Paper Citation Record · LEDGER

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families

As of 19 August 2026, this Paper Citation Record lists 100 of 261 outbound references and 6 inbound Pith citation observations for arXiv:2603.14693.

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Observation 7029d49b-9ab2-4431-96e5-0ed85099ca04 · outbound

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Planck 2018 results. VI. Cosmological parameters

Reference 1

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Observation b2bd4067-8096-4e90-b44a-6336a83b26d5 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

Reference 2

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Observation 836cb319-ae85-4b95-8eb9-3ce1dc55ea02 · outbound

This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 3

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Observation cad82978-ef4f-46e8-b8cd-a0fb67c612dc · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Pantheon+ Analysis: Cosmological Constraints

Reference 4

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Observation 3a1f7445-ea02-475e-aa15-d945ff161b4c · outbound

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 5

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Observation 32cc7f7a-d430-47c7-904b-4dcabeba906a · outbound

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 6

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Observation 86fca90f-2f1c-461b-aa03-64f5dd29d9b7 · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $\Lambda$CDM Parameters

Reference 7

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Observation 8ec52f96-b2d4-4047-807a-27b5de2a4336 · outbound

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Observation 26410ed5-ca71-4bd3-ab59-dc14b59c1701 · outbound

This paper cites SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field

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Observation 0b47dee9-6c3a-4c67-bcb0-2448d01c5990 · outbound

This paper cites The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Dark Energy Survey Supernova Program: A Reanalysis Of Cosmology Results And Evidence For Evolving Dark Energy With An Updated Type Ia Supernova Calibration

Reference 10

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Observation 59a2d9da-9a75-4cc9-8953-4339e79e7cb8 · outbound

This paper cites Weinberg, The Cosmological Constant Problem, Rev.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Weinberg, The Cosmological Constant Problem, Rev

Reference 11

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This paper cites The Case for a Positive Cosmological Lambda-term.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Case for a Positive Cosmological Lambda-term

Reference 12

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This paper cites The Cosmological Constant Problem and Quintessence.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Cosmological Constant Problem and Quintessence

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This paper cites Tensions between the Early and the Late Universe.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Tensions between the Early and the Late Universe

Reference 14

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Observation e2125164-a669-45cf-86c9-e0f5fa359f3c · outbound

This paper cites Cosmology Intertwined II: The Hubble Constant Tension.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Cosmology Intertwined II: The Hubble Constant Tension

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Observation e4c6b582-6a30-4541-9c96-2479f19da3dd · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 16

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Observation 5f454b19-2d17-4bde-a918-0c098684bf14 · outbound

This paper cites Challenges for $\Lambda$CDM: An update.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Challenges for $\Lambda$CDM: An update

Reference 17

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This paper cites The $H_0$ Olympics: A fair ranking of proposed models.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The $H_0$ Olympics: A fair ranking of proposed models

Reference 18

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This paper cites Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

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This paper cites Di Valentino, Challenges of the Standard Cosmolog- ical Model, Universe8, 399 (2022).

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Di Valentino, Challenges of the Standard Cosmolog- ical Model, Universe8, 399 (2022)

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension

Reference 21

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Observation 2689e7de-0c2e-471f-9e1d-b20feec6f901 · outbound

This paper cites Review of Hubble tension solutions with new SH0ES and SPT-3G data.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Review of Hubble tension solutions with new SH0ES and SPT-3G data

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families $\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks

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

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

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This paper cites 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.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families 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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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Small Magellanic Cloud Cepheids Observed with the Hubble Space Telescope Provide a New Anchor for the SH0ES Distance Ladder

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This paper cites The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision

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This paper cites Cosmology Intertwined III: $f \sigma_8$ and $S_8$.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Cosmology Intertwined III: $f \sigma_8$ and $S_8$

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This paper cites Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Arbitrating the $S_8$ discrepancy with growth rate measurements from Redshift-Space Distortions

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families $S_8$ increases with effective redshift in $\Lambda$CDM cosmology

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Further support for $S_8$ increasing with effective redshift

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Cosmology from large-scale structure: Constraining $\Lambda$CDM with BOSS

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Amonet al.(DES), Dark Energy Survey Year 3 results: Cosmology from cosmic shear and robustness to data calibration, Phys

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Not all lensing is low: An analysis of DESI$\times$DES using the Lagrangian Effective Theory of LSS

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Unresolved cited work

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Interacting Scalar fields: Dark matter and early dark energy

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Early dark energy, the Hubble-parameter tension, and the string axiverse

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Early Dark Energy Can Resolve The Hubble Tension

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Oscillating scalar fields and the Hubble tension: a resolution with novel signatures

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Early dark energy from massive neutrinos -- a natural resolution of the Hubble tension

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Early Dark Energy Does Not Restore Cosmological Concordance

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Constraining Early Dark Energy with Large-Scale Structure

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Hubble Tension and Early Dark Energy

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Non-minimal dark sector physics and cosmological tensions

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Update on Coupled Dark Energy and the $H_0$ tension

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Relieving the $H_0$ tension with a new interacting dark energy model

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Model-independent reconstruction of the Interacting Dark Energy Kernel: Binned and Gaussian process

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Li, G.-H

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families New constraints on interacting dark energy from DESI DR2 BAO observations

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families van der Westhuizen, A

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Unresolved cited work

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Graduated dark energy: Observational hints of a spontaneous sign switch in the cosmological constant

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Relaxing cosmological tensions with a sign switching cosmological constant

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families $\Lambda_{\rm s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families $\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity

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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Akarsu, B

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