Paper Citation Record · LEDGER

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos

As of 17 August 2026, this Paper Citation Record lists 100 of 174 outbound references and 4 inbound Pith citation observations for arXiv:2504.15348.

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Observation e34a0906-cc1f-493b-8aa8-eada6bb394ce · outbound

This paper cites In particular, we use an optical depth τ that is produced as an output by our 21-cm simulations; it is then used to compute the CMB power spectrum for our CMB analyses.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos In particular, we use an optical depth τ that is produced as an output by our 21-cm simulations; it is then used to compute the CMB power spectrum for our CMB analyses

Reference 1

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Observation 530a27d4-f0e4-4e9c-af62-0ff70f97bccf · outbound

This paper cites We can estimateτ and its uncertainty based on the other cosmological parameters and the density-weighted ioniza- tion fraction xHII(1 +δb) [45, 46].

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos We can estimateτ and its uncertainty based on the other cosmological parameters and the density-weighted ioniza- tion fraction xHII(1 +δb) [45, 46]

Reference 2

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Observation 1854af1b-9eb0-424b-bd0b-f72af54fb00a · outbound

This paper cites It is composed of ∼ 330 packed antennas, distributed in a hexagonal shape with 14 m di- ameter dishes.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos It is composed of ∼ 330 packed antennas, distributed in a hexagonal shape with 14 m di- ameter dishes

Reference 3

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Observation 9fc43cba-97a1-45a3-afa6-a3df043f612a · outbound

This paper cites The SKAO or any other ground-based detector can only slightly extend the low-frequency range observed by HERA because of atmo- spheric effects.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The SKAO or any other ground-based detector can only slightly extend the low-frequency range observed by HERA because of atmo- spheric effects

Reference 4

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Observation eb6708c7-d421-4436-bcaf-f0d147dfcc42 · outbound

This paper cites We use noise curves from the CMB-S4: Dark Radiation Anisotropy Flowdown Team (DRAFT) tool 7, for the S4-wide Chilean LAT configuration 8, updated on Octo- ber 2023 [146–149].

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos We use noise curves from the CMB-S4: Dark Radiation Anisotropy Flowdown Team (DRAFT) tool 7, for the S4-wide Chilean LAT configuration 8, updated on Octo- ber 2023 [146–149]

Reference 5

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Observation 131a5d67-926d-4ac1-abc2-5c5bdcec8c0e · outbound

This paper cites Our results on the 15 FIG.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Our results on the 15 FIG

Reference 6

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Observation dc6280aa-afc1-4919-88b2-2cacf9beba76 · outbound

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Unresolved cited work

Reference 7

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Observation 135d78f6-ea33-484d-be29-5ec9d9331c12 · outbound

This paper cites Dipartimenti di eccellenza.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Dipartimenti di eccellenza

Reference 8

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Observation dfa8d45e-5bc5-47fd-948f-0d0ea4c30207 · outbound

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Unresolved cited work

Reference 9

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Observation 7d98283b-dacc-4d43-84ed-b0bdd82f1faa · outbound

This paper cites an unresolved cited work.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Unresolved cited work

Reference 10

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Observation 07e66775-5574-450c-8fee-73289efe3565 · outbound

This paper cites Evidence for oscillation of atmospheric neutrinos.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Evidence for oscillation of atmospheric neutrinos

Reference 11

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Observation b94db4c6-8a80-4caa-878b-66487967a4cc · outbound

This paper cites Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data

Reference 12

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Observation 13251dd7-36e6-43e8-bbe6-ce8f1c890915 · outbound

This paper cites Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Determination of Solar Neutrino Oscillation Parameters using 1496 Days of Super-Kamiokande-I Data

Reference 13

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Observation cf0e73db-4502-4baa-acf9-36722d457bc6 · outbound

This paper cites Measurement of the L/E distributions of atmospheric neutrinos in Soudan 2 and their interpretation as neutrino oscil- lations,.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Measurement of the L/E distributions of atmospheric neutrinos in Soudan 2 and their interpretation as neutrino oscil- lations,

Reference 14

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Observation 44f8ab72-6e14-4c62-ab6a-16122fa21ba1 · outbound

This paper cites Final neutrino oscillation results from LSND and KARMEN,.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Final neutrino oscillation results from LSND and KARMEN,

Reference 15

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Observation e3a7a5c1-3bf2-4de8-86f3-e00715ee0c23 · outbound

This paper cites Measurement of neutrino oscillation with KamLAND: Evidence of spectral distor- tion,.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Measurement of neutrino oscillation with KamLAND: Evidence of spectral distor- tion,

Reference 16

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Observation 08e27eca-be39-4593-9e73-3a525c917448 · outbound

This paper cites A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos A Measurement of Atmospheric Neutrino Oscillation Parameters by Super-Kamiokande I

Reference 17

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Observation f3d9fbbb-d621-4560-a142-0e43efb11ce9 · outbound

This paper cites Review of neutrino oscllations ex- periments,.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Review of neutrino oscllations ex- periments,

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Observation b4f38102-1b35-4a6e-a235-cb103b24e93a · outbound

This paper cites Observation of electron-antineutrino disappearance at Daya Bay.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Observation of electron-antineutrino disappearance at Daya Bay

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Observation 34b5c1ba-39d1-4526-b3cc-a600992d4bd3 · outbound

This paper cites Power Spectra for Cold Dark Matter and its Variants.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Power Spectra for Cold Dark Matter and its Variants

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Observation 8c80ce44-6d7c-4a0b-9cad-f018acb099d8 · outbound

This paper cites Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Neutrinos in Non-linear Structure Formation - The Effect on Halo Properties

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Observation bae051e5-5aae-4c9f-8cd0-66b7b4e7b774 · outbound

This paper cites Effects of Massive Neutrinos on the Large-Scale Structure of the Universe.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Effects of Massive Neutrinos on the Large-Scale Structure of the Universe

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Observation cb627c3a-f1ae-4e8b-987f-eaa4b07aa6db · outbound

This paper cites DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Cosmic Microwave Background Radiation

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This paper cites Astrophysical implications of the neutrino rest mass. II. The density-perturbation spec- trum and small-scale fluctuations in the microwave background,.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Astrophysical implications of the neutrino rest mass. II. The density-perturbation spec- trum and small-scale fluctuations in the microwave background,

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Observation 29191e8e-5b97-4529-8f47-f8bc916b46a9 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Planck 2018 results. VI. Cosmological parameters

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

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

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos KATRIN: Status and Prospects for the Neutrino Mass and Beyond

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Project 8 Neutrino Mass Experiment

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Limits on Neutrino-Neutrino Scattering in the Early Universe

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Updated constraints on non-standard neutrino interactions from Planck

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Cosmic microwave background constraints on secret interactions among sterile neutrinos

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Interacting neutrinos in cosmology: exact description and constraints

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Neutrino Puzzle: Anomalies, Interactions, and Cosmological Tensions

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Updated constraints on massive neutrino self-interactions from cosmology in light of the $H_0$ tension

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Dark Neutrino interactions phase out the Hubble tension

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Flavor-specific Interaction Favors Strong Neutrino Self-coupling in the Early Universe

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The magnificent ACT of flavor-specific neutrino self-interaction

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos A tale of two modes: Neutrino free-streaming in the early universe

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos A First Detection of the Acoustic Oscillation Phase Shift Expected from the Cosmic Neutrino Background

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Phases of New Physics in the CMB

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Free-Streaming Neutrinos and Their Phase Shift in Current and Future CMB Power Spec- tra,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Boltzmann hierarchy for interacting neutrinos I: formalism

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Self-interacting neutrinos in light of recent CMB and LSS data

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Self-Interacting Neutrinos in Light of Large-Scale Structure Data

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos A Fresh Look at Neutrino Self- Interactions With the Lyman- α Forest: Constraints from EFT and PRIYA,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Constraints on Dark Matter-Neutrino Interaction from 21-cm Cosmology and Forecasts on SKA1-Low

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Reference 56

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Reference 57

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Reference 58

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Reference 59

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Observation 6fbc6994-7c1d-4ab4-b4a7-373e16dc8d14 · outbound

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Observation e98eeabe-794b-4b0e-af26-103a6dbb15ff · outbound

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Reference 63

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The limits of cosmology: role of the Moon

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Observation 781c9fba-8f8f-4709-a5d7-e38b36b14d07 · outbound

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Large-scale Array for Radio Astronomy on the Farside

Reference 66

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos LuSEE-Night power requirements and power generation strategy

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Forecast measurement of the 21 cm global spectrum from Lunar orbit with the Vari-Zeroth-Order Polynomial (VZOP) method

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Cosmic black body radiation and galaxy formation,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 73

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Observation 2c5dd2ce-494c-4e98-afdf-c5b3b713d6c9 · outbound

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos 21cmFirstCLASS II. Early linear fluctuations of the 21cm signal

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Does it matter? A more careful treatment of density fluctuations in 21-cm simulations

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Massive neutrinos and cosmology

Reference 78

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Neutrinos in cosmology

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Density of relict particles with zero rest mass in the universe,

Reference 81

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Cos- mological Limits to the Number of Massive Leptons,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Dynamical Role of Light Neutral Leptons in Cosmology,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos CMB signals of neutrino mass gen- eration,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Neutrinoless Universe

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Cosmological signatures of interacting neutri- nos,

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Hubble tension and a renormalizable model of gauged neutrino self-interactions

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Resolving Hubble Tension by Self-Interacting Neutrinos with Dirac Seesaw

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15

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Resolution: verified exact; raw_fallback, observed 2026-08-16T11:34:43.148016Z

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Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos 21-cm cosmology

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