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The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang

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arxiv hep-th/0103239 v3 pith:E5OHF6BA submitted 2001-03-29 hep-th astro-phhep-ph

classification hep-thastro-phhep-ph
keywords scenariouniversebangbranescosmologicalgravitationalspectrumwave
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We propose a cosmological scenario in which the hot big bang universe is produced by the collision of a brane in the bulk space with a bounding orbifold plane, beginning from an otherwise cold, vacuous, static universe. The model addresses the cosmological horizon, flatness and monopole problems and generates a nearly scale-invariant spectrum of density perturbations without invoking superluminal expansion (inflation). The scenario relies, instead, on physical phenomena that arise naturally in theories based on extra dimensions and branes. As an example, we present our scenario predominantly within the context of heterotic M-theory. A prediction that distinguishes this scenario from standard inflationary cosmology is a strongly blue gravitational wave spectrum, which has consequences for microwave background polarization experiments and gravitational wave detectors.

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Cited by 26 Pith papers

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

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    A probability estimate for scalar-field homogeneity at the onset of inflation and slow contraction concludes that, after optimizing over initial spectra, inflation is vastly more likely than ekpyrosis to have the requ...

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    gr-qc 2019-08 conditional novelty 6.0 of 10

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  17. Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology

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  20. Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model

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