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Black holes with Weyl charge and non-Riemannian waves

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Black holes with Weyl charge and non-Riemannian waves. / Tucker, Robin; Wang, Charles.
In: Classical and Quantum Gravity, Vol. 12, No. 10, 10.1995, p. 2587-2605.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Tucker, R & Wang, C 1995, 'Black holes with Weyl charge and non-Riemannian waves', Classical and Quantum Gravity, vol. 12, no. 10, pp. 2587-2605. https://doi.org/10.1088/0264-9381/12/10/016

APA

Tucker, R., & Wang, C. (1995). Black holes with Weyl charge and non-Riemannian waves. Classical and Quantum Gravity, 12(10), 2587-2605. https://doi.org/10.1088/0264-9381/12/10/016

Vancouver

Tucker R, Wang C. Black holes with Weyl charge and non-Riemannian waves. Classical and Quantum Gravity. 1995 Oct;12(10):2587-2605. doi: 10.1088/0264-9381/12/10/016

Author

Tucker, Robin ; Wang, Charles. / Black holes with Weyl charge and non-Riemannian waves. In: Classical and Quantum Gravity. 1995 ; Vol. 12, No. 10. pp. 2587-2605.

Bibtex

@article{06fa55e487434810acff1daee57f661e,
title = "Black holes with Weyl charge and non-Riemannian waves",
abstract = "A simple modification to Einstein's theory of gravity in terms of a non-Riemannian connection is examined. A new tensor-variational approach yields field equations that possess a covariance similar to the gauge covariance of electromagnetism. These equations are shown to possess solutions analogous to those found in the Einstein-Maxwell system. In particular one finds gravi-electric and gravi-magnetic charges contributing to a spherically symmetric static Reissner - Nordstr{\"o}m metric. Such Weyl `charges' provide a source for the non-Riemannian torsion and metric gradient fields instead of the electromagnetic field. The theory suggests that matter may be endowed with gravitational charges that couple to gravity in a manner analogous to electromagnetic couplings in an electromagnetic field. The nature of gravitational coupling to spinor matter in this theory is also investigated and a solution exhibiting a plane-symmetric gravitational metric wave coupled via non-Riemannian waves to a propagating spinor field is presented. ",
author = "Robin Tucker and Charles Wang",
year = "1995",
month = oct,
doi = "10.1088/0264-9381/12/10/016",
language = "English",
volume = "12",
pages = "2587--2605",
journal = "Classical and Quantum Gravity",
issn = "0264-9381",
publisher = "IOP Publishing",
number = "10",

}

RIS

TY - JOUR

T1 - Black holes with Weyl charge and non-Riemannian waves

AU - Tucker, Robin

AU - Wang, Charles

PY - 1995/10

Y1 - 1995/10

N2 - A simple modification to Einstein's theory of gravity in terms of a non-Riemannian connection is examined. A new tensor-variational approach yields field equations that possess a covariance similar to the gauge covariance of electromagnetism. These equations are shown to possess solutions analogous to those found in the Einstein-Maxwell system. In particular one finds gravi-electric and gravi-magnetic charges contributing to a spherically symmetric static Reissner - Nordström metric. Such Weyl `charges' provide a source for the non-Riemannian torsion and metric gradient fields instead of the electromagnetic field. The theory suggests that matter may be endowed with gravitational charges that couple to gravity in a manner analogous to electromagnetic couplings in an electromagnetic field. The nature of gravitational coupling to spinor matter in this theory is also investigated and a solution exhibiting a plane-symmetric gravitational metric wave coupled via non-Riemannian waves to a propagating spinor field is presented.

AB - A simple modification to Einstein's theory of gravity in terms of a non-Riemannian connection is examined. A new tensor-variational approach yields field equations that possess a covariance similar to the gauge covariance of electromagnetism. These equations are shown to possess solutions analogous to those found in the Einstein-Maxwell system. In particular one finds gravi-electric and gravi-magnetic charges contributing to a spherically symmetric static Reissner - Nordström metric. Such Weyl `charges' provide a source for the non-Riemannian torsion and metric gradient fields instead of the electromagnetic field. The theory suggests that matter may be endowed with gravitational charges that couple to gravity in a manner analogous to electromagnetic couplings in an electromagnetic field. The nature of gravitational coupling to spinor matter in this theory is also investigated and a solution exhibiting a plane-symmetric gravitational metric wave coupled via non-Riemannian waves to a propagating spinor field is presented.

U2 - 10.1088/0264-9381/12/10/016

DO - 10.1088/0264-9381/12/10/016

M3 - Journal article

VL - 12

SP - 2587

EP - 2605

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 10

ER -