Paper Citation Record · LEDGER

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus

As of 17 August 2026, this Paper Citation Record lists 100 of 197 outbound references and 3 inbound Pith citation observations for arXiv:2607.05044.

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2607.05044 v1

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Outbound references

Observation 21551282-e1e8-4fbd-a0a7-fb2f4891c992 · outbound

This paper cites Eisenstein et al.,Detection of the baryon acoustic peak in the large-scale correlation function of sdss luminous red galaxies,The Astrophysical Journal633(2005) 560.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Eisenstein et al.,Detection of the baryon acoustic peak in the large-scale correlation function of sdss luminous red galaxies,The Astrophysical Journal633(2005) 560

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This paper cites an unresolved cited work.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Unresolved cited work

Reference 2

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Observation d0d4fa28-b109-4a19-91e3-77f9499e84bf · outbound

This paper cites Percival et al.,Baryon acoustic oscillations in the sloan digital sky survey data release 7 galaxy sample,Monthly Notices of the Royal Astronomical Society401(2010) 2148.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Percival et al.,Baryon acoustic oscillations in the sloan digital sky survey data release 7 galaxy sample,Monthly Notices of the Royal Astronomical Society401(2010) 2148

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Observation 9a0b3769-125b-4447-933e-dea0dfc1bec2 · outbound

This paper cites Tegmark et al.,The three-dimensional power spectrum of galaxies from the sloan digital sky survey,The Astrophysical Journal606(2004) 702.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Tegmark et al.,The three-dimensional power spectrum of galaxies from the sloan digital sky survey,The Astrophysical Journal606(2004) 702

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Observation 30378444-a47d-4152-86a5-6f393f7a3127 · 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.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory

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Observation d27c9c81-b211-4d59-ba67-ea198a0b69b4 · outbound

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

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Reference 6

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Observation 97b5fd6b-114b-4aa8-9be9-e8d05d67b690 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Pantheon+ Analysis: Cosmological Constraints

Reference 7

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Observation cd56c60d-784e-4d7d-a78a-5c0cbfc6ffcf · outbound

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

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 8

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Observation 198964ca-5356-4c51-b370-b1a81aa24201 · outbound

This paper cites Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

Reference 9

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Observation 8dedf12d-761a-4fba-8935-7c04b0ee75fe · outbound

This paper cites Sabogal, R.C.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Sabogal, R.C

Reference 10

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Observation 480d4b7b-2ac4-492b-af45-c5c40d8c7265 · outbound

This paper cites Constraining Cosmological Parameters Based on Relative Galaxy Ages.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Constraining Cosmological Parameters Based on Relative Galaxy Ages

Reference 11

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Observation 33087e4d-fa0c-4bf8-9b5b-bbd59d08abcf · outbound

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

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Local Distance Network: a community consensus report on the measurement of the Hubble constant at 1% precision

Reference 12

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Observation 3c579d09-6363-4e99-95cc-477e4d92ec34 · outbound

This paper cites Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes

Reference 13

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Observation f2cda52e-b0a6-411f-aed0-9375c80e1a45 · outbound

This paper cites Weinberg,The cosmological constant problem,Rev.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Weinberg,The cosmological constant problem,Rev

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Observation a38767a7-29dc-43c5-a5da-2302bdce42d9 · outbound

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

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Case for a Positive Cosmological Lambda-term

Reference 15

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Observation 60a6edfa-7de4-4a09-8117-0e637651b92d · outbound

This paper cites The Cosmological Constant Problem and Quintessence.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Cosmological Constant Problem and Quintessence

Reference 16

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Observation 029b84a8-0410-4d0d-b6c0-200fcdd99ce9 · outbound

This paper cites Ratra and P.J.E.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Ratra and P.J.E

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This paper cites Armendariz-Picon, V.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Armendariz-Picon, V

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Observation 78bfbc0b-cc8a-4289-9bc0-0f09f0a66bb8 · outbound

This paper cites Dark energy from the string axiverse.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Dark energy from the string axiverse

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This paper cites Cosmological tests of an axiverse-inspired quintessence field.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Cosmological tests of an axiverse-inspired quintessence field

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This paper cites Observational constraints on generalised axion-like potentials for the late Universe.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Observational constraints on generalised axion-like potentials for the late Universe

Reference 21

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus An alternative to quintessence

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Inflation and dark energy from three-forms

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Three-form cosmology

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This paper cites Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Cosmic infinity: A dynamical system approach

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Observational constraints on 3-forms dark energy

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Bouhmadi-López, H.-W

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Generalization of the Proca Action

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus New class of Proca interactions

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Reducing the $H_{0}$ tension with generalized Proca theory

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Cosmological tensions in Proca-Nuevo theory

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Li, G.-H

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Unresolved cited work

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Isham, A

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Minimal Theory of Bigravity: construction and cosmology

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Imperfect Dark Energy from Kinetic Gravity Braiding

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus The Imperfect Fluid behind Kinetic Gravity Braiding

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Phantom attractors in Kinetic Gravity Braiding theories: a dynamical system approach

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Dark energy with a shift-symmetric scalar field: obstacles, loophole hunting and dead ends

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus f(R) Theories Of Gravity

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Extended Theories of Gravity

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Cosmography of f(R) - brane cosmology

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Can f(R) gravity contribute to (dark) radiation?

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Dark torsion as the cosmic speed-up

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Modified teleparallel gravity: inflation without inflaton

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus f(T) teleparallel gravity and cosmology

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Bouhmadi-López, C.G

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Teleparallel Palatini theories

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Cosmology in $f(Q)$ geometry

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Relaxing cosmological tensions with a sign switching cosmological constant: Improved results with Planck, BAO, and Pantheon data

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Transition dynamics in the $\Lambda_{\rm s}$CDM model: Implications for bound cosmic structures

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus $\Lambda_{\rm s}$CDM cosmology: Alleviating major cosmological tensions by predicting standard neutrino properties

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Linear matter density perturbations in the $\Lambda_{\rm s}$CDM model: Examining growth dynamics and addressing the $S_8$ tension

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Ups and Downs in Dark Energy: phase transition in dark sector as a proposal to lessen cosmological tensions

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Revisiting a negative cosmological constant from low-redshift data

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Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus Rastall gravity extension of the standard $\Lambda$CDM model: theoretical features and observational constraints

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Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus

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$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus

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$\Lambda$XCDM: a running vacuum strategy for crossing the phantom divide Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus

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