pith:W6WKHITO
The Hubble Tension and Early Dark Energy
The Hubble tension between local and early-universe expansion-rate measurements may be resolved by early dark energy that speeds up expansion before recombination while satisfying existing constraints.
arxiv:2211.04492 v1 · 2022-11-08 · astro-ph.CO · gr-qc · hep-ph
Record completeness
Claims
Early-Universe solutions are currently favored and early dark energy provides a workable example that can be tested with future measurements while remaining consistent with the majority of the data.
That proposed systematic errors in the measurements are not supported by the breadth of available data and that unknown errors are untestable, thereby directing attention to early-Universe modifications of LambdaCDM.
The Hubble tension between local and early-universe expansion-rate measurements may be resolved by early dark energy that speeds up expansion before recombination while satisfying existing constraints.
Cited by
Receipt and verification
| First computed | 2026-05-17T23:38:12.616803Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519 (pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
b7aca3a26ec65f68689d0940521ff4db41df4954b2725bc332002da25317418b
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/W6WKHITOYZPWQ2E5BFAFEH7U3N \
| 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: b7aca3a26ec65f68689d0940521ff4db41df4954b2725bc332002da25317418b
Canonical record JSON
{
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"hep-ph"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"primary_cat": "astro-ph.CO",
"submitted_at": "2022-11-08T19:00:16Z",
"title_canon_sha256": "d797ac6a2111fd46a43d747170529df6c6459b858e157e28f1174b793ceabf85"
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"source": {
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"kind": "arxiv",
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