Probing the independence within the dark sector in the fluid approximation | Paper Citation Record

Observation 3106de42-9096-42b4-b8d7-8fb019c7a005 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Probing the independence within the dark sector in the fluid approximation Planck 2018 results. VI. Cosmological parameters

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.661916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edde2e31-3ac6-4e10-9b62-83a53da977f1 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant.

Probing the independence within the dark sector in the fluid approximation Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.669173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9577bd13-fa28-490a-bab9-e47e3bf42024 · outbound

This paper cites Measurements of Omega and Lambda from 42 High-Redshift Supernovae.

Probing the independence within the dark sector in the fluid approximation Measurements of Omega and Lambda from 42 High-Redshift Supernovae

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.675328Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fab8267d-c396-4aff-ac89-82d11d2209b3 · outbound

This paper cites What is dust? - Physical foundations of the averaging problem in cosmology.

Probing the independence within the dark sector in the fluid approximation What is dust? - Physical foundations of the averaging problem in cosmology

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.682888Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74c128f5-c3eb-4b20-910d-357561e98a8b · outbound

This paper cites Large-Scale Galaxy Bias.

Probing the independence within the dark sector in the fluid approximation Large-Scale Galaxy Bias

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.689959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eceb007f-b9c5-41b2-9e76-da02eb90429f · outbound

This paper cites Cosmological Evolution With Interaction Between Dark Energy And Dark Matter.

Probing the independence within the dark sector in the fluid approximation Cosmological Evolution With Interaction Between Dark Energy And Dark Matter

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.697441Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 953c234c-19b7-4960-a6d6-ff5430b2cfb1 · outbound

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

Probing the independence within the dark sector in the fluid approximation Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.704471Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 500e2e96-61aa-441e-9643-2791eb460c6d · outbound

This paper cites Dynamics of dark energy.

Probing the independence within the dark sector in the fluid approximation Dynamics of dark energy

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.712911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0339ac8a-02e7-4d0a-9361-71d1e680750c · outbound

This paper cites Coupled Quintessence.

Probing the independence within the dark sector in the fluid approximation Coupled Quintessence

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.720852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6ca2dbb-5580-4128-bcb8-e5f8ccc80593 · outbound

This paper cites Interacting quintessence solution to the coincidence problem.

Probing the independence within the dark sector in the fluid approximation Interacting quintessence solution to the coincidence problem

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.727604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2855b2e3-bbb8-4063-9ac9-ee4fe7886f85 · outbound

This paper cites Interacting Quintessence.

Probing the independence within the dark sector in the fluid approximation Interacting Quintessence

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.734557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 51938058-76c7-4faa-90ed-18b6299a54e3 · outbound

This paper cites Interacting Dark Matter and Dark Energy.

Probing the independence within the dark sector in the fluid approximation Interacting Dark Matter and Dark Energy

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.742259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef43ca48-8422-4c13-baf3-9b6d040aae19 · outbound

This paper cites Tracking and coupled dark energy as seen by WMAP.

Probing the independence within the dark sector in the fluid approximation Tracking and coupled dark energy as seen by WMAP

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.748933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05916fa0-b11b-4bbc-a52e-fd6ca3593b90 · outbound

This paper cites The end of unified dark matter?.

Probing the independence within the dark sector in the fluid approximation The end of unified dark matter?

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.755111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ba3833a4-59ec-4867-8e39-117f5d794af9 · outbound

This paper cites The Revival of the Unified Dark Energy-Dark Matter Model ?.

Probing the independence within the dark sector in the fluid approximation The Revival of the Unified Dark Energy-Dark Matter Model ?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.762516Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf8d9fd6-b5fe-4967-8119-ab8109240ebb · outbound

This paper cites Cosmologies with Energy Exchange.

Probing the independence within the dark sector in the fluid approximation Cosmologies with Energy Exchange

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.768033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e50082e5-b90f-41f9-b5f5-445ab3692008 · outbound

This paper cites Probing the Coupling between Dark Components of the Universe.

Probing the independence within the dark sector in the fluid approximation Probing the Coupling between Dark Components of the Universe

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.775034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b25a2aab-18b5-4a88-9ab9-a7e687f3299f · outbound

This paper cites Large-scale instability in interacting dark energy and dark matter fluids.

Probing the independence within the dark sector in the fluid approximation Large-scale instability in interacting dark energy and dark matter fluids

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.785513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9b34f58e-cedc-4180-9430-24913cb06c24 · outbound

This paper cites Interacting models may be key to solve the cosmic coincidence problem.

Probing the independence within the dark sector in the fluid approximation Interacting models may be key to solve the cosmic coincidence problem

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.794489Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9cc9c4c5-8960-43d2-98ef-55447913e0ab · outbound

This paper cites The Growth of Structure in Interacting Dark Energy Models.

Probing the independence within the dark sector in the fluid approximation The Growth of Structure in Interacting Dark Energy Models

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.811528Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e6e91da-e5a3-4579-80a6-512b51ad2951 · outbound

This paper cites Adiabatic initial conditions for perturbations in interacting dark energy models.

Probing the independence within the dark sector in the fluid approximation Adiabatic initial conditions for perturbations in interacting dark energy models

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.817078Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e733f98-f70c-480c-91d6-6e3b1ff482f1 · outbound

This paper cites Observational constraints on an interacting dark energy model.

Probing the independence within the dark sector in the fluid approximation Observational constraints on an interacting dark energy model

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.822537Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6506a3d9-27ac-4403-9638-47a103110392 · outbound

This paper cites Dynamics of dark energy with a coupling to dark matter.

Probing the independence within the dark sector in the fluid approximation Dynamics of dark energy with a coupling to dark matter

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.829093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb7d0129-2e48-493a-9592-92765a058809 · outbound

This paper cites Inhomogeneous vacuum energy.

Probing the independence within the dark sector in the fluid approximation Inhomogeneous vacuum energy

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:38.825694Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 3529d7ac-2be8-474b-ba59-e3bbc083d027 · outbound

This paper cites Cosmological constraints on a decomposed Chaplygin gas.

Probing the independence within the dark sector in the fluid approximation Cosmological constraints on a decomposed Chaplygin gas

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.848669Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ca2e204-5b41-4250-84cb-e461d13043e7 · outbound

This paper cites Post-$Planck$ constraints on interacting vacuum energy.

Probing the independence within the dark sector in the fluid approximation Post-$Planck$ constraints on interacting vacuum energy

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.855668Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 652c1a4b-c6d3-4753-ac7c-c563df2e2bb7 · outbound

This paper cites Indications of a late-time interaction in the dark sector.

Probing the independence within the dark sector in the fluid approximation Indications of a late-time interaction in the dark sector

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.862191Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 822d024c-f07d-4526-b55a-0ce131d0dcff · outbound

This paper cites Reconstruction of the dark matter-vacuum energy interaction.

Probing the independence within the dark sector in the fluid approximation Reconstruction of the dark matter-vacuum energy interaction

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.868693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6a95883-84fc-42fa-9b3b-ec0e9d67d0fe · outbound

This paper cites New constraints on interacting dark energy from cosmic chronometers.

Probing the independence within the dark sector in the fluid approximation New constraints on interacting dark energy from cosmic chronometers

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.877189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6b01312-a7e3-4e4d-9e0d-1f0892c8f190 · outbound

This paper cites Echo of interactions in the dark sector.

Probing the independence within the dark sector in the fluid approximation Echo of interactions in the dark sector

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.886038Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bed288b8-88bb-48d5-9837-b78cd9368c78 · outbound

This paper cites Can interacting dark energy solve the $H_0$ tension?.

Probing the independence within the dark sector in the fluid approximation Can interacting dark energy solve the $H_0$ tension?

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.893153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 02101e1c-db90-465c-a557-98110dc1ea9e · outbound

This paper cites Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension.

Probing the independence within the dark sector in the fluid approximation Tale of stable interacting dark energy, observational signatures, and the $H_0$ tension

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.899279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e13c27ed-b048-47bd-b102-eec576d999e9 · outbound

This paper cites Dark sectors with dynamical coupling.

Probing the independence within the dark sector in the fluid approximation Dark sectors with dynamical coupling

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.908468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f25e073-18e5-4a30-a2b7-b18770efabcb · outbound

This paper cites Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension.

Probing the independence within the dark sector in the fluid approximation Interacting scenarios with dynamical dark energy: observational constraints and alleviation of the $H_0$ tension

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.915302Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cbf8dabb-b646-4bf8-80fd-e54cd8e9cc1b · outbound

This paper cites A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models.

Probing the independence within the dark sector in the fluid approximation A Fully Self-Consistent Cosmological Simulation Pipeline for Interacting Dark Energy Models

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:38.515374Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 30a97656-4e93-4dbf-835f-563e56f791ae · outbound

This paper cites The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models.

Probing the independence within the dark sector in the fluid approximation The first constraint from SDSS galaxy-galaxy weak lensing measurements on interacting dark energy models

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.932080Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f2d5a39-76f7-4224-b0de-e6b3fe2d8f62 · outbound

This paper cites The dark degeneracy: On the number and nature of dark components.

Probing the independence within the dark sector in the fluid approximation The dark degeneracy: On the number and nature of dark components

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.941250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00f6999c-d5f7-402c-8332-644b97d8cb48 · outbound

This paper cites Late universe decaying dark matter can relieve the H_0 tension.

Probing the independence within the dark sector in the fluid approximation Late universe decaying dark matter can relieve the H_0 tension

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.946813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1289768a-e663-41d3-86b3-de2c016d8f54 · outbound

This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.

Probing the independence within the dark sector in the fluid approximation Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.954306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3496016-78f9-4f4c-a9e6-7532f215caf7 · outbound

This paper cites Two Windows on Acceleration and Gravitation: Dark Energy or New Gravity?.

Probing the independence within the dark sector in the fluid approximation Two Windows on Acceleration and Gravitation: Dark Energy or New Gravity?

Reference 40

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:38.387051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 9f49f981-bfe6-4c9f-ac0b-bc85dba0ed00 · outbound

This paper cites Probing Cosmic Acceleration Beyond the Equation of State: Distinguishing between Dark Energy and Modified Gravity Models.

Probing the independence within the dark sector in the fluid approximation Probing Cosmic Acceleration Beyond the Equation of State: Distinguishing between Dark Energy and Modified Gravity Models

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.972815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29e2579f-2baa-4c36-b54c-5f7b02359375 · outbound

This paper cites A Consistency Relation in Cosmology.

Probing the independence within the dark sector in the fluid approximation A Consistency Relation in Cosmology

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:38.333607Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 0bf46600-f225-431d-8dfd-155ee4b76ad9 · outbound

This paper cites The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant.

Probing the independence within the dark sector in the fluid approximation The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.987370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 88f68290-9711-402c-9e2e-7efff3cf0ac6 · outbound

This paper cites The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15.

Probing the independence within the dark sector in the fluid approximation The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:35.995822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc57ce83-55a7-4d9a-8715-9f61fb235b48 · outbound

This paper cites The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12.

Probing the independence within the dark sector in the fluid approximation The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the correlation function of LOWZ and CMASS galaxies in Data Release 12

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.005271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 932e63df-6fad-4c67-99d0-4dd6ccae811e · outbound

This paper cites A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey.

Probing the independence within the dark sector in the fluid approximation A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - I : Methods and Application to the Sloan Digital Sky Survey

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.012348Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a723d352-ef54-402c-9f8b-50226b32b6f7 · outbound

This paper cites The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations.

Probing the independence within the dark sector in the fluid approximation The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.019243Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc4f3607-fa26-4d07-a851-e1a6749afc78 · outbound

This paper cites Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples.

Probing the independence within the dark sector in the fluid approximation Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.026384Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a300c08-a4b4-476f-bbc0-034ee5197ef3 · outbound

This paper cites The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample.

Probing the independence within the dark sector in the fluid approximation The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.033653Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5fa4ac0-d4b1-4a8a-8677-c4a4c9bb4069 · outbound

This paper cites an unresolved cited work.

Probing the independence within the dark sector in the fluid approximation Unresolved cited work

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.040278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e28430c1-205d-49e8-982f-a58b0ed75f86 · outbound

This paper cites The Reddening-Free Decline Rate Versus Luminosity Relationship for Type Ia Supernovae.

Probing the independence within the dark sector in the fluid approximation The Reddening-Free Decline Rate Versus Luminosity Relationship for Type Ia Supernovae

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.046869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b26feb97-3e89-4ca7-813f-a966cebf2b5d · outbound

This paper cites SALT2: using distant supernovae to improve the use of Type Ia supernovae as distance indicators.

Probing the independence within the dark sector in the fluid approximation SALT2: using distant supernovae to improve the use of Type Ia supernovae as distance indicators

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.054535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 58b09ae9-f61d-49c6-8a7e-458bf10ff3b7 · outbound

This paper cites Improved constraints on cosmological parameters from SNIa data.

Probing the independence within the dark sector in the fluid approximation Improved constraints on cosmological parameters from SNIa data

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.063008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5db1a873-23cd-41fe-b76d-55047e1a0726 · outbound

This paper cites Gelman, J.

Probing the independence within the dark sector in the fluid approximation Gelman, J

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.070347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0228f6d-2393-4d0c-8303-0a96800c27a0 · outbound

This paper cites Gull, in J.

Probing the independence within the dark sector in the fluid approximation Gull, in J

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.079567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71410eb0-99ca-45fd-a136-d90d743edabf · outbound

This paper cites Model-independent cosmological constraints from the CMB.

Probing the independence within the dark sector in the fluid approximation Model-independent cosmological constraints from the CMB

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.086297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fec3aebd-6c62-4643-907e-9b23f014a58e · outbound

This paper cites Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies.

Probing the independence within the dark sector in the fluid approximation Efficient Cosmological Parameter Estimation from Microwave Background Anisotropies

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.095163Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e84b74ce-f4d3-4562-b0d7-5fc7fa04f711 · outbound

This paper cites Observational Constraints on Dark Energy and Cosmic Curvature.

Probing the independence within the dark sector in the fluid approximation Observational Constraints on Dark Energy and Cosmic Curvature

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.125702Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8d72777-b0e4-4bcd-9081-34199f289b57 · outbound

This paper cites Planck priors for dark energy surveys.

Probing the independence within the dark sector in the fluid approximation Planck priors for dark energy surveys

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.133657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8518abba-564f-40df-bc6d-b22a053b8405 · outbound

This paper cites Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies.

Probing the independence within the dark sector in the fluid approximation Cosmic Confusion: Degeneracies among Cosmological Parameters Derived from Measurements of Microwave Background Anisotropies

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.140062Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c8a0946-642e-4e4c-9b63-b3f4fdac79d4 · outbound

This paper cites Planck 2015 results. XIV. Dark energy and modified gravity.

Probing the independence within the dark sector in the fluid approximation Planck 2015 results. XIV. Dark energy and modified gravity

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.149672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0b04b38-8864-4520-a0f9-16b3b7012bca · outbound

This paper cites Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers.

Probing the independence within the dark sector in the fluid approximation Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.157358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e9ad176-bc58-4381-8f06-3ce144dd6edf · outbound

This paper cites New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75.

Probing the independence within the dark sector in the fluid approximation New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.166579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d2fbddb-ff46-4eb0-a200-f1b6c8dc8eca · outbound

This paper cites Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2.

Probing the independence within the dark sector in the fluid approximation Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.173070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e0648f1-41e4-4093-a693-8a5d42015549 · outbound

This paper cites A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration.

Probing the independence within the dark sector in the fluid approximation A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.180082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1251008d-9191-4ec2-a8a7-19657ec45d9f · outbound

This paper cites Investigating dark energy experiments with principal components.

Probing the independence within the dark sector in the fluid approximation Investigating dark energy experiments with principal components

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.187596Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9c08426-09e3-4297-ad4b-24f0660435ee · outbound

This paper cites Fables of reconstruction: controlling bias in the dark energy equation of state.

Probing the independence within the dark sector in the fluid approximation Fables of reconstruction: controlling bias in the dark energy equation of state

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.194311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80375a90-3f45-41c5-b627-94d314893a18 · outbound

This paper cites Examining the evidence for dynamical dark energy.

Probing the independence within the dark sector in the fluid approximation Examining the evidence for dynamical dark energy

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.201554Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b1ef98aa-782d-4085-b2f0-2fd2b383b8a1 · outbound

This paper cites Dynamical dark energy in light of the latest observations.

Probing the independence within the dark sector in the fluid approximation Dynamical dark energy in light of the latest observations

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.209387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db62ba6c-5524-4d27-887d-f14c3c40f257 · outbound

This paper cites Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities.

Probing the independence within the dark sector in the fluid approximation Testing $\Lambda$CDM at the lowest redshifts with SN Ia and galaxy velocities

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.215072Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a12336c5-9249-486e-b84f-0a725bb78437 · outbound

This paper cites The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8.

Probing the independence within the dark sector in the fluid approximation The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.221622Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a41f1c2-a8d3-4c53-bef7-873fd477109f · outbound

This paper cites The Clustering of the SDSS Main Galaxy Sample II: Mock galaxy catalogues and a measurement of the growth of structure from Redshift Space Distortions at $z=0.15$.

Probing the independence within the dark sector in the fluid approximation The Clustering of the SDSS Main Galaxy Sample II: Mock galaxy catalogues and a measurement of the growth of structure from Redshift Space Distortions at $z=0.15$

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.228026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fb1cc590-97d4-439f-afca-2ea2cec027bf · outbound

This paper cites Simultaneous constraints on the growth of structure and cosmic expansion from the multipole power spectra of the SDSS DR7 LRG sample.

Probing the independence within the dark sector in the fluid approximation Simultaneous constraints on the growth of structure and cosmic expansion from the multipole power spectra of the SDSS DR7 LRG sample

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.233831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1e6b6ec-73bd-4fa8-b49f-cbf3127c97fc · outbound

This paper cites Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure.

Probing the independence within the dark sector in the fluid approximation Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.239960Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad225ea3-1f15-417c-8e02-c90a09f13a97 · outbound

This paper cites The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.

Probing the independence within the dark sector in the fluid approximation The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.246631Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d03a1d4f-0a16-4802-a62b-65201f1ca923 · outbound

This paper cites The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1.

Probing the independence within the dark sector in the fluid approximation The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.256237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5511b93-7203-48b2-9164-fd79b244ff70 · outbound

This paper cites The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample.

Probing the independence within the dark sector in the fluid approximation The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.262839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6d9bf969-3897-46fe-91fe-8a5b8939ec6d · outbound

This paper cites The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$.

Probing the independence within the dark sector in the fluid approximation The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at $z\sim 1.4$

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.273189Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f702074-3955-43d2-9772-3df1ee616b7f · outbound

This paper cites The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2.

Probing the independence within the dark sector in the fluid approximation The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.288640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7d88002-c474-4c58-9ec9-4c5eaacfa36c · outbound

This paper cites Parameterization of Dark-Energy Properties: a Principal-Component Approach.

Probing the independence within the dark sector in the fluid approximation Parameterization of Dark-Energy Properties: a Principal-Component Approach

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.298825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6c93c7d-fa48-4497-95b7-6772da948484 · outbound

This paper cites Uncorrelated Estimates of Dark Energy Evolution.

Probing the independence within the dark sector in the fluid approximation Uncorrelated Estimates of Dark Energy Evolution

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.304829Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0fd65acb-7c6d-498e-b6f3-ca9fe136f0a0 · outbound

This paper cites Beyond Two Dark Energy Parameters.

Probing the independence within the dark sector in the fluid approximation Beyond Two Dark Energy Parameters

Reference 82

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:37.282762Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation cf7b61ef-ee7c-4a1c-bf04-3071634a077e · outbound

This paper cites Direct reconstruction of dark energy.

Probing the independence within the dark sector in the fluid approximation Direct reconstruction of dark energy

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.327192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23ed6fd4-b18b-4b0e-84a7-3262d53ef9d3 · outbound

This paper cites New Constraints On The Dark Energy Equation of State.

Probing the independence within the dark sector in the fluid approximation New Constraints On The Dark Energy Equation of State

Reference 84

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:37.203863Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 57360db1-44bd-49d1-96f5-42e21866cc0c · outbound

This paper cites an unresolved cited work.

Probing the independence within the dark sector in the fluid approximation Unresolved cited work

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.343052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 18d2f70c-6721-43e1-9370-4b6652111bee · outbound

This paper cites Bayes in the sky: Bayesian inference and model selection in cosmology.

Probing the independence within the dark sector in the fluid approximation Bayes in the sky: Bayesian inference and model selection in cosmology

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.353443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e1d5bbaf-b2de-4b6b-8ce8-25eb6a721c7b · outbound

This paper cites Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?.

Probing the independence within the dark sector in the fluid approximation Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.493502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 56ed5ab7-6db9-4337-9778-9fbfa5366137 · outbound

This paper cites Measuring the effective complexity of cosmological models.

Probing the independence within the dark sector in the fluid approximation Measuring the effective complexity of cosmological models

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.505118Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 773004a6-b497-4db8-8815-901e6e9e63cb · outbound

This paper cites emcee: The MCMC Hammer.

Probing the independence within the dark sector in the fluid approximation emcee: The MCMC Hammer

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.513222Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 723ebc4c-8efb-4b65-a7b1-36a5724f48d9 · outbound

This paper cites An alternative to quintessence.

Probing the independence within the dark sector in the fluid approximation An alternative to quintessence

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.518944Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28d15286-38c4-4fa9-8b22-ec41e308c4a3 · outbound

This paper cites Can the Chaplygin gas be a plausible model for dark energy?.

Probing the independence within the dark sector in the fluid approximation Can the Chaplygin gas be a plausible model for dark energy?

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.524340Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2927aa88-0d4c-4265-b895-fd19eb407c85 · outbound

This paper cites Constraints on the generalized Chaplygin gas from supernovae observations.

Probing the independence within the dark sector in the fluid approximation Constraints on the generalized Chaplygin gas from supernovae observations

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.530236Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c6adcdb-1d5c-48ec-b6f1-aac77d3d0118 · outbound

This paper cites Parameterized Beyond-Einstein Growth.

Probing the independence within the dark sector in the fluid approximation Parameterized Beyond-Einstein Growth

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.539362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 27d32653-a347-474d-97b5-9024bbfe6242 · outbound

This paper cites Cosmic Growth History and Expansion History.

Probing the independence within the dark sector in the fluid approximation Cosmic Growth History and Expansion History

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.546016Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8283aa13-abfb-4664-bb3e-2ccf038869bd · outbound

This paper cites How many cosmological parameters?.

Probing the independence within the dark sector in the fluid approximation How many cosmological parameters?

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.551662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d15010f0-5e83-46cb-97bd-93ee6b555e5b · outbound

This paper cites LSST Science Book, Version 2.0.

Probing the independence within the dark sector in the fluid approximation LSST Science Book, Version 2.0

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.558143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4827b87b-96a8-47f7-a423-62e5796edc86 · outbound

This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.

Probing the independence within the dark sector in the fluid approximation The DESI Experiment Part I: Science,Targeting, and Survey Design

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.565948Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69e59c85-d5df-4154-9a8f-ca4fbda110c6 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter.

Probing the independence within the dark sector in the fluid approximation Accelerating Universes with Scaling Dark Matter

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.574936Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89680b4b-9c3e-43dd-a219-822825ae9908 · outbound

This paper cites Exploring the Expansion History of the Universe.

Probing the independence within the dark sector in the fluid approximation Exploring the Expansion History of the Universe

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-14T15:10:36.580543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7431663c-3777-4440-9e1e-62796678ee9a · outbound

This paper cites Cosmological constraints on coupled dark energy.

Probing the independence within the dark sector in the fluid approximation Cosmological constraints on coupled dark energy

Reference 100

Resolution: verified exact; local_arxiv, observed 2026-08-14T15:10:36.840250Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Coverage vector

Reference resolution

Outbound references

Pith citing papers