An accurate model for the primordial black hole mass distribution from a peak in the power spectrum (2020)

First Author: Gow A

Attributed to: University of Sussex Astronomy Consolidated Grant 2020-2023 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2009.03204

Publication URI: https://arxiv.org/abs/2009.03204

Type: Other