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Loop quantum cosmology: relation between theory and observations

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arxiv 2301.10215 v1 pith:TLI2IRLV submitted 2023-01-24 gr-qc

Loop quantum cosmology: relation between theory and observations

classification gr-qc
keywords loopquantumcosmologyrelationtheoryambiguitiesanisotropiesapplications
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This chapter provides a review of the frameworks developed for cosmological perturbation theory in loop quantum cosmology, and applications to various models of the early universe including inflation, ekpyrosis and the matter bounce, with an emphasis on potential observational consequences. It also includes a discussion on extensions to include non-Gaussianities and background anisotropies, as well as on its limitations concerning trans-Planckian perturbations and quantization ambiguities. It concludes with a summary of recent work studying the relation between loop quantum cosmology and full loop quantum gravity.

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Cited by 3 Pith papers

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

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    γ-duality in the EPRL spinfoam model determines the relation between parity-even and parity-odd terms in an effective gravity theory, allowing the Barbero-Immirzi parameter to be measured from inflationary tensor observables.

  2. Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology

    gr-qc 2025-09 unverdicted novelty 5.0

    A quasi-dust ekpyrotic two-field model in Loop Quantum Cosmology produces viable primordial power spectra via coupled scalar and tensor perturbations.

  3. Stable initial conditions and analytical investigations of cosmological perturbations in a modified loop quantum cosmology

    gr-qc 2025-05 unverdicted novelty 5.0

    A stable initial state is identified in mLQC-I that diagonalizes the Hamiltonian and minimizes particle creation, with mode functions approximated analytically by Airy or cylindrical functions whose constants are fixe...