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From General Relativity to Quantum Gravity

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arxiv 1408.4336 v1 pith:XYPRUVBD submitted 2014-08-19 gr-qc hep-thmath-phmath.MPquant-ph

classification gr-qchep-thmath-phmath.MPquant-ph
keywords quantumgeneralgravityrelativityadvancesapproachesarenaavenues
verification ladder T0 review T1 audit T2 compute T3 formal
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In general relativity (GR), spacetime geometry is no longer just a background arena but a physical and dynamical entity with its own degrees of freedom. We present an overview of approaches to quantum gravity in which this central feature of GR is at the forefront. However, the short distance dynamics in the quantum theory are quite different from those of GR and classical spacetimes and gravitons emerge only in a suitable limit. Our emphasis is on communicating the key strategies, the main results and open issues. In the spirit of this volume, we focus on a few avenues that have led to the most significant advances over the past 2-3 decades.

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Cited by 2 Pith papers

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

  1. Cosmological consequences of scale-dependent Barrow-Tsallis entropy

    gr-qc 2026-07 conditional novelty 6.0 of 10

    A scale-dependent Barrow-Tsallis entropy cosmology fits cosmic data but is statistically disfavored versus ΛCDM, with only a modest and partially circular Hubble-tension 'alleviation'.

  2. The one-loop effective action from the coherent state path integral of loop quantum gravity

    gr-qc 2025-02 conditional novelty 6.0 of 10

    The one-loop effective action from the LQG coherent state path integral is computed and found to be UV-finite, with the dynamical area j0 > 0 at the quantum level.

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