Spontaneous scalarization
Daniela D. DonevaINRNE -Bulgarian Academy of Sciences, 1784 Sofia, BulgariaFethi M. RamazanoğluTheoretical Astrophysics, Eberhard Karls University of Tübingen, 72076 Tübingen, Germany Department of Theoretical Physics,Hector O. SilvaNottingham Centre of Gravity & School of Mathematical Sciences & School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, United KingdomThomas P. SotiriouUniversity of TübingenStoytcho S. YazadjievInstitute of Mathematics and Informatics, Bulgarian Academy of Sciences, Acad. G. Bonchev Street 8, 1113 Sofia, Bulgaria
ABI
Annotatsiya
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 appears only when a certain quantity that characterizes the compact object, for example, its compactness or spin, is beyond a threshold. 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, is provided.
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