Comment on ``Perturbative Method to solve fourth-order Gravity Field Equations"

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dc.creatorCampanelli, Manuela
dc.date1995-06-22
dc.date.accessioned2026-07-07T03:30:42Z
dc.date.available2026-07-07T03:30:42Z
dc.descriptionWe reconsider the cosmic string perturbative solution to the classical fourth-order gravity field equations, obtained in Ref.\cite{CLA94}, and we obtain that static, cylindricaly symmetric gauge cosmic strings, with constant energy density, can contain only $β$-terms in the first order corrections to the interior gravitational field, while the exact exterior solution is a conical spacetime with deficit angle $D=8πμ$.
dc.description6 pages, Revtex
dc.identifierhttps://arxiv.org/abs/gr-qc/9506045
dc.identifierhttp://arxiv.org/abs/gr-qc/9506045
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35612
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleComment on ``Perturbative Method to solve fourth-order Gravity Field Equations"
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