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pith:UT46KV6V

pith:2026:UT46KV6V7SK7BZ2JQO7GYLFTQ2
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Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6

C. Pallis

Supergravity model of induced-gravity Higgs inflation matches ACT DR6 while breaking B-L symmetry at 10^16 GeV scales.

arxiv:2602.05623 v3 · 2026-02-05 · hep-ph · astro-ph.CO · hep-th

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4 Citations open
5 Replications open
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Claims

C1strongest claim

We formulate within Supergravity a model of induced-gravity inflation, excellently consistent with ACT DR6, inspired by the Palatini gravity. The inflaton belongs in the decomposition of a conjugate pair of Higgs superfields which lead to the spontaneous breaking of a U(1)B-L symmetry at a scale close to the range (0.102-5.85)x10^16 GeV.

C2weakest assumption

The Kaehler potential contains a real shift-symmetric contribution together with separate holomorphic and antiholomorphic logarithmic terms whose argument is interpreted as the inflaton-Ricci scalar coupling; these terms are assumed to produce canonical normalization, subplanckian field values, and energy scales below the effective-theory cutoff.

C3one line summary

A Palatini-inspired induced-gravity inflation model in supergravity fits ACT DR6 data while embedding into a B-L extended MSSM with split SUSY and leptogenesis.

References

137 extracted · 137 resolved · 60 Pith anchors

[1] The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters 2025 · arXiv:2503.14452
[2] The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models 2025 · arXiv:2503.14454
[3] Planck 2018 results. X. Constraints on inflation 2018 · arXiv:1807.06211
[4] R. Kallosh, A. Linde and D. Roest, Atacama Cosmology T elescope, South Pole T elescope, and Cha otic Inflation, Phys. Rev. Lett. 135, no.16, 161001 (2025) [ arXiv:2503.21030] 2025
[5] Po- tential Reconstruction from ACT Observations Lead- ing to Polynomialα-Attractor

Formal links

2 machine-checked theorem links

Cited by

2 papers in Pith

Receipt and verification
First computed 2026-05-26T01:02:31.988075Z
Builder pith-number-builder-2026-05-17-v1
Signature Pith Ed25519 (pith-v1-2026-05) · public key
Schema pith-number/v1.0

Canonical hash

a4f9e557d5fc95f0e74983be6c2cb386b4989aa4c80d66636eaecfa70655b053

Aliases

arxiv: 2602.05623 · arxiv_version: 2602.05623v3 · doi: 10.48550/arxiv.2602.05623 · pith_short_12: UT46KV6V7SK7 · pith_short_16: UT46KV6V7SK7BZ2J · pith_short_8: UT46KV6V
Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/UT46KV6V7SK7BZ2JQO7GYLFTQ2 \
  | 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: a4f9e557d5fc95f0e74983be6c2cb386b4989aa4c80d66636eaecfa70655b053
Canonical record JSON
{
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      "astro-ph.CO",
      "hep-th"
    ],
    "license": "http://creativecommons.org/licenses/by/4.0/",
    "primary_cat": "hep-ph",
    "submitted_at": "2026-02-05T12:58:52Z",
    "title_canon_sha256": "e97f94637e02164f8bd88006ea9af9955c1dc4c5e03481e9dfcf5b8453d9514b"
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}