21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter | Paper Citation Record

Observation 0966b04b-1119-4878-8ebf-ddd4173b7b7e · outbound

This paper cites 21-cm cosmology.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter 21-cm cosmology

Reference 1

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Observation 3d20d456-d7c9-4b8f-bd1b-32187da66894 · outbound

This paper cites Small-Scale Challenges to the $\Lambda$CDM Paradigm.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Small-Scale Challenges to the $\Lambda$CDM Paradigm

Reference 4

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Observation ddc0acc2-23fb-428b-8b5d-e1deb7ceddce · outbound

This paper cites The Structure of cold dark matter halos,.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Structure of cold dark matter halos,

Reference 5

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Observation eb820a7a-7383-4f85-916f-ec936241e5fa · outbound

This paper cites Observational and Theoretical Constraints on Singular Dark Matter Halos.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Observational and Theoretical Constraints on Singular Dark Matter Halos

Reference 6

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Observation b102d67e-53d2-4c5d-bbf1-898795dbeceb · outbound

This paper cites Halo Formation in Warm Dark Matter Models.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Halo Formation in Warm Dark Matter Models

Reference 7

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Observation c0240fac-1e0c-423a-b612-dcc1b54f9029 · outbound

This paper cites How supernova feedback turns dark matter cusps into cores.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter How supernova feedback turns dark matter cusps into cores

Reference 8

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Observation b8f6be1a-5023-485a-a7c6-e87c85d6efa2 · outbound

This paper cites Dark Matter Heating and Early Core Formation in Dwarf Galaxies.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark Matter Heating and Early Core Formation in Dwarf Galaxies

Reference 9

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Observation 61a9f4e8-3a78-440b-8bfb-85d11b9dcb63 · outbound

This paper cites The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Impact of Baryonic Physics on the Structure of Dark Matter Halos: the View from the FIRE Cosmological Simulations

Reference 10

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Observation 984c47ac-41b3-4d02-918c-83829f6320eb · outbound

This paper cites Forged in FIRE: cusps, cores, and baryons in low-mass dwarf galaxies.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Forged in FIRE: cusps, cores, and baryons in low-mass dwarf galaxies

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:32.341281Z

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Observation 7a24f8da-3c73-4a3a-a04b-35ac179488e0 · outbound

This paper cites Dark matter cores all the way down.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark matter cores all the way down

Reference 12

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Observation e1fb7262-9394-4c8f-8b49-cf982c0c8f00 · outbound

This paper cites The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The origin of the mass discrepancy-acceleration relation in $\Lambda$CDM

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:32.500769Z

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Observation 32d20ea2-ab35-48aa-b45d-db91bac122f6 · outbound

This paper cites The radial acceleration relation in a $\Lambda$CDM universe.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The radial acceleration relation in a $\Lambda$CDM universe

Reference 14

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Observation ab092091-733a-4b00-abbc-d8c70ad8db36 · outbound

This paper cites Entropy generation and the survival of protogalaxies in an expanding universe,.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Entropy generation and the survival of protogalaxies in an expanding universe,

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:32.683432Z

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Observation fba36b73-e956-4027-9f89-3583e85de78f · outbound

This paper cites Constraining Dark Matter candidates from structure formation.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Dark Matter candidates from structure formation

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:32.768577Z

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Observation ea706380-718a-449a-ab2f-1034a9f47c2e · outbound

This paper cites Interacting Dark Matter disguised as Warm Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Interacting Dark Matter disguised as Warm Dark Matter

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:32.880107Z

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Observation 0c7dcef4-f1a0-478e-b7ff-0530d296509b · outbound

This paper cites Constraints on Dark Matter interactions from structure formation: Damping lengths.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on Dark Matter interactions from structure formation: Damping lengths

Reference 18

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Observation 61435402-53e1-4628-afbd-740186b7cd30 · outbound

This paper cites The Small-Scale Power Spectrum of Cold Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Small-Scale Power Spectrum of Cold Dark Matter

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.101909Z

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Observation ad8f5216-e6bc-4ca5-8002-c56e5efe7127 · outbound

This paper cites Cosmic black body radiation and galaxy formation,.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Cosmic black body radiation and galaxy formation,

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.260328Z

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Observation 181d3720-83cb-4e06-a648-aceccaf6eea2 · outbound

This paper cites A fresh look into the interacting dark matter scenario.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter A fresh look into the interacting dark matter scenario

Reference 21

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Observation 263619c5-4ef1-481e-a811-c68210aad902 · outbound

This paper cites Constraints on millicharged particles from Planck.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on millicharged particles from Planck

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.461183Z

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Observation efcd6735-71b2-4e42-92da-4984ec9f5a7b · outbound

This paper cites The Cosmology of Atomic Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Cosmology of Atomic Dark Matter

Reference 23

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Observation 193ce619-0c3a-42cb-9d09-fa88db2b962a · outbound

This paper cites Dark-Matter Electric and Magnetic Dipole Moments.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark-Matter Electric and Magnetic Dipole Moments

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.568369Z

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Observation 8a589665-daa3-484c-8711-4d3995d5bb43 · outbound

This paper cites Using the CMB angular power spectrum to study Dark Matter-photon interactions.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Using the CMB angular power spectrum to study Dark Matter-photon interactions

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.655026Z

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Observation 622fa892-43b1-481e-954f-632e0d985694 · outbound

This paper cites Using the Milky Way satellites to study interactions between cold dark matter and radiation.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Using the Milky Way satellites to study interactions between cold dark matter and radiation

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.758408Z

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Observation 3d1e953d-eb4f-4a7f-88cd-b08be1bdded4 · outbound

This paper cites Dark matter-radiation interactions: the impact on dark matter haloes.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark matter-radiation interactions: the impact on dark matter haloes

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.812525Z

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Observation 19df7115-9ac0-425f-8be3-041adde0413e · outbound

This paper cites Dark matter-radiation interactions: the structure of Milky Way satellite galaxies.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark matter-radiation interactions: the structure of Milky Way satellite galaxies

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:33.872664Z

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Observation 2979cf6d-d561-433b-940f-7451f45039b3 · outbound

This paper cites Exploring dark matter microphysics with galaxy surveys.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Exploring dark matter microphysics with galaxy surveys

Reference 29

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Observation 306be123-3293-4dcf-a586-cb441e5bbd53 · outbound

This paper cites Turning off the Lights: How Dark is Dark Matter?.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Turning off the Lights: How Dark is Dark Matter?

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.013141Z

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Observation 830641e6-6faf-4030-91e1-a124a900c29e · outbound

This paper cites Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.081832Z

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Observation e4c7ad40-7374-4f9d-9476-d8471788d384 · outbound

This paper cites Constraints on dark matter interactions with standard model particles from CMB spectral distortions.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on dark matter interactions with standard model particles from CMB spectral distortions

Reference 32

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Observation db0dd44b-ae41-4b3a-ba1d-58e7b1b2c92c · outbound

This paper cites Constraints on $\gamma$-CDM interactions matching the Planck data precision.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on $\gamma$-CDM interactions matching the Planck data precision

Reference 33

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Observation 049c02c2-13d7-4690-b829-0c1b9a857cea · outbound

This paper cites Dark Matter microphysics and 21 cm observations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark Matter microphysics and 21 cm observations

Reference 34

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Observation 85b2af5b-b00a-4192-911d-9e42fb5aeb2d · outbound

This paper cites Cosmological bounds on dark matter-neutrino interactions.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Cosmological bounds on dark matter-neutrino interactions

Reference 35

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Observation 0937b1f0-d318-42ab-b6af-ccc7b29e3dda · outbound

This paper cites Constraints on neutrino -- dark matter interactions from cosmic microwave background and large scale structure data.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on neutrino -- dark matter interactions from cosmic microwave background and large scale structure data

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.484772Z

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Observation be5910a1-32a3-4009-a346-8b090f8b6f12 · outbound

This paper cites Constraining Dark Matter-Neutrino Interactions using the CMB and Large-Scale Structure.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Dark Matter-Neutrino Interactions using the CMB and Large-Scale Structure

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.560302Z

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Observation abfa80fa-0e54-4d06-88e2-b34b7fa4be48 · outbound

This paper cites Reducing the $H_0$ and $\sigma_8$ tensions with Dark Matter-neutrino interactions.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Reducing the $H_0$ and $\sigma_8$ tensions with Dark Matter-neutrino interactions

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.614616Z

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Observation b45398dd-007a-491f-bff7-75f16736e54a · outbound

This paper cites Comprehensive Study of Neutrino-Dark Matter Mixed Damping.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Comprehensive Study of Neutrino-Dark Matter Mixed Damping

Reference 39

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Observation f5f8ea73-44f9-4da1-9b5c-9f48b9e08163 · outbound

This paper cites The full Boltzmann hierarchy for dark matter-massive neutrino interactions.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The full Boltzmann hierarchy for dark matter-massive neutrino interactions

Reference 40

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Observation 49c87afb-af58-4a8d-968d-e97b9b210110 · outbound

This paper cites Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Hints of dark matter-neutrino interactions in Lyman-$\alpha$ data

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.779925Z

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Observation ff3d6154-46de-4a9a-b7b3-69596a6dd4e9 · outbound

This paper cites Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on dark matter-neutrino scattering from the Milky-Way satellites and subhalo modeling for dark acoustic oscillations

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:34.832157Z

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Observation d963bcf2-8a85-446b-9256-7da97e2621f7 · outbound

This paper cites Atomic Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Atomic Dark Matter

Reference 43

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Observation a6654526-384c-4b93-b361-e7182713de02 · outbound

This paper cites Cosmological Limits on Hidden Sector Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Cosmological Limits on Hidden Sector Dark Matter

Reference 44

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Observation 5eed0c1f-a036-4df1-8f0b-0ea5ae7f65fb · outbound

This paper cites Dark Radiation and interacting scenarios.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark Radiation and interacting scenarios

Reference 45

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Observation 7c095183-0a64-46aa-9cd4-8e50c5f90896 · outbound

This paper cites Non-Abelian dark matter and dark radiation.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Non-Abelian dark matter and dark radiation

Reference 46

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Observation ee04bb9e-c68b-48c0-b85f-df348195b6d1 · outbound

This paper cites Evidence for dark matter interactions in cosmological precision data?.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Evidence for dark matter interactions in cosmological precision data?

Reference 47

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Observation 84f696a7-d8cc-4adc-8b2e-ccfcb978b92f · outbound

This paper cites On dark matter - dark radiation interaction and cosmic reionization.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter On dark matter - dark radiation interaction and cosmic reionization

Reference 48

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Observation f61814f1-3ac7-4c74-8df8-e424a79a972d · outbound

This paper cites Hidden Charged Dark Matter and Chiral Dark Radiation.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Hidden Charged Dark Matter and Chiral Dark Radiation

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:35.580051Z

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Observation 984edccb-8df8-4ab9-98bb-3afff0ed2d09 · outbound

This paper cites Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Dark Matter -- Dark Radiation interactions with CMB, BAO, and Lyman-$\alpha$

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:35.645684Z

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Observation 5437ca8b-5160-44ec-9acb-ce8ef87f25bf · outbound

This paper cites Thermal decoupling of WIMPs from first principles.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Thermal decoupling of WIMPs from first principles

Reference 51

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Observation 5c4178e1-a790-4382-87f9-3a949907c35b · outbound

This paper cites Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Probing Dark Relativistic Species and Their Interactions with Dark Matter through CMB and 21cm surveys

Reference 52

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Observation 62d1c434-fd40-4fd2-8f1c-c7d0bf159445 · outbound

This paper cites Probing the Small-Scale Matter Power Spectrum with Large-Scale 21-cm Data.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Probing the Small-Scale Matter Power Spectrum with Large-Scale 21-cm Data

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:35.885166Z

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Observation 6b5b470e-2021-4c46-a52b-3d080f02eae3 · outbound

This paper cites Separating Dark Acoustic Oscillations from Astrophysics at Cosmic Dawn.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Separating Dark Acoustic Oscillations from Astrophysics at Cosmic Dawn

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:35.964743Z

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Observation 7c70953c-3c97-4604-9388-d793730ef58d · outbound

This paper cites How small were the first cosmological objects?.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter How small were the first cosmological objects?

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.051973Z

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Observation 0cd0cea9-a7a4-4b4d-8020-2bb113080701 · outbound

This paper cites The Impact of the First Galaxies on Cosmic Dawn and Reionization.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Impact of the First Galaxies on Cosmic Dawn and Reionization

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.152104Z

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Observation e642df1f-680a-43ea-86bd-251acae75a39 · outbound

This paper cites Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.275001Z

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Observation 100b9234-75bc-4ac6-8d27-9d0de4b040c3 · outbound

This paper cites Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.332891Z

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Observation fe653984-7f78-4e6b-afaa-65d56cba3288 · outbound

This paper cites Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.423445Z

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Observation cfe6ab2d-5edf-40aa-b152-c644cafbf6d6 · outbound

This paper cites JWST Lensed quasar dark matter survey II: Strongest gravitational lensing limit on the dark matter free streaming length to date.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter JWST Lensed quasar dark matter survey II: Strongest gravitational lensing limit on the dark matter free streaming length to date

Reference 60

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Observation 9b6fd153-6609-483a-8022-157fe2d5fb1e · outbound

This paper cites Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts

Reference 61

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Observation 45e5f214-f734-49cf-8c0a-99370476ae7b · outbound

This paper cites JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios

Reference 62

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Observation f1b75601-e3bf-42e1-87a4-02d97eb83490 · outbound

This paper cites Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Imprints of fermionic and bosonic mixed dark matter on the 21-cm signal at cosmic dawn

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.797963Z

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Observation 9a3649a4-567f-4ac1-88d6-42a34e999570 · outbound

This paper cites Simulation-based inference on warm dark matter from HERA forecasts.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Simulation-based inference on warm dark matter from HERA forecasts

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.872636Z

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Observation d1e36a0d-dc5d-4d89-bfa7-febcfca42fb4 · outbound

This paper cites Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:36.928051Z

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Observation b42d6d06-5564-4cc9-99a8-06737097d056 · outbound

This paper cites Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.031400Z

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Observation 94a4b407-eea8-425a-9fcf-f0a9a7270c71 · outbound

This paper cites Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.093252Z

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Observation 40af8a47-3f9f-40af-bc82-38717c10654d · outbound

This paper cites The Signature of Sub-galactic Dark Matter Clumping in the Global 21-cm Signal of Hydrogen.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Signature of Sub-galactic Dark Matter Clumping in the Global 21-cm Signal of Hydrogen

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.185418Z

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Observation f2f68c7e-7162-4322-a6e0-333b928063d2 · outbound

This paper cites Probing dark matter interactions with 21cm observations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Probing dark matter interactions with 21cm observations

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.295770Z

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Observation 9a64038a-39ec-43de-81c0-d95d6fd568f0 · outbound

This paper cites Constraints on Dark Matter-Neutrino Interaction from 21-cm Cosmology and Forecasts on SKA1-Low.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Constraints on Dark Matter-Neutrino Interaction from 21-cm Cosmology and Forecasts on SKA1-Low

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.430634Z

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Observation 72818846-b85d-42f3-a1b2-8be24f004920 · outbound

This paper cites Damping scales of neutralino cold dark matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Damping scales of neutralino cold dark matter

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.556109Z

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Observation c710005d-0e56-47e8-ae51-45b1f42a6b20 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The first WIMPy halos

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.659187Z

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Observation e5a01cf7-07d6-4210-92a3-f99ceadfa8d5 · outbound

This paper cites Effects of cold dark matter decoupling and pair annihilation on cosmological perturbations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Effects of cold dark matter decoupling and pair annihilation on cosmological perturbations

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.772233Z

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Observation 48dd5348-0e16-4dc2-9cfc-e3d5ace80efd · outbound

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

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:37.911738Z

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Observation 3c778f5c-1605-499b-930b-9bb9358f21ea · outbound

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

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.020917Z

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Observation e0192695-5ec9-4e49-8e4a-e1c25d39cdb0 · outbound

This paper cites Small scale aspects of warm dark matter : power spectra and acoustic oscillations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Small scale aspects of warm dark matter : power spectra and acoustic oscillations

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.159289Z

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Observation eff344dd-39fe-4f64-b99a-5cb12484d031 · outbound

This paper cites 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.300763Z

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Observation 2618cadf-11c5-448a-b541-514744cb8fc0 · outbound

This paper cites Neural network emulation of reionization to constrain new physics with early- and late-time probes.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Neural network emulation of reionization to constrain new physics with early- and late-time probes

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.453491Z

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Observation e5bd7b33-f8fe-4c04-8f4b-9ef1a246355c · outbound

This paper cites Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation,.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation,

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.594607Z

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Observation e56eb3d9-5e7f-475a-bfd2-e3a254ffaa48 · outbound

This paper cites Large scale bias and the peak background split.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Large scale bias and the peak background split

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.713315Z

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Observation 7e362a0c-69e3-4364-8fe8-826c1c2b94c4 · outbound

This paper cites Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Dark Matter Halo Merger Histories Beyond Cold Dark Matter: I - Methods and Application to Warm Dark Matter

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.778296Z

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Observation a76036f2-8da6-41c3-b8b6-b8006a0d0eb3 · outbound

This paper cites Halo Mass Function and the Free Streaming Scale.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Halo Mass Function and the Free Streaming Scale

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.867600Z

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Observation 0bc23658-d26a-4c7e-a470-44356a51c176 · outbound

This paper cites Structure formation with suppressed small-scale perturbations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Structure formation with suppressed small-scale perturbations

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:38.944362Z

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Observation eb26ea64-e1c0-4cef-88d0-534a1390c14d · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter A new smooth-$k$ space filter approach to calculate halo abundances

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.081940Z

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Observation fb8b8214-a74f-4ab3-8b0c-1a25b98a165c · outbound

This paper cites Does it matter? A more careful treatment of density fluctuations in 21-cm simulations.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Does it matter? A more careful treatment of density fluctuations in 21-cm simulations

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.188048Z

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Observation adcaa008-91d5-4e5a-8148-8985bc6c6bd3 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Wouthuysen-Field coupling strength and application to high-redshift 21 cm radiation

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.309883Z

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Observation bb181b05-9536-40b3-9f1b-89a1e6b094b9 · outbound

This paper cites Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.427543Z

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Observation 1e72ee29-4a7c-466a-bc05-2bd2d8426fa7 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter powerbox: A python package for creating structured fields with isotropic power spectra,

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.567388Z

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Observation 604c6df8-0724-4e60-95d4-3e1451deb7c3 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.673052Z

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Observation 4e474f12-e9c3-498c-9474-4c5b7a7d6797 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.832224Z

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Observation dd62e0db-ccdf-4af9-8aa2-110444303dd4 · outbound

This paper cites Stefanon, R.

21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Stefanon, R

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:39.947365Z

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Observation 5c70abcf-0db2-44b7-9860-9fcc64a33412 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.052809Z

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Observation e9019847-f86c-4b31-89da-604bf0059859 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter In the Beginning: The First Sources of Light and the Reionization of the Universe

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.198916Z

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Observation 8961fb33-bb0a-4eb3-9d4c-a0a4badfba2f · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter How does radiative feedback from a UV background impact reionization?

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.373116Z

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Observation 0227513f-a517-40b6-b80a-d92ff9ef977c · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter High Mass X-ray Binaries and the Cosmic 21-cm Signal: Impact of Host Galaxy Absorption

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.542166Z

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Observation 490b6550-daeb-4d7c-9f2e-862ba67faab9 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter 21cm signal sensitivity to dark matter decay

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.680033Z

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Observation 64f73e51-a9fa-49fc-b6a3-9ac5b6a31fa4 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Sur l’extension de certaines evaluations statistiques au cas de petits echantillons,

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.818475Z

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Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:40.974583Z

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Observation 7d1b4990-314c-4e68-9f58-ac20ffa1751a · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Xv.—on the estimation of statistical parameters,

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:41.096765Z

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Observation edb94681-252f-4d50-ac27-0ad34faa133f · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter The Baryon Acoustic Oscillation Broadband and Broad-beam Array: Design Overview and Sensitivity Forecasts

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:41.204924Z

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Observation c747e1e5-2369-4a75-99d9-e783ad9e3848 · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-03T21:29:41.322571Z

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Observation a43d6620-163c-43c1-8480-3ac4f5ba9cef · outbound

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21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter Revealing the Dark Matter Halo with Axion Direct Detection

Reference 104

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