Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy | Paper Citation Record

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy (25) to calculate the scale-dependent bias

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This paper cites Furthermore, the scale-dependence induced by the sound mode is also present in the bispectrum owing to its dependence on the galaxy bias parameters.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Furthermore, the scale-dependence induced by the sound mode is also present in the bispectrum owing to its dependence on the galaxy bias parameters

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This paper cites Concretely, we assume a redshift-dependent halo mass M(z) =M 0(1 +z) αeβz (B2) whereM 0 is the present-day halo mass.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Concretely, we assume a redshift-dependent halo mass M(z) =M 0(1 +z) αeβz (B2) whereM 0 is the present-day halo mass

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This paper cites Cosmological Imprint of an Energy Component with General Equation of State.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Cosmological Imprint of an Energy Component with General Equation of State

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Zlatev, L

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Ratra and P

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Measuring the Speed of Sound of Quintessence

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Armendariz-Picon, T

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Armendariz-Picon, V

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Ghost Inflation

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Dust of Dark Energy

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This paper cites The phenomenological approach to modeling the dark energy.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy The phenomenological approach to modeling the dark energy

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Observation 87f1cc1b-9a26-457b-8d5f-fb2ac8141564 · outbound

This paper cites Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective

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Observation f2dabd2e-a029-4976-b0f3-d1db0e9ce52d · outbound

This paper cites Variable sound speed in interacting dark energy models.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Variable sound speed in interacting dark energy models

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This paper cites $k$-evolution: a relativistic N-body code for clustering dark energy.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy $k$-evolution: a relativistic N-body code for clustering dark energy

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This paper cites Biased tracers as a probe of beyond-$\Lambda$CDM cosmologies.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Biased tracers as a probe of beyond-$\Lambda$CDM cosmologies

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This paper cites Evolution of clustering in cosmological models with time-varying dark energy.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Evolution of clustering in cosmological models with time-varying dark energy

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This paper cites Limits on Clustering and Smooth Quintessence from the EFTofLSS.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Limits on Clustering and Smooth Quintessence from the EFTofLSS

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This paper cites A low-redshift preference for an interacting dark energy model.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy A low-redshift preference for an interacting dark energy model

Reference 29

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Observation 1c80de05-8c1f-49e6-a0c9-e9502bc50287 · outbound

This paper cites DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Observation 49637326-2324-43cd-be19-f6c23c9ea299 · outbound

This paper cites Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Cosmological implications of DESI DR2 BAO measurements in light of the latest ACT DR6 CMB data

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Wang and D

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Implications of distance duality violation for the $H_0$ tension and evolving dark energy

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Capozziello, H

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Accelerating Universes with Scaling Dark Matter

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This paper cites To CPL, or not to CPL? What we have not learned about the dark energy equation of state.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy To CPL, or not to CPL? What we have not learned about the dark energy equation of state

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This paper cites Nonparametric reconstructions of dynamical dark energy via flexknots.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Nonparametric reconstructions of dynamical dark energy via flexknots

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy An overview of what current data can (and cannot yet) say about evolving dark energy

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This paper cites Optimal parameterizations for observational constraints on thawing dark energy.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Optimal parameterizations for observational constraints on thawing dark energy

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Artola, I

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 45

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This paper cites The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy The Preference for Evolving Dark Energy from Cosmological Distance Measurements and Possible Signatures in the Growth Rate of Perturbations

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Dynamical dark energy in the light of DESI 2024 data

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This paper cites Reconstructing the dark energy density in light of DESI BAO observations.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Reconstructing the dark energy density in light of DESI BAO observations

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Bansal and D

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Scalar field dark energy models: Current and forecast constraints

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This paper cites Mena-Fern´ andezet al.(DES), Dark Energy Sur- vey: DESI-Independent Angular BAO Measurement, (2026), arXiv:2601.14864 [astro-ph.CO].

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Mena-Fern´ andezet al.(DES), Dark Energy Sur- vey: DESI-Independent Angular BAO Measurement, (2026), arXiv:2601.14864 [astro-ph.CO]

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This paper cites KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature

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This paper cites Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Chen and M

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Silva and R

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

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?

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This paper cites Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy

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This paper cites Camarena, K.

Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Camarena, K

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Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy Basse, O

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