Stabilization of spherically symmetric static Boson stars by Coleman-Weinberg self-interaction potential
Our motivation in this work is due to the great importance of relativistic boson stars as fierce competitors of black holes. From theoretical perspective, they described by complex Klein Gordon (KG) scalar fields interacting with curved background in general form. In this work we use the Einstein-Kl...
Saved in:
Main Authors: | Firoozeh Eidizadeh, Hossein Ghaffarnejad |
---|---|
Format: | Article |
Language: | English |
Published: |
Elsevier
2025-01-01
|
Series: | Nuclear Physics B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0550321324003304 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Modified Gauge Invariant Einstein-Maxwell Gravity and Stability of Spherical Perfect Fluid Stars with Magnetic Monopoles
by: Hossein Ghaffarnejad, et al.
Published: (2024-01-01) -
Thermodynamic Analysis of the Static Spherically Symmetric Field Equations in Rastall Theory
by: Hooman Moradpour, et al.
Published: (2016-01-01) -
An Alternative Approach to the Static Spherically Symmetric, Vacuum Global Solution to the Einstein Equations
by: Luis Herrera, et al.
Published: (2018-01-01) -
Coleman Automorphisms of Some Metabelian Groups
by: Jingjing Hai, et al.
Published: (2022-01-01) -
Circular light orbits of a general, static, and spherical symmetrical wormhole with $$Z_2$$ Z 2 symmetry
by: Naoki Tsukamoto
Published: (2024-12-01)