pith:S3SFGEA4
Gas-rich ultra-diffuse galaxies: alleviating the MOND tension with hyperconical modified gravity
Outer-radius HMG reduces MOND tension for gas-rich ultra-diffuse galaxies but still overpredicts most observed velocities.
arxiv:2604.09652 v2 · 2026-03-30 · astro-ph.GA · gr-qc
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Claims
We conclude that the present outer-radius HMG implementation alleviates the difficulties of MOND, but is still not sufficient to account for the published central values of the UDG sample. Gas-rich UDGs therefore provide a useful discriminant between MOND and HMG.
That scanning the neighbourhood-scale parameter to select the asymptotic branch of HMG constitutes a valid, non-post-hoc application of the model to these galaxies without further tuning or justification.
HMG asymptotic predictions fit UDG outer velocities better than MOND (chi-squared 18 vs 616) but worse than Newtonian baryons (chi-squared 10), yielding per-galaxy tensions of 0.2-2.1 sigma.
Formal links
Receipt and verification
| First computed | 2026-05-26T01:02:34.086311Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
96e453101c358a073de8a3b054e515ee4bfd9b173b2aad612dbdd346ada5bc6c
Aliases
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/S3SFGEA4GWFAOPPIUOYFJZIV5Z \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
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Canonical record JSON
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