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arxiv hep-ph/9812483 v1 pith:MQ4RSNRM submitted 1998-12-22 hep-ph

Brane Inflation

classification hep-ph
keywords branesenergybranedimensionslargeextrafieldgravity
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We present a novel inflationary scenario in theories with low scale (TeV) quantum gravity, in which the standard model particles are localized on the branes whereas gravity propagates in the bulk of large extra dimensions. This inflationary scenario is natural in the brane world picture. In the lowest energy state, a number of branes sit on top of each other (or at an orientifold plane), so the vacuum energy cancels out. In the cosmological setting, some of the branes "start out" relatively displaced in the extra dimensions and the resulting vacuum energy triggers the exponential growth of the 3 non-compact dimensions. The number of e-foldings can be very large due to the very weak brane-brane interaction at large distances. In the effective four-dimensional field theory, the brane motion is described by a slowly rolling scalar field with an extremely flat plateau potential. When branes approach each other to a critical distance, the potential becomes steep and inflation ends rapidly. Then the branes "collide" and oscillate about the equilibrium point, releasing energy mostly into radiation on the branes.

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Cited by 3 Pith papers

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

  1. Unification of polynomial and exponential cosmological attractors

    hep-th 2026-07 conditional novelty 4.0

    Embedding polynomial attractor potentials within α-attractor geometry yields a unified model class that interpolates between exponential and polynomial inflationary predictions via a single parameter μ.

  2. Cosmological history after higher dimensional inflation

    hep-th 2026-06 unverdicted novelty 4.0

    Proposes a post-inflation cosmological evolution in large-extra-dimension models that prevents bulk graviton overproduction up to reheating while preserving scale-invariant perturbations for 1-2 micron-sized dimensions.

  3. Inflationary models in a minimally coupled $f(R,T)$ gravity: Constraints from $Planck$, BICEP/$Keck$, and ACT

    gr-qc 2025-11 unverdicted novelty 3.0

    Three standard inflationary potentials remain compatible with Planck, BICEP/Keck, DESI DR2, and ACT DR6 data when placed in minimally coupled f(R,T)=R+16πGλT gravity for suitable ranges of the model parameters and coupling λ.