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Swampland Program for Hypergeometric Inflation Scenarios in Rescaled Gravity

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arxiv 2407.00785 v1 pith:XCB5C2ME submitted 2024-06-30 hep-th gr-qcmath-phmath.MP

classification hep-thgr-qcmath-phmath.MP
keywords hypergeometricswamplandgravitypotentialsprogramrescaledscalarbehaviors
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In this paper, we investigate hypergeometric stringy corrections in the swampland program for rescaled gravity. Precisely, we study inflationary models from Gauss-Bonnet hypergeometric scalar couplings via the falsification scenario. We first derive generalized exponential potentials from such hypergeometric behaviors. Then, we examine certain selected scalar potentials by computing the relevant cosmological quantities using the slow-roll mechanism. Choosing specific points in the corresponding moduli space, we provide viable findings corroborated by Planck observational data and checked by the swampland criteria.

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  1. CUDA Assisted Swampland and Black Hole Thermodynamics

    hep-th 2025-08 unverdicted novelty 4.0 of 10

    Charged black holes in a Gauss-Bonnet-modified theory are claimed to become unstable when Q/M > 2√π, linking black hole thermodynamics to swampland constraints.

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