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Possible Indication of Momentum-Dependent Asymmetric Dark Matter in the Sun

2014/11/30 by Aaron C. Vincent, Pat Scott, Aldo Serenelli · 1 citation
Physics and Astronomy · #Astrophysics #Collider #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Dark matter #Helium #Momentum (technical analysis) #Neutrino #Neutrino oscillation #Nuclear physics #Nucleon #Observable #Particle physics #Physics #Quantum mechanics #Sigma #Solar and Space Plasma Dynamics #Solar neutrino #Standard solar model #astro-ph.CO #astro-ph.SR #hep-ph

paper · pdf · doi:10.1103/physrevlett.114.081302

published as Phys. Rev. Lett. 114, 081302 (2015) · 5 pages, 2 figures, 1 table. v2: small revisions; accepted for publication in PRL

arxiv created 2015/02/20 · openalex publication_date 2015/02/26 · arxiv updated 2015/03/04 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Broad disagreement persists between helioseismological observables and predictions of solar models computed with the latest surface abundances. Here we show that most of these problems can be solved by the presence of asymmetric dark matter coupling to nucleons as the square of the momentum q exchanged in the collision. We compute neutrino fluxes, small frequency separations, surface helium abundances, sound speed profiles, and convective zone depths for a number of models, showing more than a 6σ preference for q2 models over others, and over the standard solar model. The preferred mass (3 GeV) and reference dark matter-nucleon cross section (10-37 cm2 at q0=40 MeV) are within the region of parameter space allowed by both direct detection and collider searches.

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