Nuclear spin structure in dark matter search: The zero momentum transfer limit
arXiv:hep-ph/0406218
Abstract
We review the calculation of spin-dependent matrix elements relevant to scattering of weakly interacting massive particles on nuclei. A comprehensive list, to our knowledge, of the proton and neutron total spin expectation values ( and ) calculated within different nuclear models is presented. These values allow a conclusion about the event rate expected in direct dark matter search experiments due to spin-dependent neutralino-nucleon interaction, provided neutralino is a dark matter particle.
24 pages, 10 tables, revtex4
Cited by in corpus (12)
- Saturated Overburden Scattering and the Multiscatter Frontier: Discovering Dark Matter at the Planck Mass and Beyond
- Evaporation of dark matter from celestial bodies
- Solar reflection of light dark matter with heavy mediators
- Foraging for dark matter in large volume liquid scintillator neutrino detectors with multiscatter events
- Terrestrial and Martian Heat Flow Limits on Dark Matter
- Present and projected sensitivities of Dark Matter direct detection experiments to effective WIMP-nucleus couplings
- A tale of dark matter capture, sub-dominant WIMPs, and neutrino observatories
- Is it possible to discover a dark matter particle with an accelerator?
- New Projections for Dark Matter Searches with Paleo-Detectors
- XQC and CSR constraints on strongly interacting dark matter with spin and velocity dependent cross sections
- Constraining dark matter-nucleon scattering cross section by the background electron anti-neutrino flux data
- Multi-frequency test of dark matter annihilation into long-lived particles in Sirius