Paper Citation Record · LEDGER

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter

As of 13 August 2026, this Paper Citation Record lists 100 of 132 outbound references and 2 inbound Pith citation observations for arXiv:2411.17320.

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

pith.paper-citation-record.v1
2411.17320 v2

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measured 100 of 132 reference resolution

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Outbound references

Observation 19fa48cc-d34b-49a9-9482-6e43017ac64e · outbound

This paper cites Baumann,Cosmology, Cambridge University Press (7, 2022), 10.1017/9781108937092.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Baumann,Cosmology, Cambridge University Press (7, 2022), 10.1017/9781108937092

Reference 1

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Observation 6372600d-ba9f-4863-a825-5270f7f307d9 · outbound

This paper cites Dark Matter.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Dark Matter

Reference 2

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Observation db2cdbcb-b82f-452a-b1df-43e7a732c47b · outbound

This paper cites Lee and S.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Lee and S

Reference 3

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Observation f7523482-6570-465d-a840-4b27c78d1f3e · outbound

This paper cites Griest and M.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Griest and M

Reference 4

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Observation ff96441c-86a5-4264-82f3-ec18a59e9882 · outbound

This paper cites The quest to discover supersymmetry at the ATLAS experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The quest to discover supersymmetry at the ATLAS experiment

Reference 5

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Observation 409703db-920b-4b81-868f-7ee96199f25f · outbound

This paper cites First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

Reference 6

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Observation 18d5d151-fefe-49e8-8c1a-aaba9dac77ac · outbound

This paper cites First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter First Dark Matter Search with Nuclear Recoils from the XENONnT Experiment

Reference 7

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Observation 132bd146-2172-45f2-8b94-6b1f3e1fbc17 · outbound

This paper cites Dark Matter Search Results from 1.54 Tonne$\cdot$Year Exposure of PandaX-4T.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Dark Matter Search Results from 1.54 Tonne$\cdot$Year Exposure of PandaX-4T

Reference 8

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Observation 4731dc2d-5415-406d-8f8f-a1be7b0c25d1 · outbound

This paper cites Peccei and H.R.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Peccei and H.R

Reference 9

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Observation 42a35a47-b5cc-4ade-9610-bf32c9096861 · outbound

This paper cites Peccei and H.R.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Peccei and H.R

Reference 10

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Observation 24141ac9-464a-47c7-b790-9636d3fcef64 · outbound

This paper cites Weinberg,A New Light Boson?, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Weinberg,A New Light Boson?, Phys

Reference 11

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Observation 355193ca-9947-4558-b721-bc6cf83eac2d · outbound

This paper cites Wilczek,Problem of StrongP and T Invariance in the Presence of Instantons, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Wilczek,Problem of StrongP and T Invariance in the Presence of Instantons, Phys

Reference 12

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Observation 35ebcfd7-f3be-43c8-9c16-f650f2e1c62c · outbound

This paper cites Preskill, M.B.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Preskill, M.B

Reference 13

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Observation 72fcc0be-8cc7-4eb2-8f78-8ebaa6f9fcb4 · outbound

This paper cites Dine and W.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Dine and W

Reference 14

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Observation 585f2b74-244a-45d7-88b1-fb1550d6fbff · outbound

This paper cites Abbott and P.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Abbott and P

Reference 15

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Observation 99d8a5ac-d1e3-489e-9c6f-7100240dd614 · outbound

This paper cites New experimental approaches in the search for axion-like particles.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter New experimental approaches in the search for axion-like particles

Reference 16

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Observation e87bf632-26ce-478d-af6e-9b057c62f875 · outbound

This paper cites Invisible Axion Search Methods.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Invisible Axion Search Methods

Reference 17

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Observation a3e0c0d9-db11-4579-90af-7c88e20c3692 · outbound

This paper cites Direct Detection of Dark Matter -- APPEC Committee Report.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Direct Detection of Dark Matter -- APPEC Committee Report

Reference 18

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Observation ecea6615-a8d4-4029-8d4d-c28cb6d08faf · outbound

This paper cites Axion Dark Matter.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Dark Matter

Reference 19

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Observation 900f4d7b-2277-4168-bbe2-49c1f90f422c · outbound

This paper cites Zeldovich, I.Y.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Zeldovich, I.Y

Reference 20

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Observation e7c6486b-a5b0-4737-833c-3e9fec3802de · outbound

This paper cites Sikivie,Of Axions, Domain Walls and the Early Universe, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Sikivie,Of Axions, Domain Walls and the Early Universe, Phys

Reference 21

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Observation 25aa52ff-579a-448f-be85-ed9c520d4eab · outbound

This paper cites Redefining the Axion Window.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Redefining the Axion Window

Reference 22

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Observation 1ec44646-964a-4673-b5e8-2efdfe9f44f3 · outbound

This paper cites Window for preferred axion models.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Window for preferred axion models

Reference 23

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Observation 4913c8a4-6715-41cc-84c2-79f9d5596446 · outbound

This paper cites Planck 2018 results. X. Constraints on inflation.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Planck 2018 results. X. Constraints on inflation

Reference 24

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Observation 895ed5ac-289e-4c2e-8953-55a49f62df4e · outbound

This paper cites On Axion Thermalization in the Early Universe.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter On Axion Thermalization in the Early Universe

Reference 25

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Observation 1238d594-7750-4dde-9973-5532e01553fc · outbound

This paper cites Cosmological mass limits on neutrinos, axions, and other light particles.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Cosmological mass limits on neutrinos, axions, and other light particles

Reference 26

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Observation dd221404-d1a5-4606-8e75-79ced1240ee4 · outbound

This paper cites An improved cosmological bound on the thermal axion mass.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter An improved cosmological bound on the thermal axion mass

Reference 27

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Observation 4d14e7e3-54d7-44d6-b5ac-81479b741533 · outbound

This paper cites Thermal axion production in the primordial quark-gluon plasma.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Thermal axion production in the primordial quark-gluon plasma

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Observation 5b71e6df-4cd4-4edc-b834-20f6ccb94bdb · outbound

This paper cites Thermal axion production.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Thermal axion production

Reference 29

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Observation 7d384f65-03f2-478c-81c3-6c310296e1db · outbound

This paper cites Observable windows for the QCD axion through $N_\text{eff}$.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Observable windows for the QCD axion through $N_\text{eff}$

Reference 30

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Observation 51bdfa56-0e76-4f6e-a0dd-355a419425bd · outbound

This paper cites Production of Thermal Axions across the ElectroWeak Phase Transition.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Production of Thermal Axions across the ElectroWeak Phase Transition

Reference 31

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Observation 10e84b3e-157b-4520-9bbc-917fbe097d0e · outbound

This paper cites New cosmological bounds on hot relics: Axions $\&$ Neutrinos.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter New cosmological bounds on hot relics: Axions $\&$ Neutrinos

Reference 32

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Observation 772e80fb-ae6a-49e5-8f7d-6049ea2a0919 · outbound

This paper cites Thermal QCD Axions across Thresholds.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Thermal QCD Axions across Thresholds

Reference 33

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Observation 61428147-b30e-438c-8e63-91000f21662e · outbound

This paper cites Novel cosmological bounds on thermally-produced axion-like particles.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Novel cosmological bounds on thermally-produced axion-like particles

Reference 34

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Observation a6940d0c-b611-4924-8a03-8a81d998509c · outbound

This paper cites The QCD Axion: Some Like It Hot.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The QCD Axion: Some Like It Hot

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Observation 2e48099f-b4ed-472d-9753-0d39127df910 · outbound

This paper cites Thermal production of astrophobic axions.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Thermal production of astrophobic axions

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Observation 2dff15d3-9452-49fc-882d-1a630b8e60bb · outbound

This paper cites Thermal Production of Axions from Heavy Higgs Bosons.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Thermal Production of Axions from Heavy Higgs Bosons

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Observation 00883726-1fde-4971-b5f0-a68edd5cbca8 · outbound

This paper cites The Flavor of QCD Axion Dark Matter.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The Flavor of QCD Axion Dark Matter

Reference 38

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Observation 0cda5dc0-aad9-4d46-9e1d-6c02afdbec9f · outbound

This paper cites Guth,The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Guth,The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems, Phys

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Observation a5170435-9f43-44f3-a557-09b1d744c95a · outbound

This paper cites New confining force solution of QCD axion domain wall problem.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter New confining force solution of QCD axion domain wall problem

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Observation 51dab8ed-14c5-4c09-89b4-d151e8b8ef68 · outbound

This paper cites On the high-scale instanton interference effect: axion models without domain wall problem.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter On the high-scale instanton interference effect: axion models without domain wall problem

Reference 41

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Observation c533fc13-ced5-43c6-8f3e-5b9d4974e9b8 · outbound

This paper cites Cosmic implications of a low-scale solution to the axion domain wall problem.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Cosmic implications of a low-scale solution to the axion domain wall problem

Reference 42

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Observation d63f361d-21ce-4e17-ab3b-60eb7e5f60ed · outbound

This paper cites Zhitnitsky,On Possible Suppression of the Axion Hadron Interactions.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Zhitnitsky,On Possible Suppression of the Axion Hadron Interactions

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Unresolved cited work

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Observation 1dcf9d5f-487f-412e-9376-27a134ba78b9 · outbound

This paper cites Bardeen, S.H.H.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Bardeen, S.H.H

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Observation fe3179ec-48ef-4e1e-a349-acdbec827b59 · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Davidson and M.A.H

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Observation 09b0237c-7b38-4607-80c2-2920f53e5d76 · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Davidson and M.A.H

Reference 47

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Observation 6bab0f2a-d721-4df8-b9f4-5a12767afae6 · outbound

This paper cites Classification of three-family flavoured DFSZ axion models that have no domain wall problem.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Classification of three-family flavoured DFSZ axion models that have no domain wall problem

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Observation 3ecdd324-be6a-4004-a688-179a4ca8fae5 · outbound

This paper cites Kim,Weak Interaction Singlet and Strong CP Invariance, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Kim,Weak Interaction Singlet and Strong CP Invariance, Phys

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Observation f75d4880-40f5-4577-850c-02b11c315c16 · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Shifman, A.I

Reference 50

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Observation 65631851-39db-4658-a79c-a9d63d58d0b3 · outbound

This paper cites Raffelt,Astrophysical methods to constrain axions and other novel particle phenomena, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Raffelt,Astrophysical methods to constrain axions and other novel particle phenomena, Phys

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Observation 991e3ae6-960e-48b0-a83e-f09af1e6218f · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Astrophysical Axion Bounds

Reference 52

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Observation a7f88ba5-7b9e-4a5e-bbc5-e2249f7e1466 · outbound

This paper cites Astrophysical Axion Bounds: The 2024 Edition.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Astrophysical Axion Bounds: The 2024 Edition

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Observation 6cd1698a-fd14-474a-ae51-142237f27c74 · outbound

This paper cites Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Improved axion emissivity from a supernova via nucleon-nucleon bremsstrahlung

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Observation cad5500e-ce21-44fa-9c26-c11decc75935 · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The Beam and detector of the NA62 experiment at CERN

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Observation 5a5eb3ae-66d0-4e9f-91c6-dc00cba6f072 · outbound

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Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Unresolved cited work

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Observation 392469fd-fb91-4f8a-a7df-f0834089f819 · outbound

This paper cites Quark Flavor Phenomenology of the QCD Axion.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Quark Flavor Phenomenology of the QCD Axion

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This paper cites Sikivie,Experimental Tests of the Invisible Axion, Phys.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Sikivie,Experimental Tests of the Invisible Axion, Phys

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Observation 58344e6e-5495-47f7-8416-effad431236e · outbound

This paper cites The landscape of QCD axion models.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The landscape of QCD axion models

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Observation 4b7d6683-beeb-46b4-bafc-6e40a78d4cea · outbound

This paper cites A SQUID-based microwave cavity search for dark-matter axions.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter A SQUID-based microwave cavity search for dark-matter axions

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.689893Z

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Observation 263e0da3-c2a0-45a5-9ca6-1462a134fbd3 · outbound

This paper cites Extended Search for the Invisible Axion with the Axion Dark Matter Experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Extended Search for the Invisible Axion with the Axion Dark Matter Experiment

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.695950Z

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Observation 37b4ab50-b836-44bf-914a-18f62867e6ce · outbound

This paper cites Experimental search for invisible dark matter axions around 22 {\mu}eV.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Experimental search for invisible dark matter axions around 22 {\mu}eV

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.702164Z

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Observation 3724547e-1722-4c65-b7c0-a7f5de891f0d · outbound

This paper cites First results from a second generation galactic axion experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter First results from a second generation galactic axion experiment

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.708595Z

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Observation 5eb768db-1f58-43ff-b67c-a0314ef8f309 · outbound

This paper cites First Results from the Taiwan Axion Search Experiment with Haloscope at 19.6 $\mu$eV.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter First Results from the Taiwan Axion Search Experiment with Haloscope at 19.6 $\mu$eV

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.714150Z

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Observation 3f41afeb-5e55-4c39-a033-6b0f2550e2a2 · outbound

This paper cites Results from phase 1 of the HAYSTAC microwave cavity axion experiment.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Results from phase 1 of the HAYSTAC microwave cavity axion experiment

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.720906Z

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Observation 4be6d2fe-78c1-4bae-b64b-a7fb5bdac198 · outbound

This paper cites Search for galactic axions with a traveling wave parametric amplifier.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Search for galactic axions with a traveling wave parametric amplifier

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.727349Z

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Observation 5cdeda31-a79c-46c7-a593-94b35af301a0 · outbound

This paper cites Search for Axion dark matter with the QUAX-LNF tunable haloscope.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Search for Axion dark matter with the QUAX-LNF tunable haloscope

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.733664Z

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Unavailable: canonical work link unavailable.

Observation 85cf613c-a67c-40d5-8f2e-ea0afc27dee3 · outbound

This paper cites cajohare/axionlimits: Axionlimits.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter cajohare/axionlimits: Axionlimits

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.741223Z

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Observation 65d530ae-2dbd-4d3a-ae77-ce11845e1579 · outbound

This paper cites Axion Cosmology.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Cosmology

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.747829Z

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Observation 612cb965-d4b0-4c63-be29-67bfae1a116c · outbound

This paper cites Axion Cosmology.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Cosmology

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.755819Z

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Unavailable: canonical work link unavailable.

Observation 3ce0e545-ef6a-4fa7-89a0-c754901a56a0 · outbound

This paper cites The QCD axion, precisely.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter The QCD axion, precisely

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.763093Z

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Observation 20b46f7c-0cb9-414b-852a-0b25886579bf · outbound

This paper cites Axion Cosmology and the Energy Scale of Inflation.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Cosmology and the Energy Scale of Inflation

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.769598Z

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Observation 9b734a25-249d-435c-8cae-e9dc8a092fb9 · outbound

This paper cites Steinhardt and M.S.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Steinhardt and M.S

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.775859Z

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Observation d11d65e9-e2a1-43ed-9e29-e616f45ccf63 · outbound

This paper cites Lazarides, R.K.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Lazarides, R.K

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.782264Z

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Observation 321bee70-1878-435c-b64c-90687c28877b · outbound

This paper cites Can Decaying Particles Raise the Upperbound on the Peccei-Quinn Scale?.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Can Decaying Particles Raise the Upperbound on the Peccei-Quinn Scale?

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.787951Z

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Unavailable: canonical work link unavailable.

Observation efc76683-100c-4b20-a12c-f3ac15e13ed8 · outbound

This paper cites Axion cold dark matter in non-standard cosmologies.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion cold dark matter in non-standard cosmologies

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.794116Z

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Unavailable: canonical work link unavailable.

Observation 9d131eeb-faa2-4fa3-b93b-53d8556c6cce · outbound

This paper cites Axion Cosmology with Early Matter Domination.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Cosmology with Early Matter Domination

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.800251Z

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Observation e681005b-600c-4ea5-9ba7-1ccde5cf033d · outbound

This paper cites Probing the Early Universe with Axion Physics and Gravitational Waves.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Probing the Early Universe with Axion Physics and Gravitational Waves

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.806315Z

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Observation 712b153f-50c4-4af9-b4fd-faa4b30b39da · outbound

This paper cites New opportunities for axion dark matter searches in nonstandard cosmological models.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter New opportunities for axion dark matter searches in nonstandard cosmological models

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.811802Z

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Observation e0695476-625d-483b-9dd2-447d60969d3d · outbound

This paper cites Dark Matter Axions in the Early Universe with a Period of Increasing Temperature.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Dark Matter Axions in the Early Universe with a Period of Increasing Temperature

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.817940Z

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Observation 9ea3687d-2c03-48c0-9817-4ecb5d9b7637 · outbound

This paper cites Constraining Axion and ALP Dark Matter from Misalignment during Reheating.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Constraining Axion and ALP Dark Matter from Misalignment during Reheating

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.824095Z

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Observation 2394dd57-f312-46ff-88b9-81645afa3064 · outbound

This paper cites Extending preferred axion models via heavy-quark induced early matter domination.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Extending preferred axion models via heavy-quark induced early matter domination

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.829822Z

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Observation 02cf1840-d6b2-4d18-b582-05546862068c · outbound

This paper cites Axion Radiation from Strings.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Radiation from Strings

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.835189Z

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Observation 879ed8e0-4cd5-496d-a2f4-559f0165918b · outbound

This paper cites Axion Cosmology Revisited.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Cosmology Revisited

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.840673Z

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Observation 393e4d15-d27f-4837-b925-e3e94cd435a2 · outbound

This paper cites Improved estimation of radiated axions from cosmological axionic strings.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Improved estimation of radiated axions from cosmological axionic strings

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.847984Z

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Observation 72ffcf1a-2471-44f0-9db1-4aae41aa70c7 · outbound

This paper cites Axion dark matter from topological defects.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion dark matter from topological defects

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.853842Z

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Observation be4282e8-6878-4d01-96fe-f1924d569c79 · outbound

This paper cites More Axions from Strings.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter More Axions from Strings

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.859956Z

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Observation f92f4647-6346-46b1-b481-297cbacfe843 · outbound

This paper cites Dark Matter from Axion Strings with Adaptive Mesh Refinement.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Dark Matter from Axion Strings with Adaptive Mesh Refinement

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.869497Z

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Observation f9b570cc-7bbe-4923-955c-68a34c2471f0 · outbound

This paper cites Spectrum of global string networks and the axion dark matter mass.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Spectrum of global string networks and the axion dark matter mass

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.875880Z

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Observation 9ce54ac6-868d-4485-a50f-f8205a15a9da · outbound

This paper cites Axion Dark Matter from Cosmic String Network.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Axion Dark Matter from Cosmic String Network

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.881824Z

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Observation fcb1e328-97d0-4517-86b4-7287aaae79e8 · outbound

This paper cites Colored Dark Matter.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Colored Dark Matter

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.887936Z

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Unavailable: canonical work link unavailable.

Observation 19a9a3c5-38fa-49fe-b3ab-d7b431ce956b · outbound

This paper cites an unresolved cited work.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Unresolved cited work

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.895938Z

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Unavailable: canonical work link unavailable.

Observation 7c285af7-ebab-4d41-ae17-d2663848009d · outbound

This paper cites Direct Detection Constraints on Superheavy Dark Matter.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Direct Detection Constraints on Superheavy Dark Matter

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-08-12T12:24:05.195351Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 48d05c9e-fa8e-453d-be18-d24cab5c427f · outbound

This paper cites Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Towards Closing the Window on Strongly Interacting Dark Matter: Far-Reaching Constraints from Earth's Heat Flow

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.912976Z

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Observation 5acae91d-19f7-4a22-a31b-eaf78cf3806c · outbound

This paper cites Earth-Scattering of super-heavy Dark Matter: updated constraints from detectors old and new.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Earth-Scattering of super-heavy Dark Matter: updated constraints from detectors old and new

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.920253Z

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Unavailable: canonical work link unavailable.

Observation 7d6c15d2-491b-4dbd-a989-261cd696ef43 · outbound

This paper cites Symmetries and Strings in Field Theory and Gravity.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Symmetries and Strings in Field Theory and Gravity

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.927027Z

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Observation 4fad5028-1cd4-4a65-8a4c-8acd2f04cb5b · outbound

This paper cites TASI Lectures: (No) Global Symmetries to Axion Physics.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter TASI Lectures: (No) Global Symmetries to Axion Physics

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.937438Z

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Unavailable: canonical work link unavailable.

Observation 9beefe0f-0ad4-43f6-934c-0b6ae90a15cc · outbound

This paper cites Planck-Scale Physics and the Peccei-Quinn Mechanism.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Planck-Scale Physics and the Peccei-Quinn Mechanism

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.945031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45afc6fe-3fd0-4155-b2ed-f2f9c1fdb762 · outbound

This paper cites Solutions to the strong CP problem in a world with gravity.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Solutions to the strong CP problem in a world with gravity

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.952762Z

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Unavailable: canonical work link unavailable.

Observation 257a9a68-dcd3-4648-a0e4-457fff158c2d · outbound

This paper cites Barr and D.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Barr and D

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-12T12:24:03.960672Z

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Pith citing papers

Observation d7121a1b-0f18-46a4-9e5f-15616ffbc19c · inbound

Catalogues of Cosmologically Self-Consistent Hadronic QCD Axion Models cites this paper.

Catalogues of Cosmologically Self-Consistent Hadronic QCD Axion Models Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter

Reference 127

Resolution: unresolved; no resolver link, observed 2026-08-11T05:18:07.217007Z

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Observation 0e1ed311-4e85-4237-86d6-efca79fd5962 · inbound

High-Quality Axion Dark Matter at Gravitational Wave Interferometers cites this paper.

High-Quality Axion Dark Matter at Gravitational Wave Interferometers Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter

Reference 124

Resolution: verified exact; arxiv_id, observed 2026-05-18T15:36:33.472712Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.