Asset Details
Do you wish to reserve the book?
High-dimensional Schwarzschild black holes in scalar–tensor–vector gravity theory
Hey, we have placed the reservation for you!
By the way, why not check out events that you can attend while you pick your title.
Oops! Something went wrong.
Looks like we were not able to place the reservation. Kindly try again later.
Are you sure you want to remove the book from the shelf?
High-dimensional Schwarzschild black holes in scalar–tensor–vector gravity theory
Do you wish to request the book?
High-dimensional Schwarzschild black holes in scalar–tensor–vector gravity theory
Please be aware that the book you have requested cannot be checked out. If you would like to checkout this book, you can reserve another copy
We have requested the book for you!
Your request is successful and it will be processed during the Library working hours. Please check the status of your request in My Requests.
Oops! Something went wrong.
Looks like we were not able to place your request. Kindly try again later.
Journal Article
High-dimensional Schwarzschild black holes in scalar–tensor–vector gravity theory
2021
Overview
We obtain a high-dimensional Schwarzschild black hole solution in the scalar–tensor–vector gravity (STVG), and then analyze the influence of parameter α associated with a deviation of the STVG theory from General Relativity on event horizons and Hawking temperature. We calculate the quasinormal mode frequencies of massless scalar field perturbations for the high-dimensional Schwarzschild STVG black hole by using the sixth-order WKB approximation method and the unstable null geodesic method in the eikonal limit. The results show that the increase of parameter α makes the scalar waves decay slowly, while the increase of the spacetime dimension makes the scalar waves decay fast. In addition, we study the influence of parameter α on the shadow radius of this high-dimensional Schwarzschild STVG black hole and find that the increase of parameter α makes the black hole shadow radius increase, but the increase of the spacetime dimension makes the black hole shadow radius decrease. Finally, we investigate the energy emission rate of the high-dimensional Schwarzschild STVG black hole, and find that the increase of parameter α makes the evaporation process slow, while the increase of the spacetime dimension makes the process fast.
Publisher
Springer Nature B.V
Subject
