Testing the nature of dark compact objects: a status report

被引：685

作者：

Cardoso, Vitor ^{[1
,2
]}

Pani, Paolo ^{[3
,4
]}

机构：

[1] Univ Lisbon, Inst Super Tecn, Dept Fis, CENTRA, Ave Rovisco Pais 1, P-1049 Lisbon, Portugal

[2] CERN, 1 Esplanade Particules, CH-1211 Geneva 23, Switzerland

[3] Sapienza Univ Roma, Dipartimento Fis, Piazzale Aldo Moro 5, I-00185 Rome, Italy

[4] Sez INFN Roma1, Piazzale Aldo Moro 5, I-00185 Rome, Italy

来源：

LIVING REVIEWS IN RELATIVITY | 2019年 / 22卷 / 1期

基金：

欧盟地平线“2020”;

关键词：

Black holes; Event horizon; Gravitational waves; Quantum gravity; Singularities; SUPERMASSIVE BLACK-HOLE; BOSON-FERMION STARS; X-RAY BINARIES; QUASI-NORMAL MODES; EQUATION-OF-STATE; GENERAL-RELATIVITY; GRAVITATIONAL-RADIATION; ANISOTROPIC STARS; MULTIPOLE MOMENTS; WAVE-EQUATIONS;

D O I：

10.1007/s41114-019-0020-4

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

Very compact objects probe extreme gravitational fields and may be the key to understand outstanding puzzles in fundamental physics. These include the nature of dark matter, the fate of spacetime singularities, or the loss of unitarity in Hawking evaporation. The standard astrophysical description of collapsing objects tells us that massive, dark and compact objects are black holes. Any observation suggesting otherwise would be an indication of beyond-the-standard-model physics. Null results strengthen and quantify the Kerr black hole paradigm. The advent of gravitational-wave astronomy and precise measurements with very long baseline interferometry allow one to finally probe into such foundational issues. We overview the physics of exotic dark compact objects and their observational status, including the observational evidence for black holes with current and future experiments.

引用

页数：104

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