Spherically symmetric elastic bodies in general relativity

被引:5
|
作者
Alho, Artur [1 ]
Natario, Jose [1 ]
Pani, Paolo [2 ,3 ]
Raposo, Guilherme [4 ]
机构
[1] Univ Lisbon, Ctr Math Anal Geometry & Dynam Syst, Inst Super Tecn, Av Rovisco Pais, P-1049001 Lisbon, Portugal
[2] Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 5, I-00185 Rome, Italy
[3] INFN Roma1, PiazzaleAldo Moro 5, I-00185 Rome, Italy
[4] Ctr Res & Dev Math & Applicat CIDMA, CIDMA Ctr Res & Dev Math & Applicat, Campus de Santiago, P-3810183 Aveiro, Portugal
基金
欧盟地平线“2020”;
关键词
elasticity; polytropes; self-gravitating; buchdahl limit; scale invariance; spherical symmetry; radial stability; NAKED SINGULARITIES; EINSTEIN EQUATIONS; GRAVITATION FIELD; STATIC SOLUTIONS; STARS; MODELS; FLUIDS; FOUNDATIONS; EXISTENCE; SPHERES;
D O I
10.1088/1361-6382/ad1e4b
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The purpose of this review it to present a renewed perspective of the problem of self-gravitating elastic bodies under spherical symmetry. It is also a companion to the papers (2022 Phys. Rev. D 105 044025, 2022 Phys. Rev. D 106 L041502) and (arXiv:2306.16584 [gr-qc]), where we introduced a new definition of spherically symmetric elastic bodies in general relativity, and applied it to investigate the existence and physical viability, including radial stability, of static self-gravitating elastic balls. We focus on elastic materials that generalize fluids with polytropic, linear, and affine equations of state, and discuss the symmetries of the energy density function, including homogeneity and the resulting scale invariance of the TOV equations. By introducing invariant characterizations of physically admissible initial data, we numerically construct mass-radius-compactness diagrams, and conjecture about the maximum compactness of stable physically admissible elastic balls.
引用
收藏
页数:109
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