Author:
Banerjee Indra Kumar,Dey Ujjal Kumar
Abstract
AbstractIn this article we investigate the cumulative stochastic gravitational wave spectra as a tool to gain insight on the creation mechanism of primordial black holes. We consider gravitational waves from the production mechanism of primordial black holes and from the gravitational interactions of those primordial black holes among themselves and other astrophysical black holes. We specifically focus on asynchronous bubble nucleation during a first order phase transition as the creation mechanism. We have used two benchmark phase transitions through which the primordial black holes and the primary gravitational wave spectra have been generated. We have considered binary systems and close hyperbolic interactions of primordial black holes with other primordial and astrophysical black holes as the source of the secondary part of the spectra. We have shown that this unique cumulative spectra have features which directly and indirectly depend on the specifics of the production mechanism.
Subject
Astronomy and Astrophysics
Reference101 articles.
1. The Hypothesis of Cores Retarded during Expansion and the Hot Cosmological Model;Zel'dovich;Soviet Astron. AJ (Engl. Transl. ),,1967
2. Observation of Gravitational Waves from a Binary Black Hole Merger;Abbott;Phys. Rev. Lett.,2016
3. Black holes in the early Universe;Carr;Mon. Not. Roy. Astron. Soc.,1974
4. Primordial Black Holes and Baryon Production in Grand Unified Theories;Grillo;Phys. Lett. B,1980
5. PRIMORDIAL BLACK HOLES AS A COSMOLOGICAL TEST OF GRAND UNIFICATION;Khlopov;Phys. Lett. B,1980
Cited by
8 articles.
订阅此论文施引文献
订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献