Quasinormal modes of renormalization group improved Dymnikova regular black holes

@article{76401,
   author = {Konoplya, Roman and Stuchlík, Zdeněk and Zhidenko, A. and Zinhailo, Antonina Frantsivna},
   article_number = {10},
   doi = {http://dx.doi.org/10.1103/PhysRevD.107.104050},
   keywords = {free gravitatonial collapse;normal frequencies;perturbation; scalar},
   language = {eng},
   issn = {2470-0010},
   journal = {Physical Review D},
   title = {Quasinormal modes of renormalization group improved Dymnikova regular black holes},
   url = {https://journals.aps.org/prd/abstract/10.1103/PhysRevD.107.104050},
   volume = {107},
   year = {2023}
}

TY  - JOUR
ID  - 76401
AU  - Konoplya, Roman - Stuchlík, Zdeněk - Zhidenko, A. - Zinhailo, Antonina Frantsivna
PY  - 2023
TI  - Quasinormal modes of renormalization group improved Dymnikova regular black holes
JF  - Physical Review D
VL  - 107
IS  - 10
SP  - "104050-1"-"104050-12"
EP  - "104050-1"-"104050-12"
SN  - 24700010
KW  - free gravitatonial collapse;normal frequencies;perturbation
KW  - scalar
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.107.104050
N2  - We find accurate quasinormal frequencies of a quantum corrected black hole constructed in the renormalization group theory via the coordinate-independent iterative procedure, leading to the Dymnikova regular black hole. We show that while the fundamental mode is only slightly affected by the quantum correction, the overtones change at a much stronger rate. This outburst of overtones occurs because of the deformation of the geometry of the Schwarzschild black hole solely near the event horizon. For finding accurate values of overtones we developed a general procedure allowing one to use the Leaver method to metrics which, initially, are not expressed in terms of rational functions.
ER  - 

KONOPLYA, Roman, Zdeněk STUCHLÍK, A. ZHIDENKO a Antonina Frantsivna ZINHAILO. Quasinormal modes of renormalization group improved Dymnikova regular black holes. \textit{Physical Review D}. 2023, roč.~107, č.~10, s.~''104050-1''-''104050-12'', 12 s. ISSN~2470-0010. Dostupné z: https://dx.doi.org/10.1103/PhysRevD.107.104050.