pith:DWYW732L
MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts
The radial acceleration relation in galaxies shows a higher characteristic scale at higher redshifts.
arxiv:2604.22613 v1 · 2026-04-24 · astro-ph.GA
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Claims
Parametrizing the z-dependence as a0(z)= a0(0) + a1 * z, we obtain a1 = 1.59+/-0.1 *10^-10 m/s^2, providing evidence for a z-evolution.
The 3D forward modeling with disk-halo decomposition and pressure-support corrections accurately recovers the intrinsic accelerations without significant systematic bias from the choice of dark-matter halo profile or sample selection.
The radial acceleration relation persists at intermediate redshifts but with a characteristic acceleration scale that increases linearly with redshift.
References
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| First computed | 2026-05-20T14:03:27.055288Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
1db16fef4bc74321500c647e81c05321d09771f5ad1a75dc4ead75c3d7ce57bc
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/DWYW732LY5BSCUAMMR7IDQCTEH \
| 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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