The gravitational field of a massless particle on the horizon of a stationary black hole
In this work, the field of a gravitational shockwave generated by a massless point-like particle is calculated at the event horizon of a stationary Kerr–Newman black hole. Using the geometric framework of generalized Kerr–Schild deformations in combination with the spin-coefficient formalism of Newm...
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| Published in | Classical and quantum gravity Vol. 38; no. 8; p. 85006 |
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| Main Author | |
| Format | Journal Article |
| Language | English |
| Published |
22.04.2021
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| Online Access | Get full text |
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| Abstract | In this work, the field of a gravitational shockwave generated by a massless point-like particle is calculated at the event horizon of a stationary Kerr–Newman black hole. Using the geometric framework of generalized Kerr–Schild deformations in combination with the spin-coefficient formalism of Newman and Penrose, it is shown that the field equations of the theory, at the event horizon of the black hole, can be reduced to a single linear ordinary differential equation for the so-called profile function of the geometry. This differential relation is solved exactly. Based on the results obtained, a physical interpretation is given for the found shockwave spacetime, and it is clarified how these results lead back to those of previous works on the subject, which deal with the much simpler cases of gravitational shockwaves in static black hole backgrounds. |
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| AbstractList | In this work, the field of a gravitational shockwave generated by a massless point-like particle is calculated at the event horizon of a stationary Kerr–Newman black hole. Using the geometric framework of generalized Kerr–Schild deformations in combination with the spin-coefficient formalism of Newman and Penrose, it is shown that the field equations of the theory, at the event horizon of the black hole, can be reduced to a single linear ordinary differential equation for the so-called profile function of the geometry. This differential relation is solved exactly. Based on the results obtained, a physical interpretation is given for the found shockwave spacetime, and it is clarified how these results lead back to those of previous works on the subject, which deal with the much simpler cases of gravitational shockwaves in static black hole backgrounds. |
| Author | Huber, Albert |
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| Cites_doi | 10.1088/0264-9381/17/9/303 10.1007/s10714-008-0722-5 10.1103/physrevlett.95.111102 10.1103/physrevd.62.104025 10.1007/bf00758149 10.1007/s10714-019-2512-7 10.1103/physrevd.52.7053 10.1103/physrevlett.85.3564 10.12942/lrr-2004-10 10.1063/1.523851 10.1088/0264-9381/16/2/027 10.1006/jmaa.1997.5903 10.1140/epjc/s10052-020-08714-0 10.1103/physrevd.35.1798 10.1088/0264-9381/32/13/132001 10.1016/0003-4916(81)90213-x 10.1088/1742-6596/600/1/012037 10.1017/CBO9780511564048 10.1063/1.1704788 10.1016/0550-3213(94)00573-w 10.1016/0550-3213(85)90525-5 10.1103/physrevd.64.044016 10.1017/CBO9780511535185 10.1088/1361-6382/ab7614 10.1088/0264-9381/19/6/311 |
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