pith. sign in

arxiv: gr-qc/0206054 · v1 · submitted 2002-06-18 · 🌀 gr-qc · astro-ph· hep-th

Inflation from Quantum Geometry

classification 🌀 gr-qc astro-phhep-th
keywords quantumgeometrymatterphaseaccelerationadditionalapplicationbecause
0
0 comments X p. Extension
read the original abstract

Quantum geometry predicts that a universe evolves through an inflationary phase at small volume before exiting gracefully into a standard Friedmann phase. This does not require the introduction of additional matter fields with ad hoc potentials; rather, it occurs because of a quantum gravity modification of the kinetic part of ordinary matter Hamiltonians. An application of the same mechanism can explain why the present-day cosmological acceleration is so tiny.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  1. Quasinormal modes of a rotating loop quantum black hole

    gr-qc 2026-05 unverdicted novelty 5.0

    Quasinormal modes of a massless scalar field on a rotating loop quantum black hole background exhibit reduced real frequencies and damping rates with increasing quantum corrections, with rotation introducing crossover...