Paper Citation Record · LEDGER

Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1506.01011.

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

pith.paper-citation-record.v1
1506.01011 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T19:35:28.381844Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

46
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a3c9f3aa-eb76-4a9e-a8ba-44adc5b3a302 · inbound

Fully viable DHOST bounce with extra scalar cites this paper.

Fully viable DHOST bounce with extra scalar Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T19:35:28.381844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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

Probability of the Initial Conditions for Inflation and Slow Contraction cites this paper.

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 253dcc0f-6e3b-431a-8682-e59f5f6555f9 · inbound

Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model cites this paper.

Non-Gaussianity and Strong-Coupling Problem in a Two-Field DHOST Bouncing Model Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-07-02T04:16:36.125696Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 8ced4847-2984-4536-82de-092854170df7 · inbound

Causal Horizons, Geodesic Completeness and Stability in Slow Contraction Cosmology cites this paper.

Causal Horizons, Geodesic Completeness and Stability in Slow Contraction Cosmology Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-07-10T17:37:26.042860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 6ed02579-3d2e-4107-bbda-c477dcea8243 · inbound

Causal Horizons, Geodesic Completeness and Stability in Slow Contraction Cosmology cites this paper.

Causal Horizons, Geodesic Completeness and Stability in Slow Contraction Cosmology Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 12

Resolution: unresolved; no resolver link, observed 2026-07-13T06:40:48.571152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 726e9b39-9f6b-4b8c-8194-71578e0ca003 · inbound

Is there ghost and tachyon free bounce in UV complete gravity theory? cites this paper.

Is there ghost and tachyon free bounce in UV complete gravity theory? Scale-invariant perturbations in ekpyrotic cosmologies without fine-tuning of initial conditions

Reference 47

Resolution: unresolved; no resolver link, observed 2026-07-14T03:20:56.366428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.