Snowmass2021 Cosmic Frontier Dark Matter Direct Detection to the Neutrino Fog - INSPIRE

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Snowmass2021 Cosmic Frontier Dark Matter Direct Detection to the Neutrino Fog

D.S. Akerib
(
- SLAC and
- KIPAC, Menlo Park
)
,
P.B. Cushman
(
- Minnesota U.
)
,
C.E. Dahl
(
- Northwestern U. and
- Fermilab
)
,
R. Ebadi
(
- Maryland U.
)
,
A. Fan
(
- SLAC and
- KIPAC, Menlo Park
)

Mar 15, 2022

34 pages

Contribution to:

Snowmass 2021

e-Print:

2203.08084 [hep-ex]

Report number:

FERMILAB-CONF-22-180-V

View in:

reference search89 citations

Citations per year

Abstract: (arXiv)

We present a summary of future prospects for direct detection of dark matter within the GeV/c2 to TeV/c2 mass range. This is paired with a new definition of the neutrino fog in order to better quantify the rate of diminishing returns on sensitivity due to irreducible neutrino backgrounds. A survey of dark matter candidates predicted to fall within this mass range demonstrates that fully testing multiple well-motivated theo-ries will require expanding the currently-funded generation of experiments down to and past the neutrino fog. We end with the status and plans for next-generation exper-iments and novel R&D concepts which will get us there.

Note:

contribution to Snowmass 2021

dark matter: direct detection
dark matter: mass
neutrino: background
sensitivity
numerical calculations: Monte Carlo

References(135)

Figures(8)

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(
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)

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•
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[21]

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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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)
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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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