Paper Citation Record · LEDGER

$SL(2,\mathbb{Z})$ Cosmological Attractors

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2408.05203.

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

pith.paper-citation-record.v1
2408.05203 v2

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 2026-08-07T06:34:17.273281+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:12:32.720969Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T10:56:52.158703Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8b2e49f3-c3a1-4dc8-8050-0f146aaae036 · inbound

Post-inflationary enhancement of adiabatic perturbations in modular cosmology cites this paper.

Post-inflationary enhancement of adiabatic perturbations in modular cosmology $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-06T20:12:32.720969Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af96530d-8150-40d4-a048-96e725e7a332 · inbound

Ultra slow-turn inflation cites this paper.

Ultra slow-turn inflation $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-02T19:14:19.947380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1837271b-ec92-4eb3-8ead-80bde27e1d12 · inbound

Some Properties and Uses of the Species Scale cites this paper.

Some Properties and Uses of the Species Scale $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 40

Resolution: verified exact; arxiv_id, observed 2026-05-12T10:21:30.866487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation df841f43-a5f0-4908-82d5-7446ce0dc5a8 · inbound

Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.

Breaking Free from the Swampland of Impossible Universes through the DESI Portal $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 267

Resolution: unresolved; no resolver link, observed 2026-08-02T14:29:41.205568Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db9ad729-21b9-477d-85f1-034957fc41e1 · inbound

Finite modular Coleman-Weinberg inflation cites this paper.

Finite modular Coleman-Weinberg inflation $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.159983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation ea7c1ee5-982b-44d7-8f1d-4abc9f1f9112 · inbound

Gravitational waves from self-resonance during reheating with a quantum-corrected inflaton potential cites this paper.

Gravitational waves from self-resonance during reheating with a quantum-corrected inflaton potential $SL(2,\mathbb{Z})$ Cosmological Attractors

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T15:42:53.454825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.