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pith:2026:AHUOMHPYG2XMBRW32L5KRHTUNN
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A No-Go Theorem for Quantum Cosmologies with Non-natural Hamiltonians

Brazil), Christine C. Dantas (Astrophysics Division, INPE

Non-quadratic cosmological dynamics cannot be geometrized via Eisenhart-Duval lifts.

arxiv:2605.13921 v1 · 2026-05-13 · gr-qc

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Claims

C1strongest claim

We thus establish a kinematical no-go theorem: non-quadratic cosmological dynamics cannot be geometrized via ED constructions.

C2weakest assumption

The Eisenhart-Duval lift applies exclusively to natural Hamiltonians that are quadratic in the canonical momenta, and that polymer-modified Hamiltonians in loop quantum cosmology are genuinely non-polynomial in those momenta.

C3one line summary

Non-quadratic Hamiltonians in cosmological models prevent geometrization via the Eisenhart-Duval lift.

References

29 extracted · 29 resolved · 5 Pith anchors

[1] Eisenhart L P 1928 Annals of Mathematics 30 591–606 ISSN 0003486X, 19398980 URL http: //www.jstor.org/stable/1968307 1928
[2] Duval , author G 1985 · doi:10.1103/physrevd.31.1841
[3] Celestial mechanics, conformal structures, and gravitational waves 1991 · doi:10.1103/physrevd.43.3907
[4] Duval C, Henkel M, Horvathy P A, Rouhani S and Zhang P M 2024International Journal of Theoret- ical Physics 63 184 (Preprint 2403.20316) URL https://doi.org/10.1007/s10773-024-05673-0 · doi:10.1007/s10773-024-05673-0
[5] Cariglia M and Alves F K 2015 European Journal of Physics 36 025018 URL https://doi.org/ 10.1088/0143-0807/36/2/025018 2015 · doi:10.1088/0143-0807/36/2/025018

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First computed 2026-05-17T23:39:15.574171Z
Builder pith-number-builder-2026-05-17-v1
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Schema pith-number/v1.0

Canonical hash

01e8e61df836aec0c6dbd2faa89e746b65c84e0c6b6d12facd1f6631b5161636

Aliases

arxiv: 2605.13921 · arxiv_version: 2605.13921v1 · doi: 10.48550/arxiv.2605.13921 · pith_short_12: AHUOMHPYG2XM · pith_short_16: AHUOMHPYG2XMBRW3 · pith_short_8: AHUOMHPY
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/AHUOMHPYG2XMBRW32L5KRHTUNN \
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Canonical record JSON
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