Two Dynamical Scenarios for Binned Master Sample Interpretation | Paper Citation Record

Observation 0d63c570-cbac-4f65-b414-4bd98901a898 · outbound

This paper cites A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation.

Two Dynamical Scenarios for Binned Master Sample Interpretation A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation

Reference 1

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Observation 386dfaaf-8d5d-45f8-860f-2b5a2c6d2e96 · outbound

This paper cites Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results.

Two Dynamical Scenarios for Binned Master Sample Interpretation Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results

Reference 2

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Observation 0a72535b-903e-408f-a77b-6610451a6734 · outbound

This paper cites A comprehensive measurement of the local value of the Hubble constant with 1 km s−1 Mpc−1 uncertainty from the Hubble Space Telescope and the SH0ES team.

Two Dynamical Scenarios for Binned Master Sample Interpretation A comprehensive measurement of the local value of the Hubble constant with 1 km s−1 Mpc−1 uncertainty from the Hubble Space Telescope and the SH0ES team

Reference 3

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Observation e1a5970f-2a7c-43e1-bb19-c07a7fa18603 · outbound

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

Two Dynamical Scenarios for Binned Master Sample Interpretation Planck 2018 results-VI. Cosmological parameters

Reference 4

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Observation 9c464988-77b2-4854-8cc2-d961f05482fa · outbound

This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

Two Dynamical Scenarios for Binned Master Sample Interpretation The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 5

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Observation 55fa7495-3319-4289-8f8b-ceb68adbe61a · outbound

This paper cites In the realm of the Hubble tension—a review of solutions.

Two Dynamical Scenarios for Binned Master Sample Interpretation In the realm of the Hubble tension—a review of solutions

Reference 6

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Observation ce487de4-7094-400a-be50-56debeb2fea3 · outbound

This paper cites Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension.

Two Dynamical Scenarios for Binned Master Sample Interpretation Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 7

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Observation 7364cfd4-c568-4832-99bf-88dfb108f25d · outbound

This paper cites Exploring the Hubble tension with a late time Modified Gravity scenario.

Two Dynamical Scenarios for Binned Master Sample Interpretation Exploring the Hubble tension with a late time Modified Gravity scenario

Reference 8

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Observation e24e69db-9231-43a7-b582-9bce3f5dc5a8 · outbound

This paper cites Kinetic model for dark energy—dark matter interaction: Sce- nario for the hubble tension.

Two Dynamical Scenarios for Binned Master Sample Interpretation Kinetic model for dark energy—dark matter interaction: Sce- nario for the hubble tension

Reference 9

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Observation c183a76e-9f9f-4070-b542-3ce02e1e2bdb · outbound

This paper cites Slow-rolling scalar dynamics as solution for the Hubble tension.

Two Dynamical Scenarios for Binned Master Sample Interpretation Slow-rolling scalar dynamics as solution for the Hubble tension

Reference 10

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Observation 4e76c7af-6ab7-417d-9f00-c748c0f7211c · outbound

This paper cites Metric f (R) gravity with dynamical dark energy as a scenario for the Hubble tension.

Two Dynamical Scenarios for Binned Master Sample Interpretation Metric f (R) gravity with dynamical dark energy as a scenario for the Hubble tension

Reference 11

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Observation eaefcd8b-9212-4996-9f76-26460bd5f3b5 · outbound

This paper cites f(R) gravity in the Jor- dan frame as a paradigm for the Hubble tension.

Two Dynamical Scenarios for Binned Master Sample Interpretation f(R) gravity in the Jor- dan frame as a paradigm for the Hubble tension

Reference 12

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Observation 1de4e84b-9f87-440a-af75-95423ba8dc44 · outbound

This paper cites Running Hubble constant from the SNe Ia Pantheon sample?.

Two Dynamical Scenarios for Binned Master Sample Interpretation Running Hubble constant from the SNe Ia Pantheon sample?

Reference 13

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Observation bceaac6b-2f5b-43e6-bf3b-2fab1e469ff7 · outbound

This paper cites Introduction to modified gravity and gravita- tional alternative for dark energy.

Two Dynamical Scenarios for Binned Master Sample Interpretation Introduction to modified gravity and gravita- tional alternative for dark energy

Reference 14

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Observation 4c159c22-5086-4412-92c6-4aa4ae86b7a6 · outbound

This paper cites New constraints on interacting dark energy from DESI DR2 BAO observations.

Two Dynamical Scenarios for Binned Master Sample Interpretation New constraints on interacting dark energy from DESI DR2 BAO observations

Reference 15

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Observation c5e65f48-070a-4347-a0bd-be5d23996e29 · outbound

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

Two Dynamical Scenarios for Binned Master Sample Interpretation Implications of distance duality violation for the $H_0$ tension and evolving dark energy

Reference 16

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Observation f5484a2c-1b8f-4bcc-9602-5949ec806afb · outbound

This paper cites Inflation, the Hubble tension, and early dark energy: An alternative overview.

Two Dynamical Scenarios for Binned Master Sample Interpretation Inflation, the Hubble tension, and early dark energy: An alternative overview

Reference 17

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Observation 643fae76-0335-4c12-be8f-907475d824e5 · outbound

This paper cites Small amplitude red giants elucidate the nature of the Tip of the Red Giant Branch as a standard candle.

Two Dynamical Scenarios for Binned Master Sample Interpretation Small amplitude red giants elucidate the nature of the Tip of the Red Giant Branch as a standard candle

Reference 18

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Observation d73e60be-8235-44bc-94aa-75aab7533406 · outbound

This paper cites The Pantheon+ Analysis: The Full Data Set and Light-curve Release.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Pantheon+ Analysis: The Full Data Set and Light-curve Release

Reference 19

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Observation f443fb74-6f88-45e5-b489-4fb107e5d47b · 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.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

Reference 20

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Observation f0de2dac-b6b4-480d-8139-6f748fcbd459 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Pantheon+ Analysis: Cosmological Constraints

Reference 21

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Observation 770830d4-6d59-475c-98b9-a0077a687237 · outbound

This paper cites CATS: The Hubble Constant from Standardized TRGB and Type Ia Supernova Measurements.

Two Dynamical Scenarios for Binned Master Sample Interpretation CATS: The Hubble Constant from Standardized TRGB and Type Ia Supernova Measurements

Reference 22

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Observation b34fb641-ceb3-4781-89ac-5b39d152f3f4 · outbound

This paper cites Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State.

Two Dynamical Scenarios for Binned Master Sample Interpretation Cosmological Results from the RAISIN Survey: Using Type Ia Supernovae in the Near Infrared as a Novel Path to Measure the Dark Energy Equation of State

Reference 23

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Observation 7bd26b70-7826-4359-8781-c2bdf9c5d6c8 · outbound

This paper cites Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant.

Two Dynamical Scenarios for Binned Master Sample Interpretation Comparing Tip of the Red Giant Branch Distance Scales: An Independent Reduction of the Carnegie-Chicago Hubble Program and the Value of the Hubble Constant

Reference 24

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Observation c52d8d87-0b99-47a8-8906-124be32dacc4 · outbound

This paper cites Carnegie Supernova Project-I and -II: Measurements of $H_0$ using Cepheid, TRGB, and SBF Distance Calibration to Type Ia Supernovae.

Two Dynamical Scenarios for Binned Master Sample Interpretation Carnegie Supernova Project-I and -II: Measurements of $H_0$ using Cepheid, TRGB, and SBF Distance Calibration to Type Ia Supernovae

Reference 26

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Observation de814987-c2ab-4a74-996e-c359d9ab0000 · outbound

This paper cites The Mira Distance to M101 and a 4% Measurement of H0.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Mira Distance to M101 and a 4% Measurement of H0

Reference 27

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Observation 16fec508-a136-405d-bf78-3d7ff842d455 · outbound

This paper cites Reconnaissance with JWST of the J-region Asymptotic Giant Branch in Distance Ladder Galaxies: From Irregular Luminosity Functions to Approximation of the Hubble Constant.

Two Dynamical Scenarios for Binned Master Sample Interpretation Reconnaissance with JWST of the J-region Asymptotic Giant Branch in Distance Ladder Galaxies: From Irregular Luminosity Functions to Approximation of the Hubble Constant

Reference 28

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Observation 611d5793-01d9-423f-902a-2d455185c322 · outbound

This paper cites Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations.

Two Dynamical Scenarios for Binned Master Sample Interpretation Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations

Reference 29

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Observation 2431457b-da0a-434b-9db5-c075a4e20a8f · outbound

This paper cites Using The Baryonic Tully-Fisher Relation to Measure $H_o$.

Two Dynamical Scenarios for Binned Master Sample Interpretation Using The Baryonic Tully-Fisher Relation to Measure $H_o$

Reference 30

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Observation 8c127316-f2b9-4205-b2ec-a20ee5153053 · outbound

This paper cites Leveraging SN Ia spectroscopic similarity to improve the measurement of H0.

Two Dynamical Scenarios for Binned Master Sample Interpretation Leveraging SN Ia spectroscopic similarity to improve the measurement of H0

Reference 31

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Observation bfd9e8e0-c3f2-4979-80e0-ecf34422781c · outbound

This paper cites Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder.

Two Dynamical Scenarios for Binned Master Sample Interpretation Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder

Reference 32

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Observation 369f2800-f5b8-468f-a47f-ee94530985b4 · outbound

This paper cites A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set.

Two Dynamical Scenarios for Binned Master Sample Interpretation A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set

Reference 33

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Observation fa0132b0-83bf-452c-815e-4e4c0ca2c021 · outbound

This paper cites The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters

Reference 34

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Observation 59cd988b-978f-4bff-922d-d5d2ee35decd · outbound

This paper cites A proposal to improve the accuracy of cosmolog- ical observables and address the Hubble tension problem.

Two Dynamical Scenarios for Binned Master Sample Interpretation A proposal to improve the accuracy of cosmolog- ical observables and address the Hubble tension problem

Reference 35

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Observation fa81e3b8-1828-473d-9f17-58e49d6ccd52 · outbound

This paper cites DeterminingH0 from distance sum rule combining gamma-ray bursts with observational Hubble data and strong gravitational lensing.

Two Dynamical Scenarios for Binned Master Sample Interpretation DeterminingH0 from distance sum rule combining gamma-ray bursts with observational Hubble data and strong gravitational lensing

Reference 36

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Observation 51dcd8dd-5870-4f75-8577-2eabe1839fa7 · outbound

This paper cites Deep Learning Based Recalibration of SDSS and DESI BAO Alleviates Hubble and Clustering Tensions.

Two Dynamical Scenarios for Binned Master Sample Interpretation Deep Learning Based Recalibration of SDSS and DESI BAO Alleviates Hubble and Clustering Tensions

Reference 37

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Observation d87efcd7-fa68-46a0-96b6-390065427e8e · outbound

This paper cites Tensions between the early and late Universe.

Two Dynamical Scenarios for Binned Master Sample Interpretation Tensions between the early and late Universe

Reference 38

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Observation 4bb61f12-1e7c-47ee-ad6d-5a94ff7c529f · outbound

This paper cites The Carnegie-Chicago Hubble Program. VIII. An Inde- pendent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch*.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Carnegie-Chicago Hubble Program. VIII. An Inde- pendent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch*

Reference 39

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Observation ba2e099f-6d86-4ac4-aa18-76a00df284e2 · outbound

This paper cites Calibration of the Tip of the Red Giant Branch (TRGB).

Two Dynamical Scenarios for Binned Master Sample Interpretation Calibration of the Tip of the Red Giant Branch (TRGB)

Reference 40

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Observation 0c6666f7-656d-439e-86b0-829d522bd730 · outbound

This paper cites The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Parallax of Omega Centauri Measured from Gaia EDR3 and a Direct, Geometric Calibration of the Tip of the Red Giant Branch and the Hubble Constant

Reference 41

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Observation 1a2bc4bc-c2bc-4951-9667-47e335ad8040 · outbound

This paper cites Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model.

Two Dynamical Scenarios for Binned Master Sample Interpretation Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model

Reference 42

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Observation f8e02713-d75d-47d8-a37a-9588a1de2bbd · outbound

This paper cites Exploring the evidence for a large local void with supernovae Ia data.

Two Dynamical Scenarios for Binned Master Sample Interpretation Exploring the evidence for a large local void with supernovae Ia data

Reference 43

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Observation a3756952-5f80-426b-8e72-d4a392546397 · outbound

This paper cites New constraint of the Hubble constant by proper motions of radio components observed in AGN twin-jets.

Two Dynamical Scenarios for Binned Master Sample Interpretation New constraint of the Hubble constant by proper motions of radio components observed in AGN twin-jets

Reference 44

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Observation 79f92934-356e-458b-bdef-60232efcce1e · outbound

This paper cites Unbiased likelihood-free inference of the Hubble constant from light standard sirens.

Two Dynamical Scenarios for Binned Master Sample Interpretation Unbiased likelihood-free inference of the Hubble constant from light standard sirens

Reference 45

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Observation 0ac85d26-b165-4f28-9767-99625f5daae4 · outbound

This paper cites Leveraging SN Ia spectroscopic similarity to improve the measurement of $H_0$.

Two Dynamical Scenarios for Binned Master Sample Interpretation Leveraging SN Ia spectroscopic similarity to improve the measurement of $H_0$

Reference 46

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This paper cites an unresolved cited work.

Two Dynamical Scenarios for Binned Master Sample Interpretation Unresolved cited work

Reference 47

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Observation 501a2d54-dbc3-47b5-9996-e7497906ce7e · outbound

This paper cites Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?.

Two Dynamical Scenarios for Binned Master Sample Interpretation Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?

Reference 48

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Observation 8d4c5db3-161f-41cf-9d06-afe7b4e28951 · outbound

This paper cites Forecast of observing time delay of the strongly lensed quasars with Muztagh-Ata 1.93m telescope.

Two Dynamical Scenarios for Binned Master Sample Interpretation Forecast of observing time delay of the strongly lensed quasars with Muztagh-Ata 1.93m telescope

Reference 50

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Observation 83a583f5-9de8-4383-a000-470146b92ab7 · outbound

This paper cites A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey.

Two Dynamical Scenarios for Binned Master Sample Interpretation A standard siren measurement of the Hubble constant using gravitational wave events from the first three LIGO/Virgo observing runs and the DESI Legacy Survey

Reference 51

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Observation f2d7abd2-a081-42a7-9875-dcb2f9793294 · outbound

This paper cites A 5% measurement of the Hubble constant from Type II supernovae.

Two Dynamical Scenarios for Binned Master Sample Interpretation A 5% measurement of the Hubble constant from Type II supernovae

Reference 52

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Observation 77da7e5f-4deb-4c21-9250-d5d64aa3e9b4 · outbound

This paper cites Assessing the effect of mass-model assumptions on measuring the Hubble constant from the cluster-lensed supernova Refsdal.

Two Dynamical Scenarios for Binned Master Sample Interpretation Assessing the effect of mass-model assumptions on measuring the Hubble constant from the cluster-lensed supernova Refsdal

Reference 53

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Observation c173d9a1-cfb6-4e95-8ddd-c53da8623e96 · outbound

This paper cites The Hubble Constant from Infrared Surface Brightness Fluc- tuation Distances*.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Hubble Constant from Infrared Surface Brightness Fluc- tuation Distances*

Reference 54

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Observation 349a6e07-7ed4-40e1-8820-5a0df0b1cbec · outbound

This paper cites TheMegamaserCosmologyProject.XIII.CombinedHubbleConstant Constraints.

Two Dynamical Scenarios for Binned Master Sample Interpretation TheMegamaserCosmologyProject.XIII.CombinedHubbleConstant Constraints

Reference 55

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Observation 3d5fdfea-e66e-46cb-8286-86d49a226ada · outbound

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

Two Dynamical Scenarios for Binned Master Sample Interpretation DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 56

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Observation 3d8f08dd-f58d-4835-bc16-bcbe77315b92 · outbound

This paper cites Accelerating universes with scaling dark matter.

Two Dynamical Scenarios for Binned Master Sample Interpretation Accelerating universes with scaling dark matter

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This paper cites Exploring the expansion history of the universe.

Two Dynamical Scenarios for Binned Master Sample Interpretation Exploring the expansion history of the universe

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Two Dynamical Scenarios for Binned Master Sample Interpretation DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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Observation 118bae08-504f-4ae0-9ca8-ff7cb821add7 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation An overview of what current data can (and cannot yet) say about evolving dark energy

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Observation 61d36221-6792-4bb6-a896-3d4e8a9e6984 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Dynamical Dark Energy Beyond Planck? Constraints from multiple CMB probes, DESI BAO and Type-Ia Supernovae

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Observation 83c62fb9-6d8b-4c80-9704-41d7211efa04 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Extended Dark Energy analysis using DESI DR2 BAO measurements

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Two Dynamical Scenarios for Binned Master Sample Interpretation Phenomenology of $\Lambda$-CDM model: a possibility of accelerating Universe with positive pressure

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Two Dynamical Scenarios for Binned Master Sample Interpretation Decay of cosmological constant as Bose condensate evaporation

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Observation 2f508a8e-8ecd-49b1-8718-cc8c1aad4871 · outbound

This paper cites Formation of structure in a universe with unstable neutrinos.

Two Dynamical Scenarios for Binned Master Sample Interpretation Formation of structure in a universe with unstable neutrinos

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Observation 8f3cd59b-fabd-46be-8cfe-97f964ca2f91 · outbound

This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.

Two Dynamical Scenarios for Binned Master Sample Interpretation Does DESI 2024 Confirm $\Lambda$CDM?

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Two Dynamical Scenarios for Binned Master Sample Interpretation On the evolution of the Hubble constant with the SNe Ia pantheon sample and baryon acoustic oscillations: a feasibility study for GRB-cosmology in 2030

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Two Dynamical Scenarios for Binned Master Sample Interpretation A New Master Supernovae Ia sample and the investigation of the $H_0$ tension

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Observation eb076b18-3241-4ce4-9f0c-d8d8e95d0ae3 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation The effective running Hubble constant in SNe Ia as a marker for the dark energy nature

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Observation f5bef57f-3d91-4e9d-9e80-52768befd20c · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation On the Hubble constant tension in the SNe Ia Pantheon sample

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Observation a29a1165-0829-44bd-922a-66bff1a5d245 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation On the statistical assumption on the distance moduli of Supernovae Ia and its impact on the determination of cosmological parameters

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Observation 564ab7ad-6e71-41ba-919e-b86f42da60d6 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Redshift evolution of the underlying type Ia supernova stretch dis- tribution

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Two Dynamical Scenarios for Binned Master Sample Interpretation Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes

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Observation 59d1ee83-d351-41dc-a1c7-45da1e76af84 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Evolution of an effective Hubble constant in $f(R)$ modified gravity

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Observation e72258b4-854d-4fcc-88c9-9fb4f73d4e0c · outbound

This paper cites Can we learn from matter creation to solve theH0 tension problem?.

Two Dynamical Scenarios for Binned Master Sample Interpretation Can we learn from matter creation to solve theH0 tension problem?

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Observation 8e3156c0-c6d0-4307-a8a5-f360770a6964 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Investigating f (R)-Inflation: background evolution and constraints

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Observation 7af06706-083f-42b5-b58a-ce131f2e9ef4 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition

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Observation 8859eec3-3290-441d-a2e8-b473ae015b8b · outbound

This paper cites The Gamma-ray Bursts fundamental plane correlation as a cosmological tool.

Two Dynamical Scenarios for Binned Master Sample Interpretation The Gamma-ray Bursts fundamental plane correlation as a cosmological tool

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Observation 338d6b8d-ed71-42f3-a8f1-6c1e0038c117 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Influence of particle creation on flat and negative curved FLRW universes

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Observation c704117e-6ad0-4fe1-98ef-5ad37e73b7b3 · outbound

This paper cites A new binning method to choose a standard set of Quasars.

Two Dynamical Scenarios for Binned Master Sample Interpretation A new binning method to choose a standard set of Quasars

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Two Dynamical Scenarios for Binned Master Sample Interpretation The evidence for a spatially flat Universe

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Observation 73467ac0-c528-4444-8881-dc4a1a01fe85 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Weinberg

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Observation 8d526e54-47d6-442b-bafb-75abf6d7d0e5 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation On the thermodynamics of matter creation in cosmology

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This paper cites Coupled Quintessence.

Two Dynamical Scenarios for Binned Master Sample Interpretation Coupled Quintessence

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Two Dynamical Scenarios for Binned Master Sample Interpretation Cosmological evolution with interaction between dark energy and dark matter

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This paper cites Dark matter and dark energy interactions: theoretical challenges, cos- mological implications and observational signatures.

Two Dynamical Scenarios for Binned Master Sample Interpretation Dark matter and dark energy interactions: theoretical challenges, cos- mological implications and observational signatures

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Observation 82be39e6-a260-4c72-951a-09ed65a45ee0 · outbound

This paper cites Transition of the dark energy equation of state in an interacting holographic dark energy model.

Two Dynamical Scenarios for Binned Master Sample Interpretation Transition of the dark energy equation of state in an interacting holographic dark energy model

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Resolution: verified exact; doi, observed 2026-08-06T16:16:24.086848Z

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Observation f7e4fa39-bfe0-4b18-8d5e-51d2739697a4 · outbound

This paper cites Phantom behavior via cosmological creation of par- ticles.

Two Dynamical Scenarios for Binned Master Sample Interpretation Phantom behavior via cosmological creation of par- ticles

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Two Dynamical Scenarios for Binned Master Sample Interpretation Acosmographicanalysis ofholographic darken- ergymodels

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Observation 56f8bf40-1441-4861-8a63-53f3e29e8b3c · outbound

This paper cites Cosmologies with energy exchange.

Two Dynamical Scenarios for Binned Master Sample Interpretation Cosmologies with energy exchange

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Observation 639dafe7-6f62-4e94-bdba-732f8567774c · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Consequences of dark matter-dark energy interaction on cosmological parameters derived from SNIa data

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Observation e757c0d9-2ddb-4efb-a9ca-c110091a4bab · outbound

This paper cites Effects of the interaction between dark energy and dark matter on cosmological parameters.

Two Dynamical Scenarios for Binned Master Sample Interpretation Effects of the interaction between dark energy and dark matter on cosmological parameters

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Observation 3f6d3aeb-fcfb-4b8e-8946-8c9a9964cf73 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Superacceleration as the signature of a dark sector interaction

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

Two Dynamical Scenarios for Binned Master Sample Interpretation Observational constraints on an interacting dark energy model

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Observation aee6b173-1591-44ab-a437-823d73383b06 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Linear and nonlinear interactions in the dark sector

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Observation b5441a66-c997-44fa-93c2-1f5828a3bca0 · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Large-scale instability in inter- acting dark energy and dark matter fluids

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Observation 35cdabcf-8ced-4955-a493-4f7cf7458c0e · outbound

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Two Dynamical Scenarios for Binned Master Sample Interpretation Interacting dark sector with transversal inter- action

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Two Dynamical Scenarios for Binned Master Sample Interpretation Testing coupled dark energy with large scale structure observation

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Resolution: verified exact; doi, observed 2026-08-06T16:16:23.825544Z

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Observation a0d33072-5283-42b6-a4f1-4b123525e985 · outbound

This paper cites New constraints on inter- acting dark energy from cosmic chronometers.

Two Dynamical Scenarios for Binned Master Sample Interpretation New constraints on inter- acting dark energy from cosmic chronometers

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Two Dynamical Scenarios for Binned Master Sample Interpretation Testing the interaction between dark energy and dark matter via the latest observations

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Two Dynamical Scenarios for Binned Master Sample Interpretation Dynamics of nonlinear interacting dark energy models

Reference 105

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This paper cites url: http://dx.doi.org/10.1063/1.4913335.

Two Dynamical Scenarios for Binned Master Sample Interpretation url: http://dx.doi.org/10.1063/1.4913335

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