No skyrmion hair for stationary spherically symmetric reflecting stars

DOI10.1016/j.physletb.2019.134922zbMath1427.83011arXiv1908.04591OpenAlexW2966970805MaRDI QIDQ2281143

M. Khodaei, H. Mohseni Sadjadi

Publication date: 19 December 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1908.04591

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20)

Related Items

On instabilities of stationary scalar field configurations supported by reflecting compact stars ⋮ Stationary scalar hairy configurations supported by Neumann compact stars ⋮ No scalar hair in nonminimal derivative coupling model for Neumann and Dirichlet reflecting star ⋮ Scalarization of compact stars in the scalar-Gauss-Bonnet gravity

Cites Work

• Skyrmion black hole hair: conservation of baryon number by black holes and observable manifestations
• Scalar field configurations supported by charged compact reflecting stars in a curved spacetime
• Stationary black holes: uniqueness and beyond
• Charged massive scalar field configurations supported by a spherically symmetric charged reflecting shell
• Colored black holes
• Topological Solitons