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Paper Citation Record · LEDGER
Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations
As of 10 August 2026, this Paper Citation Record lists 48 of 48 outbound references and 0 inbound Pith citation observations for arXiv:2502.01751.
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Reference resolution
48 of 48 outbound references displayed
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Outbound references
Observation 7fbe4002-ad08-49a3-be82-f6a61dac9f9c · outbound
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Kamenshchik, U
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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This paper cites A Particle Field Theorist's Lectures on Supersymmetric, Non-Abelian Fluid Mechanics and d-Branes.
Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations A Particle Field Theorist's Lectures on Supersymmetric, Non-Abelian Fluid Mechanics and d-Branes
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The median density of the Universe
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unified Dark Matter models with fast transition
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unified Dark Matter scalar field models with fast transition
Reference 17
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Cosmological constraints on a decomposed Chaplygin gas
Reference 19
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Nonlinear Chaplygin Gas Cosmologies
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The growth of fluctuations in Chaplygin gas cosmologies: A nonlinear Jeans scale for unified dark matter
Reference 21
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Del Popolo and M
Reference 22
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The distribution of dark matter in galaxies
Reference 24
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations As the first nonlinear structures form, the unified dark fluid splits into two sectors, one remaining nearly homogeneous and another made of the nonlinear structures
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Planck 2018 results. VI. Cosmological parameters
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Cosmological Perturbation Theory in the Synchronous and Conformal Newtonian Gauges
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The Cosmic Linear Anisotropy Solving System (CLASS) I: Overview
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Integrated Sachs Wolfe Effect and Rees Sciama Effect
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Looking for $\Lambda$ with the Rees-Sciama Effect
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Planck ISW-lensing likelihood and the CMB temperature
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Constraining dark energy with the integrated Sachs-Wolfe effect
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The Pantheon+ Analysis: Cosmological Constraints
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations One percent determination of the primordial deuterium abundance
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Cosmological Constraints from the Clustering of the Sloan Digital Sky Survey DR7 Luminous Red Galaxies
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations An Updated Tomographic Analysis of the Integrated Sachs-Wolfe Effect and implications for Dark Energy
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations GetDist: a Python package for analysing Monte Carlo samples
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations The 2dF Galaxy Redshift Survey: The power spectrum and the matter content of the universe
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Unresolved cited work
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Clustered unified dark sector cosmology: Background evolution and linear perturbations in light of observations Efficient Photometric Selection of Quasars from the Sloan Digital Sky Survey: II. ~1,000,000 Quasars from Data Release Six
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Pith citing papers
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