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1 | \documentclass [12pt]{article} |
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2 | \usepackage[latin1]{inputenc} |
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3 | \setlength {\textwidth}{14cm} |
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4 | \setlength {\textheight}{19cm} |
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5 | \renewcommand{\baselinestretch}{1.25} |
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6 | %\topmargin -1cm |
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7 | %\oddsidemargin -5pt |
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8 | %\evensidemargin -5pt |
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9 | \begin{document} |
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10 | \title{ { |
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11 | Flux normalization in GLoBES 2.0.11 |
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12 | } } |
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13 | \author{J.E Campagne - LAL} |
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14 | \maketitle |
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15 | % |
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16 | \section*{Introduction} |
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17 | The present situation is the following: we use the files sploptiplusmauro.dat (sploptiminusmauro.dat) which are fluxes ($dN(E)$) expressed in terms of numbers of neutrino species per $100 m^2$ per year and binned every $BWF\equiv0.02GeV$ and computed at $L=130km$. |
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18 | |
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19 | Internally, GLoBES v2.0.11 uses these fluxes with some {\it a priori} and at the end of the day it turns out that: |
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20 | \begin{equation} |
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21 | dN(E)\times \frac{1}{L^2} \times \mathrm{norme2}(0) \times \mathrm{@norm} \times \Delta T |
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22 | \end{equation} |
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23 | with $\mathrm{norme2}(0) = 5.198927 = 6.02204 10^{-12}\ 295^2\ 9.92033 10^6$ the result of a function in \verb|glb_fluxes.c|. |
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24 | |
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25 | |
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26 | |
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27 | \end{document} |
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