Abstract

It is shown that the paper “Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model” (Kanzi and Sakallı in Eur Phys J C 81:501, 2021) recently published in this journal is based on an incorrect result obtained by Ding et al. (Eur Phys J C 80:178, 2020) for a Kerr-like black hole solution.

Details

Title
Comment on “Greybody radiation and quasinormal modes of Kerr-like black hole in Bumblebee gravity model”
Author
Maluf, R V 1 ; Muniz, C R 2   VIAFID ORCID Logo 

1  Universidade Federal do Ceará (UFC), Departamento de Física, Fortaleza, Brazil (GRID:grid.8395.7) (ISNI:0000 0001 2160 0329) 
2  Universidade Estadual do Ceará (UECE), Faculdade de Educação, Ciências e Letras de Iguatu, Iguatu, Brazil (GRID:grid.412327.1) (ISNI:0000 0000 9141 3257) 
Publication year
2022
Publication date
Jan 2022
Publisher
Springer Nature B.V.
ISSN
14346044
e-ISSN
14346052
Source type
Scholarly Journal
Language of publication
English
DOI
https://doi.org/10.1140/epjc/s10052-022-10039-z
ProQuest document ID
2624035013
Copyright
© The Author(s) 2022. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.