pith:3KCSQQCW
The cosmological inflation inside the cyclic model of the universe
A two-scalar-field model lets inflation recur after every bounce inside a cyclic universe.
arxiv:2605.15374 v1 · 2026-05-14 · gr-qc
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\pithnumber{3KCSQQCW2CEHUQXIAY27IEMF65}
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Claims
In a cosmological scenario involving two scalar fields, one field governs the cyclic evolution of the universe while the other drives an inflationary phase after each cosmological bounce, suggesting that inflation may be a recurring feature of a cyclic universe.
That suitable potentials and interactions for the two scalar fields can be chosen so that one produces stable cyclic behavior while the other reliably triggers inflation immediately after each bounce without destabilizing the cycles or violating observations.
A two-scalar-field model integrates inflation as a recurring feature after each bounce in a cyclic universe.
References
Formal links
Receipt and verification
| First computed | 2026-05-20T00:00:55.159884Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
da85284056d0887a42e80635f41185f740d0443248dc7ab19b2527de01731dcc
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/3KCSQQCW2CEHUQXIAY27IEMF65 \
| 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: da85284056d0887a42e80635f41185f740d0443248dc7ab19b2527de01731dcc
Canonical record JSON
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