Inhomogeneous seeding of quark bubbles in Neutron Stars
arXiv:1504.03292
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.
9 pages, 3 figures, Invited talk at the COMPACT STARS IN THE QCD PHASE DIAGRAM IV (CSQCD IV), September 26 - 30, 2014, Prerow, Germany