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Emergent Models for Gravity: an Overview of Microscopic Models

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arxiv 1110.0686 v2 pith:KYBSTR4X submitted 2011-10-04 gr-qc hep-th

classification gr-qchep-th
keywords modelsdescribeemergentgravityoverviewarriveattemptscollective
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We give a critical overview of various attempts to describe gravity as an emergent phenomenon, starting from examples of condensed matter physics, to arrive to more sophisticated pregeometric models. The common line of thought is to view the graviton as a composite particle/collective mode. However, we will describe many different ways in which this idea is realized in practice.

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Cited by 5 Pith papers

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

  1. Collective excitations in quantum gravity condensates

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    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.

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  3. Gravitational waves and cosmic boundary

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    If the cosmos has a reflective boundary beyond redshift 15, gravitational waves from repeated black hole mergers could reveal it, with a TianQin+LISA network best at fixing the boundary's orientation.

  4. First Law of Thermodynamics and Emergence of Cosmic Space in a Non-Flat Universe

    gr-qc 2019-08 conditional novelty 5.0 of 10

    In a non-flat Friedmann universe, the unified first law dE = TdS + WdV and the energy-flux form -dE = TdS are consistent only when the horizon volume is taken as the areal volume, not the proper invariant volume.

  5. Emergent Gravity in a Holographic Universe

    hep-th 2019-08 conditional novelty 3.0 of 10

    Causal diamonds in symmetric spacetimes obey a thermodynamic first law with negative temperature, and the Einstein equations can be recast as an entropy equilibrium condition, with a long-string CFT picture for non-Ad...

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