Concept information
Terme préférentiel
Kerr-Newman metric
Définition(s)
- The Kerr–Newman metric is the most general asymptotically flat, stationary solution of the Einstein–Maxwell equations in general relativity that describes the spacetime geometry in the region surrounding an electrically charged, rotating mass. It generalizes the Kerr metric by taking into account the field energy of an electromagnetic field, in addition to describing rotation. It is one of a large number of various different electrovacuum solutions, that is, of solutions to the Einstein–Maxwell equations which account for the field energy of an electromagnetic field. Such solutions do not include any electric charges other than that associated with the gravitational field, and are thus termed vacuum solutions. (Wikipedia, The Free Encyclopedia, https://en.wikipedia.org/wiki/Kerr%E2%80%93Newman_metric)
Concept(s) générique(s)
Synonyme(s)
- Kerr-Newman black hole
- Kerr-Newman cosmology
- Kerr-Newman model
- Kerr-Newman space
- Kerr-Newman spacetime
- Kerr-Newman universe
Traductions
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français
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cosmologie de Kerr-Newman
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espace de Kerr-Newman
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espace-temps de Kerr-Newman
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modèle de Kerr-Newman
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trou noir de Kerr-Newman
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univers de Kerr-Newman
URI
http://data.loterre.fr/ark:/67375/MDL-QNSK9FFH-V
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