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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Bibliographic Details
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
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