Abstract

We investigate the weak and strong deflection gravitational lensing by a quantum deformed Schwarzschild black hole and find their observables. These lensing observables are evaluated and the detectability of the quantum deformation is assessed, after assuming the supermassive black holes Sgr A* and M87* respectively in the Galactic Center and at the center of M87 as the lenses. We also intensively compare these findings with those of a renormalization group improved Schwarzschild black hole and an asymptotically safe black hole. We find that, among these black holes, it is most likely to test the quantum deformed Schwarzschild black hole via its weak deflection lensing observables in the foreseen future.

Highlights

  • Einstein’s general relativity (GR) has been tested and verified in many experiments [1], it is commonly believed that GR is incomplete

  • Inspired by these previous works and hoping to gain a whole picture of the weak and strong deflection gravitational lensing [118,119,120,121,122,123,124], we will investigate these two scenarios of gravitational lensing by the quantum deformed Schwarzschild black hole for detecting and searching its quantum signatures

  • Which will be adopted in the following investigation on the weak and strong deflection gravitational lensing by the quantum deformed Schwarzschild black hole

Read more

Summary

Introduction

Einstein’s general relativity (GR) has been tested and verified in many experiments [1], it is commonly believed that GR is incomplete. In order to obtain a full understanding of the quantum effects, both weak and strong deflection gravitational lensing have been studied for some black holes in the asymptotically safe gravity [113,114], in the loop quantum gravity [115], under the Extended Uncertainty Principle [116] and in the rainbow gravity [117] Inspired by these previous works and hoping to gain a whole picture of the weak and strong deflection gravitational lensing [118,119,120,121,122,123,124], we will investigate these two scenarios of gravitational lensing by the quantum deformed Schwarzschild black hole for detecting and searching its quantum signatures.

Metric
Essentials of gravitational lensing
Weak deflection gravitational lensing
Position of lensed image
Magnification
Time delay
Relations among positions and magnification
Relations of images positions
Relations of magnification
Total magnification and centroid
D2β6 3
Differential time delay
Practical observables
Example of Sgr A*
Strong deflection gravitational lensing
Photon sphere and shadow
Observables
Example of M87*
Findings
Conclusions and discussion

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.