Volume 118, Number 6, June 2017
|Number of page(s)||7|
|Published online||04 September 2017|
Hawking radiation and deflection of light from Rindler modified Schwarzschild black hole
1 Physics Department, Eastern Mediterranean University - Famagusta, Northern Cyprus, Turkey
2 Instituto de Física, Pontificia Universidad Católica de Valparaíso - Casilla 4950, Valparaíso, Chile
Received: 21 February 2017
Accepted: 8 August 2017
We investigate the Hawking radiation of massive spin-1 vector particles, which are coupled to vacuum fluctuations of a quantum field, from a Rindler modified Schwarzschild black hole. Rindler acceleration is used to produce the post-general relativistic theory of gravity for the distant field of a point mass. The gravitational lensing problem of the Rindler modified Schwarzschild black hole is also studied. We compute the deflection angle for the IR region (large distance limit as infrared) by using the Gaussian curvature of the optical metric of this back hole. Our investigations clarify how the Rindler acceleration plays a role on the Hawking radiation and gravitational lensing.
PACS: 04.20.Gz – Spacetime topology, causal structure, spinor structure / 04.70.Dy – Quantum aspects of black holes, evaporation, thermodynamics / 02.40.Hw – Classical differential geometry
© EPLA, 2017
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.