Pith. sign in

Paper Citation Record · LEDGER

Matching current observational constraints with nonminimally coupled dark energy

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 52 inbound Pith citation observations for arXiv:2409.17019.

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

pith.paper-citation-record.v1
2409.17019 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 52 of 52 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 52 of 52 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:27:54.478011Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T18:27:31.668688Z

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 aecc7d57-a6bb-4c0c-ad43-0c56d27a84e5 · inbound

Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis cites this paper.

Upper limits on dark energy-dark matter interaction from DESI DR2 in a field-theoretic analysis Matching current observational constraints with nonminimally coupled dark energy

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-12T18:58:29.949083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T18:58:29.949083Z digest=sha256:77144b14b0e3bc8814ea0acfaca0afaafc2d98d591209ef1dc5735e30934103c

Observation 9e936993-89e2-4de1-9ba7-ebe9b5f8b9ba · inbound

Bridge the Cosmological Tensions with Thawing Gravity cites this paper.

Bridge the Cosmological Tensions with Thawing Gravity Matching current observational constraints with nonminimally coupled dark energy

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-12T18:17:21.561330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T18:17:21.561330Z digest=sha256:eb65235acb8bf33568ea7b56c50f8dd28ad95f644063d487b45ad3531448febb

Observation d14a1f9f-5567-4342-8877-c4cfacde321b · inbound

General parametrization for energy density of quintessence field cites this paper.

General parametrization for energy density of quintessence field Matching current observational constraints with nonminimally coupled dark energy

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-12T13:51:30.465549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T13:51:30.465549Z digest=sha256:ffc4a57af571cc7722137a547d5c5f80f5755fd17c770dbf68b972845d3e9207

Observation 0eb2b26c-1033-4a11-bc1b-d61dd9f1ad01 · inbound

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity cites this paper.

Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity Matching current observational constraints with nonminimally coupled dark energy

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-12T04:57:06.857958Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T04:57:06.857958Z digest=sha256:0f70ce7846f5e241f93e82a4847a2b5cf644feff9aa97d1f57a78694102a83cc

Observation ed1a930f-3f3f-4db0-9839-7893a69e5d2a · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Matching current observational constraints with nonminimally coupled dark energy

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-11T13:41:23.851637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:41:23.851637Z digest=sha256:a750e8ba3017a0bc146e96897a29d1d2a3a189684353f6d09e038495bcb12aca

Observation 5dd0d43c-56ab-42bb-8238-edb1ebe34bd7 · inbound

The Spectre of Underdetermination in Modern Cosmology cites this paper.

The Spectre of Underdetermination in Modern Cosmology Matching current observational constraints with nonminimally coupled dark energy

Reference 130

Resolution
unresolved
no resolver link, observed 2026-08-10T21:11:17.757010Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T21:11:17.757010Z digest=sha256:1463580a3bef09cb22760e0fa78e9d4e5272c814a4131fafe479f3771fc74022

Observation c55f429e-ff1e-44ab-a259-f4b89fbca49a · inbound

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Matching current observational constraints with nonminimally coupled dark energy

Reference 164

Resolution
unresolved
no resolver link, observed 2026-08-10T18:12:34.445170Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T18:12:34.445170Z digest=sha256:df3fc0d54942b50ce239262b3435dcd9ecbfcdfb677e2bde4183a441dff454b5

Observation 1bf91917-ff0e-4c57-9073-084a80fb2a59 · inbound

Cosmic distance duality after DESI 2024 data release and dark energy evolution cites this paper.

Cosmic distance duality after DESI 2024 data release and dark energy evolution Matching current observational constraints with nonminimally coupled dark energy

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-10T14:34:39.679326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:34:39.679326Z digest=sha256:4770b8c3eebac7af93c360f9e5235f95eead1450c3d0e88400210fc7a88b58f5

Observation 040638ee-55e3-43d6-a698-577ede672652 · inbound

Scalar-Tensor Gravity and DESI 2024 BAO data cites this paper.

Scalar-Tensor Gravity and DESI 2024 BAO data Matching current observational constraints with nonminimally coupled dark energy

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T14:29:27.554293Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:29:27.554293Z digest=sha256:037bcc2d5a38c93105bc4f7ce5cf161e999771abb19c7b656487391710b398a4

Observation 163373ea-d6a7-457d-9970-037b778e4857 · inbound

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.

The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Matching current observational constraints with nonminimally coupled dark energy

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-08T23:12:26.293360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T23:12:26.293360Z digest=sha256:3f557914f6a4dd5e9ad2f374744e21322b689bbf0d120b0dc52ca38a2a868b9c

Observation ffccd60f-d895-46b4-b70b-e07924daeb07 · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Matching current observational constraints with nonminimally coupled dark energy

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-08T22:04:59.501356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T22:04:59.501356Z digest=sha256:9ca2fd21ad388feb1fe89cb0d401efd2640d09301f3f36219b0011c4fc5bee74

Observation 0b2fcb52-0837-4b50-933b-0f82987ed827 · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Matching current observational constraints with nonminimally coupled dark energy

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-08T21:04:17.572305Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T21:04:17.572305Z digest=sha256:60a0bbee1d7ca1155b8e33a6453d524a23a61aab27387ab43f435ade69370150

Observation f9610b2a-7977-4080-b59d-af56f87ccba1 · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 234

Resolution
unresolved
no resolver link, observed 2026-08-07T18:51:44.155254Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T18:51:44.155254Z digest=sha256:dd68d8ce7ca3e5d0151cc74389a3617f0012e7978fcd489679a57d36ab2c2ea5

Observation 23452f1d-46ec-4404-83b2-ce2b12741ceb · inbound

DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints cites this paper.

DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints Matching current observational constraints with nonminimally coupled dark energy

Reference 139

Resolution
verified exact
arxiv_id, observed 2026-05-11T09:56:03.497555Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-11T09:56:01.601036Z digest=sha256:aab8ca1458aab9e75277536ef68a1ed917fc011cf261a50112dbe0effafc4a74

Observation 6d5c6448-8562-4215-b8f4-c4c140f20679 · inbound

Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.

Extended Dark Energy analysis using DESI DR2 BAO measurements Matching current observational constraints with nonminimally coupled dark energy

Reference 208

Resolution
verified exact
arxiv_id, observed 2026-05-14T21:04:03.317904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-14T21:04:02.994288Z digest=sha256:8be085f0a32b7ee20cb257f94ae520d5079ddaef7f08b072e0c4dc8692dca60b

Observation 866db58d-148e-4686-aa20-2194491ad797 · inbound

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition cites this paper.

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition Matching current observational constraints with nonminimally coupled dark energy

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-16T05:27:54.478011Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:27:54.478011Z digest=sha256:f2710aad49e3b6b6c7fb8ca867e64ed8606159877f3e97ed987af0ae367f7a7b

Observation d36c95a1-15ea-4a44-8fa8-03934af6cefa · inbound

On the tension between DESI DR2 BAO and CMB cites this paper.

On the tension between DESI DR2 BAO and CMB Matching current observational constraints with nonminimally coupled dark energy

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-16T01:06:27.824343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T01:06:27.824343Z digest=sha256:c6f45768eadaf1920fd9cb1356545a3b03f0de664015ece2b69b75789cdf12bf

Observation 1c0356da-abd7-4baa-8a96-45ca1b7cd604 · inbound

The matter with(in) CPL cites this paper.

The matter with(in) CPL Matching current observational constraints with nonminimally coupled dark energy

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-15T22:00:18.127447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T22:00:18.127447Z digest=sha256:3e6d85130d05167f27d9b62c160b4c6c2028926310dd3ce5098bf67090304c6a

Observation a70476c8-8b78-443c-8bf0-9163e2b4dcda · inbound

Examining Quintessence Models with DESI Data cites this paper.

Examining Quintessence Models with DESI Data Matching current observational constraints with nonminimally coupled dark energy

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-07T14:30:37.533728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:30:37.533728Z digest=sha256:423c95c16bf929969c7f0126434b97f3079fa6e24f6634ef301a8d05efd9f4fb

Observation cd000c6a-f2a4-48c8-b7f4-a144397e9f78 · inbound

The Quintom theory of dark energy after DESI DR2 cites this paper.

The Quintom theory of dark energy after DESI DR2 Matching current observational constraints with nonminimally coupled dark energy

Reference 114

Resolution
verified exact
arxiv_id, observed 2026-05-19T13:12:18.919592Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-19T13:08:20.192767Z digest=sha256:83a96ec1608c466c052d3a4930b6237e9acde17da38c006319994aa6268cc795

Observation a5a4a3d8-b003-4821-a14d-5ef8a8b0fa1a · inbound

About electroweak domain walls in Majoron models cites this paper.

About electroweak domain walls in Majoron models Matching current observational constraints with nonminimally coupled dark energy

Reference 172

Resolution
unresolved
no resolver link, observed 2026-08-07T11:21:39.789066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:21:39.789066Z digest=sha256:b595940d966e7ca4b9864548ccbfc1842364ca891b64ea46672cf87ba04591a2

Observation 8b617535-1f59-4686-8543-c0754501ac0c · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Matching current observational constraints with nonminimally coupled dark energy

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-07T10:52:56.303551Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T10:52:56.303551Z digest=sha256:1b10f388006aaab6bb5bacb1bf398d5e456c0ef06871902d23e6771693f6e42d

Observation ff2b95ea-187f-44d1-b461-11bf6bec386b · inbound

Implications for dark energy of cosmic transparency in light of DESI data cites this paper.

Implications for dark energy of cosmic transparency in light of DESI data Matching current observational constraints with nonminimally coupled dark energy

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-06T22:08:47.627480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:08:47.627480Z digest=sha256:1897579181cb1819c4f6bf148df5bf6f2f806b575faa098abb9184b0d035c6b9

Observation b36b888e-a1c3-4266-8aaf-42d5192bcf47 · inbound

Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.

Resolving the Planck-DESI tension by nonminimally coupled quintessence Matching current observational constraints with nonminimally coupled dark energy

Reference 36

Resolution
verified exact
arxiv_id, observed 2026-05-19T01:36:58.053556Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-19T01:35:36.430109Z digest=sha256:4d38a3425427cb5106f86a091cf0d9b177e5929f8f95271b9c0e8a89e3caf87a

Observation 1f0d7f8c-084a-4506-905c-ea53b8566c78 · inbound

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data cites this paper.

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data Matching current observational constraints with nonminimally coupled dark energy

Reference 25

Resolution
verified exact
arxiv_id, observed 2026-05-18T15:51:35.155856Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-18T15:46:46.916264Z digest=sha256:c42b2620aba512a991cce25ce2564bea677fb62c7322201a08508ae3a593f229

Observation 17b83479-894b-4da8-846a-e2738564c020 · inbound

Cosmological constraints on Galileon dark energy with broken shift symmetry cites this paper.

Cosmological constraints on Galileon dark energy with broken shift symmetry Matching current observational constraints with nonminimally coupled dark energy

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-15T15:54:50.959669Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T15:54:50.959669Z digest=sha256:bd9dc127ff407ceaaa6cc43d60221642775ad0f394a11b22377a24bc0570064e

Observation 736681ab-99df-40ae-839d-de975fbc4aca · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Matching current observational constraints with nonminimally coupled dark energy

Reference 34

Resolution
verified exact
arxiv_id, observed 2026-05-18T10:46:16.485377Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-18T10:45:16.985887Z digest=sha256:8f029c70786c8624ad8b459847151fd7e449df4b8e2e2fe16b61a4c7784c35ad

Observation dcfcac12-8c8f-42cf-afc0-0c735587b069 · inbound

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses Matching current observational constraints with nonminimally coupled dark energy

Reference 39

Resolution
verified exact
arxiv_id, observed 2026-05-17T04:19:00.955174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-17T04:15:18.730245Z digest=sha256:50743dd9825780b9ba251432290417af4e53ad847e0abac088facc4a8d071d0b

Observation d6035768-1661-41f5-a4fb-7a3d4e000525 · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Matching current observational constraints with nonminimally coupled dark energy

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-03T14:40:55.402925Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T14:40:55.402925Z digest=sha256:60d26c44104585282fa73e974fc1c2979f89d6c2e36db3c942dd17cd6947e3b9

Observation f98d2954-8f21-4ed4-8dff-60d7d0b7d956 · inbound

Realizing the phantom-divide crossing with vector and scalar fields cites this paper.

Realizing the phantom-divide crossing with vector and scalar fields Matching current observational constraints with nonminimally coupled dark energy

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-03T07:07:18.055664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T07:07:18.055664Z digest=sha256:5fe6a6bc6226fa5cff32e4453c0ae76a857064337bb5583a5f849bb237eb4e62

Observation f4930fcc-1658-4525-972b-e36da236f36d · inbound

Accelerated expansion of the universe purely driven by scalar field fluctuations cites this paper.

Accelerated expansion of the universe purely driven by scalar field fluctuations Matching current observational constraints with nonminimally coupled dark energy

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-03T01:24:41.027893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T01:24:41.027893Z digest=sha256:17017445b07a802fe0cd3d38979ae717048a7b8c15c33ede4d5eef023393e316

Observation ba11b156-89b6-48c3-9f12-55dc798fc9fb · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 203

Resolution
verified exact
arxiv_id, observed 2026-05-21T13:30:12.279656Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:68e581ec370ddd0788d128297b04ca4badc736896b47def4ae3fe5cc182c7727

Observation 6417aad3-5616-4aa6-bec1-42996a7866cd · inbound

Neutrino mass limits and decaying dark matter: background evolution versus perturbations cites this paper.

Neutrino mass limits and decaying dark matter: background evolution versus perturbations Matching current observational constraints with nonminimally coupled dark energy

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-02T19:14:25.229970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T19:14:25.229970Z digest=sha256:ac5f10bb89681c7a80e3f262b2f23ecaf32bde8c44afaf232ad34e3496c0d9ec

Observation be860628-cd05-4bc2-ac90-596b56e0b30d · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 203

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:dceab021cfa8b101636cbeb969e7d744bdf8644b7cacd24c67b6935cd7c22974

Observation 740d9314-b53c-4a22-a37d-db04ece34bd1 · inbound

Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy Matching current observational constraints with nonminimally coupled dark energy

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-05-11T08:06:00.548336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-10T16:49:15.994565Z digest=sha256:bda2cefb4b0a6a00c30ed0e9c780ae647d3f8673f815965c841e8be01c41ea13

Observation 9a13174f-5577-4b97-8850-f9930bf2721f · inbound

Post-Newtonian Constraints on Scalar-Tensor Gravity cites this paper.

Post-Newtonian Constraints on Scalar-Tensor Gravity Matching current observational constraints with nonminimally coupled dark energy

Reference 12

Resolution
verified exact
arxiv_id, observed 2026-05-10T07:47:12.051715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-10T07:46:58.535167Z digest=sha256:a26773a44d9a81e53f3f192e2f705f5589ab806ba7c04b0adfb539ec74e709d5

Observation 73af16ee-7adf-4461-b473-7b7912a6a722 · inbound

A Master Equation for Screening in Luminal Horndeski Gravity cites this paper.

A Master Equation for Screening in Luminal Horndeski Gravity Matching current observational constraints with nonminimally coupled dark energy

Reference 10

Resolution
verified exact
arxiv_id, observed 2026-05-09T06:10:40.410890Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-08T18:51:06.425840Z digest=sha256:9ce0798014012399ebec8e1ec4635516a6b64f5e50c749da6e2e7799c93d43a0

Observation 065c760b-9b5f-4b6d-80f3-d0522c6e5a95 · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-05-13T04:07:13.282064Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-13T04:04:08.752924Z digest=sha256:2cf2d728a8fadf33880a1ee7341f9641747f651c0eae135fe68c34968213a3df

Observation ee9816eb-cbf0-4aa0-9afe-fc8066f34e0f · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Matching current observational constraints with nonminimally coupled dark energy

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-22T05:41:08.740644Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-22T05:36:41.912431Z digest=sha256:769eeaf0098c6eb972736382f6e748d4f106290fdaaa3e761e06b91b56a6dd12

Observation 3763e071-2411-4cb4-bcd1-16833bb8bf16 · inbound

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background cites this paper.

Signatures of Modified Gravity on Linear Scales in a Dynamical Dark Energy Background Matching current observational constraints with nonminimally coupled dark energy

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-02T13:29:54.539031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T13:29:54.539031Z digest=sha256:115d67013042686e990a44dc86a331d72a8dc23ce1f7162c70a1877c13b04c63

Observation e93d71de-7741-4198-adc3-6a187231f904 · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-05-22T03:51:01.987889Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-05-22T03:48:48.036434Z digest=sha256:a99d5b23ac8030fc875f19117254e0bc1ba10cf208aed8865f5efdf159f5e7f8

Observation 6727afa6-d889-4187-9a8a-41d8f868a84f · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 60

Resolution
verified exact
arxiv_id, observed 2026-06-30T14:34:45.479879Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-30T14:32:13.675156Z digest=sha256:5dcff51d552e9083a57336c0051d5b1f97d07ec42c4ac3bad4be5f8ac8760f25

Observation 66fe3108-5af0-4c32-9090-72170e2730c4 · inbound

Charging Across the Phantom Divide with Modified Gravity cites this paper.

Charging Across the Phantom Divide with Modified Gravity Matching current observational constraints with nonminimally coupled dark energy

Reference 3

Resolution
verified exact
arxiv_id, observed 2026-06-29T22:54:01.754844Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-29T20:30:09.955685Z digest=sha256:4fe766d1c8b85b0182227c37ebe47de6e78f13b4d7d5958acc97e948a7b344c1

Observation 9c64d75f-2132-43f4-8134-ef4cefe4d341 · inbound

Matter influence on large-scale scalar dynamics cites this paper.

Matter influence on large-scale scalar dynamics Matching current observational constraints with nonminimally coupled dark energy

Reference 27

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:16:10.929095Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-28T21:32:02.397039Z digest=sha256:f40889c649750fcebdbac41913ff7a22244c7944b80af3a5b0ba7060db9c5cef

Observation 24fb9f01-ccc0-427c-a63d-cf883f1aa8da · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Matching current observational constraints with nonminimally coupled dark energy

Reference 49

Resolution
verified exact
arxiv_id, observed 2026-07-01T21:46:16.094985Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-06-28T16:17:39.285285Z digest=sha256:b127b701040d85a0b4ec98cf73e82f42921fcfb7cf92e76a07d9d35be1b3b72e

Observation cfeeeee7-558c-48f6-aa36-38359c01a643 · inbound

A short review on Quintom dark energy theory cites this paper.

A short review on Quintom dark energy theory Matching current observational constraints with nonminimally coupled dark energy

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-02T12:40:03.367984Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T12:40:03.367984Z digest=sha256:ffca04631ce92c982360c3ce342f1bf767e38386539e8530d1749e19b24ea274

Observation 9ed95943-ef58-49e9-b69f-657689a61e91 · inbound

Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Matching current observational constraints with nonminimally coupled dark energy

Reference 42

Resolution
verified exact
local_arxiv, observed 2026-07-08T15:55:05.063809Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-07-08T15:47:53.145943Z digest=sha256:c04ba08755362e0a5d1c54428b97147a33327a839d23e141ff362ba6f9e109af

Observation 3ae5cdfa-2d10-4a34-abad-e81f92885697 · inbound

The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Matching current observational constraints with nonminimally coupled dark energy

Reference 32

Resolution
verified exact
local_arxiv, observed 2026-07-10T18:27:31.669949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.

source=pdf_text observed=2026-07-10T18:19:17.740185Z digest=sha256:8e59b1be59a44238b2366b14a0652c702013a8422e4ad87b24ab5e759252a764

Observation 0cf9c860-2588-4479-ac5d-94a9bb46df74 · inbound

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction cites this paper.

Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction Matching current observational constraints with nonminimally coupled dark energy

Reference 49

Resolution
unresolved
no resolver link, observed 2026-07-14T03:00:21.146194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T03:00:21.146194Z digest=sha256:edc0e06edfe8ceef557b7192c50e8f453c17b3f47ac61a2dec368e6e5ef38e80

Observation 7093e2c7-b987-4fec-adac-d74919bdfb4e · inbound

Rolling Galileons: Evolving Braiding Strength for Viable Dark Energy cites this paper.

Rolling Galileons: Evolving Braiding Strength for Viable Dark Energy Matching current observational constraints with nonminimally coupled dark energy

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-01T21:09:41.987996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T21:09:41.987996Z digest=sha256:3edc51f361b9feab415025c61bb319261a4daa06231e089760e3b0406e5860f0

Observation 305882d4-e0d9-4490-af53-a10d70444aa6 · 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 Matching current observational constraints with nonminimally coupled dark energy

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-01T15:41:47.323890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T15:41:47.323890Z digest=sha256:90e005d8ee7848039338f1f6272c2987a7d4681c1f86b37d008bb6252be8cc75

Observation a8413c4c-74f1-4c3b-9c05-f8d004258a5a · inbound

N-body Simulations of Large-Scale Structure in the Generalized Cubic Covariant Galileon Model cites this paper.

N-body Simulations of Large-Scale Structure in the Generalized Cubic Covariant Galileon Model Matching current observational constraints with nonminimally coupled dark energy

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-15T14:38:14.226090Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-15T14:38:14.226090Z digest=sha256:1a05d63e8afc8d532e147e778e47857aa5c759d0e3652ca63ab881d8df6d8c98