| 1 | # $Id: README,v 1.21 2005/03/17 19:48:27 daquinog Exp $
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| 2 | # -------------------------------------------------------------------
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| 3 | # GEANT4 tag $Name: $
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| 4 | # -------------------------------------------------------------------
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| 5 |
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| 6 | Simulation of the TIARA experiment using importance sampling
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| 7 | ============================================================
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| 8 |
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| 9 | This example is a simulation of the neutron shielding experiment TIARA
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| 10 | see http://idsun1.kek.jp/nakao/research/tiara/tiara.htm.
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| 11 | The example is meant to provide a realistic example for
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| 12 | applying geometrical importance sampling (geometrical splitting and
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| 13 | Russian roulette).
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| 14 | In the TIARA experiment neutrons of two different energy distributions
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| 15 | created by 43 MeV and 68 MeV protons bombarding a 7Li target are measured
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| 16 | behind several shields. The simulation starts from the neutron spectra.
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| 17 | In this example the interactions of the neutrons with the (concrete)
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| 18 | shields are simulated and energy dependent neutron fluxes are measured
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| 19 | behind the shields. Users may choose to run the simulation for different
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| 20 | shielding configuration with or without importance sampling.
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| 21 | The simulated neutron fluxes are compared to the published
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| 22 | experimental data. The efficiency of applying importance sampling
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| 23 | depends strongly on the shield thickness and importance configuration.
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| 24 | The efficiency of the simulations may be obtained as FOM values.
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| 25 |
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| 26 | See also "Geant4 User's Guide
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| 27 | For Application Developers", Chapter "Toolkit Fundamentals"
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| 28 | Section "Event Biasing Techniques" and references there.
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| 29 |
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| 30 | The example has been tested on CERN RH 7.3 with the
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| 31 | gcc-3.2.3 and gcc-2.95.2 compilers.
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| 32 |
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| 33 | Note for system testing without analysis: see points 1.1, 1.3 and 3.2.
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| 34 |
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| 35 |
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| 36 |
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| 37 | 1) Setting the environment
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| 38 | ==========================
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| 39 |
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| 40 | You must compile Geant4 with:
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| 41 | "G4LIB_BUILD_SHARED" set to 1.
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| 42 | You need to set:
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| 43 | "NeutronHPCrossSections" (e.g. pointing to a directory containing G4NDL3.7)
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| 44 |
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| 45 |
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| 46 | Three examples are given of how to set environment variables
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| 47 | in the three cases:
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| 48 |
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| 49 | 1.1) PI via AFS (most simple):
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| 50 | --------------------
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| 51 | You have access to afs and you want to use PI for the
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| 52 | analysis:
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| 53 | Set the following environment variables:
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| 54 | "G4ANALYSIS_USE"
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| 55 | "PI_BASE_DIR" (where PI has been installed)
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| 56 | "SWIG_BASE_DIR" (where SWIG has been installed)
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| 57 |
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| 58 | Finally source the script envCommon.csh from the directory where you have Tiara
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| 59 | installed, e.g. ${G4INSTALL}/examples/advanced/Tiara
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| 60 |
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| 61 |
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| 62 | 1.2) No afs but a local PI and SWIG installation:
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| 63 | -----------------------------------------------------
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| 64 | You don't use afs but you have a local installation of SWIG and PI
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| 65 | Set the following environment variables:
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| 66 | "G4ANALYSIS_USE"
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| 67 | "PI_BASE_DIR"
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| 68 | "SWIG_BASE_DIR"
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| 69 |
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| 70 | Finally source the script envCommon.csh from the directory where
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| 71 | you have Tiara installed, e.g. ${G4INSTALL}/examples/advanced/Tiara
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| 72 |
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| 73 |
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| 74 | 1.3) No afs, no PI and no SWIG (e.g. for system testing):
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| 75 | -------------------------------------------------------------
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| 76 | You don't want to use PI and SWIG and you don't have afs access.
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| 77 | Make sure "G4ANALYSIS_USE" is unset (e.g. unsetenv G4ANALYSIS_USE or setenv G4ANALYSIS_USE 0)
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| 78 |
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| 79 | Note 1: python must be built against a "libc".
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| 80 | You may do this by creating a shared library by a command
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| 81 | similar to this
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| 82 | "ld -shared -o libpython2.3.so --whole-archive libpython2.3.a /usr/lib/libc.so"
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| 83 |
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| 84 | Set the following environment variables:
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| 85 | "PYTHONVERSION" (2.3 or higher)
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| 86 | "PYTHON_BASE_DIR" (e.g. to /usr)
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| 87 | "SWIG_VERSION" (e.g. 1.3 or higher)
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| 88 | "SWIG_BASE_DIR" (e.g. /usr)
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| 89 | "CLHEP_BASE_DIR" (e.g. to /opt/local)
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| 90 |
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| 91 | Finally source the script envCommon.csh from the directory where
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| 92 | you have Tiara installed, e.g. ${G4INSTALL}/examples/advanced/Tiara
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| 93 |
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| 94 | NOTE 2: Passing from a simulation WITH to another WITHOUT analysis implies
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| 95 | that the G4ANALYSIS_use should be unset and that the SWIG-wrapper scripts
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| 96 | in the directory TiaraWrapper should be deleted. Normally, the whole code
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| 97 | should be compiled again using gmake clean_all and, afterwards, gmake.
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| 98 | The same procedure should be followed also passing from a simulation WITHOUT
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| 99 | to another WITH analysis.
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| 100 |
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| 101 | 2) Building the example
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| 102 | =======================
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| 103 |
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| 104 | Geant4 has to be compiled using G4LIB_BUILD_SHARED 1 and the one of the
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| 105 | above environment settings have to be set.
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| 106 | Type "gmake".
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| 107 |
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| 108 |
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| 109 | 2.1) In more detail
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| 110 | -------------------
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| 111 |
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| 112 | Geant4 must be compiled into granular shared libraries.
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| 113 | Therefore before compiling Geant4 set "G4LIB_BUILD_SHARED" to "1".
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| 114 |
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| 115 | External packages used in this example are PI, SWIG and Python.
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| 116 |
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| 117 |
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| 118 | 2.2) Cleaning up
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| 119 | ----------------
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| 120 | To remove the files created by swig ( *_wrap.cc, the corresponding
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| 121 | .py files) use "gmake swigClean".
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| 122 | To remove the directories of compiled code related to this example under
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| 123 | $G4WORKDIR/tmp/$G4SYSTEM/ use "gmake tiaraClean".
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| 124 | To remove all the files created during the previous compilation, use
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| 125 | "gmake clean_all".
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| 126 |
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| 127 |
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| 128 | 3) Running the example:
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| 129 | =======================
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| 130 |
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| 131 |
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| 132 | 3.1) Using PI
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| 133 | -----------------
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| 134 | Change to the sub directory "run" and execute "runSim.py".
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| 135 | "runSim.py" runs an example configuration which may be
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| 136 | changed by the user. The results of the simulation are stored in
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| 137 | the directory "simData".
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| 138 | The script "runSim.py" periodically prints scoring information to the
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| 139 | screen.
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| 140 | It also prints out the relative path of a ".shelve" file.
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| 141 | This file can be used to access results of the simulation.
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| 142 |
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| 143 | In case the example was build using analysis
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| 144 | results may be viewed e.g. using python or ROOT:
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| 145 | 1) Start python
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| 146 | 2) type: import dataAcess
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| 147 | 3) type: p = dataAcess.ExpMcPlot (shelveFileName,detectorposition)
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| 148 | where "shelveFileName" is the name (enclosed in quotes) of the
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| 149 | shelve file created during the execution of runSim.py.
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| 150 | The name is printed on the screen during execution of runSim.py.
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| 151 | "detectorposition" may be "00, "20" or "40" and stand for the
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| 152 | detectors 00, 20, 40 cm off beam axis respectively.
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| 153 | 4) type: p.display ()
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| 154 | 5) type: import extractShelve
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| 155 | 6) type: extractShelve.getFluxes (p.she)
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| 156 | p.she is the shelve object containing simulation results.
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| 157 | This prints the FOM values for the used detectors
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| 158 | for two energy regions below and in the peak region.
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| 159 | The FOM should be compared to unbiased simulations. To run
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| 160 | an unbiased simulation set the importance values to one (see
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| 161 | runSim.py)
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| 162 |
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| 163 | Note: the output files written after every run are incremental! Meaning
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| 164 | the file with the highest run number contains the data from
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| 165 | all the runs!
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| 166 |
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| 167 | The modules (dataAcess, extractShelve) imported in the above steps are
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| 168 | placed in source/py_modules in files named after the module ending with
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| 169 | ".py".
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| 170 |
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| 171 | Since the simulation time used by "runSim.py" is only 5 minutes the
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| 172 | calculated results have large errors. If you want to see a better result
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| 173 | do the following changes in "runSim.py".
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| 174 | Extend the total run time to e,g, 2 hours by setting:
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| 175 | "totalTime = 2 * myUtils.hour",
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| 176 | set the print out period to 30 minutes by setting:
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| 177 | "timeForOneRun = 30 * myUtils.min".
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| 178 |
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| 179 |
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| 180 |
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| 181 |
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| 182 | 3.2) Not using PI (mainly for system testing)
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| 183 | -------------------------------------------------
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| 184 | Change to the sub directory "run" and execute
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| 185 | runSimNoAnalysis.py.
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| 186 |
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| 187 |
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| 188 |
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| 189 |
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| 190 |
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| 191 | 4) Content of the directory:
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| 192 | ============================
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| 193 |
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| 194 |
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| 195 | envCommon.csh - a script to setup environment variables
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| 196 | in case the above one of the above environment settings have been
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| 197 | done beforehand.
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| 198 |
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| 199 | GNUmakefile - for building the example
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| 200 |
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| 201 |
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| 202 | data / - directory containing experimental data
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| 203 |
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| 204 | expDataOrig - experimental data taken from
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| 205 | http://idsun1.kek.jp/nakao/research/tiara/tiara.htm
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| 206 |
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| 207 | expDataConverted - some of the experimental data and the source
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| 208 | spectra converted into Anaphes DataPointSet
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| 209 | and stored in Anaphes xml format
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| 210 |
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| 211 |
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| 212 | source / - directory containing the source code
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| 213 |
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| 214 | tiara - C++ source code
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| 215 |
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| 216 | CLHEPWrapper - wrapper classes for usage in python
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| 217 | \include\CLHEP.i - specification file for swig
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| 218 | \src\CLHEP_wrap.cc - wrapper created with swig
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| 219 |
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| 220 | G4KernelWrapper - wrapper classes for usage in python
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| 221 |
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| 222 | TiaraWrapper - wrapper classes for usage in python
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| 223 |
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| 224 | py_modules - python modules for running and analysing
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| 225 |
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| 226 | swig.gmk - makefile rules for using swig
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| 227 |
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| 228 | run / - directory for running the example
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| 229 | runSim.py - executable example script
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| 230 | runSimNoAnalysis.py - executable script for running without
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| 231 | analysis
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| 232 |
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| 233 |
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| 234 |
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| 235 | 5) Technicalities about this example
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| 236 | ===================================
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| 237 |
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| 238 | This example is composed out of a layer of classes written in C++
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| 239 | (source/tiara/include, source/tiara/src), a layer of python
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| 240 | shadow classes created by swig (source/CLHEPWrapper,
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| 241 | source/G4KernelWrapper, source/TiaraWrapper) and a layer of
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| 242 | python modules (source/py_modules).
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| 243 | The C++ layer under source/tiara provides lower level classes closely
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| 244 | related to the Geant4 kernel.
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| 245 | The shadow classes in the source/*Wrapper directories provide classes
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| 246 | that may be instantiated in a python script or session. This way the
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| 247 | lower level C++ code can be used directly for scripting in python. The
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| 248 | shadow classes are declared in the files with extensions ".i" in the
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| 249 | source/*Wrapper/include directories. Swig is used to create C++ code for
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| 250 | a library that can be loaded into python and python modules (files with
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| 251 | extensions .py in the source/*Wrapper directories). When the python
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| 252 | modules created by swig are imported into python (in a session or a
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| 253 | script) the corresponding C++ library is automatically loaded as well.
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| 254 | The python modules in source/py_modules provide classes and functions
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| 255 | that may be changed or customized more frequently than the C++ classes
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| 256 | in source/tiara. These classes complete the construction of geometries,
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| 257 | take care of the procedure of setting up the simulation, the run sequence
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| 258 | and the analysis after the simulation has been ran.
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| 259 | The script runSim.py is an commented example of using the python modules
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| 260 | to run a simulation.
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| 261 |
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| 262 |
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| 263 | 6) Note about how to call the hadronic physics lists in runSim.py and runSimNoAnalysis.py
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| 264 | =========================================================================================
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| 265 |
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| 266 | It is only necessary to change the physList value in runSim.py or runSimNoAnalysis.py. In the example, there are 4 available physics lists, but of course the user can use whatever physics lists he/she likes and present in the Geant4-7.0 repository. In such a case, the user should also modify the
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| 267 | /source/TiaraWrapper/include/Tiara.i file in order to create an instantiation of the
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| 268 | physics list class. In particular, just follow the same lines already used for the six
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| 269 | available physics lists.
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| 270 |
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