Paper Citation Record · LEDGER

Robust Preference for Dark Sector Interactions

As of 12 August 2026, this Paper Citation Record lists 100 of 163 outbound references and 37 inbound Pith citation observations for arXiv:2601.07361.

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

pith.paper-citation-record.v1
2601.07361 v2

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measured 100 of 163 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-03T11:11:48.875018Z

measured 137 of 137 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 37 of 37 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T18:32:59.310242Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T11:59:51.269150Z

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100 of 163 outbound references displayed

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Outbound references

Observation 8bb3188a-9e1a-40eb-98e6-1a1ecada9d83 · outbound

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

Robust Preference for Dark Sector Interactions DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 1

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Observation 3812bb02-757e-40d1-942c-889613212c25 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Robust Preference for Dark Sector Interactions Accelerating Universes with Scaling Dark Matter

Reference 2

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Observation 33373cb1-6f4a-4855-9624-a4c55cbf5d1c · outbound

This paper cites Exploring the Expansion History of the Universe.

Robust Preference for Dark Sector Interactions Exploring the Expansion History of the Universe

Reference 3

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Observation 1678349d-fcbd-4c25-870a-4c4b15515aba · outbound

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

Robust Preference for Dark Sector Interactions Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 4

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Observation 5bdb1f2a-fa06-4071-8430-c67bfac7ff91 · outbound

This paper cites The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration.

Robust Preference for Dark Sector Interactions The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration

Reference 5

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Observation 2c609d8f-6961-4fd5-bcd9-b81432a8b946 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Robust Preference for Dark Sector Interactions DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 6

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Observation 1a396bbe-4af2-4c50-9da2-bbc9a9a5875f · outbound

This paper cites Guet al.(DESI), Nature Astron.9, 1879 (2025), arXiv:2504.06118 [astro-ph.CO].

Robust Preference for Dark Sector Interactions Guet al.(DESI), Nature Astron.9, 1879 (2025), arXiv:2504.06118 [astro-ph.CO]

Reference 7

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Observation e83e5362-998f-4557-a1d8-c77ddafde189 · outbound

This paper cites Interpreting DESI's evidence for evolving dark energy.

Robust Preference for Dark Sector Interactions Interpreting DESI's evidence for evolving dark energy

Reference 8

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Observation 9101f2cd-16d9-4197-8be0-9f94b9272f0e · outbound

This paper cites Assessing observational constraints on dark energy.

Robust Preference for Dark Sector Interactions Assessing observational constraints on dark energy

Reference 9

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Observation d779575b-50b0-4cf9-9ee0-bd7c2560830d · outbound

This paper cites Model independent cosmographic constraints from DESI 2024.

Robust Preference for Dark Sector Interactions Model independent cosmographic constraints from DESI 2024

Reference 10

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Observation 53664f9d-0097-4710-9b95-07d86e261326 · outbound

This paper cites Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?.

Robust Preference for Dark Sector Interactions Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

Reference 11

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Observation 2f741a6c-1d70-4e6f-8a2d-8cac530b8bab · outbound

This paper cites Dark energy in light of recent DESI BAO and Hubble tension.

Robust Preference for Dark Sector Interactions Dark energy in light of recent DESI BAO and Hubble tension

Reference 12

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Observation d4f7eac0-ce4e-452a-a908-c77562812e31 · outbound

This paper cites Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements.

Robust Preference for Dark Sector Interactions Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements

Reference 13

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Observation 4c65b49a-e7c8-4a3d-a25d-31d24633fa10 · outbound

This paper cites Quintessential interpretation of the evolving dark energy in light of DESI.

Robust Preference for Dark Sector Interactions Quintessential interpretation of the evolving dark energy in light of DESI

Reference 14

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Observation 3c1dd8b5-0ed1-4bfd-bc4c-3a829f52fc90 · outbound

This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.

Robust Preference for Dark Sector Interactions DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data

Reference 15

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Observation 3a5f9428-57f4-4156-a8d6-b38c11c6ec34 · outbound

This paper cites Cosmological constraints on curved quintessence.

Robust Preference for Dark Sector Interactions Cosmological constraints on curved quintessence

Reference 16

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Observation 826d4d74-b1ba-492d-80d7-c984b9307dd3 · outbound

This paper cites DESI Constraints on Exponential Quintessence.

Robust Preference for Dark Sector Interactions DESI Constraints on Exponential Quintessence

Reference 17

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Observation 8bf1b2fe-7922-4b50-bc59-74a09017557d · outbound

This paper cites Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology.

Robust Preference for Dark Sector Interactions Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology

Reference 18

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Observation 690ffada-9405-44c5-ad73-59a543801b8a · outbound

This paper cites Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements.

Robust Preference for Dark Sector Interactions Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements

Reference 19

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Observation d2ec724f-a3bb-476f-a3ab-94cfc9203640 · outbound

This paper cites Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO.

Robust Preference for Dark Sector Interactions Investigating Late-Time Dark Energy and Massive Neutrinos in Light of DESI Y1 BAO

Reference 20

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Observation a0ea6af6-caad-47e5-b35c-a79a534f2404 · outbound

This paper cites Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?.

Robust Preference for Dark Sector Interactions Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?

Reference 21

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Observation 90ccf01e-248f-4adf-aa30-6424f0dd6a2b · outbound

This paper cites Revisiting holographic dark energy after DESI 2024.

Robust Preference for Dark Sector Interactions Revisiting holographic dark energy after DESI 2024

Reference 22

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Observation 8030533c-43f5-40c7-885d-b105914669c0 · outbound

This paper cites Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data.

Robust Preference for Dark Sector Interactions Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

Reference 23

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Observation 567b6892-43ab-46b5-9d0f-f1c18415c357 · outbound

This paper cites Quintom cosmology and modified gravity after DESI 2024.

Robust Preference for Dark Sector Interactions Quintom cosmology and modified gravity after DESI 2024

Reference 24

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Observation 68879a64-704d-4fe4-a4fa-edada0b4b782 · outbound

This paper cites Li, G.-H.

Robust Preference for Dark Sector Interactions Li, G.-H

Reference 25

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Observation 90c866fb-dd57-43a4-b094-9a2dfb9588d4 · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Robust Preference for Dark Sector Interactions Assessing cosmological evidence for non-minimal coupling

Reference 26

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Observation a74e0ce1-c841-4723-aa15-c0c1c09bfa04 · outbound

This paper cites Scalar field dark energy models: Current and forecast constraints.

Robust Preference for Dark Sector Interactions Scalar field dark energy models: Current and forecast constraints

Reference 27

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Observation a673b713-e67a-42f1-97a7-63e45358868e · outbound

This paper cites An overview of what current data can (and cannot yet) say about evolving dark energy.

Robust Preference for Dark Sector Interactions An overview of what current data can (and cannot yet) say about evolving dark energy

Reference 28

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Observation 33a15bea-8def-40f6-9d6b-1272e4b5dcd0 · outbound

This paper cites Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO.

Robust Preference for Dark Sector Interactions Early time solution as an alternative to the late time evolving dark energy with DESI DR2 BAO

Reference 29

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Observation 6acbdcb8-47bd-4bc4-830a-a8b597657cb1 · outbound

This paper cites The Impact of the Hubble Tension on the Evidence for Dynamical Dark Energy.

Robust Preference for Dark Sector Interactions The Impact of the Hubble Tension on the Evidence for Dynamical Dark Energy

Reference 30

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Observation c171c57d-adeb-476c-9cd2-5f2518e21399 · outbound

This paper cites Roy Choudhury, Astrophys.

Robust Preference for Dark Sector Interactions Roy Choudhury, Astrophys

Reference 31

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Observation ff22d859-6c68-4e7d-8532-bb957290085d · outbound

This paper cites Paliathanasis, Phys.

Robust Preference for Dark Sector Interactions Paliathanasis, Phys

Reference 32

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Observation f2d4b4ad-2830-4ffb-ac7d-2a731793b87e · outbound

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

Robust Preference for Dark Sector Interactions Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

Reference 33

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Observation 34fb5d73-82af-418f-829e-7ca80375249b · outbound

This paper cites Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae.

Robust Preference for Dark Sector Interactions Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae

Reference 34

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Observation a8a66bb6-bea8-4c3b-9392-1b919bcf17ea · outbound

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Robust Preference for Dark Sector Interactions Unresolved cited work

Reference 35

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Observation 232d01c9-b72a-4a77-a963-3de28f261b64 · outbound

This paper cites Implications of distance duality violation for the $H_0$ tension and evolving dark energy.

Robust Preference for Dark Sector Interactions Implications of distance duality violation for the $H_0$ tension and evolving dark energy

Reference 36

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Observation 1fb16bee-4fd5-4cac-9c18-7b57fc45b8de · outbound

This paper cites Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data.

Robust Preference for Dark Sector Interactions Updated Constraints on Omnipotent Dark Energy: A Comprehensive Analysis with CMB and BAO Data

Reference 37

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Observation e70e1dba-64b9-425a-8f56-e35ccbb6ad0f · outbound

This paper cites Cheng, E.

Robust Preference for Dark Sector Interactions Cheng, E

Reference 38

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Observation 532f9086-ce21-4351-b3a9-f0d8e52ec2e6 · outbound

This paper cites Bayesian and frequentist perspectives agree on dynamical dark energy.

Robust Preference for Dark Sector Interactions Bayesian and frequentist perspectives agree on dynamical dark energy

Reference 39

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Observation 91cc90a0-06fd-4efb-b1e8-edac86e8bf4c · outbound

This paper cites Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing.

Robust Preference for Dark Sector Interactions Dark Energy Crosses the Line: Quantifying and Testing the Evidence for Phantom Crossing

Reference 40

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Observation 6f161763-1a13-4f69-97f5-97643df7bc66 · outbound

This paper cites Comparison of dynamical dark energy with {\Lambda}CDM in light of DESI DR2.

Robust Preference for Dark Sector Interactions Comparison of dynamical dark energy with {\Lambda}CDM in light of DESI DR2

Reference 41

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Observation ed93511e-a74a-46e9-983c-a41da9f428b3 · outbound

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Robust Preference for Dark Sector Interactions Silva and R

Reference 42

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Observation 48953c2a-29d6-4746-90bf-8ea3aa503a04 · outbound

This paper cites Ishak and L.

Robust Preference for Dark Sector Interactions Ishak and L

Reference 43

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Observation 49732f55-14e0-4d66-83da-47b7ade43de3 · outbound

This paper cites Fazzari, W.

Robust Preference for Dark Sector Interactions Fazzari, W

Reference 44

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This paper cites Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes.

Robust Preference for Dark Sector Interactions Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes

Reference 45

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Observation a14c2cbe-dcc3-4015-b869-cc31f9f09e89 · outbound

This paper cites Cosmic Strings as Dynamical Dark Energy: Novel Constraints.

Robust Preference for Dark Sector Interactions Cosmic Strings as Dynamical Dark Energy: Novel Constraints

Reference 46

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

Robust Preference for Dark Sector Interactions The Quintom theory of dark energy after DESI DR2

Reference 47

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This paper cites Song, G.-H.

Robust Preference for Dark Sector Interactions Song, G.-H

Reference 48

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Observation 63aac61d-b79d-4744-8cac-5ee1d21038e1 · outbound

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Robust Preference for Dark Sector Interactions Li and S

Reference 49

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Robust Preference for Dark Sector Interactions Unresolved cited work

Reference 50

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Observation ca177449-b273-4b9d-9f83-756e6487cfb2 · outbound

This paper cites Wu, T.-N.

Robust Preference for Dark Sector Interactions Wu, T.-N

Reference 51

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Observation d9214f80-ed16-47d2-bd89-182d198eb529 · outbound

This paper cites A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations.

Robust Preference for Dark Sector Interactions A New Window on Dynamical Dark Energy: Combining DESI-DR2 BAO with future Gravitational Wave Observations

Reference 52

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Observation e013b5ef-c466-4300-bac7-1b59c25ba0a0 · outbound

This paper cites Khoury, M.-X.

Robust Preference for Dark Sector Interactions Khoury, M.-X

Reference 53

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Observation f8de92fe-2cf8-458c-9d2d-3cc57a19966d · outbound

This paper cites Li and X.

Robust Preference for Dark Sector Interactions Li and X

Reference 54

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Observation 54768c51-f495-4f51-a7de-21955e880e2f · outbound

This paper cites One-parameter dynamical dark energy: Hints for oscillations.

Robust Preference for Dark Sector Interactions One-parameter dynamical dark energy: Hints for oscillations

Reference 55

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Observation e68676eb-abbc-4733-8283-9fbd82697d5f · outbound

This paper cites Smith, E.

Robust Preference for Dark Sector Interactions Smith, E

Reference 56

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Robust Preference for Dark Sector Interactions Coupled Quintessence

Reference 57

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Observation 112cadfb-3988-42b0-8d18-880e9b0e644c · outbound

This paper cites Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures.

Robust Preference for Dark Sector Interactions Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures

Reference 58

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Observation 1bd2d17e-c0e0-4137-b45e-4e3a93a7269b · outbound

This paper cites Disformal invariance of second order tensor-scalar theories: framing the Horndeski action.

Robust Preference for Dark Sector Interactions Disformal invariance of second order tensor-scalar theories: framing the Horndeski action

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.775359Z

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Observation c20dc520-4c8c-494a-98c6-cded8c4bb7f0 · outbound

This paper cites Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian.

Robust Preference for Dark Sector Interactions Transforming gravity: from derivative couplings to matter to second-order scalar-tensor theories beyond the Horndeski Lagrangian

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Observation e82fc87a-96f2-49d6-acc4-83febcca5535 · outbound

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Robust Preference for Dark Sector Interactions The Effective Field Theory of Dark Energy

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.780451Z

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Robust Preference for Dark Sector Interactions Effective Field Theory of Dark Energy: a Review

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.782868Z

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Robust Preference for Dark Sector Interactions Further understanding the interaction between dark energy and dark matter: current status and future directions

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.785247Z

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Robust Preference for Dark Sector Interactions Statefinder diagnosis for the interacting model of holographic dark energy

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.787660Z

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.790181Z

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Robust Preference for Dark Sector Interactions Testing models of vacuum energy interacting with cold dark matter

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.792547Z

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Robust Preference for Dark Sector Interactions Constraints on the Coupling between Dark Energy and Dark Matter from CMB data

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.795360Z

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Robust Preference for Dark Sector Interactions Echo of interactions in the dark sector

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.797676Z

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Robust Preference for Dark Sector Interactions Can interacting dark energy solve the $H_0$ tension?

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.800342Z

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Observation 8375c46b-4f52-4938-94a0-d375d6b28af1 · outbound

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Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.802680Z

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Robust Preference for Dark Sector Interactions Relieving the $H_0$ tension with a new interacting dark energy model

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.805079Z

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Observation d3e731ab-8677-49b8-9209-3fe8b5f39565 · outbound

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Robust Preference for Dark Sector Interactions On the interacting dark energy scenarios $-$ the case for Hubble constant tension

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Resolution: malformed identifier; no resolver link, observed 2026-08-03T11:11:48.807359Z

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Observation 3c5adb0a-a66d-4f08-a26b-25d80763cf98 · outbound

This paper cites A double take on early and interacting dark energy from JWST.

Robust Preference for Dark Sector Interactions A double take on early and interacting dark energy from JWST

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.809741Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions Reconciling CMB and structure growth measurements with dark energy interactions

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.812128Z

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Robust Preference for Dark Sector Interactions Dark sector interaction and the supernova absolute magnitude tension

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.814655Z

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This paper cites Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars.

Robust Preference for Dark Sector Interactions Constraints on interacting dark energy models from time-delay cosmography with seven lensed quasars

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Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.817365Z

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Observation 02629d67-b167-40d8-a1c9-4a935b815d35 · outbound

This paper cites Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions.

Robust Preference for Dark Sector Interactions Tensions in the dark: shedding light on Dark Matter-Dark Energy interactions

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.819919Z

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Unavailable: canonical work link unavailable.

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This paper cites A Consistent View of Interacting Dark Energy from Multiple CMB Probes.

Robust Preference for Dark Sector Interactions A Consistent View of Interacting Dark Energy from Multiple CMB Probes

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.822435Z

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Unavailable: canonical work link unavailable.

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This paper cites Cosmological constraints on multi-interacting dark matter.

Robust Preference for Dark Sector Interactions Cosmological constraints on multi-interacting dark matter

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.825052Z

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This paper cites Constraints on interacting dark energy revisited: implications for the Hubble tension.

Robust Preference for Dark Sector Interactions Constraints on interacting dark energy revisited: implications for the Hubble tension

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.827436Z

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This paper cites Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state.

Robust Preference for Dark Sector Interactions Tightening the reins on non-minimal dark sector physics: Interacting Dark Energy with dynamical and non-dynamical equation of state

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.829729Z

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Robust Preference for Dark Sector Interactions Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.832078Z

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Robust Preference for Dark Sector Interactions Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.834554Z

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Robust Preference for Dark Sector Interactions Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.836853Z

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This paper cites Phase space analysis of sign-shifting interacting dark energy models.

Robust Preference for Dark Sector Interactions Phase space analysis of sign-shifting interacting dark energy models

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.839182Z

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Unavailable: canonical work link unavailable.

Observation d908af72-de34-4673-a8a7-b2c5673e6ae3 · outbound

This paper cites Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy.

Robust Preference for Dark Sector Interactions Gravitational Redshift Constraints on the Effective Theory of Interacting Dark Energy

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.841485Z

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Robust Preference for Dark Sector Interactions Can interacting dark energy with dynamical coupling resolve the Hubble tension

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.843808Z

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Observation 1c7c0c6e-fceb-4a7e-b771-1317b68ea4c3 · outbound

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Robust Preference for Dark Sector Interactions Prospects for probing the interaction between dark energy and dark matter using gravitational-wave dark sirens with neutron star tidal deformation

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.846121Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions Cosmological implications of an interacting model of dark matter \& dark energy

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.848552Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions New constraints on interacting dark energy from cosmic chronometers

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.850888Z

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Robust Preference for Dark Sector Interactions New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.853317Z

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Robust Preference for Dark Sector Interactions van der Westhuizen, A

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.855867Z

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Robust Preference for Dark Sector Interactions Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.858167Z

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Robust Preference for Dark Sector Interactions Resolving the Planck-DESI tension by nonminimally coupled quintessence

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.860361Z

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Robust Preference for Dark Sector Interactions Li, G.-H

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.863035Z

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Unavailable: canonical work link unavailable.

Observation 04a99f66-0173-49f5-8114-9f08e87e962b · outbound

This paper cites Li, G.-H.

Robust Preference for Dark Sector Interactions Li, G.-H

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.865164Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions Constraining interacting dark energy models with black hole superradiance

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.867389Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.869917Z

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Unavailable: canonical work link unavailable.

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Robust Preference for Dark Sector Interactions Unresolved cited work

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.872936Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c5ebd60-a5a3-4318-8891-579aad5f1de8 · outbound

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Robust Preference for Dark Sector Interactions Unresolved cited work

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.875018Z

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Unavailable: canonical work link unavailable.

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Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-06T15:12:35.152374Z

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Unavailable: canonical work link unavailable.

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Unavailable: canonical work link unavailable.

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Reference 110

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Reference 66

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

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Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9d60288c-9568-4aa0-9b0b-953948a32ef0 · 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 Robust Preference for Dark Sector Interactions

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-02T13:29:58.863005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ada2c23-9311-4dae-bed2-38ad03e3affb · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Robust Preference for Dark Sector Interactions

Reference 206

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 5885aa1a-970b-4655-8566-956d88b11783 · inbound

Dissipative Dark Energy can explain the DESI phantom crossing cites this paper.

Dissipative Dark Energy can explain the DESI phantom crossing Robust Preference for Dark Sector Interactions

Reference 46

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation a237f955-2699-4140-8c48-37897860672a · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Robust Preference for Dark Sector Interactions

Reference 155

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 35a60938-cad0-4146-854b-6aa4faa8242e · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Robust Preference for Dark Sector Interactions

Reference 80

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation e3669387-f957-47f0-b2f7-333f07de181a · inbound

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.

Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Robust Preference for Dark Sector Interactions

Reference 96

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation af720a9a-c5d8-40eb-90ba-85b1b5387bc3 · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Robust Preference for Dark Sector Interactions

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation cd9a7635-3fba-4d7b-bc69-01f8f17465ca · inbound

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions cites this paper.

Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\Lambda$CDM Interpretations, and Tensions Robust Preference for Dark Sector Interactions

Reference 200

Resolution: unresolved; no resolver link, observed 2026-08-02T10:41:42.491805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3569e51-d7d3-4599-8af6-00502e54480f · inbound

Phantom-Divide Crossing in Exponentially Coupled Quintessence and the Role of Neutrino-Mass Freedom cites this paper.

Phantom-Divide Crossing in Exponentially Coupled Quintessence and the Role of Neutrino-Mass Freedom Robust Preference for Dark Sector Interactions

Reference 21

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 2bbd8aed-3e60-4e38-8dc4-d066766bcb45 · inbound

Unifying the Dark Sector with the New Generalized Chaplygin Gas: Observational Constraints cites this paper.

Unifying the Dark Sector with the New Generalized Chaplygin Gas: Observational Constraints Robust Preference for Dark Sector Interactions

Reference 85

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 2df89882-58c6-4401-a7a8-97aa47909efb · inbound

HIcosmo: a differentiable JAX-based framework for cosmology inference cites this paper.

HIcosmo: a differentiable JAX-based framework for cosmology inference Robust Preference for Dark Sector Interactions

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 11aca50c-2d85-47f1-b949-94de792d8d9b · inbound

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

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Robust Preference for Dark Sector Interactions

Reference 179

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 503624ea-e194-402c-aec9-cace22c718c7 · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Robust Preference for Dark Sector Interactions

Reference 231

Resolution: verified exact; arxiv_id, observed 2026-07-16T02:21:44.515574Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 714e1c5a-4fdc-46b8-b50b-aa93571c8aaa · 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 Robust Preference for Dark Sector Interactions

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T21:12:29.974831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b81ceed9-fe85-449d-b10c-eddba20e1165 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Robust Preference for Dark Sector Interactions

Reference 171

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:50.644894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97154877-9237-4ae7-8717-803a93be4ef1 · inbound

$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide cites this paper.

$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide Robust Preference for Dark Sector Interactions

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-01T00:51:55.821453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c0d3e97a-9299-49fc-9d8d-ba386c070ecb · inbound

$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide cites this paper.

$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide Robust Preference for Dark Sector Interactions

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T01:33:36.773607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 62188cfe-7775-42a8-98f5-74926210e078 · inbound

Coupled quintessence from an axion dark sector cites this paper.

Coupled quintessence from an axion dark sector Robust Preference for Dark Sector Interactions

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-06T11:18:55.326928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1987b343-c374-4ea7-992f-2c1476966e1d · inbound

Observational constraints on fractional holographic dark energy in the light of DESI DR2 cites this paper.

Observational constraints on fractional holographic dark energy in the light of DESI DR2 Robust Preference for Dark Sector Interactions

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T18:32:59.310242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.