Testing General Relativity with Pulsar Timing

Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8615

Full metadata record

DC Field	Value	Language
dc.creator	Stairs Ingrid H.	-
dc.date	2003	-
dc.date.accessioned	2013-06-01T11:39:49Z	-
dc.date.available	2013-06-01T11:39:49Z	-
dc.date.issued	2013-06-01	-
dc.identifier	http://www.livingreviews.org/lrr-2003-5	-
dc.identifier	http://www.doaj.org/doaj?func=openurl&genre=article&issn=14338351&date=2003&volume=6&issue=&spage=5	-
dc.identifier.uri	http://koha.mediu.edu.my:8181/jspui/handle/123456789/8615	-
dc.description	Pulsars of very different types, including isolated objects and binaries (with short- and long-period orbits, and white-dwarf and neutron-star companions) provide the means to test both the predictions of general relativity and the viability of alternate theories of gravity. This article presents an overview of pulsars, then discusses the current status of and future prospects for tests of equivalence-principle violations and strong-field gravitational experiments.	-
dc.publisher	Albert Einstein Institut, Max-Planck Institute for Gravitati	-
dc.source	Living Reviews in Relativity	-
dc.subject	Experimental Foundations of Gravitation	-
dc.title	Testing General Relativity with Pulsar Timing	-
Appears in Collections:	Physics and Astronomy

Files in This Item:

There are no files associated with this item.

DSpace JSPUI