PP-waves with torsion and metric-affine gravity

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dc.creatorPasic, Vedad
dc.creatorVassiliev, Dmitri
dc.date2005-05-31
dc.date.accessioned2026-07-07T06:24:38Z
dc.date.available2026-07-07T06:24:38Z
dc.descriptionA classical pp-wave is a 4-dimensional Lorentzian spacetime which admits a nonvanishing parallel spinor field; here the connection is assumed to be Levi-Civita. We generalise this definition to metric compatible spacetimes with torsion and describe basic properties of such spacetimes. We use our generalised pp-waves for constructing new explicit vacuum solutions of quadratic metric-affine gravity.
dc.description17 pages, LaTeX2e
dc.identifierhttps://arxiv.org/abs/gr-qc/0505157
dc.identifierhttp://arxiv.org/abs/gr-qc/0505157
dc.identifierClass.Quant.Grav. 22 (2005) 3961-3976
dc.identifierdoi:10.1088/0264-9381/22/19/010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96613
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectDifferential Geometry
dc.titlePP-waves with torsion and metric-affine gravity
dc.typetext

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