Paper Citation Record · LEDGER

Turning a negative neutrino mass into a positive optical depth

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 29 inbound Pith citation observations for arXiv:2504.21813.

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

pith.paper-citation-record.v1
2504.21813 v1

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measured 29 of 29 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T14:45:35.935226Z

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Source: pith, observed 2026-07-10T18:27:31.591345Z

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Pith citing papers

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Type II Seesaw Leptogenesis in a Majoron background cites this paper.

Type II Seesaw Leptogenesis in a Majoron background Turning a negative neutrino mass into a positive optical depth

Reference 105

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Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect cites this paper.

Probing the ionizing photon output of galaxies near cosmic dawn with the patchy kSZ effect Turning a negative neutrino mass into a positive optical depth

Reference 106

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Rapid late-time reionization: constraints and cosmological implications cites this paper.

Rapid late-time reionization: constraints and cosmological implications Turning a negative neutrino mass into a positive optical depth

Reference 76

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A New Boundary Condition on Reionization cites this paper.

A New Boundary Condition on Reionization Turning a negative neutrino mass into a positive optical depth

Reference 26

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Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth cites this paper.

Cosmic $\tau$ensions Indirectly Correlate with Reionization Optical Depth Turning a negative neutrino mass into a positive optical depth

Reference 35

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Observation e3e6fb6b-eeeb-485f-8101-e6e1dec12fd6 · inbound

The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth cites this paper.

The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth Turning a negative neutrino mass into a positive optical depth

Reference 28

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Observation b1a04054-bf04-42ce-a4f6-2203d83328c6 · inbound

Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data cites this paper.

Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data Turning a negative neutrino mass into a positive optical depth

Reference 25

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Observation e4d09542-e726-46ee-a9c7-e11e3a896471 · inbound

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity cites this paper.

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity Turning a negative neutrino mass into a positive optical depth

Reference 111

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Observation c0f0da9f-bedb-4f94-bdc3-f59edaa3190a · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Turning a negative neutrino mass into a positive optical depth

Reference 154

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Disentangling cosmic distance tensions with early and late dark energy cites this paper.

Disentangling cosmic distance tensions with early and late dark energy Turning a negative neutrino mass into a positive optical depth

Reference 52

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Observation 4ed6ee86-4c88-46e2-ac67-75b3de5e0747 · inbound

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses cites this paper.

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses Turning a negative neutrino mass into a positive optical depth

Reference 9

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Observation 866068e3-e868-4145-894d-56393a7194ff · inbound

Faster CMB lensing with control variates cites this paper.

Faster CMB lensing with control variates Turning a negative neutrino mass into a positive optical depth

Reference 31

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Observation 449d02e0-5184-4e87-aec7-52678156b101 · inbound

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

Compressed Gaussian likelihood for the Planck low-$\ell$ data Turning a negative neutrino mass into a positive optical depth

Reference 15

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Observation 9b420002-bff3-46c2-9ba6-55937a6228a7 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Turning a negative neutrino mass into a positive optical depth

Reference 86

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A self-consistent analytical model for both the photoionization rate and reionization history cites this paper.

A self-consistent analytical model for both the photoionization rate and reionization history Turning a negative neutrino mass into a positive optical depth

Reference 109

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Observation a0d51ddf-30ba-4fb3-a788-e59765a3c5e0 · inbound

Raising the reionization optical depth with inflationary CMB features cites this paper.

Raising the reionization optical depth with inflationary CMB features Turning a negative neutrino mass into a positive optical depth

Reference 10

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Observation 6c31358c-f312-4af8-a7a6-915a9de37d03 · inbound

A hidden reionization prior biases cosmological inference cites this paper.

A hidden reionization prior biases cosmological inference Turning a negative neutrino mass into a positive optical depth

Reference 30

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Observation 860eed58-0719-4801-9fd1-329be82a8d32 · inbound

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM Turning a negative neutrino mass into a positive optical depth

Reference 53

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Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM cites this paper.

Cosmological Concordance in an Especially Opaque Universe: A Tentative Cosmological Detection of Physical Neutrino Mass in $\Lambda$CDM Turning a negative neutrino mass into a positive optical depth

Reference 53

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

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Turning a negative neutrino mass into a positive optical depth

Reference 225

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Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Turning a negative neutrino mass into a positive optical depth

Reference 185

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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 Turning a negative neutrino mass into a positive optical depth

Reference 191

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The Status of Single Scalar Field Dark Energy cites this paper.

The Status of Single Scalar Field Dark Energy Turning a negative neutrino mass into a positive optical depth

Reference 80

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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 Turning a negative neutrino mass into a positive optical depth

Reference 172

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No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Turning a negative neutrino mass into a positive optical depth

Reference 8

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No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization cites this paper.

No way ou$\tau$: Epoch of Reionization Observations Do not Support Large Values of the Optical Depth to Reionization Turning a negative neutrino mass into a positive optical depth

Reference 8

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DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints Turning a negative neutrino mass into a positive optical depth

Reference 137

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DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints cites this paper.

DESI DR2 Results IV: Alcock-Paczy\'nski Measurements from the Lyman Alpha Forest and Cosmological Constraints Turning a negative neutrino mass into a positive optical depth

Reference 137

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Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.

Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift Turning a negative neutrino mass into a positive optical depth

Reference 26

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