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Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2406.14554.

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2406.14554 v2

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:34:40.731657Z

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Pith citing papers

Observation ffad2bd9-7ee5-47a8-bcba-db4b031af360 · inbound

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension cites this paper.

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 6

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DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements cites this paper.

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 185

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Observation 418d81b4-bf56-4d3d-baf7-6ba05e500b1b · inbound

Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations cites this paper.

Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 60

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Observation 691b028a-4ed7-4f52-b0d8-2791dd60c7d0 · inbound

Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data cites this paper.

Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 80

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Towards a multi-tracer neutrino mass measurement with line-intensity mapping cites this paper.

Towards a multi-tracer neutrino mass measurement with line-intensity mapping Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 20

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Neutrino masses from large-scale structures: future sensitivity and theory dependence cites this paper.

Neutrino masses from large-scale structures: future sensitivity and theory dependence Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 42

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Observation f3debfa7-d361-43b6-a772-9993f9fb5516 · inbound

Neutrino models with a zero mass eigenvalue cites this paper.

Neutrino models with a zero mass eigenvalue Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 7

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Illustrating the consequences of a misuse of $\sigma_8$ in cosmology cites this paper.

Illustrating the consequences of a misuse of $\sigma_8$ in cosmology Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 266

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Tuning the cosmic instrument: robust cosmology through combined probes cites this paper.

Tuning the cosmic instrument: robust cosmology through combined probes Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 148

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Observation 650044b5-869c-4b81-8807-7ab0528ca18b · inbound

Dark energy and lensing anomaly in Planck CMB data cites this paper.

Dark energy and lensing anomaly in Planck CMB data Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 64

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Observation 4e85acca-96be-43c1-b149-30902e213b08 · inbound

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

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 76

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos cites this paper.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 28

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Testing an unstable cosmic neutrino background cites this paper.

Testing an unstable cosmic neutrino background Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 14

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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 Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 59

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Observation 39713a19-8532-4868-8dd2-ed01a7287618 · inbound

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 29

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Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra cites this paper.

Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 2

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Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis cites this paper.

Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 78

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Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

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Minimal dark $SU(2)$ origin of a massless Dirac neutrino cites this paper.

Minimal dark $SU(2)$ origin of a massless Dirac neutrino Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 39

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The Future of Lepton Flavor Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Reference 39

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Leptonic CP Conservation and the Quark CP Phase from Octonionic Flavor Structure Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

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Radiative corrections in neutral-current (anti)neutrino elastic scattering at $\text{GeV}$ energies I: Nucleon targets cites this paper.

Radiative corrections in neutral-current (anti)neutrino elastic scattering at $\text{GeV}$ energies I: Nucleon targets Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

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