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Spherically Symmetric Solutions of Gravitational Field Equations in Kalb-Ramond Background

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arxiv gr-qc/0102095 v1 pith:W5YRC2GU submitted 2001-02-22 gr-qc

classification gr-qc
keywords fieldbackgroundgravitationalkalb-ramondsolutionsphericallysymmetrictorsion
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Static spherically symmetric solution in a background spacetime with torsion is derived explicitly. The torsion considered here is identified with the field strength of a second rank antisymmetric tensor field namely the Kalb-Ramond field and the proposed solution therefore has much significance in a string inspired gravitational field theory.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Branch structure and nonextensive thermodynamics of Kalb-Ramond-ModMax black holes: observational signatures

    gr-qc 2026-01 reject novelty 4.0 of 10

    A multi-channel phenomenological study of Einstein-Kalb-Ramond-ModMax black holes whose Tsallis internal energy does not reduce to the black-hole mass in the standard-entropy limit.

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