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Isospin-Violating Dark Matter Benchmarks for Snowmass 2013

2013/07/06 by Jonathan L. Feng, Jason Kumar, Feng, Jonathan L. +5 · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #Dark Matter and Cosmic Phenomena #Dark matter #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Isospin #Particle physics #Particle physics theoretical and experimental studies #Physics #astro-ph.CO #hep-ph

paper · pdf · doi:10.48550/arxiv.1307.1758

LaTeX, 5 pages, 4 figures. v2: minor figure revisions

openalex publication_date 2013/07/06 · arxiv created 2013/08/01 · arxiv updated 2013/08/02 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

Isospin-violating dark matter (IVDM) generalizes the standard spin-independent scattering parameter space by introducing one additional parameter, the neutron-to-proton coupling ratio fn/fp. 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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