pith. sign in

arxiv: gr-qc/9410014 · v1 · pith:QZHE5XAUnew · submitted 1994-10-11 · 🌀 gr-qc

Real Ashtekar Variables for Lorentzian Signature Space-times

classification 🌀 gr-qc
keywords variablesashtekarapproachcomplexconstrainthamiltonianintroductionlorentzian
0
0 comments X
read the original abstract

I suggest in this letter a new strategy to attack the problem of the reality conditions in the Ashtekar approach to classical and quantum general relativity. By writing a modified Hamiltonian constraint in the usual $SO(3)$ Yang-Mills phase space I show that it is possible to describe space-times with Lorentzian signature without the introduction of complex variables. All the features of the Ashtekar formalism related to the geometrical nature of the new variables are retained; in particular, it is still possible, in principle, to use the loop variables approach in the passage to the quantum theory. The key issue in the new formulation is how to deal with the more complicated Hamiltonian constraint that must be used in order to avoid the introduction of complex fields.

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 9 Pith papers

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

  1. Toller matrices and the Feynman $i\varepsilon$ in spinfoams

    gr-qc 2026-04 unverdicted novelty 7.0

    Toller matrices T^(±) in causal spinfoam amplitudes satisfy T^(+) + T^(-) = D and admit equivalent definitions via analyticity, iε prescription, and boost-eigenvalue integrals that reproduce the Euclidean-to-Lorentzia...

  2. Collective excitations in quantum gravity condensates

    gr-qc 2026-05 unverdicted novelty 6.0

    Collective excitations analogous to phonons are derived in quantum gravity condensates within a group field theory model, yielding leading beyond-mean-field corrections to emergent Friedmann dynamics.

  3. Covariant quantization of the Einstein-Hilbert theory in first-order form

    gr-qc 2026-04 unverdicted novelty 6.0

    A covariant BV quantization of first-order Einstein-Hilbert gravity is constructed, yielding a novel trivial symmetry and establishing on-shell quantum equivalence to the metric formulation.

  4. Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis

    astro-ph.CO 2026-05 unverdicted novelty 5.0

    Einstein-Cartan pseudoscalaron inflation coupled to type-I seesaw neutrinos makes nonthermal leptogenesis a necessary mechanism for the baryon asymmetry, yielding ns ~ 0.97, r ~ 0.004 and nB/s ~ 8.7e-11 for gamma ~ -1...

  5. Covariant quantization of the Einstein-Hilbert theory in first-order form

    gr-qc 2026-04 unverdicted novelty 5.0

    A covariant path-integral quantization of first-order Einstein-Hilbert gravity is constructed using BV formalism, yielding structural identities from Dyson-Schwinger equations and equivalence to the second-order formu...

  6. Charges of supergravity

    hep-th 2026-04 unverdicted novelty 5.0

    In N=1 supergravity as constrained BF theory, the algebra of boundary charges matches the superalgebra with translational charges vanishing on-shell from the super-torsion constraint.

  7. Quantum Backreaction in Effective Brans-Dicke Bianchi I Cosmology

    gr-qc 2026-01 unverdicted novelty 5.0

    Cross-correlations between quantum degrees of freedom are required for consistent effective dynamics in Brans-Dicke Bianchi I cosmology, smoothing bounces and keeping energy density finite.

  8. Effective dynamics of Janis-Newman-Winicour spacetime

    gr-qc 2025-12 unverdicted novelty 5.0

    Loop quantum gravity effective dynamics resolves classical singularities in the JNW spacetime via bounces in the μ0 scheme but produces new singularities in the Dirac-observable scheme.

  9. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.