Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-21T22:49:29.622622Z
Paper Citation Record · LEDGER
As of 5 August 2026, this Paper Citation Record lists 66 of 66 outbound references and 2 inbound Pith citation observations for arXiv:2509.06148.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-05-21T22:49:29.622622Z
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T09:05:14.017240Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-29T10:23:17.568859Z
66 of 66 outbound references displayed
External citation measurements
No source-named external measurement is stored.
Observation d056b96d-77d4-4387-89bf-fbfe413fcdea · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Unresolved cited work
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Reference 3
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Observation a4aa3c37-bd6d-4da4-913d-bfe71d0b9c3e · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology We compute the scalar spectral index given in (35) using our numerical results for the curvature power spectrumP R att f in the expanding phase
Reference 4
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Observation 25d0dbb1-93e7-4ae1-87c7-cac60f966e5d · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Small variations of the ekpyrotic parameters have little impact on the evolution of perturbations
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Observation 574360bc-02c2-4375-a99d-aa748e61857f · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Initially, modesk≲10 −7 that have exited the horizon display a nearly scale-invariant power spectrum, with a slight red-tilt favouring smallerk
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Source-reported events for the cited work
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Observation 8b555909-3e8f-4a08-92b6-0df9471d9f39 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology During the quasi-dust-dominated phase of contraction, this mode’s ampli- tude grows fast, withP t ∝ |t| −2+4wT untilt eq1
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Source-reported events for the cited work
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Observation 8b41de00-d46a-4780-b26d-a4ac46df2165 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology The evolution of the power spectrum for this tensor mode is shown in the right panel of Figure 12
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Observation 85fb5281-8762-4c53-8c7f-f69a33bf8a59 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Loop Quantum Gravity: from Computation to Phe- nomenology
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Observation 95abd394-47b1-48cd-8d22-58e49d188a7c · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology As was discussed in section III C, all modes in the red-tilted regime have the same qualitative behaviour
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Observation ec3198c1-d3fa-42d3-a35f-7b8ec115583d · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology A new type of isotropic cosmological models without singularity
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Observation 01404d44-7915-45fc-ac43-d2de58e822b0 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology First order phase transition of a vacuum and expansion of the universe
Reference 12
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Observation 552dd058-a71b-4d3d-a77d-27f2b12deae1 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Inflationary universe: A possible solution to the horizon and flatness problems
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Observation 50541cb1-d479-4bd2-ac9f-6d16197ef3fa · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems
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Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
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Source-reported events for the cited work
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Observation f4599565-1cad-4574-803e-41821e6614a9 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Chaotic inflation
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Source-reported events for the cited work
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Observation 784b5436-1ce0-4a26-89f2-6e1c6ae61bf0 · outbound
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Observation 968576a0-2e4d-48c5-b1f7-e85a12433661 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology The Vacuum energy and large scale structure of the universe
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Observation b6adecb8-cae7-44ad-ad87-9c548abb233a · outbound
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Observation 68463261-41e0-4f33-ac6f-5909f18a7fe6 · outbound
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Observation 8df23d41-05b5-445b-b558-1ca2ae3d9a7c · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology The development of irregularities in a single bubble inflationary universe
Reference 21
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Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
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Observation a315ff52-004a-4343-9097-adf59f2d1efd · outbound
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Reference 23
Source-reported events for the cited work
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Observation 2655b4b8-ef46-40d3-9c19-3c861048fd4f · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Discreteness of area and volume in quantum gravity
Reference 24
Source-reported events for the cited work
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Observation 21e20466-d22d-4057-94ef-ed20b21416cd · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Evidence for Maximal Acceleration and Singularity Resolution in Covariant Loop Quantum Gravity
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Observation 8b444ce5-bf77-42b5-b441-d7ece2cb720f · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Loop Quantum Cosmology: Physics of Singularity Resolution and its Implications
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Observation d91e2b6b-99aa-4745-b870-ca3f1a00b4c9 · outbound
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Observation 8e930823-f5fa-44e8-9ff1-422f19f249b2 · outbound
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Observation 284b1a1b-2ef4-4816-8c4e-14206f75a9bd · outbound
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Observation 1168cff4-cc28-41af-b35d-eccbb77c50ae · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Hybrid Loop Quantum Cosmology: An Overview
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Observation 4556f025-5ee4-47c5-a0f7-fee47eac40a3 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology An Overview on the Nature of the Bounce in LQC and PQM
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Observation 52efcc4f-7d8b-4cef-84d5-0f12eac04c0d · outbound
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Observation 0d5851af-303f-4ebf-8181-d62bb8989e65 · outbound
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Observation 55b27eb1-60b4-4416-8f51-c14703a9ff86 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Inflation in Loop Quantum Cosmology
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Observation bd22c757-9faf-43cd-a45e-171976e567ba · outbound
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Observation 273a4419-ea78-4d8f-abb1-3b4c8f66363a · outbound
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Observation 4fe29239-96a3-4894-926b-352b838ef83e · outbound
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Observation 51283c5b-c0a0-4a89-980b-af6d019ec45a · outbound
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Observation b6266899-1e77-4434-93c4-7c02fc200da5 · outbound
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Observation f4de3312-aa69-425e-aab1-0760b85f6b19 · outbound
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Observation de2acfb8-7b68-497a-a798-c20b24a9e953 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology The Temperature of the Cosmic Microwave Background
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Observation 3ec3807b-ae8c-44e2-8a3d-ac70aab9ae93 · outbound
Quasi-dust ekpyrotic scenario in Loop Quantum Cosmology Observational constraints on anisotropies for bouncing alternatives to inflation
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Observation 9907c17c-223c-47b2-a716-2a61c1ce1d04 · inbound
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Unavailable: canonical work link unavailable.