Effect of electromagnetic dipole dark matter on energy transport in the solar interior
Date
2017
Authors
Geytenbeek, B.
Rao, S.
Scott, P.
Serenelli, A.
Vincent, A.
White, M.
Williams, A.
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Journal article
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Journal of Cosmology and Astroparticle Physics, 2017; 2017(3):1-37
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Ben Geytenbeek, Soumya Rao, Pat Scott, Aldo Serenelli, Aaron C. Vincent, Martin White and Anthony G. Williams
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Abstract
In recent years, a revised set of solar abundances has led to a discrepancy in the sound-speed profile between helioseismology and theoretical solar models. Conventional solutions require additional mechanisms for energy transport within the Sun. Vincent et al. have recently suggested that dark matter with a momentum or velocity dependent cross section could provide a solution. In this work, we consider three models of dark matter with such cross sections and their effect on the stellar structure. In particular, the three models incorporate dark matter particles interacting through an electromagnetic dipole moment: an electric dipole, a magnetic dipole or an anapole. Each model is implemented in the DarkStec stellar evolution program, which incorporates the effects of dark matter capture and heat transport within the solar interior. We show that dark matter with an anapole moment of ∼1 GeV⁻² or magnetic dipole moment of ∼10⁻³μp can improve the soundspeed profile, small frequency separations and convective zone radius with respect to the Standard Solar Model. However, the required dipole moments are strongly excluded by direct detection experiments.
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© 2017 IOP Publishing Ltd and Sissa Medialab srl