Paper Citation Record · LEDGER

Braneworld models of dark energy

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 15 inbound Pith citation observations for arXiv:astro-ph/0202346.

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

pith.paper-citation-record.v1
astro-ph/0202346 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 15 of 15 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 15 of 15 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T20:46:05.959481Z

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

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External citation measurements

738
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 5d109340-1e48-41a8-b58d-25430d9f2b9c · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions Braneworld models of dark energy

Reference 249

Resolution: verified exact; local_arxiv, observed 2026-05-15T11:50:32.859999Z

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 3b54d579-0415-4f2d-a872-1f3da45e019b · inbound

Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies cites this paper.

Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies Braneworld models of dark energy

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-05-24T12:54:30.283737Z

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 cbfaedb9-958e-4dfc-92f3-16d41cba4259 · inbound

Cosmological Frequency Combs cites this paper.

Cosmological Frequency Combs Braneworld models of dark energy

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T20:46:05.959481Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b2db5dc-9803-481e-84b1-4cdd4924a9b4 · 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 Braneworld models of dark energy

Reference 140

Resolution: verified exact; local_arxiv, observed 2026-05-18T04:50:55.001670Z

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 c8eb79de-8062-44ed-b281-bbcffc8530c0 · inbound

F(R,..) theories from the point of view of the Hamiltonian approach: non-vacuum Anisotropic Bianchi type I cosmological model cites this paper.

F(R,..) theories from the point of view of the Hamiltonian approach: non-vacuum Anisotropic Bianchi type I cosmological model Braneworld models of dark energy

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-05-16T23:03:39.045832Z

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 45580881-dabe-4755-9af4-48a9089b47f4 · 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 Braneworld models of dark energy

Reference 106

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 48f21d01-25f0-4427-85b8-048f744fd192 · inbound

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data cites this paper.

Latent-Space Gaussian Processes for Dark-Energy Reconstruction from Observational $H(z)$ Data Braneworld models of dark energy

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-05-14T18:47:36.932832Z

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 0e93b40c-0d7d-48db-bb2b-d7d79d7e4f59 · inbound

Thick branes and fermion localization in five-dimensional $f(T,T_G)$ gravity cites this paper.

Thick branes and fermion localization in five-dimensional $f(T,T_G)$ gravity Braneworld models of dark energy

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-05-20T05:18:03.446762Z

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 2532372c-4159-47c0-8df0-6c1bac458bce · inbound

Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply cites this paper.

Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply Braneworld models of dark energy

Reference 91

Resolution: verified exact; local_arxiv, observed 2026-06-29T15:33:32.286450Z

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 14918334-385f-4738-9630-b583b27e729e · inbound

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias cites this paper.

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias Braneworld models of dark energy

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-06-28T03:41:35.555841Z

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 22a6d38c-ad16-4686-843d-e483c1d9f496 · inbound

An Interplay Between Fractional Calculus and Holographic Dark Energy cites this paper.

An Interplay Between Fractional Calculus and Holographic Dark Energy Braneworld models of dark energy

Reference 133

Resolution: verified exact; local_arxiv, observed 2026-06-26T10:19:18.721468Z

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 a314baea-0f7a-44ca-a9d4-3659c1638177 · inbound

Quintom Model Perturbations cites this paper.

Quintom Model Perturbations Braneworld models of dark energy

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-06-26T04:18:58.545418Z

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 833cab9d-ae74-47c5-b4e9-5ec3df889e4b · 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 Braneworld models of dark energy

Reference 86

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 d710541d-94b1-460f-b11f-f0ce2472534c · inbound

Compact stars in a large-tension braneworld: mildly negative Weyl coupling consistent with NICER and gravitational-wave data cites this paper.

Compact stars in a large-tension braneworld: mildly negative Weyl coupling consistent with NICER and gravitational-wave data Braneworld models of dark energy

Reference 23

Resolution: unresolved; no resolver link, observed 2026-07-14T15:11:08.453732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 644ff6ae-c4c4-46f7-9d48-d4354b6e6ffb · 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 Braneworld models of dark energy

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T16:30:02.471263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.