Theory of Neutrino-Atom Collisions: The History, Present Status, and BSM Physics

<table>The SM (weak) and NMM contributions to the differential cross section of <svg height="16.2125" id="M415" style="vertical-align:-3.2316pt" version="1.1" viewbox="0 0 14.7125 16.2125" width="14.7125" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg>-Ge ionization at <svg height="15.4" id="M416" style="vertical-align:-3.21404pt" version="1.1" viewbox="0 0 45.400002 15.4" width="45.400002" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> MeV [<a href="/journals/ahep/2014/569409/#B64">60</a>] in comparison with the corresponding stepping-approximation results (FEA). The NMM value is set to be the current upper limit <svg height="21.012501" id="M417" style="vertical-align:-3.21404pt" version="1.1" viewbox="0 0 126.4125 21.012501" width="126.4125" xmlns="http://www.w3.org/2000/svg" xmlns:xlink="http://www.w3.org/1999/xlink">
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</svg> [<a href="/journals/ahep/2014/569409/#B19">19</a>].</table>

Advances in High Energy Physics

fig6

Figure 6

Figure 6: Theory of Neutrino-Atom Collisions: The History, Present Status, and BSM Physics 