A critical look at cosmions

Computer Science – Sound

Scientific paper

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Dark Matter, Elementary Particle Interactions, Solar Interior, Solar Neutrinos, Baryons, Stellar Evolution, Sunspots

Scientific paper

A thorough numerical investigation of the cosmion hypothesis as a solution to the solar neutrino puzzle was performed using the Saclay solar evolution code. The ensuing constraints on cosmion parameters appear as domains in the plane of cosmion-proton cross section versus cosmion mass. Various hypotheses on cosmion couplings are considered. Comparison with available experimental data on direct dark matter detection excludes most of the domain in the 'vector' case. In the 'axial' case the results provide useful hints for experiments. The effect of cosmions on the sound speed near the center of the sun, confronted with present knowledge and data on helioseismology, does not improve the comparison between standard predictions and helioseismological inversion.

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