Relativistic model of an anisotropic star with Bose-Einstein dark matter density profile in f(T) gravity
This article presents a new model for anisotropic compact stars that are confined to physical dark matter in the background of f(T) teleparallel gravity. The model is based on the equation of state (EoS) of the bag model type and the Bose-Einstein dark matter density profile. The derived solutions m...
Saved in:
Main Authors: | Samprity Das, Prabir Rudra, Surajit Chattopadhyay |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2025-03-01
|
Series: | Nuclear Physics B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S055032132500029X |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
The stability of anisotropic compact stars influenced by dark matter under teleparallel gravity: an extended gravitational deformation approach
by: Sneha Pradhan, et al.
Published: (2025-02-01) -
From relativistic gravity to the Poisson equation
by: Eric A. Bergshoeff, et al.
Published: (2025-02-01) -
Testing quantum gravity with dilute dipolar Bose gases
by: Asma Tahar Taiba, et al.
Published: (2025-02-01) -
GR-Athena++: General-relativistic Magnetohydrodynamics Simulations of Neutron Star Spacetimes
by: William Cook, et al.
Published: (2025-01-01) -
Gravity-mediated scalar Dark Matter in warped extra-dimensions
by: Miguel G. Folgado, et al.
Published: (2020-01-01)