Matches in SemOpenAlex for { <https://semopenalex.org/work/W2156520281> ?p ?o ?g. }
- W2156520281 abstract "We perform a comprehensive analysis of the spectrum of proper oscillations (quasinormal modes), transmission/reflection coefficients and Hawking radiation for a massive charged scalar field in the background of the Kerr-Newman black hole immersed in an asymptotically homogeneous magnetic field. There are two main effects: the Zeeman shift of the particle energy in the magnetic field and the difference of values of an electromagnetic potential between the horizon and infinity, i.e. the Faraday induction. We have shown that turning on the magnetic field induces a stronger energy-emission rate and leads to recharging of the black hole. Thus, a black hole immersed in a magnetic field evaporates much quicker, achieving thereby an extremal state in a shorter period of time. Quasinormal modes are moderately affected by the presence of a magnetic field which is assumed to be relatively small compared to the gravitational field of the black hole." @default.
- W2156520281 created "2016-06-24" @default.
- W2156520281 creator A5011416197 @default.
- W2156520281 creator A5034397464 @default.
- W2156520281 creator A5085046045 @default.
- W2156520281 date "2011-01-26" @default.
- W2156520281 modified "2023-10-02" @default.
- W2156520281 title "Quasinormal modes, scattering, and Hawking radiation of Kerr-Newman black holes in a magnetic field" @default.
- W2156520281 cites W1629749464 @default.
- W2156520281 cites W1968369949 @default.
- W2156520281 cites W1982349891 @default.
- W2156520281 cites W1987881050 @default.
- W2156520281 cites W1997874012 @default.
- W2156520281 cites W1998292677 @default.
- W2156520281 cites W2005263011 @default.
- W2156520281 cites W2015207475 @default.
- W2156520281 cites W2015757619 @default.
- W2156520281 cites W2018084472 @default.
- W2156520281 cites W2019400496 @default.
- W2156520281 cites W2021706553 @default.
- W2156520281 cites W2023347320 @default.
- W2156520281 cites W2027298238 @default.
- W2156520281 cites W2031976080 @default.
- W2156520281 cites W2035105419 @default.
- W2156520281 cites W2037097324 @default.
- W2156520281 cites W2038955315 @default.
- W2156520281 cites W2040729881 @default.
- W2156520281 cites W2059126891 @default.
- W2156520281 cites W2059236649 @default.
- W2156520281 cites W2069764580 @default.
- W2156520281 cites W2075367341 @default.
- W2156520281 cites W2080705137 @default.
- W2156520281 cites W2082241931 @default.
- W2156520281 cites W2083347038 @default.
- W2156520281 cites W2091302669 @default.
- W2156520281 cites W2091940450 @default.
- W2156520281 cites W2104443781 @default.
- W2156520281 cites W2107259515 @default.
- W2156520281 cites W2114830198 @default.
- W2156520281 cites W2128626098 @default.
- W2156520281 cites W2142314120 @default.
- W2156520281 cites W2144095749 @default.
- W2156520281 cites W2145326299 @default.
- W2156520281 cites W2149420708 @default.
- W2156520281 cites W2159827406 @default.
- W2156520281 cites W2168424351 @default.
- W2156520281 cites W2594121836 @default.
- W2156520281 cites W2949923492 @default.
- W2156520281 cites W3098226165 @default.
- W2156520281 cites W3099252948 @default.
- W2156520281 cites W3103204141 @default.
- W2156520281 cites W3123637741 @default.
- W2156520281 doi "https://doi.org/10.1103/physrevd.83.024031" @default.
- W2156520281 hasPublicationYear "2011" @default.
- W2156520281 type Work @default.
- W2156520281 sameAs 2156520281 @default.
- W2156520281 citedByCount "33" @default.
- W2156520281 countsByYear W21565202812012 @default.
- W2156520281 countsByYear W21565202812013 @default.
- W2156520281 countsByYear W21565202812014 @default.
- W2156520281 countsByYear W21565202812015 @default.
- W2156520281 countsByYear W21565202812017 @default.
- W2156520281 countsByYear W21565202812018 @default.
- W2156520281 countsByYear W21565202812019 @default.
- W2156520281 countsByYear W21565202812020 @default.
- W2156520281 countsByYear W21565202812021 @default.
- W2156520281 countsByYear W21565202812023 @default.
- W2156520281 crossrefType "journal-article" @default.
- W2156520281 hasAuthorship W2156520281A5011416197 @default.
- W2156520281 hasAuthorship W2156520281A5034397464 @default.
- W2156520281 hasAuthorship W2156520281A5085046045 @default.
- W2156520281 hasBestOaLocation W21565202812 @default.
- W2156520281 hasConcept C104062141 @default.
- W2156520281 hasConcept C104954878 @default.
- W2156520281 hasConcept C106301342 @default.
- W2156520281 hasConcept C115260700 @default.
- W2156520281 hasConcept C121332964 @default.
- W2156520281 hasConcept C155675718 @default.
- W2156520281 hasConcept C190330329 @default.
- W2156520281 hasConcept C25227350 @default.
- W2156520281 hasConcept C26873012 @default.
- W2156520281 hasConcept C3079626 @default.
- W2156520281 hasConcept C31258907 @default.
- W2156520281 hasConcept C40745267 @default.
- W2156520281 hasConcept C41008148 @default.
- W2156520281 hasConcept C50341732 @default.
- W2156520281 hasConcept C62520636 @default.
- W2156520281 hasConcept C74172769 @default.
- W2156520281 hasConcept C82422596 @default.
- W2156520281 hasConcept C89305328 @default.
- W2156520281 hasConceptScore W2156520281C104062141 @default.
- W2156520281 hasConceptScore W2156520281C104954878 @default.
- W2156520281 hasConceptScore W2156520281C106301342 @default.
- W2156520281 hasConceptScore W2156520281C115260700 @default.
- W2156520281 hasConceptScore W2156520281C121332964 @default.
- W2156520281 hasConceptScore W2156520281C155675718 @default.
- W2156520281 hasConceptScore W2156520281C190330329 @default.
- W2156520281 hasConceptScore W2156520281C25227350 @default.
- W2156520281 hasConceptScore W2156520281C26873012 @default.
- W2156520281 hasConceptScore W2156520281C3079626 @default.