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Scalarization

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Silva,  Hector O.
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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2211.01766.pdf
(Preprint), 4MB

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Citation

Doneva, D. D., Ramazanoğlu, F. M., Silva, H. O., Sotiriou, T. P., & Yazadjiev, S. S. (in preparation). Scalarization.


Cite as: https://hdl.handle.net/21.11116/0000-000B-829A-4
Abstract
Scalarization is a mechanism that endows strongly self-gravitating bodies,
such as neutron stars and black holes, with a scalar field configuration. It
resembles a phase transition in that the scalar configuration only appears when
a certain quantity that characterizes the compact object, e.g., its compactness
or spin, is beyond a threshold. We provide a critical and comprehensive review
of scalarization, including the mechanism itself, theories that exhibit it, its
manifestation in neutron stars, black holes, and their binaries, potential
extension to other fields, and a thorough discussion of future perspectives.