Massive scalar field quasinormal modes of a Schwarzschild black hole surrounded by quintessence
Keyword(s):
AbstractWe present the quasinormal frequencies of the massive scalar field in the background of a Schwarzchild black hole surrounded by quintessence with the third-order WKB method. The mass of the scalar field u plays an important role in studying the quasinormal frequencies, the real part of the frequencies increases linearly as mass of the field u increases, while the imaginary part in absolute value decreases linearly which leads to damping more slowly than the massless scalar field. The frequencies have a limited value, so it is easier to detect the quasinormal modes. Moreover, owing to the presence of the quintessence, the massive scalar field damps more slowly.
2010 ◽
Vol 19
(01)
◽
pp. 63-78
◽
Keyword(s):
2017 ◽
Vol 32
(24)
◽
pp. 1750128
◽
2013 ◽
Vol 22
(05)
◽
pp. 1350026
◽
2006 ◽
Vol 21
(30)
◽
pp. 6183-6190
◽
2008 ◽
Vol 23
(05)
◽
pp. 359-369
◽
Keyword(s):
Keyword(s):
Keyword(s):
2019 ◽
Vol 79
(12)
◽
Keyword(s):