J 2002

Isotropic loop quantum cosmology with matter

BOJOWALD, Martin and Franz HINTERLEITNER

Basic information

Original name

Isotropic loop quantum cosmology with matter

Authors

BOJOWALD, Martin (276 Germany, guarantor) and Franz HINTERLEITNER (40 Austria)

Edition

Physical Revue D, USA, The American Physical Society, 2002, 0556-2821

Other information

Language

English

Type of outcome

Článek v odborném periodiku

Field of Study

10301 Atomic, molecular and chemical physics

Country of publisher

United States of America

Confidentiality degree

není předmětem státního či obchodního tajemství

Impact factor

Impact factor: 4.358

RIV identification code

RIV/00216224:14310/02:00006759

Organization unit

Faculty of Science

UT WoS

000179679900028

Keywords in English

Loop quantum cosmology; Euclidean Hamiltonian; discrete time evolution

Tags

Reviewed
Změněno: 9/2/2007 09:52, doc. Franz Hinterleitner, Ph.D.

Abstract

V originále

The isotropic, spatially flat Friedmann model is coupled to a massless scalar field. The hailtonian constraint equation is solved exactly in the framework of loop quantum gravity. Time evolution is constructed with respect to the radius of the universe as an internal time. Due to the discrete nature of geometry in the loop formalism this time evolution becomes discrete, too. It displays the correct classical limit but avoids the singularity of the classical counterpart.

Links

MSM 143100006, plan (intention)
Name: Kvantová teorie pole, teorie strun, kvantová teorie gravitace
Investor: Ministry of Education, Youth and Sports of the CR, Quantum Field Theory, String Theory, Quantum Theory of Gravity