Complementarity of direct detection experiments in search of light Dark Matter - INSPIRE

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Complementarity of direct detection experiments in search of light Dark Matter

J.R. Angevaare
(
- Nikhef, Amsterdam and
- NIKHEF, Amsterdam
)
,
G. Bertone
(
- Nikhef, Amsterdam
)
,
A.P. Colijn
(
- Nikhef, Amsterdam and
- NIKHEF, Amsterdam
)
,
M.P. Decowski
(
- Nikhef, Amsterdam and
- NIKHEF, Amsterdam
)
,
B.J. Kavanagh
(
- Cantabria Inst. of Phys.
)

Apr 4, 2022

19 pages

Published in:

JCAP 10 (2022) 004

Published: Oct 3, 2022

e-Print:

2204.01580 [hep-ph]

DOI:

10.1088/1475-7516/2022/10/004

View in:

ADS Abstract Service

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Abstract: (IOP)

Dark Matter experiments searching for Weakly interacting massive particles (WIMPs) primarily use nuclear recoils (NRs) in their attempt to detect WIMPs. Migdal-induced electronic recoils (ERs) provide additional sensitivity to light Dark Matter with 𝒪(GeV/c

^{2}

) masses. In this work, we use Bayesian inference to find the parameter space where future detectors like XENONnT and SuperCDMS SNOLAB will be able to detect WIMP Dark Matter through NRs, Migdal-induced ERs or a combination thereof. We identify regions where each detector is best at constraining the Dark Matter mass and spin independent cross-section and infer where two or more detection configurations are complementary to constraining these Dark Matter parameters through a combined analysis.

Note:

19 pages, 7 figures

dark matter detectors
dark matter experiments
Bayesian reasoning
dark matter experiment
dark matter simulations
dark matter theory
dark matter: mass
WIMP: dark matter
dark matter: scattering
nucleus: recoil

References(49)

Figures(7)

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,
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)
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)
,
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,
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,
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)

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