Dynamically Triangulating Lorentzian Quantum Gravity

By J. Ambjørn, J. Jurkiewicz, R. Loll. 2001

303 citations recorded by the source corpus.

Fruitful ideas on how to quantize gravity are few and far between. In this paper, we give a complete description of a recently introduced non-perturbative gravitational path integral whose continuum limit has already been investigated extensively in d < 4, with promising results. It is based on a simplicial regularization of Lorentzian space-times and, most importantly, possesses a well-defined, non-perturbative Wick rotation. We present a detailed analysis of the geometric and mathematical properties of the discretized model in d = 3,4. This includes a derivation of Lorentzian simplicial manifold constraints, the gravitational actions and their Wick rotation. We define a transfer matrix for the system and show that it leads to a well-defined self-adjoint Hamiltonian. In view of numerical simulations, we also suggest sets of Lorentzian Monte Carlo moves. We demonstrate that certain pathological phases found previously in Euclidean models of dynamical triangulations cannot be realized in the Lorentzian case.

Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/22b5202f01ca11fcf31fc3f339775c4624483190

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

  1. R. Loll
  2. M. Niedermaier
  3. Martin Reuter
  4. J. Jurkiewicz
  5. J. Ambjrn
  6. J. Ambjørn
  7. E. Wilson-Ewing
  8. D. Oriti

In Statistical and Nonlinear Physics

  1. R. Loll
  2. M. Niedermaier
  3. Martin Reuter
  4. J. Jurkiewicz
  5. Lorenzo Sindoni
  6. D. Oriti
  7. J. Ambjrn
  8. J. Ambjørn

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