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Probing String Theory with Modulated Cosmological Fluctuations

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arxiv astro-ph/0303614 v2 pith:PZNLE73L submitted 2003-03-27 astro-ph hep-phhep-th

classification astro-phhep-phhep-th
keywords constantscouplingfluctuationsmodulatedfieldsinhomogeneitiesuniversecosmological
verification ladder T0 review T1 audit T2 compute T3 formal
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Superstring theory, models with extra dimensions and other SUSY models generically predict that the coupling constants are in fact vacuum expectation values of fields like the dilaton, moduli etc. Assuming some of these fields are light during inflation, we get generation of small classical inhomogeneities in these fields from inflation. Consequently, coupling constants inherit small inhomogeneities at scales much larger than the causal horizon in the early universe. After the moduli get pinned down to their minima, the spatial variations of coupling constants in the late time universe will be erased. However, inhomogeneities in coupling constants in the very early universe would generate modulated large scale fluctuations in all relic species that are produced due to interactions and freezing out. Moreover (p)reheating of the inflaton field results in modulated curvature fluctuations. Even if the standard inflaton fluctuations are suppressed, in this picture we may have pure curvature cosmological fluctuations entirely generated by the modulated spatial variations of the coupling constants during preheating.

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Cited by 4 Pith papers

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

  1. Tachyonic Encore: A universal shift of inflationary observables

    hep-th 2026-06 unverdicted novelty 5.0 of 10

    A light axion spectator induces post-inflation tachyonic phases that produce a nearly scale-invariant boost to the curvature power spectrum and alter key inflationary observables in a largely potential-independent manner.

  2. Stochastic Gravitational Waves from Modulated Reheating

    astro-ph.CO 2025-10 unverdicted novelty 5.0 of 10

    A spectator scalar in modulated reheating with large Higgs-like couplings generates detectable scalar-induced stochastic gravitational waves for BBO and DECIGO, but only outside perturbative low-energy extrapolations.

  3. Type-III Seesaw in Non-Holomorphic Modular Symmetry and Leptogenesis

    hep-ph 2025-08 unverdicted novelty 5.0 of 10

    A Type-III seesaw model based on non-holomorphic modular symmetry fits NuFIT 6.0 neutrino data and produces baryogenesis via leptogenesis with Y_B-L about 1e-9.

  4. Lectures on Reheating after Inflation

    astro-ph.CO 2019-07 unverdicted

    Lecture notes providing a generic introduction to reheating after inflation, covering its theoretical, phenomenological, and observational aspects.

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