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3 Pith papers citing it

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2026 3

representative citing papers

Optimal paths across potentials on scalar field space

hep-th · 2026-04-27 · unverdicted · novelty 7.0

Optimal transport yields a generalized Wasserstein distance on field space, obtained from a WKB expansion of a Schrödinger equation and extended to dynamical gravity via the Wheeler-DeWitt equation in the ADM formalism.

dS$^4$ Metamorphosis

hep-th · 2026-02-23 · conditional · novelty 7.0

Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.

A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral

hep-th · 2026-02-26 · unverdicted · novelty 6.0

The paper identifies a variety of Euclidean saddle solutions including wormholes and oscillatory configurations in Einstein-Scalar-Maxwell models, demonstrates how oscillations are controlled by lifting flat potential directions, finds phase transitions, and shows analytic continuation to FLRW cosm

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Showing 3 of 3 citing papers.

  • Optimal paths across potentials on scalar field space hep-th · 2026-04-27 · unverdicted · none · ref 80

    Optimal transport yields a generalized Wasserstein distance on field space, obtained from a WKB expansion of a Schrödinger equation and extended to dynamical gravity via the Wheeler-DeWitt equation in the ADM formalism.

  • dS$^4$ Metamorphosis hep-th · 2026-02-23 · conditional · none · ref 11

    Higher spin gravity path integral on S^4 glues to an Sp(N) or superconformal S^3 boundary theory, giving leading contribution 2^N with one-loop cancellations.

  • A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral hep-th · 2026-02-26 · unverdicted · none · ref 18

    The paper identifies a variety of Euclidean saddle solutions including wormholes and oscillatory configurations in Einstein-Scalar-Maxwell models, demonstrates how oscillations are controlled by lifting flat potential directions, finds phase transitions, and shows analytic continuation to FLRW cosm