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Shortcomings of the big bounce derivation in loop quantum cosmology

Francesco Cianfrani and Giovanni Montani
Phys. Rev. D 82, 021501(R) – Published 22 July 2010

Abstract

We give a prescription to define in loop quantum gravity the electric field operator related to the scale factor of a homogeneous and isotropic cosmological space-time. This procedure allows us to link the fundamental theory with its cosmological implementation. In view of the conjugate relation existing between holonomies and fluxes, the edge length and the area of surfaces in the fiducial metric satisfy a duality condition. As a consequence, the area operator has a discrete spectrum also in loop quantum cosmology. This feature makes the super-Hamiltonian regularization an open issue of the whole formulation.

  • Received 9 June 2010

DOI:https://doi.org/10.1103/PhysRevD.82.021501

©2010 American Physical Society

Authors & Affiliations

Francesco Cianfrani1,* and Giovanni Montani2,3,4,†

  • 1ICRA-International Center for Relativistic Astrophysics, Dipartimento di Fisica (G9), Università di Roma “Sapienza,” Piazzale Aldo Moro 5, 00185 Roma, Italy
  • 2Dipartimento di Fisica (G9), Università di Roma “Sapienza,” Piazzale Aldo Moro 5, 00185 Roma, Italy
  • 3ENEA Centro Ricerche Frascati (Unità Fusione Magnetica), Via Enrico Fermi 45, 00044 Frascati, Roma, Italy
  • 4ICRANet Coordinating Center Pescara, Piazzale della Repubblica, 10, 65100 Pescara, Italy

  • *francesco.cianfrani@icra.it
  • montani@icra.it

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Vol. 82, Iss. 2 — 15 July 2010

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