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Paper detail

Non-singular inflationary universe from polymer matter

We consider a polymer quantization of a free massless scalar field in a homogeneous and isotropic cosmological spacetime. This quantization method assumes that field translations are fundamentally discrete, and is related to but distinct from that used in loop quantum gravity. The semi-classical Friedman equation yields a universe that is non-singular and non-bouncing, without quantum gravity. The model has an early de Sitter-like inflationary phase with sufficient expansion to resolve the horizon and entropy problems, and a built in mechanism for a graceful exit from inflation.

preprint2009arXivOpen access
Golam Mortuza HossainViqar HusainSanjeev S. Seahra
astro-ph.COgr-qchep-th
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Golam Mortuza HossainViqar HusainSanjeev S. Seahra

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