Speaker
Ruifeng Dong
(State University of New York at Buffalo)
Description
Primordial black holes evaporate by Hawking radiation, leaving a stochastic gravitational-wave background today. Its spectrum is affected by the formation mass, angular momentum and initial abundance. In particular, the particle emission is greatly enhanced at high frequencies for fast-rotating black holes. In this work, we calculated this spectrum for a wide range of these parameters. Besides, we used the latest constraints on the abundance and found the upper bound on today's spectral density of gravitational waves.
Summary
A stochastic gravitational-wave background from primordial black holes is studied comprehensively.
Primary authors
Ruifeng Dong
(State University of New York at Buffalo)
William Kinney
(Univ. at Buffalo, SUNY)
Dejan Stojkovic
(SUNY at Buffalo)
