# Hawking Radiation and Deflection of Light from Rindler Modified   Schwarzschild Black Hole

**Authors:** I. Sakalli, A. Ovgun

arXiv: 1702.04636 · 2017-09-05

## TL;DR

This paper explores how Rindler acceleration influences Hawking radiation and gravitational lensing in a modified Schwarzschild black hole, providing insights into quantum effects and light deflection in such spacetimes.

## Contribution

It introduces the study of Hawking radiation of massive vector particles and gravitational lensing in a Rindler modified Schwarzschild black hole, highlighting the role of Rindler acceleration.

## Key findings

- Rindler acceleration affects Hawking radiation emission.
- The deflection angle of light is computed in the IR region.
- Rindler acceleration influences gravitational lensing properties.

## Abstract

We investigate the Hawking radiation of massive spin-1 vector particles, which are coupled to vacuum fluctuations of a quantum field, from 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.

## Full text

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## Figures

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## References

92 references — full list in the complete paper: https://tomesphere.com/paper/1702.04636/full.md

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Source: https://tomesphere.com/paper/1702.04636