pith:CH2BAKO5
Generalizing the CPL Parametrization through Dark Sector Interaction
Interacting dark energy models generalized with a specific coupling kernel and CPL parametrization are not preferred over LambdaCDM by Bayesian evidence despite some frequentist tensions.
arxiv:2604.25373 v2 · 2026-04-28 · astro-ph.CO · gr-qc
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Claims
Ultimately, our Bayesian model comparison reveals that no investigated IDE scenario is statistically preferred over the concordance ΛCDM model.
The specific background interaction kernel Q = 3H(δ + η a)ρ_de is assumed to permit closed analytical expressions for the dark matter and dark energy densities while remaining physically motivated.
Dynamical couplings in interacting dark energy models reduce deviations from LambdaCDM to 1.3-1.5 sigma and yield no Bayesian preference over the standard model.
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| First computed | 2026-05-21T01:05:19.545300Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
11f41029dd1acb33350456438117a1230b446ffbe6b127e68c4c68a857f7b496
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/CH2BAKO5DLFTGNIEKZBYCF5BEM \
| 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: 11f41029dd1acb33350456438117a1230b446ffbe6b127e68c4c68a857f7b496
Canonical record JSON
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