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Testing General Relativity with Pulsar Timing

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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


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