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Isospin-Violating Dark Matter Benchmarks for Snowmass 2013

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arxiv 1307.1758 v2 pith:ZAIW46WX submitted 2013-07-06 hep-ph astro-ph.CO

Isospin-Violating Dark Matter Benchmarks for Snowmass 2013

classification hep-ph astro-ph.CO
keywords ivdmdarkdetectiondirectexperimentsisospin-violatingmatterparameter
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Isospin-violating dark matter (IVDM) generalizes the standard spin-independent scattering parameter space by introducing one additional parameter, the neutron-to-proton coupling ratio f_n/f_p. In IVDM the implications of direct detection experiments can be altered significantly. We review the motivations for considering IVDM and present benchmark models that illustrate some of the qualitatively different possibilities. IVDM strongly motivates the use of a variety of target nuclei in direct detection experiments.

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  1. Shifting the neutrino fog: studying the Isospin-violating Dark Matter case

    hep-ph 2025-12 conditional novelty 4.0

    Isospin-violating dark matter shifts the neutrino fog: in xenon, a Z-portal model (f_n/f_p ≈ -22) lowers the discovery limit while the Scotogenic model (f_n/f_p = 0) raises it.