Paper Citation Record · LEDGER

The case for a low dark matter density in dynamical dark energy model from local probes

As of 11 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 4 inbound Pith citation observations for arXiv:2501.08915.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2501.08915 v1

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Source: arxiv_reference, observed 2026-05-19T05:22:06.103057Z

Reference resolution

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Outbound references

Observation 8dba96a2-ab37-42ef-8510-4dfe00d53681 · outbound

This paper cites Testing the hypothesis of a matter density discrepancy within LCDM model using multiple probes.

The case for a low dark matter density in dynamical dark energy model from local probes Testing the hypothesis of a matter density discrepancy within LCDM model using multiple probes

Reference 1

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Observation 031eabdb-f36a-428a-902e-4cd46a01329d · outbound

This paper cites On Evidence for Elastic Interactions in the Dark Sector.

The case for a low dark matter density in dynamical dark energy model from local probes On Evidence for Elastic Interactions in the Dark Sector

Reference 2

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Observation d155ce22-01a8-4726-b6ac-b24170a10524 · outbound

This paper cites Can decaying vacuum solve the H_0 Tension?.

The case for a low dark matter density in dynamical dark energy model from local probes Can decaying vacuum solve the H_0 Tension?

Reference 3

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Observation 0fd8f325-51b7-4755-b4d3-71349a49aae6 · outbound

This paper cites Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes.

The case for a low dark matter density in dynamical dark energy model from local probes Uniting the Observed Dynamical Dark Energy Preference with the Discrepancies in $\Omega_m$ and $H_0$ Across Cosmological Probes

Reference 4

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Observation ae5cba1e-419b-495c-8ed7-630709c85ab4 · outbound

This paper cites Modified recombination and the Hubble tension.

The case for a low dark matter density in dynamical dark energy model from local probes Modified recombination and the Hubble tension

Reference 5

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Observation 1be80e87-928f-4cae-b6ef-1c3353ec426a · outbound

This paper cites Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis.

The case for a low dark matter density in dynamical dark energy model from local probes Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis

Reference 6

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Observation 624c23a7-a64b-4f61-9147-aa55252d829c · outbound

This paper cites Bridge the Cosmological Tensions with Thawing Gravity.

The case for a low dark matter density in dynamical dark energy model from local probes Bridge the Cosmological Tensions with Thawing Gravity

Reference 7

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Observation bd28581a-faca-487d-b081-3a8f6d005924 · outbound

This paper cites Running gravitational constant induced dark energy as a solution to $\sigma_8$ tension.

The case for a low dark matter density in dynamical dark energy model from local probes Running gravitational constant induced dark energy as a solution to $\sigma_8$ tension

Reference 8

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Observation 2f565075-da42-40d2-b59f-bb32b179cb67 · outbound

This paper cites A doublet of cosmological models to challenge the H0 tension in the Pantheon Supernovae Ia catalog.

The case for a low dark matter density in dynamical dark energy model from local probes A doublet of cosmological models to challenge the H0 tension in the Pantheon Supernovae Ia catalog

Reference 9

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Observation f6744d62-94e9-4124-bf2b-0b816fb824b9 · outbound

This paper cites Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag.

The case for a low dark matter density in dynamical dark energy model from local probes Towards alleviating the $H_0$ and $S_8$ tensions with Early Dark Energy - Dark Matter drag

Reference 10

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Observation 06a0e255-e314-4670-8306-4bb384a9facf · outbound

This paper cites Toda and O.

The case for a low dark matter density in dynamical dark energy model from local probes Toda and O

Reference 11

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Observation 5ec77fae-af26-42a8-8e2d-2e34ab4e3b11 · outbound

This paper cites Composite running vacuum in the Universe: implications on the cosmological tensions.

The case for a low dark matter density in dynamical dark energy model from local probes Composite running vacuum in the Universe: implications on the cosmological tensions

Reference 12

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Observation c52ef787-4f06-4971-83fb-2e53c96e0c5f · outbound

This paper cites Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant.

The case for a low dark matter density in dynamical dark energy model from local probes Combining pre- and post-recombination new physics to address cosmological tensions: case study with varying electron mass and sign-switching cosmological constant

Reference 13

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Observation 7fdb39e3-f8d0-4a3f-ae49-33cc852a561d · outbound

This paper cites $\Lambda_{\rm s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties.

The case for a low dark matter density in dynamical dark energy model from local probes $\Lambda_{\rm s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties

Reference 14

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Observation 499aeea4-7ca2-437b-9693-2d01ff332acd · outbound

This paper cites Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample.

The case for a low dark matter density in dynamical dark energy model from local probes Alleviating the Hubble-constant tension and the growth tension via a transition of absolute magnitude favored by the Pantheon+ sample

Reference 15

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Observation 7b570abe-e1f4-4d14-9110-9cf13ad281e4 · outbound

This paper cites Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model.

The case for a low dark matter density in dynamical dark energy model from local probes Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

Reference 16

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Observation 11a27e3e-157f-4512-a942-83c6afda35c3 · outbound

This paper cites Alleviating $H_0$ and $S_8$ Tensions Simultaneously in K-essence Cosmology.

The case for a low dark matter density in dynamical dark energy model from local probes Alleviating $H_0$ and $S_8$ Tensions Simultaneously in K-essence Cosmology

Reference 17

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Observation 882a2ecb-764a-42fb-91ec-1663bed84fc5 · outbound

This paper cites Investigating the Hubble Tension and $\sigma_8$ Discrepancy in f(Q) Cosmology.

The case for a low dark matter density in dynamical dark energy model from local probes Investigating the Hubble Tension and $\sigma_8$ Discrepancy in f(Q) Cosmology

Reference 18

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Observation b8f30891-eae7-476c-97a8-35598793a843 · outbound

This paper cites Phantom matter: a challenging solution to the cosmological tensions.

The case for a low dark matter density in dynamical dark energy model from local probes Phantom matter: a challenging solution to the cosmological tensions

Reference 19

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Observation 5934afe8-facc-4fb8-b2fb-53935167bd16 · outbound

This paper cites The Lambda-CDM-NG cosmological model: A possible resolution of the Hubble tension.

The case for a low dark matter density in dynamical dark energy model from local probes The Lambda-CDM-NG cosmological model: A possible resolution of the Hubble tension

Reference 20

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Observation 7834fc8a-4b18-42a2-be81-585878990232 · outbound

This paper cites Refitting cosmological data with neutrino mass and degeneracy.

The case for a low dark matter density in dynamical dark energy model from local probes Refitting cosmological data with neutrino mass and degeneracy

Reference 21

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Observation 98b056a5-4df2-4c25-b873-0c9e6fe1e79c · outbound

This paper cites $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks.

The case for a low dark matter density in dynamical dark energy model from local probes $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks

Reference 22

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Observation 53450ebe-9a61-48e2-9f58-a4438995b69e · outbound

This paper cites The Cosmological Constant Potential: a resolution to the Hubble tension via the cosmological sound horizon.

The case for a low dark matter density in dynamical dark energy model from local probes The Cosmological Constant Potential: a resolution to the Hubble tension via the cosmological sound horizon

Reference 23

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Observation b8951f4b-bb97-4572-8a9d-a2652a97ae46 · outbound

This paper cites Solving the Hubble tension at intermediate redshifts with dynamical dark energy.

The case for a low dark matter density in dynamical dark energy model from local probes Solving the Hubble tension at intermediate redshifts with dynamical dark energy

Reference 24

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Observation 07a29c7c-b807-4e0a-a191-6b5562f20ef1 · outbound

This paper cites Extensions to $\Lambda$CDM at Intermediate Redshifts to Solve the Tensions ?.

The case for a low dark matter density in dynamical dark energy model from local probes Extensions to $\Lambda$CDM at Intermediate Redshifts to Solve the Tensions ?

Reference 25

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Observation 3d634b08-97e9-4319-9f23-5bbe12f5a911 · outbound

This paper cites Using the Kaniadakis horizon entropy in the presence of neutrinos to alleviate the Hubble and $ S_{8} $ Tensions.

The case for a low dark matter density in dynamical dark energy model from local probes Using the Kaniadakis horizon entropy in the presence of neutrinos to alleviate the Hubble and $ S_{8} $ Tensions

Reference 26

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Observation 8c7d1306-33bc-4b76-a1b5-53d794c7726e · outbound

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

The case for a low dark matter density in dynamical dark energy model from local probes Deep Learning Based Recalibration of SDSS and DESI BAO Alleviates Hubble and Clustering Tensions

Reference 27

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Observation 61a5b89d-95bf-4e55-bb19-7b91c35f6efa · outbound

This paper cites Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results.

The case for a low dark matter density in dynamical dark energy model from local probes Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results

Reference 28

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Observation eb4c2adf-a9b8-4406-81e6-e21a735d91a9 · outbound

This paper cites H0 tension in Tsallis and Renyi statistics.

The case for a low dark matter density in dynamical dark energy model from local probes H0 tension in Tsallis and Renyi statistics

Reference 29

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Observation 35cfb81a-9915-4218-b429-9ba452cf762f · outbound

This paper cites Barrow Interacting holographic dark energy cosmology with Hubble horizon as IR cutoff: A model can Alleviating the Hubble and $S_{8}$ Tension.

The case for a low dark matter density in dynamical dark energy model from local probes Barrow Interacting holographic dark energy cosmology with Hubble horizon as IR cutoff: A model can Alleviating the Hubble and $S_{8}$ Tension

Reference 30

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Observation 0147c172-ae4f-4687-9213-343fc1171658 · outbound

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

The case for a low dark matter density in dynamical dark energy model from local probes Planck 2018 results. VI. Cosmological parameters

Reference 31

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Observation 5e7596b0-78d9-4629-858a-9f0705c66be4 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

The case for a low dark matter density in dynamical dark energy model from local probes The Pantheon+ Analysis: Cosmological Constraints

Reference 32

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This paper cites Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework.

The case for a low dark matter density in dynamical dark energy model from local probes Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 33

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This paper cites The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset.

The case for a low dark matter density in dynamical dark energy model from local probes The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 34

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

The case for a low dark matter density in dynamical dark energy model from local probes DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 35

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The case for a low dark matter density in dynamical dark energy model from local probes Unresolved cited work

Reference 36

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Observation ba32744d-9aaa-4e9c-9272-1b560cc83c04 · outbound

This paper cites Solving the Hubble tension \`a la Ellis & Stoeger 1987.

The case for a low dark matter density in dynamical dark energy model from local probes Solving the Hubble tension \`a la Ellis & Stoeger 1987

Reference 37

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This paper cites Can late-time extensions solve the $H_0$ and $\sigma_8$ tensions?.

The case for a low dark matter density in dynamical dark energy model from local probes Can late-time extensions solve the $H_0$ and $\sigma_8$ tensions?

Reference 38

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Observation 9af6bd66-3091-4952-bb36-cf195d650600 · outbound

This paper cites DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?.

The case for a low dark matter density in dynamical dark energy model from local probes DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics?

Reference 39

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This paper cites $\Lambda$CDM is alive and well.

The case for a low dark matter density in dynamical dark energy model from local probes $\Lambda$CDM is alive and well

Reference 40

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This paper cites Multidimensionality of the Hubble tension: the roles of $\Omega_m$ and $\omega_c$.

The case for a low dark matter density in dynamical dark energy model from local probes Multidimensionality of the Hubble tension: the roles of $\Omega_m$ and $\omega_c$

Reference 41

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This paper cites $\Lambda$CDM model against redshift-binned data: A mock analysis based on SNIa and Cosmic Chronometers.

The case for a low dark matter density in dynamical dark energy model from local probes $\Lambda$CDM model against redshift-binned data: A mock analysis based on SNIa and Cosmic Chronometers

Reference 42

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Observation 6f53ea2c-61af-4c80-851e-0345e23e7f58 · outbound

This paper cites DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons.

The case for a low dark matter density in dynamical dark energy model from local probes DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons

Reference 43

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This paper cites Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1.

The case for a low dark matter density in dynamical dark energy model from local probes Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1

Reference 44

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This paper cites The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system.

The case for a low dark matter density in dynamical dark energy model from local probes The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system

Reference 45

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Observation bfac3a80-a2ee-4224-92af-f1bcd6a28fba · outbound

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

The case for a low dark matter density in dynamical dark energy model from local probes New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75

Reference 46

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Observation 8d2b6218-6932-4bb6-a384-b80fd7a6d6f4 · outbound

This paper cites Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters.

The case for a low dark matter density in dynamical dark energy model from local probes Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters

Reference 47

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Observation 027e4c97-dde7-431c-9b94-145261c52e15 · outbound

This paper cites Prospect for cosmological parameter estimation using future Hubble parameter measurements.

The case for a low dark matter density in dynamical dark energy model from local probes Prospect for cosmological parameter estimation using future Hubble parameter measurements

Reference 48

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This paper cites Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation.

The case for a low dark matter density in dynamical dark energy model from local probes Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

Reference 49

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The case for a low dark matter density in dynamical dark energy model from local probes Unresolved cited work

Reference 50

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Observation e022e464-6158-4564-96ca-67cfefb32d65 · outbound

This paper cites Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints.

The case for a low dark matter density in dynamical dark energy model from local probes Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints

Reference 51

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This paper cites MontePython 3: boosted MCMC sampler and other features.

The case for a low dark matter density in dynamical dark energy model from local probes MontePython 3: boosted MCMC sampler and other features

Reference 52

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Observation 63b51a42-ef25-4e7b-a387-0b60f9e9d35a · outbound

This paper cites Exploring the Expansion History of the Universe.

The case for a low dark matter density in dynamical dark energy model from local probes Exploring the Expansion History of the Universe

Reference 53

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This paper cites Accelerating Universes with Scaling Dark Matter.

The case for a low dark matter density in dynamical dark energy model from local probes Accelerating Universes with Scaling Dark Matter

Reference 54

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Can the sound horizon-free measurement of $H_0$ constrain early new physics? The case for a low dark matter density in dynamical dark energy model from local probes

Reference 106

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Robustness of dark energy phenomenology across different parameterizations The case for a low dark matter density in dynamical dark energy model from local probes

Reference 61

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New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.

New Insights into Dark Energy from DESI DR2 with CMB and SNIa The case for a low dark matter density in dynamical dark energy model from local probes

Reference 44

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Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB The case for a low dark matter density in dynamical dark energy model from local probes

Reference 30

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