Thermal Gravitational Waves from Primordial Black Holes

Sivaram, C; Arun, K

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dc.contributor.author	Sivaram, C
dc.contributor.author	Arun, K
dc.date.accessioned	2012-02-07T14:13:31Z
dc.date.available	2012-02-07T14:13:31Z
dc.date.issued	2011-08
dc.identifier.citation	The Open Astronomy Journal, Vol. 4, pp. 72-74	en
dc.identifier.issn	1874-3811
dc.identifier.uri	http://hdl.handle.net/2248/5692
dc.description	This is an open access article licensed under the terms of the Creative Commons Attribution Non-Commercial License (http://creativecommons.org/licenses/by-nc/3.0/) which permits unrestricted, non-commercial use, distribution and reproduction in any medium, provided the work is properly cited.	en
dc.description.abstract	Thermal gravitational waves can be generated in various sources such as, in the cores of stars, white dwarfs and neutron stars due to the fermion collisions in the dense degenerate Fermi gas [1-3]. Such high frequency thermal gravitational waves can also be produced during the collisions in a gamma ray burst [3] or during the final stages of the evaporation of primordial black holes [4]. Here we estimate the thermal gravitational waves from primordial black holes and estimate the integrated energy of the gravitational wave emission over the entire volume of the universe and over Hubble time. We also estimate the gravitational wave flux from gamma ray bursts and jets.	en
dc.language.iso	en	en
dc.publisher	Bentham Open	en
dc.relation.uri	http://dx.doi.org/10.2174/1874381101004010072	en
dc.rights	© Sivaram and Arun; Licensee Bentham Open	en
dc.subject	Thermal gravitational waves	en
dc.subject	Primordial black holes	en
dc.subject	Integrated Hawking flux.	en
dc.title	Thermal Gravitational Waves from Primordial Black Holes	en
dc.type	Article	en