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pith:2025:FTKG5G5KLNAVV25656BDCN27BU
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Hawking radiation: black hole vs de Sitter

G.E. Volovik

In higher-dimensional de Sitter spacetime the entropy inside the cosmological horizon becomes (d-1)A/8G instead of the usual Gibbons-Hawking value.

arxiv:2510.24502 v7 · 2025-10-28 · gr-qc

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Claims

C1strongest claim

We found that the entropy of the Hubble volume is S_H=(d-1)A/8G, which modifies the Gibbons-Hawking entropy of horizon. The original form of the Gibbons-Hawking entropy is valid only for d=3.

C2weakest assumption

The local de Sitter temperature is T_dS = H/π, is universal, and does not depend on dimension d; this temperature is used to define the local entropy density that is then integrated over the Hubble volume. (Abstract paragraph on local thermodynamics and the comparison to T_GH = H/2π.)

C3one line summary

Entropy of the Hubble volume in de Sitter spacetime is S_H=(d-1)A/8G in general dimensions, so the original Gibbons-Hawking entropy holds only for d=3.

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First computed 2026-06-01T01:02:24.607507Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

2cd46e9baa5b415aebbeef8231375f0d14cd02e128b99c6325ededb6b99f4fa4

Aliases

arxiv: 2510.24502 · arxiv_version: 2510.24502v7 · doi: 10.48550/arxiv.2510.24502 · pith_short_12: FTKG5G5KLNAV · pith_short_16: FTKG5G5KLNAVV256 · pith_short_8: FTKG5G5K
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/FTKG5G5KLNAVV25656BDCN27BU \
  | 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: 2cd46e9baa5b415aebbeef8231375f0d14cd02e128b99c6325ededb6b99f4fa4
Canonical record JSON
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    "primary_cat": "gr-qc",
    "submitted_at": "2025-10-28T15:14:56Z",
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