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10	<title>Networking Activity of the CARE Integrating Activity project</title>
11	<!-- saved from url=(0071)http://www.lal.in2p3.fr/recherche/delphi/bambade/esgard/NA_skeleton.htm -->
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15
16	<blockquote>
17	<blockquote>
18	<blockquote>
19	<div align="left"><b><font face="Arial,Helvetica"><font size="+3"><font
20	color="#ff0000">B</font><font color="#000000">eams</font><font
21	color="#ff0000"> </font><font color="#000000">for</font><font
22	color="#ff0000"> European N</font><font color="#000000">eutrino </font><font
23	color="#ff0000">E</font><font color="#000000">xperiments (</font><font
24	color="#ff0000">BE</font></font></font></b><font size="+3"><font
25	color="#cc0000">ν</font></font><b><font face="Arial,Helvetica"><font
26	size="+3"><font color="#ff0000">E</font><font color="#000000">)</font></font></font></b>
27	</div>
28	</blockquote>
29	</blockquote>
30	</blockquote>
31
32	<p align="center"> </p>
33
34	<hr width="100%"> <br>
35	<font size="+3">Networking Activity:<b> <font color="#ff0000">N3</font></b></font>
36	<br>
37
38	<blockquote><font size="+3">Topic:<b> <font color="#ff0000">Neutrino </font></b></font><font
39	size="+3"><b><font color="#ff0000">beams of superior intensity and quality</font></b></font>
40	<br>
41	</blockquote>
42	<font size="+3">Co-ordinator:<b> <font color="#ff0000">Vittorio Palladino
43	(INFN-Napoli, Italy)</font></b></font>
44	<p><i>Draft last updated 01/02/2003
45	</i>This page prepared by : <a
46	href="mailto://vittorio.palladino@cern.ch">Vittorio Palladino</a> <br>
47	</p>
48
49	<hr width="100%"> <br>
50	<font size="+1">Link to <a
51	href="http://esgard.lal.in2p3.fr/esgard/Project/Activities/Networking/IA_forms">proposal
52	part B</a> form prepared for the IA "Coordinating Accelerator Research in
53	Europe"</font> <br>
54	<font size="+1">Link to<b> </b><a
55	href="http://esgard.lal.in2p3.fr/esgard/Project/Activities/Networking/EBNE_info.htm">more
56	information</a> provided on the subjects covered by : N4</font> <br>
57
58	<hr width="100%"> <br>
59	<b><font color="#009900"><font size="+2">Description:</font></font></b>
60	<br>
61	<br>
62
63	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
64	<caption><br>
65	</caption><tbody>
66
67	</tbody> <tbody>
68	<tr>
69	<td><b><font color="#ff0000"><i><font color="#000000">NB Text in Italic
70	should be viewed as preliminary generic text, likely to be replaced soon
71	by a more specific and suitable formulation. </font></i><br>
72	</font></b><i>Introduction and summary of the activity</i><br>
73	<br>
74	<b><font color="#ff0000"> <i>Short description meant as an
75	input to  Table 2?</i></font><br>
76	</b><br>
77
78	<div align="left"> Landmark discoveries have recently confirmed
79	that <b>the investigation of the properties of neutrinos </b><font
80	color="#000000"><small><small><big><big><big>(ν</big></big></big></small></small>)</font><b>
81	</b><b>is and will be</b> <b>revealing to us fundamental and unique
82	information on </b>the basic nature and texture of <b>fundamental matter</b>.
83	We, the <a
84	href="http://muonstoragerings.web.cern.ch/muonstoragerings/Welcome.html">Muon
85	Study Groups, endorsed by ECFA </a>since 2000,  active since 1998,
86	apply for EC support of our <b>Networking Activity. </b> Our mandate
87	is <b>to prepare the evolution of European research in the field of <font
88	color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font>
89	physics</b> beyond the present CNGS facility.  Accelerator and particle
90	physicists together and coherently intend to plan the technical effort,
91	comparing the physics reach of the different approaches, while closely
92	monitoring the rapid evolution of the field.  <br>
93	</div>
94	<br>
95	While Europe is presently building a <font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font><font
96	size="-2">μ</font><small><small>  </small></small>facility (<b>CNGS</b>)
97	based on a conventional π decay tunnel, the concept of a <b>Neutrino Factory</b>,
98	novel multi-accelerator complex whose final stage is a high energy <big><big><font
99	size="-2"><big><big>μ</big></big></font></big></big> storage & decay
100	ring, has been proposed as the ultimate tool for precise study of <font
101	color="#000000"><small><small><big><big><big><small>both</small> ν</big></big></big></small></small></font><font
102	size="-2">μ</font><font color="#ff0000"> </font>& <font
103	color="#000000"><small><small><big><big><big>ν<small><small>e </small></small></big></big></big></small></small></font>properties.
104	Its high power p-driver would also offer, however, early on the way,
105	the possibility of a <b>SuperBeam</b>, a superior conventional <font
106	color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font><font
107	size="-2">μ</font> beam (as well as of an  unprecedented facility
108	for fundamental  experiments  with  slow <big><big><font
109	size="-2"><big><big>μ</big></big></font></big></big>). In addition, the
110	unique complentary physics reach of the <b>BetaBeam</b>, pure <font
111	color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font><small>e</small>
112	beam from a high energy storage & decay ring for β-active ions, has
113	recently been pointed out at CERN, as a possible evolution of existing
114	accelerators. Our NA will investigate coherently these few attractive main
115	options<b>. </b>Integrating all the proposed studies<b>, we intend
116	to outline a </b><b>road-map </b>of technical milestones<b> leading
117	both to the most rewarding utilization of the existing facilities and to
118	</b><b>the realization of the most attractive and intense new European
119	</b><b> <font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font></b><b>
120	facility.  </b>Of this<b>, we intend to complete </b><b>a complete
121	Conceptual Design Report</b><b> by 2008. </b>We intend to foster, prepare,
122	launch and perform, assembling the necessary human and material resources,
123	all the R&D and technical preparatory work indispensable to these achievements.<br>
124	<br>
125	<b><i><font color="#ff0000">Longer description to stay here?</font></i><br>
126	</b><br>
127	<b>The investigation of the properties of the <font
128	color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font>,</b>
129	70 years after its invention, 46 after the discovery of the <font
130	color="#000000"><small><small><big><big><big><small>its first</small> ν</big></big></big></small></small></font><small>e</small>
131	species , 27 after the first indirect evidence of its third and so far last
132	<font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font><small>τ
133	</small>species, <b>is and will still long be</b> <b>revealing
134	to us fundamental and unique information </b>on the basic nature and
135	texture of fundamental matter. <br>
136	<br>
137	Recent experiments have established transitions in flight of one <b><font
138	color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font></b>
139	into another, very likely to be oscillations, over two independent long
140	baselines (LBL), Thus <b><font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font></b>
141	<b>do have</b> non zero <b>mixing </b>rates <b>and </b>non zero <b>masses</b><b>.
142	</b>The exceptional smallness of the masses points to the existence
143	of <b>new fundamental physics </b>occurring at a very high-energy scale,
144	providing indeed the first experimental data constraining it. The pattern
145	of large mixings is likely to carry the imprint of this new specific physics
146	and, even more importantly, points to the possibility of a <b>large leptonic
147	CP violation phase</b>. If true, this may be a key ingredient in the understanding
148	of the matter-antimatter asymmetry of the universe (including the existence
149	of our own physical bodies!), rooting it in a fundamental <b>asymmetry
150	of the mechanism of primordial lepto-genesis</b> by decay of very heavy
151	<b><font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font></b>.
152	<br>
153	<br>
154	This opens a field of research which will last several decades,
155	perform the complete mapping of the patterns of masses and mixings and
156	culminate with the discovery of leptonic CP violation. Long baselines
157	impose very high power, constraints on the physics at the new scale will
158	come only from statistically significant data samples. <b>These studies
159	will thus require an important investment in accelerator-based neutrino
160	beams and experiments</b>, improving significantly the present facilities
161	and/or developing new ones. <i>Proposed underground neutrino detector
162	locations, both existing and new, will also need careful scrutiny.</i><br>
163	<br>
164	The present European program (CNGS) is expected to produce decisive
165	evidence of nutau appearance. It will operate in 2006 and will, after that,
166	benefit from R&D towards improved performance. In addition. not much
167	later its operation, <b>we must have</b> a clear view of the nature, characteristics
168	and logistics of the investments necessary for a further major upgrade
169	of our discovery potential in this sector. <b> This Networking
170	Activity</b> on neutrino beams, <b>integrating all the proposed studies,
171	aims at developping</b>, from the present basic conceptual road map, <b>a
172	true road-map of technical milestones for the realization </b><b>of  an
173	upgraded and/or new European neutrino facility</b>. We plan to channel
174	all our efforts towards the <b>global strategic objective </b>of submitting,
175	to the  European funding agencies and laboratory Directors,  <b>a
176	complete Conceptual Design Report (CDR ) of  such a facility by 2008</b>,
177	that appears the earliest conceivable date for new significant investments
178	in an European particle physics program. <b><br>
179	<br>
180	</b><b>We plan to  continue to investigate coherently</b> the
181	requirements posed on accelerators by this long term program of experimental
182	LBL neutrino physics, and to define and prepare, after HARP, MUSCAT and
183	other current activities, the R&D necessary for <b>the our present few
184	main options </b>of future <b><font color="#000000"><small><small><big><big><big>ν</big></big></big></small></small></font></b>
185	beams of unprecedented intensity and quality. <font color="#cc0000">This
186	implies a number of items to be assembled</font>.<br>
187	<br>
188	<font color="#cc0000">A.<b>Consensual physics requirements</b>, mainly
189	emerging from collective studies of <b><small><small><big><big><big>ν</big></big></big></small></small></b>
190	oscillation physics, on the ultimate reach of the CNGS and on the value of
191	a Neutrino Factory,  Super-beam,  Beta-beam or combinations of
192	them (but also on the value of additional powerful facilities made possible
193	by a high power proton driver, slow muons and much  more).  It
194	will have to take  into account the likely availability of funding and
195	the state of the relevant technologies and provide indications on:
196	<br>
197	B.<b>The choice and design of a proton driver. </b>Several possibilities
198	are being considered: Superconductive Proton Linacs and similar CW machines
199	in linear or cyclotron mode and/or  Rapid Cycling Synchrotron.
200	A careful study of the pros and cons of the various option, using the HARP
201	data on particle production, could bring to definition of the baseline option
202	<b>by NUFACT05 (</b><b>spring 2005</b>)<b> followed by complete design
203	in view of the CDR</b>: <br>
204	C. and D. <b>The design of a Target and Collection Station</b>. Considerable
205	progress was achieved, in collaboration with the US, for the option
206	of a liquid metal target with collection by a high field solenoid. This requires
207	now the design and construction or refurbishment of large (20T or so) solenoid.
208	Alternative options include other targets (liquid jet, solid levitating rings,
209	solid granular targets) imbedded in a solenoid or a horn. Use of several
210	target & horn systems in parallel is also proposed. <b>Work on a proposal
211	to set up a </b><b>target test area (TTA)</b> in Europe including a beam,
212	a liquid jet and a high field solenoid <b>is in progress</b>. <b>A proposal
213	for a test area </b>to test the limits <b>of  horns </b>in term of rep.
214	rate and sustainable beam power (resistance to radiation) <b>is also being
215	prepared</b>. <b> A viable final design</b> of target and collection
216	area <b>for 4->10 MW</b> beam power, perhaps the most formidable challenge
217	of the entire program,  including aspects of safety, radiation and waste
218	disposal, <b>may thus be achieved by 2008</b>. <br>
219	D. <b>The design of the Neutrino Factory Front-end </b>(Ionization Cooling,
220	Phase rotation) <b>and of acceleration. </b>The <b>MICE experiment is being
221	proposed</b> and constitutes the major experimental effort in the area of
222	muon cooling. <b>R&D</b> <b>towards </b>cheap, high peak power, pulsed
223	<b>RF power sources and fast kickers with large acceptance</b><b> for
224	future ring coolers is being undertaken</b>. Comparative studies will be
225	necessary of the two different European and American preliminary baseline
226	front end designs (tboth based on cooling), as well as of the Japanese scheme
227	that relies on little or no cooling, by means of a cascade of  very
228	large aperture (Fixed Field Alternated Gradient) accelerators.</font> <font
229	color="#cc0000"><b>A viable final design</b> of the front end <b>can thus
230	be achieved by 2008</b>. The acceleration scheme, with re-circulating linacs
231	or with FFAG, must also be defined down to complete conceptual design. </font><br>
232	<font color="#cc0000">E <b>A first design study of a Betabeam.</b><font
233	color="#330033"> <font color="#cc0000">In preparation for that,</font></font>
234	we are considering  target development studies at ISOLDE and possibly
235	at at ISAC with high intensity proton bea,  pre-acceleration, accumulation
236	and storage studies at existing facilities (TSL in Uppsala, ESR at GSI,
237	LEIR at CERN), and low intensity test (possibly in the SPS) of the high
238	energy accumulation scheme using stable ions. <b>This could result in ?????????????</b></font><font
239	color="#cc0000"><br>
240	It should finally be kept in view that the launch of neutrino detector studies
241	and R&D, for future neutrino beams, will also become a necessity, at
242	some point.<br>
243	</font><br>
244	Such a coherent and coordinated European program on neutrino
245	beams will involve the large majority of the European experts in this
246	field and will allow Europe to play a world leader role. It will enhance
247	considerably the collaboration between accelerator physicists on the one
248	hand and will develop a synergy between particle physicists and accelerator
249	physicists on the other, ensuring the long-term sustainability of the field.<br>
250	<br>
251	Very limited resources are presently available in Europe for accelerator
252	neutrino physics. The LHC crisis appears to inevitably imply reduced support
253	from the European agencies, even to the approved CNGS program. <b>Decisive
254	added  value would result, from </b>the <b>EC support </b>that we are
255	requesting here, <b>to the strategic goal of producing a timely European
256	initiative and leadership in the fondamental area of neutrino science</b>.
257	This applies both to this Networking Activity and to R&D Projects. Among
258	those,  HIPPI, proposed within this IA, and MICE, entering soon its
259	final design phase, appear as the natural continuation of the R&D projects
260	(MUSCAT, HARP and the first BNL-CERN target experiment) that, as ECFA Muon
261	Study Groups, we have initiated in the recent past.  <br>
262
263	<br>
264	</td>
265	</tr>
266
267	</tbody>
268	</table>
269
270	<p><b><font color="#009900"><font size="+2">Objectives and Work Packages:</font></font></b>
271	<br>
272	<br>
273
274	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
275	<caption><br>
276	</caption><tbody>
277
278	</tbody> <tbody>
279	<tr>
280	<td><i>Summary of the objectives, described in terms of work packages
281	(where relevant) <br>
282	</i>The practical implementation of the program will be carried
283	out by forming <b>the following specific working groups.</b><br>
284	<i>A few words about Management and Communications should
285	be inserted here?</i>
286	<ul>
287	<li><i></i><b>Physics demands on neutrino accelerator facilities</b><i>
288	</i>Coordinator: <b>M. Mezzetto(Padova) </b><b> </b>shortname:
289	<b>PHYSICS</b>
290
291	<table cellpadding="2" cellspacing="2" border="1" width="100%">
292	<tbody>
293	<tr>
294	<td valign="top">
295
296
297	<ul>
298	<li>Monitor the development of the field of <font
299	color="#ff0000">n</font>-physics (SNO, Kamland, K2K, NuMI, ) and identify
300	the most rewarding experimental and technical strategy</li>
301	<li>Follow closely realization & operation of the
302	CNGS. Assess, at a later stage, gains in performance resulting from the HIPPI
303	Joint Research Project, enhancements of neutrino yield per proton, in particular
304	for future searches of the subdominant transition leading to nue appearance,
305	ultimate intensity limitations. Explore nature, characteristics and logistics
306	of the investments necessary for further major upgrades of the facilitiy<font
307	color="#cc33cc">.</font><b>A. Guglielmi (Padova) </b><font
308	color="#000000">is the <i>proposed </i></font><font color="#cc33cc"><font
309	color="#000000">coordinator of this subset of the effort ...</font>..</font><br>
310	</li>
311	<li> Evaluate the impact on physics of <font
312	color="#ff0000">n</font> beam characteristics (neutrino energy, baseline,
313	power & flux, energy spread, beam emittance, timing) for different
314	type of beam (Superbeam, Neutrino Factory, Betabeam).  Define a
315	strategy of successive measurements of neutrino oscillation rates with
316	different beams and baselines capable of a complete mapping of the mixing
317	matrix overcoming ambiguities, correlations & degeneracies.   </li>
318
319	</ul>
320
321
322
323	<ul>
324	<li> Identify realistic and concrete future options
325	building on existing or planned european accelerator facilities and undergound
326	neutrino detector laboratories (LNGS, Frejus etc). </li>
327	<li>Keep other interesting physics in view; in particular
328	foster the design of a new high intensity slow muon facility <b>A. V. der
329	Schaaf (Zurich)</b> is the <i>proposed </i>coordinator of this subset
330	of the effort.<font color="#cc33cc">........................  all this
331	is being  properly reformulated by the Coordinator  ......</font>
332	<a
333	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
334	color="#cc33cc"><font color="#993399">more detailed text from him WILL ALSO
335	SOON BE available her</font>e.</font></a></li>
336	<li><font color="#cc0000">Study the optimization of future
337	n beams in terms of beam energy, beam structure, composition, flux, emittance,
338	baseline etc. Study a design of the different beam options capable to reduce
339	at minimum systematic errors.</font></li>
340	<li><font color="#cc0000">Study the coherence of the
341	neutrino detector(s) located close to the Superbeam decay tunnel with the
342	beam instrumentationin target/collector/tunnel/dump areas.</font><font
343	color="#cc0000">Do the same for the Neutrino Factory and the Beta Beam.</font><font
344	color="#cc0000"><br>
345	</font> </li>
346	<li><font color="#cc0000">Monitor the development of
347	the field of </font><font color="#cc0000">n-physics (SNO, Kamland, K2K,
348	MiniBoone and further). Their results will provide the necessary information
349	for the process of optimization.<br>
350	</font> </li>
351	<li><font color="#cc0000">Define a strategy of successive
352	measurements in the different beams capable of a complete mapping of the
353	mixing matrix, including in particular the CP violating phase delta, overcoming
354	ambiguities, correlations & degeneracies. Define the possible synergies
355	between SuperBeams, BetaBeams and Neutrino Factories.</font></li>
356	<li><font color="#cc0000">CNGS ????</font> <font
357	color="#cc0000">(A possible formulation: in collaboration with the experiments
358	consider it among the players of the previous topic)</font><br>
359	</li>
360
361	</ul>
362
363	<ul>
364	<li><font color="#cc0000"> Identify realistic and concrete
365	future options building on existing or planned european accelerator facilities
366	and undergound neutrino detector laboratories (LNGS, Frejus etc).</font></li>
367	<li><font color="#cc0000">Identify
368	and promote a serie of ancillary experiments devoted to reduce the experimental
369	systematic errors:  measurements of neutrino cross sections, particle
370	identification, charge identification etc.<br>
371	</font> </li>
372	<li><font color="#cc0000">Implement the results of dedicated
373	experiments (Muscat, Harp) in the simulation Monte Carlo codes. Promote
374	the developing of MonteCarlo codes suitable to the simulation of the future
375	beam lines.<br>
376	</font> </li>
377	<li><font color="#cc0000">Keep other interesting physics
378	in view; in particular foster the design of a new high intensity slow muon
379	facility <b>A. V. der Schaaf (Zurich)</b> is the <i>proposed </i>coordinator
380	of this subset of the effort.</font></li>
381
382	</ul>
383
384	</td>
385	</tr>
386
387
388	</tbody>
389
390	</table>
391	</li>
392	<li><b>Present neutrino facilities: CNGS and its upgrades</b><i>
393	Proposed </i>Coordinator:<b> A. Guglielmi (Padova) </b> <i>proposed
394	</i>shortname: <b>CNGS</b>       <b>............
395	MOVED ABOVE .... IT WILL DISAPPEAR IF NO NEW CIRCUMSTANCES ARISES </b>
396
397
398	<table cellpadding="2" cellspacing="2" border="1" width="100%">
399	<tbody>
400	<tr>
401	<td valign="top">
402
403
404	<ul>
405	<li><br>
406	</li>
407
408	</ul>
409	</td>
410	</tr>
411
412
413	</tbody>
414
415	</table>
416	</li>
417	<li><b>High Power proton drivers</b> Coordinator:<b> P.
418	Debu (CEA) </b>shortname: <b>DRIVER</b>
419
420
421	<table cellpadding="2" cellspacing="2" border="1" width="100%">
422	<tbody>
423	<tr>
424	<td valign="top">
425
426
427	<ul>
428	<li>Perform the studies of the several critical elements
429	demanded for R&D towards high intensity proton drivers:
430
431
432
433
434
435
436	a reliable intense source of H- ions,
437
438
439
440
441
442
443
444
445
446
447	a very fast beam chopper
448	to select the bunches to be injected inside the following synchrotron buckets,
449
450
451
452
453
454
455	the various accelerating structures, drift tube linacs, hybrid drift
456	tube linacs, coupled cavities, side coupled linacs, low b superconducting
457	structures, the RF system
458
459	the high intensity beam diagnostics and a very precise beam dynamics
460	simulation code to estimate the beam halo and losses </li>
461	<li>Share the expertise among the various laboratories
462	and establish a common R&D strategy</li>
463	<li>Assess and disseminate the results of the Joint Research
464	Project on High Intensity Pulsed Proton Injectors (HIPPI) which is proposed
465	within this IA (I3).  </li>
466	<li>Progress on the conceptual design of  a Rapid
467	Cycling Synchrotron ring alternative and/or complementary to Superconducting
468	Proton Linac  <font color="#cc33cc">.................. all this is
469	to be revised, refined and finalized  by the Coordinator  .</font><a
470	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
471	color="#cc33cc"><font color="#993399">more detailed text from him available
472	her</font>e.</font></a></li>
473
474	</ul>
475	</td>
476	</tr>
477
478
479	</tbody>
480
481	</table>
482	</li>
483	<li><b>High power targets (concept, materials, installations)</b> Coordinator<b>
484	R.Bennett (RAL) </b><b> </b>shortname: <b>TARGET</b>
485
486
487	<table cellpadding="2" cellspacing="2" border="1" width="100%">
488	<tbody>
489	<tr>
490	<td><font color="#cc33cc"> </font>
491
492
493
494	<ul>
495	<li>Review the oustandingly severe technical problems
496	in dissipating high power densities in targets for the proposed neutrino
497	factories 1)  effective heat removal  2) sustainability of
498	severe pulsing shock waves 3) operation in large B field  4) integration
499	in densely packed general layout 5) guarantee of safety in operation,
500	maintenance & disposal </li>
501	<li>Review merits & limitations of main leading
502	technologies (molten metal jet or contained flow, tantalum spheres,  rotating
503	bands ... ), none yet conclusively shown to work. Explore all new emerging
504	options.  </li>
505	<li>Define an R&D roadmap towards solutions capable
506	to overcome limitations, actively liasing with similar efforts for pulsed
507	neutron facilities and radioactive beam facilities, in Europe, the USA
508	and Japan .</li>
509	<li>Form R&D project collaborations aiming at proving
510	realistic, safe and economic feasibility of one or more option.
511	NB the target sector apperas as the one most dangerous potential show stopper
512	at the moment!  <font color="#cc33cc">.................. all this
513	is to be revised, refined and finalized  by the Coordinator  .</font>
514	<a
515	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
516	color="#cc33cc"><font color="#993399">more detailed text from him available
517	her</font>e.</font></a></li>
518	<li>The following issues need to be addressed:<br>
519	<br>
520	1.    Thermal dissipation and distribution in the target due
521	to the beam<br>
522	2.    Thermal dissipation and distribution in the beam dump
523	due to the beam<br>
524	3.    Thermal dissipation and distribution in the surroundings
525	– horn, solenoid etc.<br>
526	4.    Radiation damage to the target<br>
527	5.    Radiation damage to the beam dump<br>
528	6.    Radiation damage to the surroundings – horn, solenoid
529	etc.<br>
530	7.    Thermal cooling studies for the different target designs
531	and the beam dump<br>
532	Impact on the surroundings – horn, solenoid etc.<br>
533	Water cooling requirements; activity in water. Helium cooling and activity.<br>
534	8.    Nuclear radiation heating and cooling in the target
535	and the surroundings<br>
536	9.    Evolution of gases from the targets and surroundings.
537	<br>
538	Assess radioactive inventory and disposal.<br>
539	10.    Shock stress in solid targets and lifetime<br>
540	11.    Effects of pulsed proton beam on mercury jets<br>
541	12.    Effects of pulsed proton beam on contained flowing
542	mercury targets<br>
543	13.    Effects of the magnetic field on the jet, contained
544	mercury and rotating band targets<br>
545	14.    Mechanical design and maintenance of each target design
546	and the beam dump<br>
547	The impact on the surroundings – horn, solenoid etc.<br>
548	15.    Disposal of radioactive items<br>
549	16.    Are proton and pion beam windows required? <br>
550	Design of proton beam windows at this intensity<br>
551	17.    Health and Safety issues – radiation and chemical (with
552	mercury)<br>
553	18.    Safety legislation - requirements<br>
554	</li>
555
556	</ul>
557	</td>
558	</tr>
559
560
561	</tbody>
562
563	</table>
564	</li>
565	<li><b>High power collection systems (horns, solenoids, etc)</b><i>
566	</i>Coordinator<b>  J. E. Campagne (LAL) </b><i> </i>shortname:
567	<b>COLLECTOR</b>
568
569	<table cellpadding="2" cellspacing="2" border="1" width="100%">
570	<tbody>
571	<tr>
572	<td><font color="#cc33cc"> </font>
573
574
575
576	<ul>
577	<li>Study limitations of the present technologies
578
579
580
581
582
583
584
585
586
587
588	consequences of high
589	power dissipation in targets for the design of collection systems
590
591
592
593
594
595
596
597	resistance of different materials proposed  for
598	collectors operating under severe radiation condition
599
600
601
602
603
604
605	simulated predictions  of thermal stress, mechanical stresses
606	and fatigue from  neutron irradiation
607
608
609
610
611
612	</li>
613	<li>Estimate reliably  lifetime expectations under
614	unprecedented operation conditions (highly radiactive enviroments at high
615	repetetition rate).
616
617
618	</li>
619	<li>compare focusing and collection capabilities of the
620	few main options of collection systems, as simulated by the few main existing
621	codes</li>
622	<li>define, in collaboration with the TARGET team,
623	a viable solution to all the integration problems imposed by the need of
624	locating the target inside the collector</li>
625	<li>form R&D projects and establish collaborations
626	for the design and test of horns and other collection systems,.as they
627	are likely to evolve to cope with increasingly severe conditions, from
628	the present conventional beams up to full power neutrino factories
629	<font color="#cc33cc">........................ </font><font
630	color="#cc33cc"> a</font><font color="#cc33cc">ll this is to be revised,
631	refined and finalized  by the Coordinator  .</font>  <a
632	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
633	color="#cc33cc"><font color="#993399">more detailed text from him available
634	her</font>e.</font></a></li>
635	<li><font color="#cc0000">The major motivation of a Network
636	Activity and also R&D studies in this field  is that the collection
637	system for the future neutrino beams will have to keep up with unprecendent
638	challenging conditions as such as 1) more than one order magnitude more electric
639	stresses (expressed in A.Hz) than the MiniBOON Horn and  more than two
640	orders of magnitudes than the present K2K Horn and the future NuMI and CNGS
641	Horns and 2) a huge rapid neutron flux 10^22n/cm^2/6weeks due to the necessary
642	integration of the TARGET inside the COLLECTOR system. The NA will attack
643	the challenge by</font> </li>
644	<li><font color="#cc0000"> Defining, in collaboration with
645	the TARGET team,  a viable solution to all the integration problems
646	imposed by the need of locating the target inside the collector: neutron
647	radiation, heat load...</font></li>
648	<li><font color="#cc0000"> Comparing focusing and collection
649	capabilities of the few main options of collection systems, as simulated
650	by the few main existing codes</font></li>
651	<li><font color="#cc0000"> Conducting particle production
652	and collection simulations using different Monte Carlo programs: GEANT, MARS,... </font></li>
653	<li><font color="#cc0000"> Conducting simulation of
654	thermal and mechanical stresses of the collection systems to define the critical
655	points </font></li>
656	<li><font color="#cc0000"> Studing resistance of different
657	materials proposed  for collectors operating under severe radiation
658	conditions</font></li>
659	<li><font color="#cc0000"> Studing the cooling system to
660	optimize  the operating heating temperature of the alloy </font></li>
661	<li><font color="#cc0000"> Estimating reliably  lifetime
662	expectations under unprecedented operation conditions (highly radioactive
663	enviroments at high repetetition rate). </font></li>
664	<li><font color="#cc0000"> Proposing R&D projects and
665	establishing collaborations for the design and test of horns and other collection
666	systems, as they are likely to evolve to cope with increasingly severe conditions,
667	from the present conventional beams up to full power neutrino factories </font></li>
668	<li><br>
669	</li>
670
671	</ul>
672	</td>
673	</tr>
674
675
676	</tbody>
677
678	</table>
679	</li>
680	<li><b>Muon Front End (ionization cooling , phase rotatiion etc
681	) </b>Coordinator:<b> R. Edgecock (RAL)  </b><b> </b>shortname: <b>COOLING</b>
682
683
684	<table cellpadding="2" cellspacing="2" border="1" width="100%">
685	<tbody>
686	<tr>
687	<td valign="top"><font color="#cc33cc"> </font>
688
689
690
691	<ul>
692	<li>Develop the baseline European  design of the
693	muon front end, including more realistic RF and B fields and engineering
694	context.</li>
695	<li>Investigate alternative front end designs, ranging
696	from extended (cooling rings) to no application of cooling. <br>
697	</li>
698	<li>Establish, through detailed simulation,  plans
699	for additional experiments in MICE beyond its baseline plans</li>
700	<li>Assess the potential of MICE as a general tool to
701	measure emittance reduction of  a variety of front end designs. </li>
702	<li>Outline the road map for assessing muon front ends
703	and defining the R&D towards the realization of one</li>
704	<li>Consolidate the links with the front end R&D
705	geoups  in US and Japan <font color="#cc33cc">.......................
706	</font><font color="#cc33cc"> a</font><font color="#cc33cc">ll
707	this is to be revised, refined and finalized  by the Coordinator
708	.</font>  <a
709	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
710	color="#cc33cc"><font color="#993399">more detailed text from him available
711	her</font>e.</font></a></li>
712
713	</ul>
714
715
716
717	</td>
718	</tr>
719
720
721	</tbody>
722
723	</table>
724	</li>
725	<li><b>Beta-beams R&D (ion sources, acceleration, storage)</b><i>
726	</i>Coordinator: <b>M. Lindroos(CERN) </b><b> </b>shortname:
727	<b>BETABEAM</b>
728
729	<table width="100%" border="1" cellspacing="2" cellpadding="2">
730	<tbody>
731	<tr>
732	<td valign="top">
733
734
735	<ul>
736	<li>A "green field" study of a betabeam facility to
737	establish limits imposed by using existing facilities and to create
738	a site independent alternative </li>
739	<li> A R&D roadmap including preparation (or execution,
740	where possible) of R&D project collaborations, like
741
742
743
744	1) target development studies
745	at ISOLDE with possible tests at ISAC with high intensity proton beam
746
747
748
749	2) pre-acceleration, accumulation
750	and storage studies at existing facilities (TSL in Uppsala, ESR at GSI,
751	LEIR at CERN)
752
753	3) low intensity test (in the SPS ? )
754	of the high energy accumulation scheme using stable ions</li>
755	<li>Preparation of a proposal for a Design Study of all
756	different parts of a complete beta beam facility.      <font
757	color="#cc33cc">.......................  </font><font
758	color="#cc33cc"> a</font><font color="#cc33cc">ll this is to be revised,
759	refined and finalized  by the Coordinator  .</font>  <a
760	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/Network,%20TARGETS.doc"><font
761	color="#cc33cc"><font color="#993399">more detailed text from him available
762	her</font>e.</font></a>
763	</li>
764
765	</ul>
766	</td>
767	</tr>
768
769	</tbody>
770
771	</table>
772	</li>
773
774	</ul>
775
776	<ul>
777
778	</ul>
779	</td>
780	</tr>
781
782	</tbody>
783	</table>
784	</p>
785
786	<p><b><font color="#009900"><font size="+2">Contracting Participants:</font></font></b>
787	<br>
788
789	<table width="100%" cols="5" border="1" bgcolor="#ffffff">
790	<tbody>
791	<tr>
792	<td width="6" align="center"><b>Participant number</b></td>
793	<td align="center"><b>Organisation name <br>
794	</b> <b>(and short name)</b></td>
795	<td align="center" width="6"><b>Local responsible</b> <b>and
796	team members, number of FTE (incl. associated members)</b></td>
797	<td align="center"><b>Interests, expertise </b> <b>(and
798	relevant WPs)</b></td>
799	<td align="center"><b>Associated members (short names), number
800	of FTEs</b></td>
801	</tr>
802	<tr>
803	<td align="center">1  (co-ordinator)</td>
804	<td align="center">Sezione <br>
805	INFN<br>
806	Napoli, Italy<br>
807	<b>(INFN-<font color="#ff0000">nu</font></b>)<br>
808	</td>
809	<td align="center" width="6">Vittorio.Palladino@napoli.infn.it<font
810	color="#3366ff"> <br>
811	<a
812	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">>8
813	scientists, >0,7 FTE</a><br>
814	</font></td>
815	<td align="justify"> <font
816	face="Times New Roman, Times, serif"><small>Organization co-ordinating
817	a consortium of physicists fr</small></font><font
818	face="Times New Roman, Times, serif" size="-1">om Italian Universities and
819	Sezioni INFN (see Table below) contributing long term expertise in the
820	field of neutrino physics, experiments & beams (design, detailed simulation,
821	operation and analysis of their data), involved in several major R&D
822	projects in progress (HARP,MICE). It will contribute  to  the
823	<b>general </b>steering </font><font size="-1">and to the <b>PHYSICS,
824	COLLECTOR, COOLING and BETABEAM</b> WPs</font><br>
825	</td>
826	<td align="center"><font color="#3366ff">Padova, Genova,
827	Legnaro, Milano and possibly more<br>
828	<br>
829	</font></td>
830	</tr>
831	<tr>
832	<td align="center">2</td>
833	<td>
834
835	<div align="center"> Laboratori. Nazionali<br>
836	INFN, Frascati, Italy <br>
837	(<b>LNF</b>)</div>
838	</td>
839	<td width="6" align="center">Michele.Castellano or<br>
840	Mauro.Migliorati@lnf.infn.it <font color="#3366ff"><a
841	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition"><br>
842	3 scientists, 0,6 FTE</a><br>
843	</font><br>
844	</td>
845	<td align="justify">
846	<div align="justify"><small>T<font size="-1">he Laboratory will contribute
847	to the studies of </font></small><font size="-1"><b>COOLING </b>techniques
848	both theoretical (simulation, design) and experimental (measurements of
849	emittances) as well as to the <b>general </b>steering <i>(and to the <b>PHYSICS
850	</b></i></font><small><font size="-1"
851	face="Times New Roman, Times, serif"><small><i>WP</i>').</small></font></small></div>
852	</td>
853	<td align="center"><font color="#3366ff"> </font><font
854	color="#3366ff"> <br>
855	<br>
856	</font></td>
857	</tr>
858	<tr>
859	<td align="center">3<br>
860	<br>
861	</td>
862	<td align="center">CERN, Geneva, Switzerland<br>
863	<b>(CERN)</b><br>
864	</td>
865	<td width="6" align="center">Helmut.Haseroth@cern.ch<br>
866	<a
867	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">12
868	scientists, 1,75 FTE</a><br>
869	</td>
870	<td align="justify"><font size="-1">The Laboratory has made
871	together with other European labs a feasibility study for a Neutrino Factory
872	and is currently building the next European neutrino beam (CNGS). It will
873	provide expertise and some leadership in the R&D for a neutrino factory
874	in general and specifically in target technology. Theoretical and experimental
875	among the users physicists will be contributing leading expertise in the
876	field of neutrino physics, experiments & beams and promotion of betabeam
877	studies. Depending on the requirements excellent test beams may be available.
878	</font><font face="Times New Roman, Times, serif" size="-1">It will
879	contribute  to  the <b>general </b>steering </font><font
880	size="-1">and to the <b>TARGET, COLLECTOR, COOLING, BETABEAM</b></font>
881	<font size="-1">WPs</font> <font size="-1"><i>and  probably
882	more</i></font>. </td>
883	<td align="center"><font color="#3366ff"> </font><font
884	color="#3366ff"><br>
885	</font></td>
886	</tr>
887	<tr>
888	<td valign="top" align="center"><br>
889	<br>
890	<br>
891	4<br>
892	<br>
893	</td>
894	<td valign="top" align="center"> Univ. of Geneva,  Geneva,
895	Switzerland<br>
896	<b>(CH-<font color="#ff0000">nu</font>)<br>
897	</b><br>
898	</td>
899	<td valign="top" width="6" align="center">Alain.Blondel@unige.ch
900	or Andre.Rubbia@cern.ch<a
901	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition"><br>
902	2 scientists, ? FTE</a><br>
903	</td>
904	<td valign="top" align="justify"><font size="-1"> Organization
905	coordinating a consortium of physicists from Swiss Universities (including
906	ETH and Zurich) contributing long term expertise in the field of neutrino
907	physics, experiments &  beams (design, detailed simulation, operation
908	and analysis of their data), expertise in horn technology and in the
909	field of intense low energy muon beams and leadership in the experimental
910	studies of muon ionisation cooling,.   It will contribute
911	to  the <b>general </b>steering and to the <b>PHYSICS, TARGET, HORN,
912	COOLING </b>WPs <i>and  probably more</i></font>.<br>
913	</td>
914	<td valign="top" align="center"><font color="#3366ff"><br>
915	<br>
916	Zurich, ETH?,      Novosibirsk?<br>
917	<br>
918	</font></td>
919	</tr>
920	<tr>
921	<td valign="top" align="center"><br>
922	5<br>
923	<br>
924	</td>
925	<td valign="top">
926
927	<div align="center"> Paul Scherrer Institute, Villigen, Switzerland<br>
928	<b>(PSI</b>)<br>
929	</div>
930	<br>
931	</td>
932	<td valign="top" width="6" align="center">Knud.Thomsen@psi.ch<br>
933	<a
934	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">2
935	scientists, 0,2 FTE</a><br>
936	</td>
937	<td valign="top" align="justify"><small> The Laboratory operates
938	the highest power proton machine presently available and can </small><font
939	size="-1">contribute long term expertise in most sectors</font><small>. It
940	will specifically contribute to the <b>general </b>steering and to the studies
941	of <b>TARGET </b>technologies. </small><small> </small><br>
942	</td>
943	<td valign="top" align="center"><font color="#3366ff"> <br>
944	</font></td>
945	</tr>
946	<tr>
947	<td valign="top" align="center"><br>
948	<br>
949	6<br>
950	</td>
951	<td valign="top" align="center"> Rutherford Appleton Laboratory,
952	Didcot,UK<br>
953	<b>(CCLRC)</b><br>
954	</td>
955	<td valign="top" width="6" align="center">P.R.Norton@rl.ac.uk
956	or  K.Peach@rl.ac.uk<br>
957	<a
958	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">?
959	scientists, ? FTE</a><br>
960	</td>
961	<td valign="top" align="justify"><small> T<font
962	size="-1">he Laboratory will contribute to the studies towards a Neutrino
963	factory in general, and specifically to studies of proton drivers and
964	targets. It is providing the home and the technical and human resources
965	to make experimental studies of muon ionisation cooling possible. </font><i><font
966	color="#ff0000" size="-1">Infrastructure providing access?</font></i></small><font
967	size="-1"> It will contribute to the <b>general </b>steeering and to the
968	<b>PHYSICS, DRIVER, TARGET, COOLING </b>WPs <i>and probably more ....</i>
969	<font face="Times New Roman, Times, serif"> <i> </i></font><i><font
970	color="#3366ff">to be revised by the local responsible</font></i></font><br>
971	</td>
972	<td valign="top" align="center"><font color="#3366ff"> all
973	the UK Universities?<br>
974	<br>
975	ITEP?<br>
976	<br>
977	<br>
978	</font></td>
979	</tr>
980	<tr>
981	<td valign="top" align="center"><br>
982	<br>
983	7<br>
984	</td>
985	<td valign="top" align="center"> Imperial College, London,
986	UK<br>
987	<b>(UK-</b><b><font color="#ff0000">nu</font></b><b>)</b><br>
988	</td>
989	<td valign="top" width="6" align="center">Kenneth.Long@ic.ac.uk<br>
990	<a
991	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">? scientists,
992	? FTE</a>  <br>
993	<br>
994	</td>
995	<td valign="top"><small> Organization coordinating a consortium
996	of physicists from UK Universities, including Oxford <i>and who else?,</i>
997	contributing long term expertise in the field of neutrino physics, experiments
998	& beams), involved in most major R&D projects in progress (HARP,
999	MUSCAT, MICE).</small><small> </small><font size="-1">It will contribute
1000	to  the <b>general </b>steeering and to the  <b>PHYSICS, DRIVER,
1001	TARGET, COOLING </b>WPs <i>and probably more.</i> <font
1002	face="Times New Roman, Times, serif">  </font><i><font
1003	color="#3366ff">to be revised by the local responsible</font></i></font><br>
1004	</td>
1005	<td valign="top" align="center"><font color="#3366ff"> Oxford?
1006	A few more?<br>
1007	<br>
1008	</font></td>
1009	</tr>
1010	<tr>
1011	<td valign="top" align="center"><br>
1012	8<br>
1013	<br>
1014	</td>
1015	<td valign="top" align="center"> Forschungszentrum, Julich,
1016	Germany <br>
1017	<b>(FZJ)</b><br>
1018	</td>
1019	<td valign="top" width="6" align="center">g.bauer@fz-juelich.de<br>
1020	<a
1021	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">?
1022	scientists, ? FTE</a><br>
1023	</td>
1024	<td valign="top">
1025	<div align="justify"><small><small><small> The Laboratory will contribute
1026	to the <b>general </b>steering and to studies of </small></small></small><small>high
1027	power</small><small><small><small><b> TARGETry </b></small></small>and related
1028	technologies with emphasis on liquid metal targets and their enclosure. The
1029	main sectors will be:</small><small> studies relating to the effects of pressure
1030	wave mitigation in targets exposed to intense short pulses of energetic particles;</small><small>
1031	radiation effects in target walls and on the wall-liquid interface;</small><small>
1032	fluid dynamics and thermal hydraulics/ thermomechanics</small><small>, spallation
1033	products and associated technology issues;</small><small> loop components,
1034	diagnostics and remote handling issues;</small><small> waste management</small>.<small><small>
1035	</small><font size="-1"><small><i><font color="#3366ff">to be revised
1036	by the local responsible</font></i></small></font></small><br>
1037	</div>
1038	</td>
1039	<td valign="top" align="center"><font color="#3366ff"><br>
1040	</font>Institute of Physics, University of Latvia(IPUL), <br>
1041	<br>
1042	<br>
1043	NRG, Petten, NL<br>
1044	</td>
1045	</tr>
1046	<tr>
1047	<td valign="top" align="center"><br>
1048	9<br>
1049	</td>
1050	<td valign="top" align="center">GSI (Gesellshaft fur Schwerionenforschung)<br>
1051	Darmstadt, Germany<br>
1052	<b>(GSI)</b><br>
1053	</td>
1054	<td valign="top" width="6" align="center">B.Franzke@gsi.de<br>
1055	<a
1056	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">5
1057	scientists, 0,5 FTE</a>  <br>
1058	</td>
1059	<td valign="top" align="justify"><small> The Laboratory will
1060	contribute to the studies of beam dynamics in general, high intensity
1061	phenomena, beam stability</small><small><font size="-1"
1062	face="Times New Roman, Times, serif"><small>. Main interest is in the <b>general
1063	</b>steering and  in the <b>BETABEAM </b>WP. .</small></font><font
1064	size="-1" face="Times New Roman, Times, serif"><small>.. </small></font></small><small><font
1065	size="-1" face="Times New Roman, Times, serif"><small><i><small> </small><font
1066	size="-1"><i><font color="#3366ff">to be revised by the local responsible</font></i></font></i></small></font></small><br>
1067	</td>
1068	<td valign="top" align="center"><font color="#3366ff"> <br>
1069	</font></td>
1070	</tr>
1071	<tr>
1072	<td valign="top" align="center"><br>
1073	10<br>
1074	</td>
1075	<td valign="top" align="center"> Technical University Muenchen,
1076	Germany<br>
1077	<b>(D-</b><b><font color="#ff0000">nu</font></b><b>)</b><br>
1078	</td>
1079	<td valign="top" width="6" align="center">Manfred.Lindner@ph.tu-muenchen.de<br>
1080	<a
1081	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">5
1082	scientists, 2,05 FTE</a><br>
1083	</td>
1084	<td valign="top">
1085	<div align="justify"> <font size="-1">Organization grouping around it
1086	a consortium of physicists from Germany Universities, <i>including Dortmund</i>,
1087	contributing long term expertise in the field of neutrino <i>and muon
1088	</i>physics and experiments.  It will contribute to the <b>general
1089	</b>steering and studies of the <b>PHYSICS </b>potential of future
1090	long baseline experiments. The studies aim at guiding the exploration, planning
1091	and construction of conceivable setups by identifying the capabilities and
1092	the crucial components and limitations.<br>
1093	</font></div>
1094	</td>
1095	<td valign="top">
1096	<i>Dortmund? </i><br>
1097	</td>
1098	</tr>
1099	<tr>
1100	<td valign="top" align="center"><br>
1101	11<br>
1102	<br>
1103	</td>
1104	<td valign="top" align="center"><br>
1105	CEA/DSM/DAPNIA, Saclay, France (CEA)<br>
1106	<b>(CEA</b><b>)</b><br>
1107	</td>
1108	<td valign="top" width="6" align="center">pascal.debu@cea.fr<a
1109	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition"><br>
1110	17 scientists, 2,0 FTE</a><br>
1111	</td>
1112	<td valign="top" align="justify"><font size="-1">The laboratory
1113	will mostly contribute to the studies of high power proton <b>DRIVERs </b>especially
1114	the low energy end, but also to <b>general </b>steering, to the definition
1115	of the <b>PHYSICS </b>demands on neutrino accelerator facilities, the <b>COLLECTOR
1116	</b>systems, the <b>COOLING </b>effort and the <b>BETABEAM </b>R&D.<br>
1117	</font> </td>
1118	<td valign="top" align="center"><font color="#3366ff"> <br>
1119	<br>
1120	</font></td>
1121	</tr>
1122	<tr>
1123	<td valign="top" align="center"><br>
1124	<br>
1125	12<br>
1126	<br>
1127	</td>
1128	<td valign="top" align="center"><br>
1129	IN2P3, France<br>
1130	<b>(IN2P3-</b><b><font color="#ff0000">nu</font></b><b>)</b><br>
1131	</td>
1132	<td valign="top" width="6" align="center">Stavros.Katsanevas@admin.in2p3.fr<br>
1133	<a
1134	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">9
1135	scientists, 2,35 FTE</a>  <br>
1136	</td>
1137	<td valign="top" align="justify"><font size="-1">The Institute
1138	will coordinate a consortium including physicists from French CNRS and University
1139	Laboratories  (IPN Lyon, LAL, LPNHE Paris VI&VII) contributing long
1140	term expertise in the field of neutrino <b>PHYSICS, </b>experiments &
1141	beams. It expects then to contribute to the <b>general </b>steering and provide
1142	technical expertise in the field of <b>COLLECTOR </b>technology (</font><font
1143	size="-1">and of  </font><font size="-1"><b><font
1144	color="#cc0000">BETABEAM ????</font></b> )</font> <font size="-1">design
1145	studies.</font><font size="-1"><small><font size="-1"
1146	face="Times New Roman, Times, serif"><small>.. </small></font></small><small><font
1147	size="-1" face="Times New Roman, Times, serif"><small><i><small> </small><font
1148	size="-1"><i><font color="#3366ff">to be revised by the local responsible</font></i></font></i></small></font></small></font><br>
1149	</td>
1150	<td valign="top" align="center"><font color="#3366ff"> IPN
1151	Lyon, LAL, LNPHE Paris 6&7<br>
1152	</font></td>
1153	</tr>
1154	<tr>
1155	<td valign="top" align="center"><br>
1156	<br>
1157	13<br>
1158	</td>
1159	<td valign="top" align="center"> Univ. of Barcelona, Barcelona,
1160	Spain<br>
1161	<b>(E-</b><b><font color="#ff0000">nu</font></b><b>)</b><br>
1162	</td>
1163	<td valign="top" width="6" align="center">Federico.Sanchez@ifae.es<br>
1164	<a
1165	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">?
1166	scientists, ? FTE</a>  <br>
1167	</td>
1168	<td valign="top"><small>Organization coordinating a consortium
1169	of physicists from Spanish contributing long term expertise in the field
1170	of neutrino <b>PHYSICS </b>experiments & beams, involved in major
1171	R&D projects in progress (HARP). This consortium  provides recognized
1172	leadership in the <b>general </b>steering and identification of the physics
1173	reach of future neutrino facilities.</small> <font size="-1"> <small><font
1174	size="-1" face="Times New Roman, Times, serif"><small> .</small></font><font
1175	size="-1" face="Times New Roman, Times, serif"><small>.. </small></font></small><small><font
1176	size="-1" face="Times New Roman, Times, serif"><small><i><small> </small><font
1177	size="-1"><i><font color="#3366ff">to be revised by the local responsible</font></i></font></i></small></font></small></font><br>
1178	</td>
1179	<td valign="top" align="center"><font color="#3366ff"> Valencia?
1180	Madrid? <br>
1181	</font></td>
1182	</tr>
1183	<tr>
1184	<td valign="top" align="center"><br>
1185	14<br>
1186	<br>
1187	</td>
1188	<td valign="top" align="center"> Univ. Catholique, Louvain-la-Neuve,
1189	Belgium<br>
1190	<b>(B-</b><b><font color="#ff0000">nu</font></b><b>)</b><br>
1191	</td>
1192	<td valign="top" width="6" align="center">Thierry.Delbar@fynu.ucl.ac.be<br>
1193	<a
1194	href="file:///C:/Documents%20and%20Settings/Administrator/Documenti/copia%20condivisa%20su%20pcpalladino2/EU%20application/NAComposition">3
1195	scientists, 0,6 FTE</a><br>
1196	</td>
1197	<td valign="top" align="justify"><small>Organization coordinating
1198	a consortium of physicists from universities and laboratories from Benelux,
1199	contributing long term expertise in the field of neutrino physics, experiments
1200	& beams, involved in major R&D projects in progress (HARP, MICE)
1201	expected to contribute to the <b>general </b>steering, to  the <font
1202	color="#000000"><b>COOLING </b>and the <b>BETABEAM </b></font></small><font
1203	color="#000000"><small><font size="-1"
1204	face="Times New Roman, Times, serif"><small>WP, where </small></font></small></font><font
1205	face="Times New Roman, Times" size="-1" color="#000000">it holds extensive
1206	experience in ion sources and in production of radioactive ion beams (6He,
1207	13N, 18Ne, 18F,...)</font><small><font size="-1"
1208	face="Times New Roman, Times, serif"><small> </small></font></small>
1209	<font size="-1"> <small><font size="-1"
1210	face="Times New Roman, Times, serif"><small> .</small></font><font
1211	size="-1" face="Times New Roman, Times, serif"><small>.. </small></font></small><small><font
1212	size="-1" face="Times New Roman, Times, serif"><small><i><small> </small><font
1213	size="-1"><i><font color="#3366ff">to be revised by the local responsible</font></i></font></i></small></font></small></font><br>
1214	</td>
1215	<td valign="top" align="center"><font color="#3366ff"> Bruxelles?
1216	NIKHEF? <br>
1217	</font></td>
1218	</tr>
1219
1220	</tbody>
1221	</table>
1222	</p>
1223
1224	<p> <b><font color="#009900"><font size="+2">Associated Members:</font></font></b>
1225	</p>
1226
1227	<table bgcolor="#ffffff" border="1" cols="4" width="100%">
1228	<tbody>
1229	<tr>
1230	<td><b>Organisation name </b> <br>
1231	<b>(and short name)</b></td>
1232	<td><b>Local team responsible, number of FTEs</b></td>
1233	<td><b>Interests, expertise </b> <br>
1234	<b>(and relevant WPs)</b></td>
1235	<td><b>Associated to:</b> <br>
1236	(participant short name)</td>
1237	</tr>
1238	<tr>
1239	<td>Sezione INFN Genoa, Italy<br>
1240	Sezione INFN Padova, Italy<br>
1241	Lab. Naz. INFN Legnaro, Italy<br>
1242	Sezione INFN Milano, Italy<br>
1243	Sezione INFN Roma 3, Italy <br>
1244	Bologna, Torino expressed interested<br>
1245	Bari, Trieste may still join<br>
1246	<br>
1247	<br>
1248	<br>
1249	<i> but what if INFN were just one organization? </i><br>
1250	</td>
1251	<td>Pasquale Fabbricatore  3 scientists, ? FTE's <br>
1252	Mauro Mezzetto         >1 scientist, ? FTE's
1253	<br>
1254	Ugo Gastaldi
1255	1 scientist, ? FTE  <br>
1256	Maurizio Bonesini        1 scientist, ? FTE <br>
1257	Domizia Orestano         ? scientists, ? FTE<br>
1258	Representative<br>
1259	Representative<br>
1260	<br>
1261	<br>
1262	<br>
1263	<br>
1264	<br>
1265	</td>
1266	<td>general, COLLECT, COOLING<br>
1267	general, PHYSICS, BETABEAM <br>
1268	general, DRIVING, COOLING<br>
1269	general, PHYSICS <br>
1270	<br>
1271	<br>
1272	<br>
1273	<br>
1274	<br>
1275	<br>
1276	<br>
1277	<br>
1278	</td>
1279	<td> INFN-nu</td>
1280	</tr>
1281	<tr>
1282	<td valign="top"><br>
1283	</td>
1284	<td valign="top"><br>
1285	</td>
1286	<td valign="top"><br>
1287	</td>
1288	<td valign="top"><br>
1289	</td>
1290	</tr>
1291	<tr>
1292	<td valign="top">Institute of Physics, University of Latvia(IPUL),
1293	<br>
1294	<br>
1295	</td>
1296	<td valign="top">Janis Freibergs
1297	4 scientist 1,7 FTE's <br>
1298	</td>
1299	<td valign="top">general, TARGET<br>
1300	IPUL has many years of expertise in designing and operating liquid metal
1301	loops and in developing necessary equipment and technologies. IPUL will contribute
1302	to the study and development of liquid metal high power targets and make
1303	available its existing facilities for work within the collaboration<br>
1304	</td>
1305	<td valign="top">FZJ<br>
1306	<br>
1307	</td>
1308	</tr>
1309	<tr>
1310	<td valign="top"> NRG, Petten, NL<br>
1311	</td>
1312	<td valign="top">Ed Komen
1313	? scientists, 2,5 FTE's<br>
1314	</td>
1315	<td valign="top">general, TARGET<br>
1316	NRG is experienced in fluid dynamics, structural mechanics and thermal hydraulics
1317	calculations and in developing suitable computer software. Their contribution
1318	will be to the optimisation of the target configuration under the above aspects.<br>
1319	</td>
1320	<td valign="top">FZJ<br>
1321	</td>
1322	</tr>
1323	<tr>
1324	<td align="center">ITEP, Moscow, Russia<br>
1325	(ITEP)<br>
1326	</td>
1327	<td align="center">Boris.Sharkov@itep.ru<br>
1328	<font color="#3366ff">and here?</font><br>
1329	</td>
1330	<td> The Laboratory will contribute to the studies of
1331	beam dynamics and RF technology NB As any Russian institute this can
1332	only be a  partner,  not  a participant. Groups of
1333	Russian particle physicists may be associated in similar way.</td>
1334	<td> RAL?</td>
1335	</tr>
1336	<tr>
1337	<td align="center">Novosibirsk, Russia  <br>
1338	( NSBRSK )</td>
1339	<td align="center">A.N.Skrinsky@inp.nsk.su<br>
1340	<font color="#3366ff">and here?</font><br>
1341	</td>
1342	<td>The Laboratory will contribute to the studies of RF technology,
1343	superconducting magnets, general accelerator technology. NB As any Russian
1344	instituts this can only be a  partner,  not  a participant.
1345	Groups of  Russian particle physicists may be associated in similar
1346	way.</td>
1347	<td> CH-n?</td>
1348	</tr>
1349	<tr>
1350	<td align="center"> US Muon Collider & NuFact Collaboration<br>
1351	(MUCOLL)<br>
1352	</td>
1353	<td align="center">S. Geer, spokesman,<br>
1354	Fermilab, USA </td>
1355	<td>We expect from contacts and synergy with the sister US
1356	Neutrino Factory Collaboration contributions of widest general scope aa
1357	well as significant technical  impact on the work of all WPs. </td>
1358	<td>Coordinating Organization?</td>
1359	</tr>
1360	<tr>
1361	<td valign="top" align="center">Japanese Nufact-J <br>
1362	Collaboration <br>
1363	(Nufact-J)<br>
1364	</td>
1365	<td valign="top" align="center">Y. Kuno, spokesman, <br>
1366	Univ. of Osaka,<br>
1367	Japan <br>
1368	</td>
1369	<td valign="top">We expect from contacts and synergy with the
1370	sister NuFact J Collaboration contributions of widest general scope aa well
1371	as significant technical  impact on the work of all WPs. <br>
1372	</td>
1373	<td valign="top">Coordinating Organization?<br>
1374	</td>
1375	</tr>
1376	<tr>
1377	<td valign="top"><br>
1378	</td>
1379	<td valign="top"><br>
1380	</td>
1381	<td valign="top"><br>
1382	</td>
1383	<td valign="top"><br>
1384	</td>
1385	</tr>
1386
1387	</tbody>
1388	</table>
1389
1390	<h2><font color="#009900">Deliverables and relevant milestones:</font><br>
1391	</h2>
1392
1393	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
1394	<caption><br>
1395	</caption><tbody>
1396
1397	</tbody> <tbody>
1398	<tr>
1399	<td><i>Describe the results expected from the NA, in terms of achieved
1400	designs, solutions to problems, etc...  </i>
1401	<p><i>Outline the milestones to be achieved by means of the NA, as
1402	relevant to each work package.  </i></p>
1403
1404	<p><i>Links to obtained results can also be given here (or a link to
1405	a site prepared for disseminating the acquired knowledge)</i><br>
1406	<br>
1407	</p>
1408	<br>
1409	<i><b>Describe the results expected from the NA, in terms of achieved
1410	designs, solutions to problems, etc..</b>. <br>
1411	</i> <br>
1412	<i>  .....  specify the  deliverables  ......<br>
1413	<br>
1414	The expected outcome of the NA will consist of technical notes,
1415	articles, reports, proceedings of workshops and meetings devoted to the
1416	solve (or prepare solution of) all problems necessary to launch in the
1417	shortest possible time complete conceptual design studies of a realistic
1418	option for each of the three mentioned types of future neutrino source.<br>
1419	<br>
1420	NB More work needed, considering that the main delivrables of a
1421	NA are described by the EC as  <br>
1422	-the organization of general meetings, workshops or specialized
1423	meeting with corresponding proceedings. Normally, the general meetings
1424	are meant to identify limitations, establish the state-of-the-art and share
1425	expertise, workshops and specialized meetings are meant to study particular
1426	issues.<br>
1427	Important deliverables will be also <br>
1428	-reports on comparative studies, <br>
1429	- development of roadmaps,<br>
1430	- definitions of joint research projects for which EU funding could
1431	be requested at a later stage. <br>
1432	Other delivrables could be <br>
1433	- the definition and selection of common protocols, for example
1434	for portability of software <br>
1435	-  databases <br>
1436	-  simulation codes and their maintenance. <br>
1437	In any case, a detailed plan of the activities for the 18 first
1438	months with clear objectives and delivrables should be proposed and the
1439	longer-term perspectives should be explicited.<br>
1440	A proposal for full Technical Design Study can also be given as
1441	a deliverable. </i> <br>
1442	<br>
1443	.<i>....<font color="#cc66cc"> to be done largely by the 7 coordinators
1444	first </font>and then in collegially by   the NA SG  ...
1445	for now, excerpts from contributions from Coordinators are being
1446	collected below </i><br>
1447	<br>
1448	<font color="#cc0000"><b>PHYSICS</b><b><br>
1449	</b></font>
1450	<ul>
1451	<li><font color="#cc0000">Organize 3-4 meetings/year continuing
1452	the existing activity of the ECFA neutrino oscillation working group. These
1453	meetings constitute an open forum of discussion with frequent contributes
1454	of overseas physicists. Transparencies of the meetings are regularly published
1455	on the web.<br>
1456	</font> </li>
1457	<li><font color="#cc0000">Three general reports will be written
1458	on a) the general problem of solving ambiguities, correlation and degeneracies
1459	with a set of measurements. b) the optimization of the design of future
1460	neutrino beams and the identification of the main sources of systematic
1461	errors and how to attack them. c)the definition of the roadmap for the mapping
1462	of the neutrino mixing matrix, the experimental choices and options providing
1463	the parameter list of the optimized neutrino beam characteristics.</font></li>
1464	<li><font color="#cc0000">Topical international workshops will be
1465	organized to focus on the subjects of the reports.</font></li>
1466	<li><font color="#cc0000">Regular contribution will be done to the
1467	NUFACT international workshops. In particular the budget will also used
1468	to subsidize young physicists to present their results at the conferences.<br>
1469	</font> </li>
1470	<li><font color="#cc0000">The "neutrino unbound" web site, which
1471	provides a complete, updated and elaborated information on experimental and
1472	theoretical work on the physics of neutrinos<b class="teal">, </b>will be
1473	mantained and improved. <br>
1474	</font> </li>
1475	<li><font color="#cc0000">Monte Carlo codes ....<br>
1476	</font> </li>
1477
1478	</ul>
1479	<font
1480	color="#cc0000"><b> </b></font><b>CNGS </b>?<br>
1481	<b>DRIVER.</b><br>
1482	Meetings will be held regularly (about once every 2 months) to discuss
1483	progresses, and a general workshop once a year is foreseen. Proceedings
1484	will be published describing the results obtained and the strategy to further
1485	develop the R&D topics. The broadening of expertise within the network
1486	will allow a better definition of technological developments to be undergone.
1487	The creation and maintenance of a website will facilitate the sharing of
1488	information.<br>
1489	Another important topic of the meetings and workshops will be a prospective
1490	to further extend the possible applications of such high intensity proton
1491	drivers in other physics domains and for practical applications. This would
1492	be an extra bonus to the R&D pursued within the HIPPI JRP. In addition,
1493	the regular publication of reports is a quality insurance of the JRP’s.<br>
1494	<b>TARGET </b>The main oustanding expected deliverable is a
1495	consensus on the best way forward for the successful construction of targets
1496	for a European Neutrino Factory. Individual deliverables are expected to
1497	be 1) a comprehensive summary report, reviewing the present status 2) solidly
1498	rooted links with the presently loosely tied existing world wide expertise
1499	3) establishment in Europe of the best possible up-to-date and durable
1500	knowledge base of world wide activities in target development 4) careful
1501	& structured dissemination of information and progress 4) detailed
1502	investigation and documentation of the possible solutions of the limitations
1503	of each of the technological options 5) expression of interest and proposals
1504	of  detailed and realistic R&D projects capable to prove the solutions
1505	<br>
1506	<b>COLLECTOR</b> The main expected deliverable is a comprehensive
1507	final report on horn designs, proposing multiple specific solutions respectivelly
1508	adequate to performance and lifetime requirements in a classical beam, a
1509	superbeam and ultimately in a neutrino factories.This will be based on detailed
1510	thermo-mechanical simulations, complete technical specification of electric
1511	supply and discharge equipment and state-of -the art knowledge of mechanical
1512	properties of alloys under high rate neutron irradiation. It will include
1513	specific solutions to the choices ( of material for the collection device,
1514	of machining, soldering and assembling techniques, of  heat removal
1515	and cooling system) necessary to achieve a lifetime  of 200 M pulses
1516	or more, as well as to the problems of real life integration of horn and
1517	target and of  periodic replacement of either or both after 200 M pulses,
1518	in the average.<br>
1519	<font color="#cc0000">The first deliverable for Summer 2004 will be
1520	a status report (R1) on existing collection systems used in the past and
1521	currently in operation (MiniBOON/K2K) and in construction (NuMI/CNGS). Then,
1522	till end 2006, studies will be condcuted,  to produce a detail report
1523	(R2) on a specific solution for the SuperBeam project. Then, till the end
1524	of the NA Jan. 2008, it is foreseen to produce a detail report (R3) on the
1525	different solutions that will be avaliable for the Neutrino Factory project.
1526	</font>
1527	<p><font color="#cc0000">The 2 last reports  (R2 and R3) will
1528	be based on </font></p>
1529	<blockquote>
1530	<ol>
1531	<li><font color="#cc0000"> a detailed particle collection simulations
1532	(Monte Carlo based simulations with state-of-the art code: GEANT4, MARS,...),</font></li>
1533	<li><font color="#cc0000"> thermo-mechanical simulations that implies
1534	for instence to experimentally measure some relevant parameters (heat diffusion
1535	coefficients, stress limit under high neutron fluxes and after 10^8 cycles...),</font></li>
1536	<li><font color="#cc0000"> complete technical specifications of
1537	electric power supply and discharge equipment</font></li>
1538	<li><font color="#cc0000"> state-of -the art knowledge of mechanical
1539	properties of alloys under high rate neutron irradiation as already mentionned.</font></li>
1540	</ol>
1541	</blockquote>
1542	<font color="#cc0000"> They  will include proposition of specific
1543	solutions or R&D to be conducted  necessary to achieve a lifetime
1544	of such system of few 100 Mega cycles or more. For instance, the documents
1545	will address solutions </font>
1546	<ul>
1547	<li><font color="#cc0000"> to the choices of material for the collection
1548	device,</font></li>
1549	<li><font color="#cc0000"> of machining, soldering and assembling
1550	techniques,</font></li>
1551	<li><font color="#cc0000"> of  heat removal and cooling system,</font></li>
1552	<li><font color="#cc0000">  to the problems of TARGET integration
1553	in the collection system</font></li>
1554	<li><font color="#cc0000"> and of  periodic replacement in a
1555	high radioactive environment.</font></li>
1556	</ul>
1557	<font color="#cc0000"> Other deliverables will be intermediate specialized
1558	notes and worshop proceedings that will be used for the final <br>
1559	document, and simulation programs that will be worth to develop for these
1560	studies. </font><br>
1561	<br>
1562	<b>COOLING </b>Main deliverables are 0) Formation of a European
1563	muon front end network , with consolidated link with US and Japan 1) Determination
1564	of the performance of the European  design incorporating realistic
1565	fields and real engineerization. 2) Simulation of cooling free  front
1566	ends in  comparison with our baseline; quantitative appraisal  of
1567	the indispensability of cooling 3) Simulation of front ends based on cooling
1568	rings 4)Assessment of the technologies required by <i>1)2) & 3)</i> and
1569	of  their feasibility 5) Proposal of a coherent R&D program as a
1570	result of this assessment 6) Determination of the resolution of MICE (in
1571	the measurement of emittance and emittance reduction) and of its potential
1572	beyond its baseline measurements plans <br>
1573	<b>BETABEAM</b><br>
1574	We aims at a team including RAL, TSL in Uppsala, GSI, GANIL, INFN Legnaro
1575	associating TRIUMF and FermiLab. Its expected deliverables in the first
1576	18 months are <br>
1577	1) Meeting at GSI in September 2003: Follow up of Moriond in March and
1578	discussions on possible synergy with the future GSI design study.2) International
1579	workshop on a beta-beam facility in June 2004 3) Theoretical study and appraisal
1580	of experimental tests of longitudinal stacking scheme for the decay ring
1581	(in the CERN PS) 4) Computer simulation and theoretical study of losses
1582	in the decay ring 5) Proposal for targets to be tested for the production
1583	of suitable beta-beam isotopes 6) Study of cyclotron injection into a storage
1584	ring using a charge injection scheme (TSL and Triumf) 7) Study of dynamic
1585	aperture in the SPS (RAL)<br>
1586	A comprehensive report, "Ideas for a beta-beam facility", would conclude
1587	the first 18 months  Further meetings would be held at least once a
1588	year but it will depend on a possible design study. Reports will be delivered
1589	as conference papers and as CERN reports. The next stage would be a conceptual
1590	design report but the likely date for that would heavily depend on a possible
1591	design study.<br>
1592	Only fresh resources, presently unavailable, would evidently permit
1593	us to address a larger number of issues such as: lattice for decay ring
1594	and storage ring, optics for transfer lines and injection line, full simulation
1595	of stacking scheme, full simulation of losses, test of injection schemes
1596	(both storage ring and decayring), construction and test of prototype target
1597	at ISOLDE and test of targets at TRIUMF with a high intensity proton.<br>
1598	<br>
1599
1600
1601	<p><i><b>Outline the milestones to be achieved by means of the NA, as
1602	relevant to each work package.</b></i> </p>
1603
1604	<p><i> .....<font color="#cc66cc"> to be done largely by the 7
1605	coordinators first </font>and then in collegially by   the NA
1606	SG</i><br>
1607	</p>
1608
1609	<p><b> PHYSICS</b><br>
1610	Dec 04 Workshop on Ambiguities, Degeneracies and Correlations in the search
1611	<br>
1612	for Leptonic CP, possible exp. strategies (Munich?)<br>
1613	JUN 05 A report on the same subject <br>
1614	FEB 06 Workshop on SuperBeams vs. Beta Beams vs NuFact, synergies and priorities
1615	(Valencia ?)<br>
1616	SEP 06 A report on the same subject<br>
1617	SEP 07 A report on an optimized parameter list for SB, BB and NF. Addressing
1618	the problems of systematic errors<font
1619	face="Times New Roman, Times, serif"><br>
1620	DEC 08 Final report with the roadmap</font><br>
1621	<b>DRIVER</b><br>
1622	-    publication of the proceedings of  the yearly workshop
1623	<br>
1624	-    2004 :  report on the state of the art for the various
1625	elements, redaction of an agreement for a common R&D strategy and sharing
1626	of work, plans to explore applications to other fields<br>
1627	-    2005 : publication of  results of the studies for
1628	most elements (source, chopper, accelerating structures, RF couplers, beam
1629	dynamics, rapid cycling cyclotron alternative)<br>
1630	-    2006 & 2007 : definition and revision of the planning
1631	for tests, prototyping, studies depending on results obtained and technical
1632	problems encountered<br>
1633	-    2008 : final general report on results, TDR for the realization
1634	of a  high power proton driver with draft costing and schedule, assessment
1635	of the outcomes of the NA, prospective, applications to other fields, proposals
1636	for further developments   <br>
1637	<b>TARGET <br>
1638	COLLECTOR milestones</b><br>
1639	1)a comprehensive status report of the current state of the art in the
1640	early phase of the NA<br>
1641	2) the formation of a collaboration to propose a complete  design
1642	study <br>
1643	2) the publication of a detailed proposal for the evolution ("road map")
1644	towards  the design  <br>
1645	of a complete collection system, properly integrated upstream with
1646	the design of the target and <br>
1647	downstream with the one of the muon  front end <br>
1648	3)yearly international workshops, assembling EU,  USA and Japanese
1649	expertise and timely<br>
1650	addressing the milestones of this evolution <br>
1651	4) a report on comparative studies of different simulation of the complete
1652	production and <br>
1653	collection of neutrino parents<br>
1654	</p>
1655	<p><b><font size="+2">Plans for the first  18 monthes </font></b><br>
1656	Before the NA will start: </p>
1657	<ul>
1658	<ul>
1659	<li> report on 6000 type alloy caracteristics on mecanical properties
1660	under high intensity neutron flux based on bibliographic documentation</li>
1661	<li> initiate collaboration with French-CEA for stress limit measurement
1662	of 6000 type alloy under high level of neutron flux.</li>
1663	<li> report on analytic solutions of the Horn thermal/mecanical
1664	design</li>
1665	<li> start of  thermal/mecanical simulation of the Horn for
1666	a SuperBeam project</li>
1667	<li> first report on electric power design of the Horn for SuperBeam
1668	project</li>
1669	<li> proposal for Horn prototype building as Design Studies Technical
1670	Work Project</li>
1671	</ul>
1672	<li> Spring 2004</li>
1673	<ul>
1674	<li> first guide of the collection systems used in the past, present
1675	and near future (along R1 publication): mechanical stresses and design, electric
1676	power caracteristics and design, heat dissipation system design, failure description,
1677	lifetime in operation</li>
1678	<li> <font color="#000000">status report of the CERN Horn prototype</font></li>
1679	<li> reports on other mechanical tests as diffusion coefficient
1680	measurements</li>
1681	<li> integration of preliminary TARGET parameters on thermal/mecanical
1682	simulation of the Horn for a SuperBeam project</li>
1683	<li> first drawing design of a new Horn prototype</li>
1684	</ul>
1685	<li> Summer 2004</li>
1686	<ul>
1687	<li> R1 repport production</li>
1688	<li> status report on thermo/mechanical simulations</li>
1689	<li> status report on electric power design to deliver 300kA/50Hz</li>
1690	</ul>
1691	<li> Spring 2005</li>
1692	<ul>
1693	<li> first result on stress limit measurement of irradiated materials</li>
1694	<li> final design of a new Horn prototype to launch realisation</li>
1695	</ul>
1696	</ul>
1697	Afterwards their will be prototype realisation by the Design Studies TWP
1698	and measurement campain that will end by the writing of R2. Then, new work
1699	will be undertaken by DS TWP in the line of R3 report goal.
1700	<p> </p>
1701
1702	<p><b> COOLING</b></p>
1703
1704	<p>(0) Q1 2004: have European network formed and working.<br>
1705	(1) Q2 2004: completion of simulation of at least one frontend without
1706	cooling<br>
1707
1708	using detailed simulation codes. Comparison with existing studies<br>
1709
1710	of the baseline European design.<br>
1711	(2) Q2 2004: complete detailed analysis of the systematic errors for
1712	the <br>
1713
1714	baseline MICE experiment and hence a determination of total <br>
1715
1716	emittance resolution.<br>
1717	(3) Q3 2004: begin assessment of US ring cooler designs and start to
1718	develop<br>
1719
1720	a ring cooler to fit into the European Neutrino Factory.<br>
1721	(4) Q4 2004: begin determination of more realistic fields for the baseline<br>
1722
1723	cooling channel.<br>
1724	(5) Q2 2005: determine performance of the baseline channel with realistic
1725	<br>
1726
1727	fields.<br>
1728	(6) Q3 2005: complete a preliminary outline design for a European ring
1729	cooler.<br>
1730	(7) Q3 2005: start assessment of the use of MICE for testing alternative<br>
1731
1732	frontends or running the cooling cell components in different<br>
1733
1734	modes.<br>
1735	(8) Q4 2005: start optimising Neutrino Factory designs for different
1736	frontend<br>
1737
1738	designs.<br>
1739	(9) Q2 2006: start to look at technological aspects of implementing
1740	the<br>
1741
1742	different frontends and preparing R&D programmes.<br>
1743	(10) Q1 2007: start assessment of first results from MICE.<br>
1744	(11) Q3 2007: complete studies of alternative MICE experiments. Start
1745	preparing<br>
1746
1747	a proposal if the results are positive.<br>
1748	(12) Q1 2008: complete technology investigations and Neutrino Factory
1749	design<br>
1750
1751	optimisation.<br>
1752	(13) Q2 2008: assess impact of full MICE results.<br>
1753	(14) Q3 2008: complete detailed comparison between the alternative frontend<br>
1754
1755	designs.<br>
1756	(15) Q4 2008: if sufficient information is not available from MICE,
1757	devise an <br>
1758
1759	R&D programme for proving the best frontend can be built and <br>
1760
1761	will work. Write a proposal.<br>
1762	<br>
1763	<b>BETABEAM<br>
1764	</b></p>
1765	<p><i>The list below is a list of global deliverables tentatively produced
1766	by Alain. <br>
1767	Deliverables <br>
1768	After this overview, it seems that the list of deliverables could be as follows
1769	<br>
1770	-- recommendation for the parameters of the proton driver (spring 2005) <br>
1771	-- Interim tool: location and home lab for a Test Target Area  (summer
1772	2003)<br>
1773	-- List and estimate of experiments to be carried out at the TTA. (summer
1774	2003) <br>
1775	-- Design of a 4 ® 10 MW target station.  (2007)<br>
1776	-- Design (2003) and realization (2006) of a horn power supply unit, horn(s),
1777	horn optics. <br>
1778	-- Paper study (2004) of high aperture kickers for cooling (or phase rotation)
1779	rings <br>
1780	-- Realization of a kicker prototype (2006). <br>
1781	-- Design of the pulsed RF power stations needed for muon front-end and acceleration
1782	(2004)<br>
1783	-- Development of a prototype pulsed RF power station (2006)  <br>
1784	-- design of an FFAG magnet for acceleration and cost estimate (2004).<br>
1785	-- recommendation for accelerator design (2005)   <br>
1786	-- construction of a prototype FFAG magnet and characterization<br>
1787	<br>
1788	There are some decision points: the launch of a super-beam experiment could
1789	probably be envisaged around 2005.</i> <br>
1790	<br>
1791	</p>
1792
1793	<p><br>
1794	<br>
1795	</p>
1796
1797
1798	<p><b>Links to obtained results can also be given here (or a link to
1799	a site prepared for disseminating the acquired knowledge)</b></p>
1800	Bibliography?
1801	.... <font color="#ff0000">throu the EBNE Website, to be set  up
1802	.</font>.... recycling the wealth of the ECFA Muon site  ... what
1803	else? <b><br>
1804	</b>
1805	<p><br>
1806	</p>
1807	</td>
1808	</tr>
1809
1810	</tbody>
1811	</table>
1812
1813	<h2> <font color="#009900">Impact and benefits to the community:</font><br>
1814	</h2>
1815
1816	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
1817	<caption><br>
1818	</caption><tbody>
1819
1820	</tbody> <tbody>
1821	<tr>
1822	<td><i>Describe the expected benefits and impact on the community.<br>
1823	</i><br>
1824	ie indicate how the participants and the relevant scientific community
1825	will benefit from the expected results of this particular networking activity.
1826	<br>
1827	<br>
1828	The NA plans to hold regular and structured Weeks of meetings and
1829	discussion organized 3 to 4 times a year. . In addition one or two dedicated
1830	workshop are foreseen per year. <br>
1831	<br>
1832	The international community meets once a year at the occasion of
1833	the ECFA-sponsored NuFact & Superbeam Workshop. A NUFACT School
1834	is held, since 2002, yearly on the same location of the Workshop ...
1835	<i>this does not seem to be eligible ...</i><br>
1836	<br>
1837	Such a coherent and coordinated European program on neutrino beams
1838	will involve the large majority of the European experts in this field
1839	and will allow Europe to play a world leader role. It will enhance considerably
1840	the collaboration between accelerator physicists on the one hand and will
1841	develop a synergy between particle physicists and accelerator physicists
1842	on the other, ensuring the long-term sustainability of the field.<br>
1843	R&D experiments and projects as the ones being performed (HARP,
1844	high intensity target R&D, horn R&D etc )  or planned (MICE),
1845	will be pursued and multiplied , will mark the technical progress of our
1846	studies and will provide training and learning opportunities to large
1847	number of students and postdocs. <br>
1848	<br>
1849	We should also contribute to the description of the overall plan
1850	to disseminate, promote and exploit the knowledge derived from the NA
1851	both within and beyond the consortium: publications, conferences, workshops
1852	and web-based activities aiming at disseminating the knowledge and technology
1853	produced.<br>
1854	<br>
1855	<br>
1856	NB Only preliminary thoughts. <br>
1857	<br>
1858	We are suggested also to explain, looking at the ensemble of the
1859	“networking activities”, how they will enhance the services provided
1860	by the research infrastructures in the proposed programme of activities
1861	under consideration.<br>
1862	<br>
1863	To be done later.<br>
1864	</td>
1865	</tr>
1866
1867	</tbody>
1868	</table>
1869
1870	<h2> <font color="#3333ff">Execution plan:</font></h2>
1871	<br>
1872
1873	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
1874	<caption><br>
1875	</caption><tbody>
1876
1877	</tbody> <tbody>
1878	<tr>
1879	<td><i><b>Describe in detail the execution plan in terms of a chart
1880	showing the time expected to be spent concluding each of the milestones
1881	specified in the different work packages. This chart can be made
1882	with standard tools and inserted here.</b><br>
1883	</i> <br>
1884	<i> .e. give an indicative multi-annual execution plan (in
1885	tabular form) for the whole duration of the I3 that cover all the networking
1886	activities. For each activity, you should specify the relevant milestones
1887	and the expected deliverables. Additional information can be provided,
1888	if necessary, in free text.<br>
1889	<br>
1890	Detailed work needed here.<br>
1891	</i>
1892
1893	<p><i>A contribution of N4 to the18 months plan will also have to be
1894	provided. <br>
1895	Should one give here a correspondingly more detailed execution
1896	plan for the first 18 months? <br>
1897	<br>
1898	We should also produce a general “road map”, detailing our view
1899	of the time scale of initiatives in the sector of neutrino beams in
1900	the medium and long-term future.<br>
1901	<br>
1902	In order to prompt discussion, I just attempt the following<br>
1903	<br>
1904	R&D and design studies from now to 2007 or 2008<br>
1905	<br>
1906	Conceptual Design Report for a Neutrino Factory in 2008 <br>
1907	Realization of  a  Superbeam, a European high power
1908	conventional neutrino facility(2012 at earliest?)<br>
1909	Realization of the first Neutrino Factory in 2015 (or later?)<br>
1910	First possible date for a running Betabeam complex? <br>
1911	</i> </p>
1912
1913	<p><i>.....<font color="#cc66cc"> collecting here from  the 7
1914	coordinators first </font><br>
1915	</i> </p>
1916
1917	<i><b> PHYSICS</b><b><br>
1918	CNGS <br>
1919	DRIVER.<br>
1920	</b><b>TARGET </b><b><br>
1921	COLLECTOR </b><br>
1922	<b> </b><b>COOLING<br>
1923	BETABEAM</b><br>
1924	</i> </td>
1925	</tr>
1926
1927	</tbody>
1928	</table>
1929
1930	<p><b><font color="#3333ff"><font size="+2"><i>Estimate of total cost per
1931	partici</i>pant and work package:</font></font></b> <br>
1932	<b><font color="#3333ff"><font size="+2">(including associate members)</font></font></b>
1933	<br>
1934	</p>
1935
1936	<center><br>
1937
1938	<table border="1" cols="7" width="100%" bgcolor="#ffffff">
1939	<caption>
1940	<center></center>
1941	<br>
1942	</caption><tbody>
1943
1944	</tbody> <tbody>
1945	<tr>
1946	<td><b>Participants </b> <br>
1947	(give short name and include ass.  <br>
1948	members)</td>
1949	<td>        <b>WP1</b>
1950
1951	<p>a.  FTE  <br>
1952	b.  networking</p>
1953	</td>
1954	<td>       <b>WP2</b>
1955	<p>a.  FTE  <br>
1956	b.  networking</p>
1957	</td>
1958	<td>        <b>WP3</b>
1959
1960	<p>a.  FTE  <br>
1961	b.  networking</p>
1962	</td>
1963	<td>      <b> ......</b></td>
1964	<td> </td>
1965	<td><b>Sum per      participant</b> <br>
1966	a.  FTE  <br>
1967	b.  networking</td>
1968	</tr>
1969	<tr>
1970	<td>       <b>1</b></td>
1971	<td>a.  <br>
1972	b. </td>
1973	<td>a.  <br>
1974	b. </td>
1975	<td>a.  <br>
1976	b. </td>
1977	<td> </td>
1978	<td> </td>
1979	<td>a.  <br>
1980	b. </td>
1981	</tr>
1982	<tr>
1983	<td>       <b>2</b></td>
1984	<td>a.  <br>
1985	b. </td>
1986	<td>a.  <br>
1987	b. </td>
1988	<td>a.  <br>
1989	b. </td>
1990	<td> </td>
1991	<td> </td>
1992	<td>a.  <br>
1993	b. </td>
1994	</tr>
1995	<tr>
1996	<td>       <b>3</b></td>
1997	<td>a.  <br>
1998	b. </td>
1999	<td>a.  <br>
2000	b. </td>
2001	<td>a.  <br>
2002	b. </td>
2003	<td> </td>
2004	<td> </td>
2005	<td>a.  <br>
2006	b. </td>
2007	</tr>
2008	<tr>
2009	<td>       <b>...</b></td>
2010	<td> </td>
2011	<td> </td>
2012	<td> </td>
2013	<td> </td>
2014	<td> </td>
2015	<td> </td>
2016	</tr>
2017	<tr>
2018	<td> </td>
2019	<td> </td>
2020	<td> </td>
2021	<td> </td>
2022	<td> </td>
2023	<td> </td>
2024	<td> </td>
2025	</tr>
2026	<tr>
2027	<td>   Sum per WP</td>
2028	<td>a.  <br>
2029	b. </td>
2030	<td>a.  <br>
2031	b. </td>
2032	<td>a.  <br>
2033	b. </td>
2034	<td> </td>
2035	<td> </td>
2036	<td>Total  FTE  <br>
2037	Total networking</td>
2038	</tr>
2039
2040	</tbody>
2041	</table>
2042	</center>
2043
2044	<p><b><font color="#3333ff"><font size="+2">Requested cost per participant
2045	and work package:</font></font></b> <br>
2046	<b><font color="#3333ff"><font size="+2">(including associate members)</font></font></b>
2047	<br>
2048	</p>
2049
2050	<center><br>
2051
2052	<table border="1" cols="7" width="100%" bgcolor="#ffffff">
2053	<caption>
2054	<center></center>
2055	<br>
2056	</caption><tbody>
2057
2058	</tbody> <tbody>
2059	<tr>
2060	<td><b>Participants </b> <br>
2061	(give short name and include ass.  <br>
2062	members)</td>
2063	<td>        <b>WP1</b>
2064
2065	<p>a.  FTE  <br>
2066	b.  networking</p>
2067	</td>
2068	<td>       <b>WP2</b>
2069	<p>a.  FTE  <br>
2070	b.  networking</p>
2071	</td>
2072	<td>        <b>WP3</b>
2073
2074	<p>a.  FTE  <br>
2075	b.  networking</p>
2076	</td>
2077	<td>      <b> ......</b></td>
2078	<td> </td>
2079	<td><b>Sum per      participant</b> <br>
2080	a.  FTE  <br>
2081	b.  networking</td>
2082	</tr>
2083	<tr>
2084	<td>       <b>1</b></td>
2085	<td>a.  <br>
2086	b. </td>
2087	<td>a.  <br>
2088	b. </td>
2089	<td>a.  <br>
2090	b. </td>
2091	<td> </td>
2092	<td> </td>
2093	<td>a.  <br>
2094	b. </td>
2095	</tr>
2096	<tr>
2097	<td>       <b>2</b></td>
2098	<td>a.  <br>
2099	b. </td>
2100	<td>a.  <br>
2101	b. </td>
2102	<td>a.  <br>
2103	b. </td>
2104	<td> </td>
2105	<td> </td>
2106	<td>a.  <br>
2107	b. </td>
2108	</tr>
2109	<tr>
2110	<td>       <b>3</b></td>
2111	<td>a.  <br>
2112	b. </td>
2113	<td>a.  <br>
2114	b. </td>
2115	<td>a.  <br>
2116	b. </td>
2117	<td> </td>
2118	<td> </td>
2119	<td>a.  <br>
2120	b. </td>
2121	</tr>
2122	<tr>
2123	<td>       <b>...</b></td>
2124	<td> </td>
2125	<td> </td>
2126	<td> </td>
2127	<td> </td>
2128	<td> </td>
2129	<td> </td>
2130	</tr>
2131	<tr>
2132	<td> </td>
2133	<td> </td>
2134	<td> </td>
2135	<td> </td>
2136	<td> </td>
2137	<td> </td>
2138	<td> </td>
2139	</tr>
2140	<tr>
2141	<td>   Sum per WP</td>
2142	<td>a.  <br>
2143	b. </td>
2144	<td>a.  <br>
2145	b. </td>
2146	<td>a.  <br>
2147	b. </td>
2148	<td> </td>
2149	<td> </td>
2150	<td>Total  FTE  <br>
2151	Total networking</td>
2152	</tr>
2153
2154	</tbody>
2155	</table>
2156	</center>
2157
2158	<p><b><font color="#3333ff"><font size="+2">Additional information concerning
2159	the cost estimate:</font></font></b> <br>
2160	<br>
2161
2162	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
2163	<caption><br>
2164	</caption><tbody>
2165
2166	</tbody> <tbody>
2167	<tr>
2168	<td>Specify additional details relevant to the structure of the budget
2169	requested (number of workshops and collaboration weeks to be attended, new
2170	events to be organised, eventual service tasks, fraction of young/senior researchers,
2171	inviting high-level experts from outside the IA, support for dissemination
2172	of the knowledge, educational tools and actions, outreach,...)<br>
2173	<b>Specify additional details relevant to the structure of the
2174	budget requested (fraction of total cost requested to be funded,
2175	number of workshops and collaboration weeks to be attended, new
2176	events to be organised, eventual service tasks, fraction of young/senior
2177	researchers, inviting high-level experts from outside the IA, support
2178	for dissemination of the knowledge, educational tools and actions,
2179	outreach,...)</b><br>
2180	<br>
2181	<br>
2182	No attempt to fill the financial table has been done yet. Only
2183	an early first rough underestimate of the level of funding useful to
2184	adequately <br>
2185	reinforce participation to these network of activities in 2004-7
2186	was performed several weeks ago and is reproposed here as such for now.
2187	<br>
2188	<br>
2189	1) assuming that about 20 people would be supported to travel for
2190	each of the  Weeks, at 1000 € each, 60 to 80 K€ per year are needed
2191	<br>
2192	<br>
2193	2) 20 to 40 researchers would be supported to travel to the NuFact
2194	Workshop (faculty and postdocs) and/or the NuFact School (postdocs <br>
2195	and students). About 40 to 80  K€ per year will be needed<br>
2196	<br>
2197	3) additional funds will be needed to cover expenses of invited
2198	speakers to the Weeks<br>
2199	<br>
2200	4) additional funds will be needed to support participation to
2201	dedicated workshops.  <br>
2202	<br>
2203	A request of 800 to 1000 K€ over 4 years emerged at the time, to
2204	be soon seriously revised. <br>
2205	<br>
2206	The Guide for proposers implies that the main cost is to be requested
2207	for the organization of meetings, travel and subsistence expenses. In
2208	some special case, the cost of for hiring a postdocs or a student can be
2209	supported provided his task is a service task (such as maintenance and
2210	exportability of code, database…). EU funding can cover up to 100% of
2211	the real costs of the networking activities. No explicit limit is indicated,
2212	however it seems that total amounts largely exceeding 1 Meuros for each
2213	NA over the entire IA period (i.e. 5 years) will be difficult to obtain.<br>
2214	<br>
2215	<i>We are seriously considering requesting also the cost
2216	for hiring a postdoc in charge of the centralization, maintenance and
2217	distribution of the NA patrimony of simulation codes and of the NA Website.
2218	</i><br>
2219	</td>
2220	</tr>
2221
2222	</tbody>
2223	</table>
2224	</p>
2225
2226	<p><b><font color="#3333ff"><font size="+2">Management structure:</font></font></b>
2227	<br>
2228	<br>
2229
2230	<table border="1" cols="1" width="100%" bgcolor="#ffffff">
2231	<caption><br>
2232	</caption><tbody>
2233
2234	</tbody> <tbody>
2235	<tr>
2236	<td>Specify the structure of the NA management, based on the guidelines
2237	provided, with names and functions of the people nominated. <br>
2238	<b>Co-ordinator: </b> <br>
2239	<b>Deputy co-ordinator: </b> <br>
2240	<b>Work-package co-ordinators:</b>  <br>
2241	A link to the <a
2242	href="http://esgard.lal.in2p3.fr/Project/Activities/Organisation/index.php">WEB-based
2243	description</a> of the central management structure of the CARE IA can be
2244	provided. Specific functions NA co-ordinators in the central management
2245	structure can be highlighted (for example the deputy co-ordinator of the
2246	NA is a member of the Knowledge Dissemination Board, etc...).</td>
2247	</tr>
2248
2249	</tbody>
2250	</table>
2251	</p>
2252	<br>
2253	<br>
2254	<br>
2255	</body>
2256	</html>

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