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.
arXiv comment9 pages, 3 figures, Invited talk at the COMPACT STARS IN THE QCD PHASE DIAGRAM IV (CSQCD IV), September 26 - 30, 2014, Prerow, Germany