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...
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Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2025-01-01
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Series: | Nuclear Physics B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0550321324003304 |
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