pith:Y7JNMQBP
Accelerating scaling solutions from dark matter particle creation
Accelerating scaling attractors emerge only when dark matter particle creation drives energy flow from dark matter to the second fluid.
arxiv:2604.21770 v2 · 2026-04-23 · gr-qc · astro-ph.CO · math-ph · math.MP
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Claims
accelerating scaling attractors, namely late-time states where both fluids coexist with fixed energy fractions, arise only when the interaction is controlled by the DM density and energy flows from DM to the second fluid.
The six widely used interaction prescriptions adequately represent the relevant physics and that the adiabatic particle creation rate remains valid at late times; the analysis further assumes a flat FLRW background in standard general relativity.
Accelerating scaling attractors where DM and barotropic fluid coexist at late times arise only for DM-density-controlled interactions with energy transfer from DM.
Receipt and verification
| First computed | 2026-06-08T01:04:05.460300Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/Y7JNMQBPUATSHHI4I7MOOLDSYU \
| 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: c7d2d6402fa027239d1c47d8e72c72c5257bbfcd7c65beaf1f14c8076afe7ad2
Canonical record JSON
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