Vacuum polarization and the spontaneous loss of charge by black holes

1975/10/01 by G. W. Gibbons · 1 voice · 6 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Relativity and Gravitational Theory

paper · doi:10.1007/bf01609829

crossref issued 1975/10/01 · crossref published 1975/10/01 · crossref published-print 1975/10/01 · openalex publication_date 1975/10/01 · crossref created 2005/04/30 · crossref deposited 2021/07/10 · openalex created_date 2025/10/10 · crossref indexed 2026/07/24 · openalex updated_date 2026/07/29

Citations

• The four laws of black hole mechanics

Cited by

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• A quasilocal Hamiltonian for gravity with classical and quantum applications
• Scalar quasinormal modes of magnetically charged black holes in a quintessence field

Discussions

• $$ f(r)=1-\frac{2GM}{c^2 r}+\frac{GQ^2}{4\pi\epsilon_0 c^4 r^2} $$ $$ r_\pm=\frac{GM}{c^2}\pm \sqrt{\left(\frac{GM}{c^2}\right)^2-\frac{GQ^2}{4\pi\epsilon_0 c^4}} $$ Again, as usual $ Q_{\rm ext}^2=4\ [stackexchange, 2 points]