How high is the neutrino floor?

In this paper, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We use this information to calculate the maximum value of the so-called neutrino floor for direct dark matter detection experiments, which dete...

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Published inJournal of cosmology and astroparticle physics Vol. 2019; no. 1; p. 43
Main Authors Bœhm, C., Cerdeño, D.G., Machado, P.A.N., Campo, A. Olivares-Del, Reid, E.
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 21.01.2019
Institute of Physics (IOP)
Subjects
ASTRONOMY AND ASTROPHYSICS
Astrophysics
Coherent scattering
Constraint modelling
Dark matter
dark matter detectors
Elastic scattering
Floors
High Energy Physics - Phenomenology
neutrino properties
Neutrinos
Physics
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Scattering cross sections
Supernovae
numerical calculations
new physics
neutrino properties
dark matter: direct detection
neutrino: background
dark matter: mediation
dark matter: mass
neutrino nucleus: elastic scattering
neutrino: model
CDMS
XENON
Z
dark matter detectors
Online AccessGet full text
ISSN1475-7516
1475-7508
1475-7516
DOI10.1088/1475-7516/2019/01/043

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Abstract In this paper, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We use this information to calculate the maximum value of the so-called neutrino floor for direct dark matter detection experiments, which determines when these detectors are sensitive to the neutrino background. After including all relevant experimental constraints in different simplified neutrino models, we have found that the neutrino floor can increase by various orders of magnitude in the region of dark matter masses below 10 GeV in the case of scalar mediators, however, this spectacular enhancement is subject to the re-examination of supernovae bounds. The increase is approximately a factor of two for vector mediators. In the light of these results, future claims by direct detection experiments exploring the low-mass window must be carefully examined if a signal is found well above the expected Standard Model neutrino floor.
AbstractList In this study, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We use this information to calculate the maximum value of the so-called neutrino floor for direct dark matter detection experiments, which determines when these detectors are sensitive to the neutrino background. After including all relevant experimental constraints in different simplified neutrino models, we have found that the neutrino floor can increase by various orders of magnitude in the region of dark matter masses below 10 GeV in the case of scalar mediators, however, this spectacular enhancement is subject to the re-examination of supernovae bounds. The increase is approximately a factor of two for vector mediators. In the light of these results, future claims by direct detection experiments exploring the low-mass window must be carefully examined if a signal is found well above the expected Standard Model neutrino floor.
In this paper, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We use this information to calculate the maximum value of the so-called neutrino floor for direct dark matter detection experiments, which determines when these detectors are sensitive to the neutrino background. After including all relevant experimental constraints in different simplified neutrino models, we have found that the neutrino floor can increase by various orders of magnitude in the region of dark matter masses below 10 GeV in the case of scalar mediators, however, this spectacular enhancement is subject to the re-examination of supernovae bounds. The increase is approximately a factor of two for vector mediators. In the light of these results, future claims by direct detection experiments exploring the low-mass window must be carefully examined if a signal is found well above the expected Standard Model neutrino floor.
Author Machado, P.A.N.
Campo, A. Olivares-Del
Reid, E.
Cerdeño, D.G.
Bœhm, C.
Author_xml – sequence: 1
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  surname: Machado
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  givenname: A. Olivares-Del
  surname: Campo
  fullname: Campo, A. Olivares-Del
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  givenname: E.
  surname: Reid
  fullname: Reid, E.
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Issue 1
Keywords numerical calculations
new physics
neutrino properties
dark matter: direct detection
neutrino: background
dark matter: mediation
dark matter: mass
neutrino nucleus: elastic scattering
neutrino: model
CDMS
XENON
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dark matter detectors
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Snippet In this paper, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We...
In this study, we compute the contribution to the coherent elastic neutrino-nucleus scattering cross section from new physics models in the neutrino sector. We...
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StartPage 43
SubjectTerms ASTRONOMY AND ASTROPHYSICS
Astrophysics
Coherent scattering
Constraint modelling
Dark matter
dark matter detectors
Elastic scattering
Floors
High Energy Physics - Phenomenology
neutrino properties
Neutrinos
Physics
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Scattering cross sections
Supernovae
Title How high is the neutrino floor?
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