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The Inflaton Field as Self-Interacting Dark Matter in the Braneworld Scenario

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arxiv astro-ph/0111292 v2 pith:KL3XCGLN submitted 2001-11-14 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords fieldbraneworlddarkinflatonmatterself-interactinguniverseblack
verification ladder T0 review T1 audit T2 compute T3 formal
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A unified model is developed within the context of the braneworld paradigm, where a single scalar field can act as both the inflaton field in the very early universe and also as strong, self-interacting dark matter in the post-inflationary universe. Reheating proceeds due to the overproduction and subsequent evaporation of primordial black holes. Observational constraints, most notably from gravitational waves, are satisfied if the probability of PBH formation is sufficiently high.

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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. Gravitational Waves from Black Hole Reheating: The Scalar-Induced Component

    hep-ph 2026-05 unverdicted novelty 7.0 of 10

    Accounting for the minimal mass spread of primordial black holes from gravitational collapse suppresses the Poltergeist GW background to the level of generic scalar-induced signals and reopens ultra-light PBH parameter space.

  2. Dark Matter and Energy-Momentum Squared Gravity

    gr-qc 2025-01 reject novelty 4.0 of 10

    Energy-momentum squared gravity can reproduce flat galactic rotation curves only because its free parameter s is set from the observed velocities.

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