pith:LOIL3LDZ
Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$
The Event Horizon Telescope image of Sagittarius A* imposes tight limits on gravity models that predict larger black hole shadows than in general relativity.
arxiv:2205.07787 v3 · 2022-05-16 · gr-qc · astro-ph.HE · hep-ph · hep-th
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Claims
the EHT image of Sgr A* places particularly stringent constraints on models predicting a shadow size larger than that of a Schwarzschild BH of a given mass, with the resulting limits in some cases surpassing cosmological ones
connecting the size of the bright ring of emission to that of the underlying BH shadow and exploiting high-precision measurements of Sgr A*'s mass-to-distance ratio
EHT observations of Sgr A* constrain deviations from GR black hole solutions including regular BHs, string-inspired spacetimes, and BH mimickers, with some limits exceeding cosmological bounds.
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| First computed | 2026-05-17T23:38:48.050367Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
5b90bdac797410cefb69a49b49208cb77634a0ba3a2987ba411ba655c785eef6
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· · · · ·Agent API
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/LOIL3LDZOQIM563JUSNUSIEMW5 \
| jq -c '.canonical_record' \
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Canonical record JSON
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