corner
corner

Phys. Rev. Lett. 85, 924–927 (2000)

Nonperturbative Lorentzian Path Integral for Gravity

Download: PDF (84 kB) Buy this article Export: BibTeX or EndNote (RIS)

J. Ambjørn1, J. Jurkiewicz2, and R. Loll3
1The Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen Ø, Denmark
2Institute of Physics, Jagellonian University, Reymonta 4, PL 30-059 Krakow, Poland
3Max-Planck-Institut für Gravitationsphysik, Am Mühlenberg 1, D-14476 Golm, Germany

Received 7 February 2000; published in the issue dated 31 July 2000

We construct a well-defined regularized path integral for Lorentzian quantum gravity in terms of dynamically triangulated causal space-times. Each Lorentzian geometry and its action have a unique Wick rotation to the Euclidean sector. All space-time histories possess a distinguished notion of a discrete proper time and, for finite lattice volume, the associated transfer matrix is self-adjoint, bounded, and strictly positive. The degenerate geometric phases found in dynamically triangulated Euclidean gravity are not present.

© 2000 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.85.924
DOI:
10.1103/PhysRevLett.85.924
PACS:
04.60.Gw, 04.20.Gz, 04.60.Kz, 04.60.Nc