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Etude de bruit de fond induit par les muons dans l'expérience ...

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tel-00724955, version 1 - 23 Aug 2012<br />

2<br />

40 Detecting the WIMP<br />

regime, even at very large WIMP-search exposures. This requires a powerful <strong>par</strong>ticle<br />

i<strong>de</strong>ntification technique that operates at low energies, but the benefits of lowbackground<br />

operation allow one to extract enormous sensitivity from relatively small<br />

<strong>de</strong>tector exposures in this way.<br />

Most mo<strong>de</strong>rn direct-<strong>de</strong>tection experiments use event-by-event discrimination techniques<br />

to i<strong>de</strong>ntify nuclear recoils from WIMPs, or neutrons, among a far larger rate of<br />

electron recoils from radioactive <strong>de</strong>cay and cosmogenic processes. Some experiments,<br />

notably bubble chambers and other phase-transition <strong>de</strong>tectors, use the difference in<br />

dE/dx between electron- and nuclear-recoil tracks to make their <strong>de</strong>tectors unresponsive<br />

to electron recoils, thus achieving a <strong>par</strong>ticularly simple sort of event-by-event<br />

discrimination. Discrimination is more commonly accomplished by measuring each<br />

event in two or more distinct <strong>de</strong>tection channels and using their ratio to i<strong>de</strong>ntify<br />

the recoil type. When the recoil occurs, the energy is <strong>par</strong>titioned in the ionization,<br />

the heat/phonons and the scintillation channels. In Figure 2.2, the main <strong>de</strong>tection<br />

techniques are shown around a triangle that <strong>de</strong>picts the energy from the interaction<br />

of a WIMP-nuclear recoil. These channels differ enormously in the mean nuclear recoil<br />

energy nee<strong>de</strong>d to create the individual quanta: A few meV per phonon, ∼ 10 eV<br />

per charge carrier, and ∼ 100 eV per scintillation photon. Each <strong>de</strong>tection technique<br />

exploits one or more of this channels or <strong>de</strong>grees of freedom to make the discrimination<br />

between nuclear recoils (neutrons and WIMPs) and electron recoils (majority<br />

of backgrounds).<br />

Xe, Ar,<br />

Ne<br />

NaI, Xe,<br />

Ar, Ne<br />

ZEPLIN II, III<br />

XENON<br />

WARP<br />

ArDM<br />

SIGN<br />

LUX<br />

NAIAD<br />

ZEPLIN I<br />

DAMA<br />

XMASS<br />

DEAP<br />

Mini-CLEAN<br />

Scintillation<br />

Few % of Energy<br />

Ge, CS2 , C3F8 DRIFT<br />

IGEX<br />

COUPP<br />

~20% of Energy<br />

Ionization<br />

Heat -<br />

Phonons<br />

CRESST II<br />

ROSEBUD<br />

CaWO4 , BGO<br />

ZnWO 4 , Al 2 O 3 …<br />

~100% of Energy<br />

CDMS<br />

EDELWEISS<br />

CRESST I<br />

Al 2 O 3 , LiF<br />

Ge, Si<br />

Figure 2.2: Main <strong>de</strong>tection techniques to track a WIMP signal. The triangle <strong>de</strong>picts<br />

the energy after a nuclear recoil interaction from a WIMP, each corner represents<br />

a channel where the energy from the interaction appears. Each <strong>de</strong>tection technique<br />

exploits one or more of these channels. Most of the energy goes into phonons and<br />

ionization, the two channels used by CDMS and EDELWEISS. Figure from [115].

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