Paper Citation Record · LEDGER

Probability of the Initial Conditions for Inflation and Slow Contraction

As of 18 August 2026, this Paper Citation Record lists 58 of 58 outbound references and 1 inbound Pith citation observation for arXiv:2505.22763.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2505.22763 v3

Coverage vector

measured 58 of 58 reference resolution

Typed states for the displayed outbound observations.

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measured 59 of 59 standing notices

One-hop event checks from named stored sources.

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T01:24:43.210811Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: cited_works

Reference resolution

58 of 58 outbound references displayed

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verified fuzzy8
unresolved37
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External citation measurements

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Outbound references

Observation fb368d82-f533-4bdc-9755-f6d4c835b843 · outbound

This paper cites an unresolved cited work.

Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 1

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This paper cites an unresolved cited work.

Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 2

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Observation d2f91178-0c56-4faf-851c-6b235cf588eb · outbound

This paper cites slow contraction.

Probability of the Initial Conditions for Inflation and Slow Contraction slow contraction

Reference 3

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Observation 83fdfee1-a7c4-4a61-9319-8d3d3ae33e22 · outbound

This paper cites s = inf.

Probability of the Initial Conditions for Inflation and Slow Contraction s = inf

Reference 4

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Observation 14fddfe9-79c1-47fe-af56-18a435453e3a · outbound

This paper cites (A6) Then, it follows from (A4) that ˜ψ(⃗k) = −4πG ˜ρ(⃗k) |⃗k|2.

Probability of the Initial Conditions for Inflation and Slow Contraction (A6) Then, it follows from (A4) that ˜ψ(⃗k) = −4πG ˜ρ(⃗k) |⃗k|2

Reference 5

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Observation 48338f9c-76d2-407f-9705-d270afd64289 · outbound

This paper cites This scale is given by Θ−1 = K 3 , (A13) where K is the trace of the extrinsic curvature of the initial-time hypersurface.

Probability of the Initial Conditions for Inflation and Slow Contraction This scale is given by Θ−1 = K 3 , (A13) where K is the trace of the extrinsic curvature of the initial-time hypersurface

Reference 6

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Observation 1d652358-b1b3-462b-85e6-228dcd336180 · outbound

This paper cites We focus on a thermal spectrum here for concreteness.

Probability of the Initial Conditions for Inflation and Slow Contraction We focus on a thermal spectrum here for concreteness

Reference 7

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 8

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 9

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Observation 8683f5ff-eb6f-467c-9221-1f823d9fdc94 · outbound

This paper cites Kazanas, apjl 241, L59 (1980).

Probability of the Initial Conditions for Inflation and Slow Contraction Kazanas, apjl 241, L59 (1980)

Reference 10

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 11

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 12

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Observation f149ecff-6e5a-4b5a-947d-7de6472420a2 · outbound

This paper cites Albrecht and P.

Probability of the Initial Conditions for Inflation and Slow Contraction Albrecht and P

Reference 13

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Observation df864695-2cb2-4920-9779-22c3eeb354a5 · outbound

This paper cites Cosmological parameters from SDSS and WMAP.

Probability of the Initial Conditions for Inflation and Slow Contraction Cosmological parameters from SDSS and WMAP

Reference 14

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Observation d5d4f24b-fa9f-439c-a618-14c55d0bf5e8 · outbound

This paper cites Inflationary Cosmology: Exploring the Universe from the Smallest to the Largest Scales.

Probability of the Initial Conditions for Inflation and Slow Contraction Inflationary Cosmology: Exploring the Universe from the Smallest to the Largest Scales

Reference 15

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Observation c253ba9f-1fe6-41a4-a43b-1bb926ca3194 · outbound

This paper cites J., Barreiro, R.

Probability of the Initial Conditions for Inflation and Slow Contraction J., Barreiro, R

Reference 16

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Observation a8524295-33ed-46aa-a204-3ef5cc95950a · outbound

This paper cites Penrose, Annals N.

Probability of the Initial Conditions for Inflation and Slow Contraction Penrose, Annals N

Reference 17

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 18

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Observation 06bbe5b1-5313-4a57-bf4d-35c222c84e2f · outbound

This paper cites Inflationary paradigm in trouble after Planck2013.

Probability of the Initial Conditions for Inflation and Slow Contraction Inflationary paradigm in trouble after Planck2013

Reference 19

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Observation 6f623992-bba4-4803-88f7-57904c8b2942 · outbound

This paper cites Inflationary paradigm after Planck 2013.

Probability of the Initial Conditions for Inflation and Slow Contraction Inflationary paradigm after Planck 2013

Reference 20

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This paper cites Quantum Fluctuations in Cosmology and How They Lead to a Multiverse.

Probability of the Initial Conditions for Inflation and Slow Contraction Quantum Fluctuations in Cosmology and How They Lead to a Multiverse

Reference 21

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Observation 5d771d1c-89c7-4a2c-b9a7-66ccfc71de1f · outbound

This paper cites Trans-Planckian Issues for Inflationary Cosmology.

Probability of the Initial Conditions for Inflation and Slow Contraction Trans-Planckian Issues for Inflationary Cosmology

Reference 22

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Observation 8e6bcbf2-f6e1-436a-a8c7-ccd93b0a4a20 · outbound

This paper cites Initial Conditions for Inflation - A Short Review.

Probability of the Initial Conditions for Inflation and Slow Contraction Initial Conditions for Inflation - A Short Review

Reference 23

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Observation 6eb54a29-bd61-4994-aa04-d8ecd06cbb47 · outbound

This paper cites Inflationary spacetimes are not past-complete.

Probability of the Initial Conditions for Inflation and Slow Contraction Inflationary spacetimes are not past-complete

Reference 24

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Probability of the Initial Conditions for Inflation and Slow Contraction Unresolved cited work

Reference 25

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Observation 258031b2-3773-4620-94fb-39c39a1d681b · outbound

This paper cites Vilenkin, Phys.

Probability of the Initial Conditions for Inflation and Slow Contraction Vilenkin, Phys

Reference 26

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This paper cites Eternal inflation and its implications.

Probability of the Initial Conditions for Inflation and Slow Contraction Eternal inflation and its implications

Reference 27

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Observation c3357e93-61a0-4570-84e4-04f44242f428 · outbound

This paper cites Supersmoothing through Slow Contraction.

Probability of the Initial Conditions for Inflation and Slow Contraction Supersmoothing through Slow Contraction

Reference 28

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Observation a13a2b63-e1cc-480d-a7bf-a1dbaca530ee · outbound

This paper cites Slow Contraction and the Weyl Curvature Hypothesis.

Probability of the Initial Conditions for Inflation and Slow Contraction Slow Contraction and the Weyl Curvature Hypothesis

Reference 29

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Observation 17a0c759-e912-497e-94c8-f8c2b291892b · outbound

This paper cites Initial conditions problem in cosmological inflation revisited.

Probability of the Initial Conditions for Inflation and Slow Contraction Initial conditions problem in cosmological inflation revisited

Reference 30

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Observation 79d34966-7d99-4e29-8a10-81c206aa9fc2 · outbound

This paper cites Smoothing and flattening the universe through slow contraction versus inflation.

Probability of the Initial Conditions for Inflation and Slow Contraction Smoothing and flattening the universe through slow contraction versus inflation

Reference 31

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This paper cites Kurki-Suonio, P.

Probability of the Initial Conditions for Inflation and Slow Contraction Kurki-Suonio, P

Reference 32

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This paper cites Beginning inflation in an inhomogeneous universe.

Probability of the Initial Conditions for Inflation and Slow Contraction Beginning inflation in an inhomogeneous universe

Reference 33

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Observation 11622a24-e8c3-4010-90df-f9479a9ddc9c · outbound

This paper cites Robustness of Inflation to Inhomogeneous Initial Conditions.

Probability of the Initial Conditions for Inflation and Slow Contraction Robustness of Inflation to Inhomogeneous Initial Conditions

Reference 34

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This paper cites Robustness of Inflation to Large Tensor Perturbations.

Probability of the Initial Conditions for Inflation and Slow Contraction Robustness of Inflation to Large Tensor Perturbations

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:45.659786Z

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This paper cites A Bumpy Start to a Smooth Ride: Onset of Inflation amid Backreaction from Inhomogeneities.

Probability of the Initial Conditions for Inflation and Slow Contraction A Bumpy Start to a Smooth Ride: Onset of Inflation amid Backreaction from Inhomogeneities

Reference 36

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This paper cites The Effects of Potential Shape on Inhomogeneous Inflation.

Probability of the Initial Conditions for Inflation and Slow Contraction The Effects of Potential Shape on Inhomogeneous Inflation

Reference 37

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This paper cites Inhomogeneous initial conditions for inflation: A wibbly-wobbly timey-wimey path to salvation.

Probability of the Initial Conditions for Inflation and Slow Contraction Inhomogeneous initial conditions for inflation: A wibbly-wobbly timey-wimey path to salvation

Reference 38

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This paper cites Gravitational dynamics in Higgs inflation: Preinflation and preheating with an auxiliary field.

Probability of the Initial Conditions for Inflation and Slow Contraction Gravitational dynamics in Higgs inflation: Preinflation and preheating with an auxiliary field

Reference 39

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This paper cites Starting inflation from inhomogeneous initial conditions with momentum.

Probability of the Initial Conditions for Inflation and Slow Contraction Starting inflation from inhomogeneous initial conditions with momentum

Reference 40

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This paper cites Robustness of inflation to kinetic inhomogeneities.

Probability of the Initial Conditions for Inflation and Slow Contraction Robustness of inflation to kinetic inhomogeneities

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:46.254699Z

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This paper cites Beginning inflation in conformally curved spacetimes.

Probability of the Initial Conditions for Inflation and Slow Contraction Beginning inflation in conformally curved spacetimes

Reference 42

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This paper cites Cosmology using numerical relativity.

Probability of the Initial Conditions for Inflation and Slow Contraction Cosmology using numerical relativity

Reference 43

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Probability of the Initial Conditions for Inflation and Slow Contraction Inhomogeneous Anisotropic Cosmology

Reference 44

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Observation 0f2e4698-b36c-494b-bca9-0a6bf31daa4c · outbound

This paper cites Asymptotic Behavior of Cosmologies with $\Lambda >0$ in 2+1 Dimensions.

Probability of the Initial Conditions for Inflation and Slow Contraction Asymptotic Behavior of Cosmologies with $\Lambda >0$ in 2+1 Dimensions

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:49.527535Z

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This paper cites A de Sitter no-hair theorem for 3+1d Cosmologies with isometry group forming 2-dimensional orbits.

Probability of the Initial Conditions for Inflation and Slow Contraction A de Sitter no-hair theorem for 3+1d Cosmologies with isometry group forming 2-dimensional orbits

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:49.358805Z

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This paper cites On the asymptotics of 3+1D cosmologies with bounded scalar potential and isometry group forming 2-dimensional orbits.

Probability of the Initial Conditions for Inflation and Slow Contraction On the asymptotics of 3+1D cosmologies with bounded scalar potential and isometry group forming 2-dimensional orbits

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:49.168427Z

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Observation 41991866-8e17-4300-9b5d-4dd61af868df · outbound

This paper cites Flows into de Sitter space from anisotropic initial conditions: An effective field theory approach.

Probability of the Initial Conditions for Inflation and Slow Contraction Flows into de Sitter space from anisotropic initial conditions: An effective field theory approach

Reference 48

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:49.023053Z

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Observation 87941435-6a9e-430b-9e10-b81a37ad8a88 · outbound

This paper cites Bouncing Cosmology made simple.

Probability of the Initial Conditions for Inflation and Slow Contraction Bouncing Cosmology made simple

Reference 49

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Observation 4ba546f3-dffd-47a8-bb44-95ffe97fac88 · outbound

This paper cites The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang.

Probability of the Initial Conditions for Inflation and Slow Contraction The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:47.172183Z

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Observation 947d5fb6-5a31-479e-a8d9-6dda23ecfcfa · outbound

This paper cites On the Initial Conditions in New Ekpyrotic Cosmology.

Probability of the Initial Conditions for Inflation and Slow Contraction On the Initial Conditions in New Ekpyrotic Cosmology

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:48.838285Z

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Observation ea73548d-9e1a-4ef4-9361-feac0d2bc738 · outbound

This paper cites Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions.

Probability of the Initial Conditions for Inflation and Slow Contraction Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:47.394805Z

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This paper cites Sourcing curvature modes with entropy perturbations in non-singular bouncing cosmologies.

Probability of the Initial Conditions for Inflation and Slow Contraction Sourcing curvature modes with entropy perturbations in non-singular bouncing cosmologies

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-07T13:11:48.612384Z

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Observation d507feb2-f928-4743-9165-a4102ce7ab96 · outbound

This paper cites Nearly scale-invariant curvature modes from entropy perturbations during graceful exit.

Probability of the Initial Conditions for Inflation and Slow Contraction Nearly scale-invariant curvature modes from entropy perturbations during graceful exit

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:47.588849Z

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Observation 677240a0-5fd9-4dc9-88d2-2b95e4c0628a · outbound

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Probability of the Initial Conditions for Inflation and Slow Contraction Ultralocality and Slow Contraction

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:47.685770Z

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Observation 3c923b30-5946-409c-89c6-7ecaf65da450 · outbound

This paper cites Fully stable cosmological solutions with a non-singular classical bounce.

Probability of the Initial Conditions for Inflation and Slow Contraction Fully stable cosmological solutions with a non-singular classical bounce

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T13:11:47.762979Z

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Observation adca39a1-7e3b-45c4-93f0-6ccaebc40296 · outbound

This paper cites Cosmological Bounces Induced by a Fermion Condensate.

Probability of the Initial Conditions for Inflation and Slow Contraction Cosmological Bounces Induced by a Fermion Condensate

Reference 57

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Observation 51a138b9-b5fe-4a25-b0a0-afef742d1cb3 · outbound

This paper cites The robustness of slow contraction and the shape of the scalar field potential.

Probability of the Initial Conditions for Inflation and Slow Contraction The robustness of slow contraction and the shape of the scalar field potential

Reference 58

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Observation 13391696-024d-4187-8855-ea220dba9114 · inbound

Accelerated expansion of the universe purely driven by scalar field fluctuations cites this paper.

Accelerated expansion of the universe purely driven by scalar field fluctuations Probability of the Initial Conditions for Inflation and Slow Contraction

Reference 27

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