Asset Details
Do you wish to reserve the book?
Traversability of Schwarzschild-Anti-de Sitter Wormhole in f(T) gravity
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?
Traversability of Schwarzschild-Anti-de Sitter Wormhole in f(T) gravity
Do you wish to request the book?
Traversability of Schwarzschild-Anti-de Sitter Wormhole in f(T) gravity
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
Traversability of Schwarzschild-Anti-de Sitter Wormhole in f(T) gravity
2024
Overview
In this paper we analyze the traversability of static and evolving Schwarzschild-Anti-de Sitter wormholes. The wormhole metric under consideration is not asymptotically flat. Hence one can only embed this metric into the Euclidean space for a limited radius
r
max
. For
r
>
r
max
, an exterior vacuum spacetime should be matched to the wormhole spacetime. In the framework of
f
(
T
) gravities, we discuss the null energy condition that the matter supporting the wormhole should satisfy and find that the nontrivial form of
f
(
T
) is necessary. For the wormholes to be suitable for human to traverse, we consider the tidal force that a traveler would have felt during his trip. This leads to an upper bound of the traveler’s velocity. Utilizing the velocity allowed, we will estimate the travel time through the wormhole. In the evolving cases, the wormhole should not be expanding too fast, otherwise the traveler may not be able to arrive at the other side of the wormhole. Besides this, for static wormholes, we briefly discuss the geodesics in the plane
θ
=
π
/
2
.
