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Features of a dark energy model in string theory

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arxiv 2212.14004 v4 pith:SUGZPIG6 submitted 2022-12-28 hep-th gr-qc

Souvik Banerjee , Ulf Danielsson , Suvendu Giri This is my paper · ORCID
classification hep-thgr-qc
keywords darkbubbleenergymodelstringtheoryclearconcerning
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In this paper we clear up misconceptions concerning the dark bubble model as a realization of dark energy in string theory. In particular we point out important differences with Randall-Sundrum, and explain why gravity neither is, nor need to be, localized on the dark bubble.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Weak gravity at micron scales from dark bubble cosmology and its cosmological consequences

    hep-th 2025-11 conditional novelty 7.0 of 10

    Dark bubble cosmology predicts gravity weakens below L~10^-5 m, yielding V=-G4M(1/rho - 3L^2/(2rho^3)+...) and a radiation-only inflationary phase.

  2. Dark bubble cosmology and the equivalence principle

    hep-ph 2025-07 conditional novelty 6.0 of 10

    In dark bubble cosmology, non-abelian gauge fields like gluons would couple to induced gravity with the wrong sign, making the proton's gravitational mass about 1% of its inertial mass and ruling out the scenario agai...

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