Paper Citation Record · LEDGER

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2501.18031.

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

pith.paper-citation-record.v1
2501.18031 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T01:08:40.896465Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:07:44.902694Z

Reference resolution

0 of 0 outbound references displayed

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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 9126d422-c620-4d8c-8a78-fc2a9495cb89 · inbound

Cosmographic analysis of sign-switching dark energy cites this paper.

Cosmographic analysis of sign-switching dark energy Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T01:08:40.896465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 886e58b0-590b-4693-811c-5fdde59c2341 · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 207

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.802127Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation c63e225d-ae7f-49c8-b2e8-fdd4e29ec43b · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 83

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.624179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation b0916da2-abf6-4c13-999e-400d20f73297 · inbound

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations cites this paper.

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 78

Resolution: verified exact; arxiv_id, observed 2026-05-16T05:20:39.631780Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 8cd0c66e-93b7-4adf-80f9-0602e741d3fc · inbound

Statistical consistency of sign-switching vacuum energy with cosmological observations cites this paper.

Statistical consistency of sign-switching vacuum energy with cosmological observations Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-02T18:35:52.836218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b0bf439-aee0-4144-ae07-21eb0e7830fb · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 92

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16b91d67-bdf3-4633-94de-804b909707c6 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 62

Resolution: verified exact; arxiv_id, observed 2026-05-10T14:20:31.064828Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 218a6e17-4bb5-485a-bc06-bfb2849fcb09 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 93

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.342413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 076f56a6-0e1c-4d9c-982e-ef09af9d2db6 · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 122

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.208229Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 18a49258-9aef-40ab-b99f-33685792bfa6 · inbound

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity cites this paper.

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 30

Resolution: unresolved; no resolver link, observed 2026-07-12T14:25:03.782538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 63d1b55a-029b-48cc-8455-64404d5674c2 · inbound

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions cites this paper.

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:07:44.903952Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 276fe673-fa14-4316-acf6-9036ba1109f8 · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 194

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.215694Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 8bac621a-1453-4a10-94cd-1f1a706cf2e1 · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 71

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bdf99a8c-29a1-41ec-8ae0-cc1080240783 · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:01.807584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.