Paper Citation Record · LEDGER

Modified recombination and the Hubble tension

As of 21 August 2026, this Paper Citation Record lists 61 of 61 outbound references and 21 inbound Pith citation observations for arXiv:2411.16678.

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2411.16678 v2

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Observation 74c38be7-1d80-4e2b-872a-adfb1b804b56 · outbound

This paper cites For ℓ ≥ 30, we use the C T T ℓ , C T E ℓ , and C EE ℓ spectra and the covariance matrix from the Cobaya [40, 41] implementation of the Planck PR4 CamSpec ( NPIPE) likelihood [42].

Modified recombination and the Hubble tension For ℓ ≥ 30, we use the C T T ℓ , C T E ℓ , and C EE ℓ spectra and the covariance matrix from the Cobaya [40, 41] implementation of the Planck PR4 CamSpec ( NPIPE) likelihood [42]

Reference 1

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Observation f561fd01-59a5-44eb-9e48-c5a39f865b89 · outbound

This paper cites baryon drag.

Modified recombination and the Hubble tension baryon drag

Reference 2

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Observation 7d26f53d-af48-4201-b866-59e139ee6563 · outbound

This paper cites (A1) The best-fit parameters and chi-squared of the modified model will be different from those of the fiducial model.

Modified recombination and the Hubble tension (A1) The best-fit parameters and chi-squared of the modified model will be different from those of the fiducial model

Reference 3

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Observation 6173505d-c429-4584-adac-e7db0c59462f · outbound

This paper cites We define Gaussian shapes used for the principal component analysis in [34], since they are smooth and easy to implement into the Boltzmann equation solver.

Modified recombination and the Hubble tension We define Gaussian shapes used for the principal component analysis in [34], since they are smooth and easy to implement into the Boltzmann equation solver

Reference 4

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Observation ca8cbaff-34b1-4345-bd96-7055224d7a54 · outbound

This paper cites We set ∆ xe = 0 outside this range, as the CMB data show negligible sen- sitivity to the changes in ionization history beyond these redshifts, as illustrated in Fig.

Modified recombination and the Hubble tension We set ∆ xe = 0 outside this range, as the CMB data show negligible sen- sitivity to the changes in ionization history beyond these redshifts, as illustrated in Fig

Reference 5

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Observation 789b41e8-d919-41bc-9ffb-7a86a18ff4f4 · outbound

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.

Modified recombination and the Hubble tension 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

Reference 6

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Observation c715b741-2cd5-409e-9a6c-ee619e2ac867 · outbound

This paper cites Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry.

Modified recombination and the Hubble tension Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry

Reference 7

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Observation 79db4c56-9602-4738-a1d7-476ee3aa55ca · outbound

This paper cites DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys.

Modified recombination and the Hubble tension DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys

Reference 8

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Observation d31b588c-c9f1-42e6-821c-7b244694d6bd · outbound

This paper cites Amon et al.

Modified recombination and the Hubble tension Amon et al

Reference 9

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Observation 2e5596c6-ecf9-46dc-b993-79cfe3578abe · outbound

This paper cites KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics.

Modified recombination and the Hubble tension KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics

Reference 10

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Observation 3c32a50e-d640-43c8-9d0e-51ae2cf6bc54 · outbound

This paper cites The Pantheon+ Analysis: Cosmological Constraints.

Modified recombination and the Hubble tension The Pantheon+ Analysis: Cosmological Constraints

Reference 11

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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.

Modified recombination and the Hubble tension The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset

Reference 12

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Observation bf83b989-eaf3-42cb-9d87-f39a03d89895 · outbound

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

Modified recombination and the Hubble tension Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework

Reference 13

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Observation 105b9567-9b58-4f7e-9e6b-9a839c2c651c · outbound

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

Modified recombination and the Hubble tension DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 14

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Observation 46d74498-0120-4689-ad11-bf4d555379dc · outbound

This paper cites A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team).

Modified recombination and the Hubble tension A Lockdown Perspective on the Hubble Tension (with comments from the SH0ES team)

Reference 15

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Observation 9e21df5f-b675-41f2-a116-a598ae692f85 · outbound

This paper cites It's Dust: Solving the Mysteries of the Intrinsic Scatter and Host-Galaxy Dependence of Standardized Type Ia Supernova Brightnesses.

Modified recombination and the Hubble tension It's Dust: Solving the Mysteries of the Intrinsic Scatter and Host-Galaxy Dependence of Standardized Type Ia Supernova Brightnesses

Reference 16

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Observation 65e2d208-fc26-4dba-8269-bb4f008ce02f · outbound

This paper cites The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties.

Modified recombination and the Hubble tension The Hubble Tension Revisited: Additional Local Distance Ladder Uncertainties

Reference 17

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Observation 432a2778-21d9-48a2-bcf3-e6dc16e1c37d · outbound

This paper cites Measurements of the Hubble Constant: Tensions in Perspective.

Modified recombination and the Hubble tension Measurements of the Hubble Constant: Tensions in Perspective

Reference 18

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Observation a4b2caec-8ce3-40b5-aed0-11e1f71b5f59 · outbound

This paper cites The Hubble Hunter's Guide.

Modified recombination and the Hubble tension The Hubble Hunter's Guide

Reference 19

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Observation 887aa990-62af-4371-8478-ba9a3e0e9c9a · outbound

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

Modified recombination and the Hubble tension In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 20

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Observation e1df5249-be3f-4d20-bdfb-92600784f532 · outbound

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

Modified recombination and the Hubble tension Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies

Reference 21

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Observation 0cb97a6a-1bba-4c76-acab-ecd1f5b7676c · outbound

This paper cites The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions.

Modified recombination and the Hubble tension The implications of an extended dark energy cosmology with massive neutrinos for cosmological tensions

Reference 22

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Observation ceb8d7fc-4d1b-421d-9405-b6c0d47779b5 · outbound

This paper cites Reconstructing Gravity on Cosmological Scales.

Modified recombination and the Hubble tension Reconstructing Gravity on Cosmological Scales

Reference 23

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Observation 78813063-e5aa-4f53-a4b3-8382019b036a · outbound

This paper cites Can Late Dark Energy Transitions Raise the Hubble constant?.

Modified recombination and the Hubble tension Can Late Dark Energy Transitions Raise the Hubble constant?

Reference 24

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Observation 46061211-64df-4ccb-903b-19b752f60bcd · outbound

This paper cites Converting dark matter to dark radiation does not solve cosmological tensions.

Modified recombination and the Hubble tension Converting dark matter to dark radiation does not solve cosmological tensions

Reference 25

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Observation e66aa031-a3bd-4276-a02c-2b50160b379c · outbound

This paper cites Imprints of cosmological tensions in reconstructed gravity.

Modified recombination and the Hubble tension Imprints of cosmological tensions in reconstructed gravity

Reference 26

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This paper cites On the implications of the `cosmic calibration tension' beyond $H_0$ and the synergy between early- and late-time new physics.

Modified recombination and the Hubble tension On the implications of the `cosmic calibration tension' beyond $H_0$ and the synergy between early- and late-time new physics

Reference 27

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Observation 5bfb776f-3ba7-44f3-a711-47bc2f598ed0 · outbound

This paper cites Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data.

Modified recombination and the Hubble tension Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data

Reference 28

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Observation 6d1d5343-b0a2-43ce-a290-cf909474696a · outbound

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

Modified recombination and the Hubble tension Multidimensionality of the Hubble tension: the roles of $\Omega_m$ and $\omega_c$

Reference 29

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Observation ddc919e7-70bd-4583-9122-75fc88523386 · outbound

This paper cites Relieving the Hubble tension with primordial magnetic fields.

Modified recombination and the Hubble tension Relieving the Hubble tension with primordial magnetic fields

Reference 30

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Observation 5954d800-2f86-44c3-8bcd-6853bd702bb2 · outbound

This paper cites Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4.

Modified recombination and the Hubble tension Can small-scale baryon inhomogeneities resolve the Hubble tension? An investigation with ACT DR4

Reference 31

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Observation 221e04b1-9f99-4276-9f27-97afd12fd5c8 · outbound

This paper cites Small-scale clumping at recombination and the Hubble tension.

Modified recombination and the Hubble tension Small-scale clumping at recombination and the Hubble tension

Reference 32

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Observation eaf3667a-2c7f-40d2-8039-2c9d963e1713 · outbound

This paper cites What it takes to solve the Hubble tension through modifications of cosmological recombination.

Modified recombination and the Hubble tension What it takes to solve the Hubble tension through modifications of cosmological recombination

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Observation 6d9f1044-4ad1-4bcf-a0e4-d1a572574376 · outbound

This paper cites Reconstructing the recombination history by combining early and late cosmological probes.

Modified recombination and the Hubble tension Reconstructing the recombination history by combining early and late cosmological probes

Reference 34

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Observation be421bc3-d8a1-4f12-90aa-32d13548b2ae · outbound

This paper cites DESI and the Hubble tension in light of modified recombination.

Modified recombination and the Hubble tension DESI and the Hubble tension in light of modified recombination

Reference 35

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This paper cites A consistency test of the cosmological model at the epoch of recombination using DESI BAO and Planck measurements.

Modified recombination and the Hubble tension A consistency test of the cosmological model at the epoch of recombination using DESI BAO and Planck measurements

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This paper cites Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension.

Modified recombination and the Hubble tension Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension

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Observation 3f42f944-97d0-442d-b342-d6a831a89ad1 · outbound

This paper cites Small Scale Cosmological Perturbations: An Analytic Approach.

Modified recombination and the Hubble tension Small Scale Cosmological Perturbations: An Analytic Approach

Reference 38

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Observation 07abc875-e0e7-474c-98f8-9d5d47c663a5 · outbound

This paper cites Improved model-independent constraints on the recombination era and development of a direct projection method.

Modified recombination and the Hubble tension Improved model-independent constraints on the recombination era and development of a direct projection method

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Observation 6a9577c8-9588-4eb5-848f-ba93982c1d52 · outbound

This paper cites A New Calculation of the Recombination Epoch.

Modified recombination and the Hubble tension A New Calculation of the Recombination Epoch

Reference 40

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This paper cites How well do we understand cosmological recombination?.

Modified recombination and the Hubble tension How well do we understand cosmological recombination?

Reference 41

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Modified recombination and the Hubble tension Seager, D

Reference 42

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This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Modified recombination and the Hubble tension Efficient Computation of CMB anisotropies in closed FRW models

Reference 43

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This paper cites Cosmic Recombination in the Presence of Primordial Magnetic Fields.

Modified recombination and the Hubble tension Cosmic Recombination in the Presence of Primordial Magnetic Fields

Reference 44

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Modified recombination and the Hubble tension Cobaya: Code for Bayesian Analysis of hierarchical physical models

Reference 45

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Modified recombination and the Hubble tension Torrado and A

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Observation a420a0d1-bb19-40de-8fcd-f94b5e39d326 · outbound

This paper cites CMB power spectra and cosmological parameters from Planck PR4 with CamSpec.

Modified recombination and the Hubble tension CMB power spectra and cosmological parameters from Planck PR4 with CamSpec

Reference 47

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Observation 5979ede9-b0d6-496b-a468-bf4e0ce9a0fa · outbound

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

Modified recombination and the Hubble tension Planck 2018 results. VI. Cosmological parameters

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This paper cites A Python compressed low-$\ell$ Planck likelihood for temperature and polarization.

Modified recombination and the Hubble tension A Python compressed low-$\ell$ Planck likelihood for temperature and polarization

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This paper cites Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies.

Modified recombination and the Hubble tension Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

Reference 50

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Observation 81d7857f-6ea6-4fce-98da-01ae7ea455a9 · outbound

This paper cites CMB lensing from Planck PR4 maps.

Modified recombination and the Hubble tension CMB lensing from Planck PR4 maps

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This paper cites A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set.

Modified recombination and the Hubble tension A Measurement of the CMB Temperature Power Spectrum and Constraints on Cosmology from the SPT-3G 2018 TT/TE/EE Data Set

Reference 52

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Observation aa86eef6-b2e3-48b2-b63f-ecff9271f879 · outbound

This paper cites The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters.

Modified recombination and the Hubble tension The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters

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This paper cites Analytic approach to the polarization of the cosmic microwave background in flat and open universes.

Modified recombination and the Hubble tension Analytic approach to the polarization of the cosmic microwave background in flat and open universes

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This paper cites Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments.

Modified recombination and the Hubble tension Consistency of Planck, ACT and SPT constraints on magnetically assisted recombination and forecasts for future experiments

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Modified recombination and the Hubble tension The Simons Observatory: Science goals and forecasts

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This paper cites CMB-S4 Science Case, Reference Design, and Project Plan.

Modified recombination and the Hubble tension CMB-S4 Science Case, Reference Design, and Project Plan

Reference 57

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Observation ee166d39-fb01-4b14-af95-57d5c9d91130 · outbound

This paper cites Early recombination as a solution to the $H_0$ tension.

Modified recombination and the Hubble tension Early recombination as a solution to the $H_0$ tension

Reference 58

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Observation de712450-d62b-4673-8f5e-32a66fdcf8b8 · outbound

This paper cites The mass effect -- Variations of the electron mass and their impact on cosmology.

Modified recombination and the Hubble tension The mass effect -- Variations of the electron mass and their impact on cosmology

Reference 59

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Observation 3b10a12c-d902-460d-ba0a-f83a808cb73c · outbound

This paper cites Cosmology with varying fundamental constants from hyperlight, coupled scalars.

Modified recombination and the Hubble tension Cosmology with varying fundamental constants from hyperlight, coupled scalars

Reference 60

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Observation c9e5a98e-aaa9-4e7d-912a-81b37a98da84 · outbound

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

Modified recombination and the Hubble tension $\Lambda$CDM is alive and well

Reference 61

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Pith citing papers

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

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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 ec165a5b-5888-419f-a787-43515d59326c · inbound

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Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Modified recombination and the Hubble tension

Reference 222

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Observation 3c31f396-0064-471e-bfb4-c7a05fc260a2 · inbound

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Alleviating the Hubble Tension via Cosmological Time Dilation in the meVSL Model Modified recombination and the Hubble tension

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-05T12:06:17.988101Z

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Observation 989e9287-606e-4f9d-bebf-dec68d454f85 · inbound

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Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Modified recombination and the Hubble tension

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-04T07:19:39.380402Z

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Observation fbe2fa59-3381-4c10-838a-961d0823c333 · inbound

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Primordial magnetic field from chiral plasma instability with sourcing Modified recombination and the Hubble tension

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-03T17:35:05.517880Z

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Observation 1842b00d-47c5-43b8-a204-7379b7d1365b · inbound

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Exploring the interplay of late-time dynamical dark energy and new physics before recombination Modified recombination and the Hubble tension

Reference 127

Resolution: verified exact; arxiv_id, observed 2026-05-14T23:13:15.552178Z

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Observation 443066c7-c142-464d-b226-e31a14d61fc7 · inbound

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Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Modified recombination and the Hubble tension

Reference 74

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:03.572582Z

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Observation ad158451-7343-4119-91b9-c1e730958fc1 · inbound

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Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Modified recombination and the Hubble tension

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.477010Z

Source-reported events for the cited work

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Observation 923e4376-e528-496d-8bae-3a377bf8d0cb · inbound

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Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity Modified recombination and the Hubble tension

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-06-30T20:15:05.470892Z

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Observation a66a48ef-dea9-4454-affc-46e3dab544b4 · inbound

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Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Modified recombination and the Hubble tension

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-06-30T00:14:04.937136Z

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Observation f928fb4f-eb3c-4b85-8c0b-08125416054e · inbound

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Compressed Gaussian likelihood for the Planck low-$\ell$ data Modified recombination and the Hubble tension

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.927644Z

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Observation f5af49e7-3a52-4b44-9d50-7e0b3608d969 · inbound

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Reference 120

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.495583Z

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Observation 7ff15ff4-1c6f-497e-806f-b85fbf751a81 · inbound

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Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements Modified recombination and the Hubble tension

Reference 18

Resolution: verified exact; arxiv_id, observed 2026-07-03T15:38:34.059857Z

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Observation dad9b158-8f1a-4a14-af75-80cd8f4a51b2 · inbound

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The Hubble tension: A decade review Modified recombination and the Hubble tension

Reference 208

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:35.463249Z

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Observation 4a89ce82-63ab-4e0f-b4a7-6a1966d1a0a8 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Modified recombination and the Hubble tension

Reference 208

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Observation 02d98405-cd91-4135-b5ec-6a92c5f57e68 · inbound

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Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Modified recombination and the Hubble tension

Reference 221

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.467667Z

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Observation 3af630cd-a239-4f1d-9202-73e74f34a97b · inbound

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The $H_0$ World Cup. I. Summary of the baseline group stage results Modified recombination and the Hubble tension

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-02T05:41:41.755272Z

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Observation 1ace7d86-8700-4ddc-a2e4-92d361ef003a · inbound

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The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions Modified recombination and the Hubble tension

Reference 127

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:17.178286Z

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Observation dd9b38c9-e595-4dac-84fc-83d4831f4452 · inbound

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The impact of Hawking radiation from primordial black holes on recombination and the Hubble tension Modified recombination and the Hubble tension

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T15:14:37.393834Z

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Observation 4f08b14a-884e-4d21-a314-7a79fef595e4 · inbound

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Hubble tension: the shape wall Modified recombination and the Hubble tension

Reference 151

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:48.269856Z

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Observation e60a674a-8cd6-43fb-abad-585eebe9bbf5 · inbound

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Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Modified recombination and the Hubble tension

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:22.691986Z

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