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Paper Citation Record · LEDGER
Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 67 inbound Pith citation observations for arXiv:2404.15232.
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Pith citing papers
Observation 4d25b231-2b9d-4c25-b27e-fad1add89644 · inbound
$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.
$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 137
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Observation 7fed6e95-d5c9-4619-a316-ac6a9c0ae3ff · inbound
Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis cites this paper.
Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 21
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General parametrization for energy density of quintessence field Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
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Observation 0f7892e2-7912-4693-8980-cb97daa23086 · inbound
Interacting phantom dark energy: new accelerating scaling attractors cites this paper.
Interacting phantom dark energy: new accelerating scaling attractors Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 99
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A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data cites this paper.
A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 39
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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.
DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 70
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Newest measurements of Hubble constant from DESI 2024 BAO observations cites this paper.
Newest measurements of Hubble constant from DESI 2024 BAO observations Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 17
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Observation cde4490a-37f3-4a03-b20f-69ccb7cbdcfc · inbound
Alleviating cosmological tensions with a hybrid dark sector cites this paper.
Alleviating cosmological tensions with a hybrid dark sector Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 36
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Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics cites this paper.
Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 46
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Observation c5d2e94d-ae66-484d-aa51-7776e8400401 · inbound
Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.
Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 137
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Scalar-Tensor Gravity and DESI 2024 BAO data cites this paper.
Scalar-Tensor Gravity and DESI 2024 BAO data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 25
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Observation 8ac42b03-5561-4f83-b4b5-17e07998f0f0 · inbound
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae cites this paper.
The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 35
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Observation 362dd013-d112-4da6-8eec-5249eb2bb7cb · inbound
Dark energy and lensing anomaly in Planck CMB data cites this paper.
Dark energy and lensing anomaly in Planck CMB data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 37
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Observation fc3788b4-a960-44ed-9aa3-1abca5b43738 · inbound
Robustness of dark energy phenomenology across different parameterizations cites this paper.
Robustness of dark energy phenomenology across different parameterizations Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 129
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Observation c4bd085a-e72f-49b3-9712-c05afb87a53c · inbound
Modified theories of gravity at different curvature scales cites this paper.
Modified theories of gravity at different curvature scales Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 231
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Observation 63b3be25-dfe2-4e88-aac5-a8dcc46322c9 · inbound
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An overview of what current data can (and cannot yet) say about evolving dark energy Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 115
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Observation 32f0d96d-091d-49b4-b17a-3935f189ec2e · inbound
Evidence for non-cold dark matter from DESI DR2 measurements cites this paper.
Evidence for non-cold dark matter from DESI DR2 measurements Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 103
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Observation ea9e50a2-7316-46a0-8ea9-aca3b3261679 · inbound
In search of an interaction in the dark sector through Gaussian Process and ANN approaches cites this paper.
In search of an interaction in the dark sector through Gaussian Process and ANN approaches Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 44
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The Quintom theory of dark energy after DESI DR2 cites this paper.
The Quintom theory of dark energy after DESI DR2 Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 101
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Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.
Can the universe experience an AdS landscape since matter-radiation equality? Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
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Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.
Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 87
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Observation 909b5787-d89a-43d9-8302-917e2c38d826 · inbound
New Insights into Dark Energy from DESI DR2 with CMB and SNIa cites this paper.
New Insights into Dark Energy from DESI DR2 with CMB and SNIa Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 24
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Observation 1a0b614f-640b-496e-adca-55b650fc5241 · inbound
Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI cites this paper.
Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 49
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Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data cites this paper.
Cosmological preference for a positive neutrino mass at 2.7$\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
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Resolving the Planck-DESI tension by nonminimally coupled quintessence Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 46
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Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime cites this paper.
Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 77
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Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.
Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 102
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Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.
Beyond CPL: Evidence for dynamical dark energy in three-parameter models Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
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Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.
Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 174
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Observation 61eef0a9-cf10-455c-bcd7-81e4872f2920 · inbound
Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.
Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 87
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Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.
Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 88
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Revisiting the Hubble tension problem in the framework of holographic dark energy cites this paper.
Revisiting the Hubble tension problem in the framework of holographic dark energy Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 30
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Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model cites this paper.
Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 14
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Observation 28bf4d10-4a1d-4c5d-88aa-3ae7925f5c53 · inbound
Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.
Observational constraints on early time non-phantom behaviour of dynamical dark energy Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 16
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Robust Preference for Dark Sector Interactions cites this paper.
Robust Preference for Dark Sector Interactions Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 111
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Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models cites this paper.
Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 12
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Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.
Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 51
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Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework cites this paper.
Probing dynamical dark energy with late-time data: Evidence, tensions, and the limits of the $w_0w_a$CDM framework Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 66
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Measuring neutrino mass in light of ACT DR6 and DESI DR2 Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 39
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Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.
Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 75
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Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae cites this paper.
Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 36
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Observation e04192f8-5876-4656-a6f8-9c9c51251049 · inbound
UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 cites this paper.
UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 15
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Observation 007cebce-67d8-40fb-87a8-08d2c73efdf5 · inbound
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.
Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 68
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Observation ce635795-f3cb-48d2-940b-1e820da0c4fb · inbound
Accelerating scaling solutions from dark matter particle creation cites this paper.
Accelerating scaling solutions from dark matter particle creation Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 91
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Observation f2b61a5d-a08d-4e3a-a7ec-06939644b9f7 · inbound
Accelerating scaling solutions from dark matter particle creation cites this paper.
Accelerating scaling solutions from dark matter particle creation Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 85
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Observation 1371249a-1844-4687-8df5-0981a224454d · inbound
The open-Universe signal: A model artifact rather than genuine curvature cites this paper.
The open-Universe signal: A model artifact rather than genuine curvature Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 26
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Observation abd2ece5-b9af-4674-9c30-cd87fe4400d5 · inbound
Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.
Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 50
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Observation 8ca5013d-ce8e-4efd-b78e-36772f31e1f2 · inbound
Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.
Breaking Free from the Swampland of Impossible Universes through the DESI Portal Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 297
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Observation 60d49e16-41b0-4613-a3f8-39c0f52603ca · inbound
Dark Energy in Ghost-free non-local Gravity cites this paper.
Dark Energy in Ghost-free non-local Gravity Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 32
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No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 94feebc8-e4ec-4271-a1ba-846fde556935 · inbound
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 146
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T16:45:51.197724Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 63971910-0fec-4137-a77a-4cb215c6761b · inbound
A short review on Quintom dark energy theory cites this paper.
A short review on Quintom dark energy theory Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T21:46:15.956582Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 02d96286-70ef-4812-b164-fabfb6cc187c · inbound
A short review on Quintom dark energy theory cites this paper.
A short review on Quintom dark energy theory Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:40:01.093221Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0030bb84-fd26-45a7-80ca-51c592f4b886 · inbound
Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.
Neutrino mass constraints in interacting dark energy models after DESI DR2 Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 151
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T10:56:52.425874Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation dc7d1628-25e1-41c2-b84f-034889a04716 · inbound
Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations cites this paper.
Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 68
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T14:17:03.631815Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 2feaebf2-f0d7-4a6d-9508-7342f3281ef2 · inbound
Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values cites this paper.
Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 61
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-07-03T02:27:35.312828Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 7e3d21ea-b57b-46c5-93f8-230b9853a0d9 · inbound
Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values cites this paper.
Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:05:39.495259Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 95acd21b-e667-41e9-907e-fc9e692e9452 · inbound
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 52
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:19:23.735673Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 412f5266-af22-4ffc-86bf-e85dcf61a409 · inbound
Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.
Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 215
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T11:25:45.477465Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 763e0bbc-5f4c-4f83-85da-c6b73c76ef71 · inbound
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 94
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:18:55.037825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a896061b-68ac-460d-b7e5-5507edf1ce64 · inbound
Imprint of swampland-inspired coupled early dark energy cites this paper.
Imprint of swampland-inspired coupled early dark energy Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 11
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T15:55:04.963643Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation e98b5eb5-941a-43a9-90cc-07e9a3191eb9 · inbound
Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey cites this paper.
Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 40
- Resolution
- malformed identifier
- local_arxiv, observed 2026-07-09T13:46:17.481323Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation c82c0a0d-5e61-4e6f-9338-177f5cecac1e · inbound
Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae cites this paper.
Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T16:44:02.461654Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f5fd74a-a52f-4515-a4be-cf318fd77473 · inbound
Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction cites this paper.
Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T03:00:21.146194Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0ecc0348-0404-4908-b72f-958b10d7cf65 · inbound
Hubble tension: the shape wall cites this paper.
Hubble tension: the shape wall Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 141
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T08:08:47.106381Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 378aef4a-9015-4ec1-8e4e-a5bd8b4201ec · inbound
Hubble tension: a short review of theoretical explanations cites this paper.
Hubble tension: a short review of theoretical explanations Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 231
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T07:20:08.240266Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9416b0fc-7247-4a2e-bf54-e3f6d2e6bd47 · inbound
Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements cites this paper.
Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T19:55:29.070461Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e55f62d4-35d0-40d7-a3ea-3bfcf699fc40 · inbound
Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift cites this paper.
Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 95
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T18:21:13.152445Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.