Updated constraints on velocity and momentum-dependent asymmetric dark matter
Abstract
We present updated constraints on dark matter models with momentum-dependent or velocity-dependent interactions with nuclei, based on direct detection and solar physics. We improve our previous treatment of energy transport in the solar interior by dark matter scattering, leading to significant changes in fits to many observables. Based on solar physics alone, DM with a spin-independent coupling provides the best fit to data, and a statistically satisfactory solution to the solar abundance problem. Once direct detection limits are accounted for however, the best solution is spin-dependent scattering with a reference cross-section of 10 cm (at a reference velocity of km s), and a dark matter mass of about 5 GeV.
Keywords
Cite
@article{arxiv.1605.06502,
title = {Updated constraints on velocity and momentum-dependent asymmetric dark matter},
author = {Aaron C. Vincent and Pat Scott and Aldo Serenelli},
journal= {arXiv preprint arXiv:1605.06502},
year = {2016}
}
Comments
34 pages, 18 figures. Accepted in JCAP. Ancillary file likelihood_solarDM.dat contains observables and chi-squared values for each model studied