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arXiv · 1504.03292

Inhomogeneous seeding of quark bubbles in Neutron Stars

M. A. Perez-Garcia
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Abstract

In this proceedings contribution we briefly discuss about the consequences of the presence of Majorana dark matter in a dense neutron star environment focusing on a particularly interesting possible indirect effect, namely that of bubble nucleation. This is somewhat similar to current techniques developed for direct detection using bubble chamber or superheated droplet detectors.

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M. A. Perez-Garcia. 2015-04-13. Inhomogeneous seeding of quark bubbles in Neutron Stars. https://arxiv.org/abs/1504.03292

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