Are carbon deflagration supernovae triggered by dark matter ?

Abstract

Collisions between stellar remnants and dark matter in the Galactic bulge are frequent, and the kinetic energy of a primordial black hole incident on a white dwarf, if it is all thermalized, will raise the degenerate core's temperature, by at least a degree in the case of a lunar mass black hole. This is an underestimate in two ways: the specific heat is less than 3k/2 per particle, and the incoming object is accelerated by gravitational focusing. Detailed physical models have recently been made of this triggering event. Present observational data are equivocal as to whether the radial distribution of type Ia supernovae in galaxies follows the starlight in the galaxies, or is more concentrated towards the center, as collisional triggering would suggest. But future samples of millions of supernovae from the Rubin telescope will change that.