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Limits on momentum-dependent asymmetric dark matter with CRESST-II · Around

2016

Limits on momentum-dependent asymmetric dark matter with CRESST-II

Angloher, G., Bento, A., Bucci, C. et al.

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The usual assumption in direct dark matter searches is to only consider the spin-dependent or spin-independent scattering of dark matter particles.

However, especially in models with light dark matter particles $\mathcal{O}(\mathrm{GeV/c^2})$, operators which carry additional powers of the momentum transfer $q^2$ can become dominant.
One such model based on asymmetric dark matter has been invoked to overcome discrepancies in helioseismology and an indication was found for a particle with preferred mass of 3 $\mathrm{GeV/c^2}$ and cross section of $10^{-37} \mathrm{cm^2}$.
Recent data from the CRESST-II experiment, which uses cryogenic detectors based on $\mathrm{CaWO_4}$ to search for nuclear recoils induced by dark matter particles, are used to constrain these momentum-dependent models.

Built on

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S. Chang, A. Pierce, and N. Weiner, · 2010
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