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

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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

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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

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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

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

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

Reference 5

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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

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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

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This paper cites Dynamics of dark energy.

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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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This paper cites Inhomogeneous vacuum energy.

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

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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

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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

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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

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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

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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

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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

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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?

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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

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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

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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

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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

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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

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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

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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

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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

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

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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

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

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

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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

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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

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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

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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

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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

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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

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

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

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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

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

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

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

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

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

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

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

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

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

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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

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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

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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

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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

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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

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

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

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

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

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

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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

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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 $z=0.15$

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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

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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

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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

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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

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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

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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 $z\sim 1.4$

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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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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