Unified Bertotti-Robinson and Melvin Spacetimes

dc.contributor.author	Halilsoy, Mustafa
dc.contributor.author	Mazharimousavi, S. Habib
dc.date.accessioned	2016-01-07T08:11:15Z
dc.date.available	2016-01-07T08:11:15Z
dc.date.issued	2013
dc.identifier.citation	M. Halilsoy and S. HabibMazharimousavi, arXiv:1211.6983 "Unified Bertotti-Robinson and Melvin Spacetimes". Phys. Rev. D 88, 064021 (2013).	en_US
dc.identifier.issn	1550-7998
dc.identifier.other	DOI: 10.1103/PhysRevD.88.064021
dc.identifier.uri	http://hdl.handle.net/11129/1926
dc.description	The file in this item is the publisher version (published version) of the article.	en_US
dc.description.abstract	We present a solution for the Einstein-Maxwell (EM) equations which unifies both the magnetic Bertotti-Robinson (BR) and Melvin (ML) solutions as a single metric in the axially symmetric coordinates t,ρ,z,φ. Depending on the strength of magnetic field the spacetime manifold, unlike the cases of separate BR and ML spacetime, develops singularity on the symmetry axis (ρ=0). Our analysis shows, beside other things that there are regions inaccessible to all null geodesics.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Physical Review D, American Physical Society (APS)	en_US
dc.relation.ispartofseries	;Phys. Rev. D 88, 064021 (2013)
dc.subject	general relativity	en_US
dc.subject	Melvin Spacetimes	en_US
dc.subject	Bertotti-Robinson	en_US
dc.subject	Einstein-Maxwell	en_US
dc.title	Unified Bertotti-Robinson and Melvin Spacetimes	en_US
dc.type	Article	en_US
dc.description.version	Publisher Version (Published Version).