pith:UTGEVXMZ
Weighing gas-rich starless halos: dark matter parameters inference from their gas distributions
Virial masses of starless dark matter halos are reliably recovered from their neutral hydrogen gas distributions
arxiv:2603.05597 v2 · 2026-03-05 · astro-ph.GA · astro-ph.CO
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Claims
the virial mass is exceptionally well constrained, establishing a highly reliable framework for weighing starless halos in upcoming surveys
The gas resides in near hydrostatic equilibrium within the dark matter potential and in thermal equilibrium with the cosmic ultraviolet background. This simplicity allows analytic frameworks to link observable HI column densities directly to fundamental dark matter halo structural parameters.
Virial masses of RELHICs are robustly recovered from their HI gas profiles via Bayesian nested sampling, with environmental density as a free parameter eliminating systematic mass biases from mass-concentration degeneracies.
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| First computed | 2026-05-17T23:39:15.862354Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a4cc4add9908c64292655587b7b60ccbd218584af5c3920fad4ae5159c3c62c2
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· · · · ·Agent API
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/UTGEVXMZBDDEFETFKWD3PNQMZP \
| 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())"
# expect: a4cc4add9908c64292655587b7b60ccbd218584af5c3920fad4ae5159c3c62c2
Canonical record JSON
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