Paper Citation Record · LEDGER

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics

As of 7 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 1 inbound Pith citation observation for arXiv:2506.01956.

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pith.paper-citation-record.v1
2506.01956 v2

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Pith citing papers itemized under the disclosed page cap.

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Outbound references

Observation 21b9a316-8e7c-4c48-96e6-756df56cab82 · outbound

This paper cites CMB-S4 Science Book, First Edition.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics CMB-S4 Science Book, First Edition

Reference 1

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Observation 00555723-2978-46bc-8ee2-34b4758a3f70 · outbound

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

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics CMB-S4 Science Case, Reference Design, and Project Plan

Reference 2

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Observation d43398ff-898d-4d47-b022-b66fdd8fb005 · outbound

This paper cites Snowmass 2021 CMB-S4 White Paper.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Snowmass 2021 CMB-S4 White Paper

Reference 3

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Observation 95eaa08c-0976-42dc-a0bd-b205d39482ef · outbound

This paper cites The Simons Observatory: Science goals and forecasts.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The Simons Observatory: Science goals and forecasts

Reference 4

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Observation 75caf80a-062e-44b0-a1fc-6a371ab8427b · outbound

This paper cites The Simons Observatory: Astro2020 Decadal Project Whitepaper.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The Simons Observatory: Astro2020 Decadal Project Whitepaper

Reference 5

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This paper cites CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky

Reference 6

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Observation 1c188daa-5e84-4b1c-ac0c-d83db75b88d7 · outbound

This paper cites Snowmass2021 CMB-HD White Paper.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Snowmass2021 CMB-HD White Paper

Reference 7

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Observation 0f22b8a5-e3c3-407a-9e6d-08064a35e78e · outbound

This paper cites The DESI Experiment Part I: Science,Targeting, and Survey Design.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The DESI Experiment Part I: Science,Targeting, and Survey Design

Reference 8

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This paper cites The Dark Energy Spectroscopic Instrument (DESI).

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The Dark Energy Spectroscopic Instrument (DESI)

Reference 9

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Observation b4d71b22-64c8-4575-b3cc-638cbb9add85 · outbound

This paper cites LSST: from Science Drivers to Reference Design and Anticipated Data Products.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics LSST: from Science Drivers to Reference Design and Anticipated Data Products

Reference 10

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Observation f03ea6b2-f0ad-4ecc-8789-015a0cd653ea · outbound

This paper cites Large Synoptic Survey Telescope: Dark Energy Science Collaboration.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Large Synoptic Survey Telescope: Dark Energy Science Collaboration

Reference 11

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Observation af0f702e-11c4-45fe-86b3-77eb33116aa6 · outbound

This paper cites The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document

Reference 12

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This paper cites Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Wide-Field InfrarRed Survey Telescope-Astrophysics Focused Telescope Assets WFIRST-AFTA 2015 Report

Reference 13

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This paper cites Euclid Definition Study Report.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Euclid Definition Study Report

Reference 14

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This paper cites Lesgourgues and S.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Lesgourgues and S

Reference 15

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Ma and E

Reference 16

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Observation 8cf22564-ca41-47c6-b777-6e9cfe1cc912 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 17

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Observation dd614d7f-3e5b-4fcd-b891-a59b4da3bb79 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics

Reference 18

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Observation 760a5478-fa46-4f45-9b14-40eb72e9f0e8 · outbound

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

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Analytic approach to the polarization of the cosmic microwave background in flat and open universes

Reference 19

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This paper cites A Line of Sight Approach to Cosmic Microwave Background Anisotropies.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics A Line of Sight Approach to Cosmic Microwave Background Anisotropies

Reference 20

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

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Efficient Computation of CMB anisotropies in closed FRW models

Reference 21

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This paper cites CMB power spectrum parameter degeneracies in the era of precision cosmology.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics CMB power spectrum parameter degeneracies in the era of precision cosmology

Reference 22

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This paper cites Damping of Tensor Modes in Cosmology.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Damping of Tensor Modes in Cosmology

Reference 23

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Observation f18b315c-fe12-4e32-b66c-b11bb3a3133d · outbound

This paper cites Imprints of Relic Gravitational Waves in Cosmic Microwave Background Radiation.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Imprints of Relic Gravitational Waves in Cosmic Microwave Background Radiation

Reference 24

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This paper cites A No-Truncation Approach to Cosmic Microwave Background Anisotropies.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics A No-Truncation Approach to Cosmic Microwave Background Anisotropies

Reference 25

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Observation 2c7c969d-cab1-4dff-a812-330a133bfa71 · outbound

This paper cites Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach

Reference 26

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This paper cites Tensor Microwave Background Fluctuations for Large Multipole Order.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Tensor Microwave Background Fluctuations for Large Multipole Order

Reference 27

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This paper cites Probing neutrino interactions and dark radiation with gravitational waves.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Probing neutrino interactions and dark radiation with gravitational waves

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Cosmological perturbations without the Boltzmann hierarchy

Reference 29

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Observation c41d2365-e0c0-4387-b82f-34538f8b7061 · outbound

This paper cites Cosmological perturbations: non-cold relics without the Boltzmann hierarchy.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Cosmological perturbations: non-cold relics without the Boltzmann hierarchy

Reference 30

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This paper cites Hu, Structure formation with generalized dark matter, Astrophys.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Hu, Structure formation with generalized dark matter, Astrophys

Reference 31

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This paper cites Evolution of cosmological dark matter perturbations.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Evolution of cosmological dark matter perturbations

Reference 32

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics An accurate fluid approximation for massive neutrinos in cosmology

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Implications of the $S_8$ tension for decaying dark matter with warm decay products

Reference 35

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Unresolved cited work

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics A parallel non-uniform fast Fourier transform library based on an "exponential of semicircle" kernel

Reference 37

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Aliasing error of the exp$(\beta \sqrt{1-z^2})$ kernel in the nonuniform fast Fourier transform

Reference 38

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Archidiacono et al

Reference 39

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Evolution of perturbations and cosmological constraints in decaying dark matter models with arbitrary decay mass products

Reference 40

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension

Reference 41

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Lower Mass Bounds on FIMP Dark Matter Produced via Freeze-In

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Banerjee, A

Reference 43

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Sterile neutrino dark matter: A tale of weak interactions in the strong coupling epoch

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Hidden Treasures: sterile neutrinos as dark matter with miraculous abundance, structure formation for different production mechanisms, and a solution to the sigma-8 problem

Reference 45

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This paper cites What can CMB observations tell us about the neutrino distribution function?.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics What can CMB observations tell us about the neutrino distribution function?

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics A cosmological case study of a tower of warm dark matter states: $N$naturalness

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Interacting neutrinos in cosmology: exact description and constraints

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics The full Boltzmann hierarchy for dark matter-massive neutrino interactions

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Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics Unresolved cited work

Reference 50

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Pith citing papers

Observation 8f8009bf-40d5-4444-88cc-0e3acd7cef5c · inbound

Cosmological evolution with decaying dark matter: an integral-equation approach cites this paper.

Cosmological evolution with decaying dark matter: an integral-equation approach Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics

Reference 25

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