Testing the nature of dark compact objects: a status report. (arXiv:1904.05363v1 [gr-qc])
<a href="http://arxiv.org/find/gr-qc/1/au:+Cardoso_V/0/1/0/all/0/1">Vitor Cardoso</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Pani_P/0/1/0/all/0/1">Paolo Pani</a>

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.

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.

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