pith:VGHUDLUW
Cosmological coupled black holes immersed in dark sector
Black hole mass grows with the cosmic expansion through coupling to a dark sector halo.
arxiv:2603.24609 v2 · 2026-03-23 · gr-qc · astro-ph.CO · hep-th
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\pithnumber{VGHUDLUW6KEKLCYW6MGVCNPMJW}
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Record completeness
Claims
We derive a solution where the black hole mass co-evolves with the cosmic expansion... the interaction is governed by the dark halo profile.
The generalization of the static seed metric to a dynamical FLRW background preserves the form of the coupling while the dark sector remains an anisotropic fluid whose halo profile directly sets the radius-dependent exponent.
Exact solution for a black hole whose mass co-evolves with Hubble expansion via radius-dependent coupling to an anisotropic dark halo in FLRW spacetime.
Formal links
Receipt and verification
| First computed | 2026-05-25T02:01:18.160629Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
a98f41ae96f288a58b16f30d5135ec4d80ca77bfe1208dd29cb532d03ddb7e4d
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/VGHUDLUW6KEKLCYW6MGVCNPMJW \
| 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: a98f41ae96f288a58b16f30d5135ec4d80ca77bfe1208dd29cb532d03ddb7e4d
Canonical record JSON
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],
"license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
"primary_cat": "gr-qc",
"submitted_at": "2026-03-23T07:21:20Z",
"title_canon_sha256": "15a21d5a53da2b119a4c6be05a30889546b38dcfd35e9910d10b108044a6c41a"
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