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Paper Citation Record · LEDGER

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

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2212.04494.

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pith.paper-citation-record.v1
2212.04494 v2

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Pith citing papers itemized under the disclosed page cap.

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Source: arxiv_reference, observed 2026-07-04T05:19:35.968978Z

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Pith citing papers

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

Modified recombination and the Hubble tension cites this paper.

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

Reference 33

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Observation da426113-dcf3-438d-a48b-82cbe653616e · inbound

Searching for coupled, hyperlight scalars across cosmic history cites this paper.

Searching for coupled, hyperlight scalars across cosmic history What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 197

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Observation e4cfa7cb-dff8-4442-bf8d-2fefb43520c4 · inbound

Alleviating the Hubble Tension via Cosmological Time Dilation in the meVSL Model cites this paper.

Alleviating the Hubble Tension via Cosmological Time Dilation in the meVSL Model What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 65

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Observation c013d602-0c2a-4713-ab18-abff3ff98001 · inbound

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 56

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arxiv_id, observed 2026-05-11T11:36:03.731035Z

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Observation 240d7a94-d887-4e36-9a3e-b843475d435f · inbound

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 125

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Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity cites this paper.

Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 33

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Observation 8e8be5b3-84d6-4041-8848-a1894d3588b0 · inbound

Compressed Gaussian likelihood for the Planck low-$\ell$ data cites this paper.

Compressed Gaussian likelihood for the Planck low-$\ell$ data What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 13

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Observation 21a31a01-c957-4f81-a63e-fcb103d57a4e · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 60

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Observation 907d878c-746c-4c76-8cbe-8a420042b0bd · inbound

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements cites this paper.

Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 17

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Observation 694c5a11-7d35-43aa-a8bd-5e0ffb06fdd3 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 240

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Observation 7ced93c9-a826-4b3b-8a17-e1bd95b846cf · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 240

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Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 145

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Observation 91b787c6-2ab5-4726-ad0e-15ea64d1954a · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 203

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Observation 58d68808-5dd3-45fc-afa1-54b05b7fb4e2 · inbound

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 89

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Observation 7dd2919c-6831-4017-89a7-14854782a098 · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 206

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Observation 15804a5b-33dc-4d7a-836c-c6871cb651fc · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 120

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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 cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions What it takes to solve the Hubble tension through modifications of cosmological recombination

Reference 25

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