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  Scalarization

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

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2211.01766.pdf (Preprint), 4MB
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2211.01766.pdf
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File downloaded from arXiv at 2022-11-24 11:52
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 Urheber:
Doneva, Daniela D., Autor
Ramazanoğlu, Fethi M., Autor
Silva, Hector O.1, Autor           
Sotiriou, Thomas P., Autor
Yazadjiev, Stoytcho S., Autor
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              

Inhalt

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,High Energy Physics - Theory, hep-th
 Zusammenfassung: 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.

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 Datum: 2022-11-03
 Publikationsstatus: Keine Angabe
 Seiten: 50 pages, 24 figures. Review commissioned by Reviews of Modern Physics, submitted version, comments welcome
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 Identifikatoren: arXiv: 2211.01766
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