Nonlocal Gravity Simulates Dark Matter

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dc.creatorHehl, Friedrich W.
dc.creatorMashhoon, Bahram
dc.date2008-12-05
dc.date2009-02-03
dc.date.accessioned2026-07-07T12:55:20Z
dc.date.available2026-07-07T12:55:20Z
dc.descriptionA nonlocal generalization of Einstein's theory of gravitation is constructed within the framework of the translational gauge theory of gravity. In the linear approximation, the nonlocal theory can be interpreted as linearized general relativity but in the presence of "dark matter" that can be simply expressed as an integral transform of matter. It is shown that this approach can accommodate the Tohline-Kuhn treatment of the astrophysical evidence for dark matter.
dc.description5 pages RevTex, v3: new material and references added, abstract somewhat extended
dc.identifierhttps://arxiv.org/abs/0812.1059
dc.identifierhttp://arxiv.org/abs/0812.1059
dc.identifierPhys.Lett.B673:279-282,2009
dc.identifierdoi:10.1016/j.physletb.2009.02.033
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224218
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleNonlocal Gravity Simulates Dark Matter
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