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Автор Fabrizio Canfora
Автор Gaetano Vilasi
Дата выпуска 2003-12-01
dc.description A model is proposed to describe a transition from a charged black hole of mass M and charge Q to one of mass M̅ and charge Q̅. The basic equations are derived from the non-vacuum Einstein field equations sourced by the Coulomb field and by a null scalar field with a nonvanishing trace anomaly. It is shown that the nonvanishing trace of the energy-momentum tensor prevents the formation of a naked singularity.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Back reaction from trace anomaly in RN-blackholes evaporation
Тип paper
DOI 10.1088/1126-6708/2003/12/055
Electronic ISSN 1029- 8479
Print ISSN 1126-6708
Журнал Journal of High Energy Physics
Том 2003
Первая страница 55
Последняя страница 055
Выпуск 12

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