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Электронный каталог: Kunz, J. - Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model
Kunz, J. - Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model
Статья
Автор: Kunz, J.
Physical Review D [Electronic resource]: Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model
б.г.
ISBN отсутствует
Автор: Kunz, J.
Physical Review D [Electronic resource]: Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model
б.г.
ISBN отсутствует
Статья
Kunz, J.
Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model / J.Kunz, Ya.Shnir // Physical Review D [Electronic resource]. – 2023. – Vol.107, No.10. – P.104062. – URL: https://doi.org/10.1103/PhysRevD.107.104062. – Bibliogr.:57.
We obtain charged spherically symmetric black holes in the two-component scalar Einstein-Maxwell-Friedberg-Lee-Sirlin model with a symmetry breaking potential. These asymptotically flat black holes carry resonant scalar Q-hair. As expected, these hairy black holes give rise to nonuniqueness. When comparing these solutions with the corresponding charged boson stars and Reissner-Nordström black holes, we find a different pattern in the case of a massive real scalar component and a massless one. We demonstrate that, as the real component becomes massless, the resonant hairy black holes bifurcate from Reissner-Nordström black holes for sufficiently small gravitational coupling.
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 44/023
Kunz, J.
Charged Hairy Black Holes in the Gauged Einstein-Friedberg-Lee-Sirlin Model / J.Kunz, Ya.Shnir // Physical Review D [Electronic resource]. – 2023. – Vol.107, No.10. – P.104062. – URL: https://doi.org/10.1103/PhysRevD.107.104062. – Bibliogr.:57.
We obtain charged spherically symmetric black holes in the two-component scalar Einstein-Maxwell-Friedberg-Lee-Sirlin model with a symmetry breaking potential. These asymptotically flat black holes carry resonant scalar Q-hair. As expected, these hairy black holes give rise to nonuniqueness. When comparing these solutions with the corresponding charged boson stars and Reissner-Nordström black holes, we find a different pattern in the case of a massive real scalar component and a massless one. We demonstrate that, as the real component becomes massless, the resonant hairy black holes bifurcate from Reissner-Nordström black holes for sufficiently small gravitational coupling.
ОИЯИ = ОИЯИ (JINR)2023
Спец.(статьи,препринты) = С 322.2 - Космология. Гравитационные волны
Бюллетени = 44/023