Planetary Perturbation with Cosmological Constant

dc.creatorNeupane, Ishwaree P.
dc.date1999-02-12
dc.date.accessioned2026-07-07T03:32:57Z
dc.date.available2026-07-07T03:32:57Z
dc.descriptionA contribution of quantum vacuum to the energy momentum tensor is inevitably experienced in the present universe. One requires the presence of non-zero cosmological constant ($Λ$) to make the various observations consistent. A case of $Λ$ in the Schwarzschild de Sitter space-time shows that precession of perihelion orbit provides a sensative solar test for non-zero $Λ$. Application of the relations involving $Λ$ to the planetery perturbation indicates the values near to the present bound on $Λ$. Also suggested are some relations in vacuum dominated flat universe with a positive $Λ$.
dc.description6 pages, RevTex, some corrections on gr-qc/9812096
dc.identifierhttps://arxiv.org/abs/gr-qc/9902039
dc.identifierhttp://arxiv.org/abs/gr-qc/9902039
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36434
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePlanetary Perturbation with Cosmological Constant
dc.typetext

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