On the formation of “supermassive” neutron stars and dynamical transition to spontaneous scalarization
It is well known that neutron stars can undergo a phase transition under a certain class of Scalar Tensor Theories of gravity (STT's) where a new order parameter, the scalar charge, appears within the star. This is the well known phenomenon of spontaneous scalarization (SC) discovered by Damour...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2020-09-01
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Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S037026932030469X |