Discriminating dark matter candidates using direct detection
Creators
- 1. LAPTH, Universite de Savoie, CNRS, B.P.110, F-74941 Annecy-le-Vieux (France)
- 2. LAM, CNRS, Universite Aix-Marseille I, 2 place le Verrier, 13248 Marseille (France)
- 3. Skobeltsyn Inst. of Nuclear Physics, Moscow State Univ., Moscow 119992 (Russian Federation)
Description
We examine the predictions for both the spin-dependent and spin-independent direct detection rates in a variety of new particle physics models with dark matter candidates. We show that a determination of both spin-independent and spin-dependent amplitudes on protons and neutrons can in principle discriminate different candidates of dark matter up to a few ambiguities. We emphasize the importance of making measurements with different spin-dependent sensitive detector materials and the need for significant improvement of the detector sensitivities. Scenarios where exchange of new colored particles contributes significantly to the elastic scattering cross sections are often the most difficult to identify, the LHC should give an indication whether such scenarios are relevant for direct detection.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.79.015008;
- arXiv
- arXiv:0810.1362v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 79
- Journal Issue
- 1
- Journal Page Range
- p. 015008-015008.16
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41005329
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- AMPLITUDES; CERN LHC; CROSS SECTIONS; DETECTION; ELASTIC SCATTERING; FORECASTING; NEUTRONS; NONLUMINOUS MATTER; PARTICLES; PROTONS; SENSITIVITY; SPIN
- Descriptors DEC
- ACCELERATORS; ANGULAR MOMENTUM; BARYONS; CYCLIC ACCELERATORS; ELEMENTARY PARTICLES; FERMIONS; HADRONS; MATTER; NUCLEONS; PARTICLE PROPERTIES; SCATTERING; STORAGE RINGS; SYNCHROTRONS
Optional Information
- Notes
- (c) 2009 The American Physical Society