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The Galactic Center as a laboratory for theories of gravity and dark matter

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arxiv 2211.07008 v3 pith:YYD6Y55D submitted 2022-11-13 astro-ph.GA astro-ph.HEgr-qc

classification astro-ph.GAastro-ph.HEgr-qc
keywords generalcentergalacticgravityrelativitybeendarklaboratory
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The Galactic Center of the Milky Way, thanks to its proximity, allows to perform astronomical observations that investigate physical phenomena at the edge of astrophysics and fundamental physics. As such, it offers a unique laboratory to probe gravity, where one can not only test the basic predictions of General Relativity, but is also able to falsify theories that, over time, have been proposed to modify or extend General Relativity; to test different paradigms of dark matter; and to place constraints on putative models that have been formulated as alternatives to the standard black hole paradigm in General Relativity. In this review we provide a general overview of the history of observations of the Galactic Center, emphasizing the importance, in particular on the smallest-observable scales, that they had in opening a new avenue to improve our understanding of the underlying theory of gravity in the surrounding of a supermassive compact object.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Pulsar timing in the Galactic Center

    gr-qc 2025-01 conditional novelty 6.0 of 10

    A fully relativistic (geodesic) pulsar timing model for the Galactic Center shows that 1PN-based timing formulas produce errors of up to seconds for tight orbits around Sgr A*.

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