Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can the dark energy equation-of-state parameter w be less than -1?
As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 26 inbound Pith citation observations for arXiv:astro-ph/0301273.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T18:08:50.454695Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-03T23:09:01.606592Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 6242db14-338d-472d-82f4-7158ee8834de · inbound
Wormhole geometries in modified gravity cites this paper.
Wormhole geometries in modified gravity Can the dark energy equation-of-state parameter w be less than -1?
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T17:20:10.654184Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation df4612ae-c6e4-4a65-b1e6-92caa0aa7c47 · inbound
Inhomogeneous model with a space dependent Cosmological Constant cites this paper.
Inhomogeneous model with a space dependent Cosmological Constant Can the dark energy equation-of-state parameter w be less than -1?
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T20:38:29.854796Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 65a0955e-dfa8-4724-92ec-f9aa886ca15b · inbound
An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.
An overview of what current data can (and cannot yet) say about evolving dark energy Can the dark energy equation-of-state parameter w be less than -1?
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T18:51:43.047035Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2577a28b-9658-4250-b6ff-bf9f754d37d1 · inbound
Cosmic Strings as Dynamical Dark Energy: Novel Constraints cites this paper.
Cosmic Strings as Dynamical Dark Energy: Novel Constraints Can the dark energy equation-of-state parameter w be less than -1?
Reference 55
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T14:22:24.327538Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 1fe3f472-0d8b-4eef-92b3-cbe86c7267b3 · inbound
The Quintom theory of dark energy after DESI DR2 cites this paper.
The Quintom theory of dark energy after DESI DR2 Can the dark energy equation-of-state parameter w be less than -1?
Reference 217
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T13:12:18.390777Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation b56a2904-f4b6-49f8-8874-c823ec148279 · inbound
Kalb-Ramond Black Holes Sourced by ModMax Electrodynamics: Some Perturbative Properties in the Phantom Sector cites this paper.
Kalb-Ramond Black Holes Sourced by ModMax Electrodynamics: Some Perturbative Properties in the Phantom Sector Can the dark energy equation-of-state parameter w be less than -1?
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T18:08:50.454695Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47e1acac-b6af-48a8-95f0-219cc3db9d2c · inbound
Realizing the phantom-divide crossing with vector and scalar fields cites this paper.
Realizing the phantom-divide crossing with vector and scalar fields Can the dark energy equation-of-state parameter w be less than -1?
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T07:07:16.168335Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9eec1e8b-f121-4f72-bcdc-ff610b1fa442 · inbound
Energy conditions of bouncing solutions in quadratic curvature gravity coupled with a scalar field cites this paper.
Energy conditions of bouncing solutions in quadratic curvature gravity coupled with a scalar field Can the dark energy equation-of-state parameter w be less than -1?
Reference 43
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T01:18:26.670792Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d666ee39-7486-48a3-b053-5df81aa1e743 · inbound
Ghost Degrees of Freedom Without Quantum Runaway: Exact Moment Bounds from an Operator Conservation Law cites this paper.
Ghost Degrees of Freedom Without Quantum Runaway: Exact Moment Bounds from an Operator Conservation Law Can the dark energy equation-of-state parameter w be less than -1?
Reference 5
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T14:21:06.662657Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation d7ae1306-29b8-41b6-9e7b-ccec0b56dcfd · inbound
Unitary Time Evolution and Vacuum for a Quantum Stable Ghost cites this paper.
Unitary Time Evolution and Vacuum for a Quantum Stable Ghost Can the dark energy equation-of-state parameter w be less than -1?
Reference 7
- Resolution
- verified exact
- arxiv_id, observed 2026-05-11T14:41:04.436800Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 69584a39-bdee-4356-b8bd-9c2ebb267c53 · inbound
Late-time reconstruction of non-minimally coupled gravity with a smoothness prior cites this paper.
Late-time reconstruction of non-minimally coupled gravity with a smoothness prior Can the dark energy equation-of-state parameter w be less than -1?
Reference 8
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T04:07:13.407382Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5c86f95f-fff7-428c-811f-02d98a12b444 · inbound
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies cites this paper.
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies Can the dark energy equation-of-state parameter w be less than -1?
Reference 58
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T20:52:58.312692Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 9cce8022-c31d-4330-b0af-66f1dd7d1379 · inbound
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies cites this paper.
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies Can the dark energy equation-of-state parameter w be less than -1?
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T05:15:03.609765Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ecabf506-395b-4981-9b98-ffa6edf39158 · inbound
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies cites this paper.
Phase-resolved field-space distance criteria in ekpyrotic, bouncing and cyclic cosmologies Can the dark energy equation-of-state parameter w be less than -1?
Reference 61
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T22:25:06.983175Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 20834ce1-29b4-43b3-80d0-b478b59ec017 · inbound
Affine ANEC selects the closed FRW branch for geodesically complete cosmology cites this paper.
Affine ANEC selects the closed FRW branch for geodesically complete cosmology Can the dark energy equation-of-state parameter w be less than -1?
Reference 57
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T09:13:10.288839Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f102b51a-bf6f-4f9b-98b4-4bae7989d44f · inbound
The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data cites this paper.
The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data Can the dark energy equation-of-state parameter w be less than -1?
Reference 45
- Resolution
- verified exact
- local_arxiv, observed 2026-05-22T03:51:01.870866Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 6e49e6fe-ed15-4985-a38f-162c1eb48330 · inbound
Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes cites this paper.
Exploring the Dark Sector: Interacting Radiation in Light of Modern Cosmological Probes Can the dark energy equation-of-state parameter w be less than -1?
Reference 56
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T14:34:45.518238Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e097a597-e140-4ddd-9e05-7f23181bfc13 · 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 Can the dark energy equation-of-state parameter w be less than -1?
Reference 2
- 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 3c82d245-adde-44d4-b787-650eeb18def1 · 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 Can the dark energy equation-of-state parameter w be less than -1?
Reference 2
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T07:07:44.943167Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation fdbd7764-cf2c-46ef-9f7a-c4293ce48611 · inbound
The Coherence Principle: A Falsifiable Prior for Model Selection from the Grammar of Theories cites this paper.
The Coherence Principle: A Falsifiable Prior for Model Selection from the Grammar of Theories Can the dark energy equation-of-state parameter w be less than -1?
Reference 64
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T23:09:01.608279Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 18a043cb-0a75-491c-820d-aa466d0b8816 · inbound
Quintom Model Perturbations cites this paper.
Quintom Model Perturbations Can the dark energy equation-of-state parameter w be less than -1?
Reference 76
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T04:18:58.498356Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 44986121-dacf-4b63-9328-8b54c22ddb28 · inbound
Cosmological Evidence for Dark Axion-Dark Baryon Interactions from Apparent Phantom Crossing cites this paper.
Cosmological Evidence for Dark Axion-Dark Baryon Interactions from Apparent Phantom Crossing Can the dark energy equation-of-state parameter w be less than -1?
Reference 19
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T21:12:28.183431Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 25fcb681-29ce-4f92-ac19-8e5bb31151d2 · 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 Can the dark energy equation-of-state parameter w be less than -1?
Reference 110
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T16:30:06.280713Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f2c8d675-eab5-49a1-9acb-f69ec8e7f853 · inbound
The silent dark sector: a field-theory approach to unified dark fluids with vanishing speed of sound cites this paper.
The silent dark sector: a field-theory approach to unified dark fluids with vanishing speed of sound Can the dark energy equation-of-state parameter w be less than -1?
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T12:48:16.683174Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2cf7a4e2-8949-4b33-824e-272fc0ae9d13 · inbound
Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange cites this paper.
Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange Can the dark energy equation-of-state parameter w be less than -1?
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T15:41:43.181495Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e40d4c22-83e4-4355-96cc-8518514b304a · inbound
Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ cites this paper.
Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ Can the dark energy equation-of-state parameter w be less than -1?
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-07-31T11:14:46.951673Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.