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Pith Number

pith:3KCSQQCW

pith:2026:3KCSQQCW2CEHUQXIAY27IEMF65
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The cosmological inflation inside the cyclic model of the universe

Jan Nov\'ak, Kanabar Jay, Maxim Khlopov

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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\usepackage{pith}
\pithnumber{3KCSQQCW2CEHUQXIAY27IEMF65}

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Record completeness

1 Bitcoin timestamp
2 Internet Archive
3 Author claim open · sign in to claim
4 Citations open
5 Replications open
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The bundle contains the canonical record plus signed events. A mirror can host it anywhere and recompute the same current state with the deterministic merge algorithm.

Claims

C1strongest claim

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.

C2weakest assumption

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.

C3one line summary

A two-scalar-field model integrates inflation as a recurring feature after each bounce in a cyclic universe.

References

18 extracted · 18 resolved · 1 Pith anchors

[1] Friedmann, On the Curvature of space, Z 1922 · doi:10.1007/bf01332580
[2] Hubble, A relation between distance and radial velocity among extra-galactic nebulae 1929 · doi:10.1073/pnas.15.3.168
[3] F. Hoyle. The Nature of the Universe (Third BBC Broadcast). The Listener41, 567 (31 March 1949) 1949
[4] The Singu- larities of gravitational collapse and cosmology, 1970
[5] Ya. B. Zeldovich and M. Yu. Khlopov. On the concentration of relic magnetic monopoles in the universe. Physics Letters B79, 239–241 (1978).https://doi.org/10.1016/ 0370-2693(78)90232-0 1978

Formal links

2 machine-checked theorem 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

arxiv: 2605.15374 · arxiv_version: 2605.15374v1 · doi: 10.48550/arxiv.2605.15374 · pith_short_12: 3KCSQQCW2CEH · pith_short_16: 3KCSQQCW2CEHUQXI · pith_short_8: 3KCSQQCW
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
{
  "metadata": {
    "abstract_canon_sha256": "141054241761ad41056b054cd46f1ec13fbc7be5c84e7b05fc3a9b362cef1e9b",
    "cross_cats_sorted": [],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "gr-qc",
    "submitted_at": "2026-05-14T20:03:43Z",
    "title_canon_sha256": "e35ba075885ce6a0c42f8cd20d0ec124667d4a21670cfbb22b36159230fda150"
  },
  "schema_version": "1.0",
  "source": {
    "id": "2605.15374",
    "kind": "arxiv",
    "version": 1
  }
}