Quasinormal modes and Hawking radiation of black holes in cubic gravity

@article{49325,
   author = {Konoplya, Roman and Zinhailo, Antonina Frantsivna and Stuchlík, Zdeněk},
   article_location = {US - Spojené státy americké},
   article_number = {4},
   doi = {http://dx.doi.org/10.1103/PhysRevD.102.044023},
   keywords = {quasinormal modes ; Hawking radiation; four-dimensional asymptotically flat black holes},
   language = {eng},
   issn = {1550-7998},
   journal = {Physical Review D},
   title = {Quasinormal modes and Hawking radiation of black holes in cubic gravity},
   url = {https://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.044023},
   volume = {102},
   year = {2020}
}

TY  - JOUR
ID  - 49325
AU  - Konoplya, Roman - Zinhailo, Antonina Frantsivna - Stuchlík, Zdeněk
PY  - 2020
TI  - Quasinormal modes and Hawking radiation of black holes in cubic gravity
JF  - Physical Review D
VL  - 102
IS  - 4
SP  - "044023-1"-"044023-11"
EP  - "044023-1"-"044023-11"
SN  - 15507998
KW  - quasinormal modes
KW  - Hawking radiation
KW  - four-dimensional asymptotically flat black holes
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.044023
N2  - We consider quasinormal modes and Hawking radiation of four-dimensional asymptotically flat black holes in the most general up to-cubic-order-in-curvature dimension-independent Einsteinian theory of gravity that shares its graviton spectrum with the Einstein theory on constant curvature backgrounds. We show that damping rate and real oscillation frequencies of quasinormal modes for scalar, electromagnetic and Dirac fields are suppressed once the coupling with the cubic term is on. The intensity of Hawking radiation is suppressed as well, leading to, roughly, one order longer lifetime at a sufficiently large coupling constant.
ER  - 

KONOPLYA, Roman, Antonina Frantsivna ZINHAILO a Zdeněk STUCHLÍK. Quasinormal modes and Hawking radiation of black holes in cubic gravity. \textit{Physical Review D}. US - Spojené státy americké, roč.~102, č.~4, s.~''044023-1''-''044023-11'', 11 s. ISSN~1550-7998. doi:10.1103/PhysRevD.102.044023. 2020.