Spontaneous scalarization

被引：31

作者：

Doneva, Daniela D. ^{[1
,2
]}

Ramazanoglu, Fethi M. ^{[3
]}

Silva, Hector O. ^{[4
]}

Sotiriou, Thomas P. ^{[5
,6
,7
]}

Yazadjiev, Stoytcho S. ^{[1
,8
,9
,10
]}

机构：

[1] Eberhard Karls Univ Tubingen, Theoret Astrophys, D-72076 Tubingen, Germany

[2] Bulgarian Acad Sci, INRNE, Sofia 1784, Bulgaria

[3] Koc Univ, Dept Phys, Rumelifeneri Yolu, TR-34450 Sariyer, Istanbul, Turkiye

[4] Albert Einstein Inst, Max Planck Inst Grav Phys, D-14476 Potsdam, Germany

[5] Univ Nottingham, Nottingham Ctr Grav, Univ Pk, Nottingham NG7 2RD, England

[6] Univ Nottingham, Sch Math Sci, Univ Pk, Nottingham NG7 2RD, England

[7] Univ Nottingham, Sch Phys & Astron, Univ Pk, Nottingham NG7 2RD, England

[8] Univ Tubingen, IAAT, Theoret Astrophys, D-72076 Tubingen, Germany

[9] Sofia Univ, Fac Phys, Dept Theoret Phys, Sofia 1164, Bulgaria

[10] Bulgarian Acad Sci, Inst Math & Informat, Acad Georgi Bonchev St 8, Sofia 1113, Bulgaria

来源：

REVIEWS OF MODERN PHYSICS | 2024年 / 96卷 / 01期

关键词：

EQUATION-OF-STATE; SCALAR-TENSOR THEORIES; MASS-RADIUS RELATION; ROTATING RELATIVISTIC STARS; X-RAY OSCILLATIONS; NEUTRON-STAR; BLACK-HOLES; DENSE MATTER; GENERAL-RELATIVITY; MAXIMUM MASS;

D O I：

10.1103/RevModPhys.96.015004

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

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.

引用

页数：45

共 50 条

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[10] Closing a spontaneous-scalarization window with binary pulsars
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