Black holes and the classical model of a particle in Einstein non-linear electrodynamics theory

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dc.contributor.author	Mazharimousavi, S. Habib
dc.contributor.author	Halilsoy, Mustafa
dc.date.accessioned	2016-01-20T11:27:29Z
dc.date.available	2016-01-20T11:27:29Z
dc.date.issued	2009
dc.identifier.citation	S. Habib Mazharimousavi and Mustafa Halilsoy, Phys. Lett. B 678 (2009) 407:arXiv:0812.0989"Black holes and the classical model of a particle in Einstein non-linear electrodynamics theory".	en_US
dc.identifier.issn	1873-2445 (online)
dc.identifier.issn	ISSN: 0370-2693 (print)
dc.identifier.other	DOI: 10.1016/j.physletb.2009.06.049
dc.identifier.uri	http://hdl.handle.net/11129/2018
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	Modified by a logarithmic term, the non-linear electrodynamics (NED) model of the Born–Infeld (BI) action is reconsidered. Unlike the standard BI action, this choice provides interesting integrals of the Einstein-NED equations. It is found that the spherical matching process for a regular black hole entails indispensable surface stresses that vanish only for a specific value of the BI parameter. This solution represents a classical model of an elementary particle whose radius coincides with the horizon. In flat spacetime, a charged particle becomes a conducting shell with a radius proportional to the BI parameter.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physics Letters B, Elsevier	en_US
dc.relation.ispartofseries	Elsevier;Physics Letters B Volume 678, Issue 4, 27 July 2009, Pages 407–410
dc.subject	gravity	en_US
dc.subject	general relativity	en_US
dc.subject	Black hole	en_US
dc.subject	non-linear electrodynamics theory	en_US
dc.title	Black holes and the classical model of a particle in Einstein non-linear electrodynamics theory	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).