Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Revisiting holographic dark energy after DESI 2024
As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 32 inbound Pith citation observations for arXiv:2411.08639.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T19:40:50.825329Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T15:55:05.042750Z
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Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation ad447a3c-5acd-446b-81cf-50443fd21d92 · inbound
Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts cites this paper.
Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts Revisiting holographic dark energy after DESI 2024
Reference 31
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Source-reported events for the cited work
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Observation 9243e175-ff4b-4013-aca4-3ed199677385 · inbound
A comprehensive numerical study on four categories of holographic dark energy models cites this paper.
A comprehensive numerical study on four categories of holographic dark energy models Revisiting holographic dark energy after DESI 2024
Reference 108
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Observation 4dcf575c-8f15-4206-a70a-b4685909d701 · inbound
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? Revisiting holographic dark energy after DESI 2024
Reference 81
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Source-reported events for the cited work
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Observation 33e5b1f7-5ab8-4774-8769-a9b681d288ad · inbound
Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.
Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Revisiting holographic dark energy after DESI 2024
Reference 51
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Observation 8b7fa834-9f64-4c0e-b2ab-aac483e2d638 · 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 Revisiting holographic dark energy after DESI 2024
Reference 52
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Observation d725cdde-3504-492b-8596-2d824371be28 · inbound
Dark energy and lensing anomaly in Planck CMB data cites this paper.
Dark energy and lensing anomaly in Planck CMB data Revisiting holographic dark energy after DESI 2024
Reference 51
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Source-reported events for the cited work
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Observation 05601f15-1e6b-4a1c-92ed-8351c02aa5fc · inbound
An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.
An overview of what current data can (and cannot yet) say about evolving dark energy Revisiting holographic dark energy after DESI 2024
Reference 223
- Resolution
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Source-reported events for the cited work
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Observation c0fabfa2-a7ed-43e0-a17b-9b4ddf82644e · inbound
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? Revisiting holographic dark energy after DESI 2024
Reference 48
- Resolution
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Source-reported events for the cited work
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Observation f14a923e-e0d7-47c8-9637-8a0456f15460 · inbound
Barrow holographic dark energy interacting model in the presence of radiation and matter cites this paper.
Barrow holographic dark energy interacting model in the presence of radiation and matter Revisiting holographic dark energy after DESI 2024
Reference 25
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 69fb7fa8-9650-4802-bbf4-1b2312973672 · inbound
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data cites this paper.
Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data Revisiting holographic dark energy after DESI 2024
Reference 34
- Resolution
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Source-reported events for the cited work
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Observation f030daf4-ba3a-4928-a2f3-d119280002d7 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 24
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9be4c1cb-77c6-4d61-9ea3-062ffd456abf · inbound
How Holographic is the Dark Energy? A Spline Nodal reconstruction approach cites this paper.
How Holographic is the Dark Energy? A Spline Nodal reconstruction approach Revisiting holographic dark energy after DESI 2024
Reference 66
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 566e281e-8bc2-4e42-a830-7b987c877862 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 54
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 653bfe8c-9c52-4fc8-8832-1071e4f75588 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 69
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f9bb374e-65d4-465f-81de-6c261a54f9f4 · inbound
Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies cites this paper.
Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies Revisiting holographic dark energy after DESI 2024
Reference 20
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 868f3853-4f67-4959-b834-0654d50a120d · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 94
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation fae009f2-d90b-4952-9ce8-779970b38ba5 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 98
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation fd53ccf2-8951-45ce-9735-0ba22c1aecd7 · 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 Revisiting holographic dark energy after DESI 2024
Reference 53
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 90ccf01e-248f-4adf-aa30-6424f0dd6a2b · inbound
Robust Preference for Dark Sector Interactions cites this paper.
Robust Preference for Dark Sector Interactions Revisiting holographic dark energy after DESI 2024
Reference 22
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 94fb8cc2-da09-4766-b33e-1ebfb0624ac6 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 58
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation d3d6f401-674c-45a6-9287-8c7b5c93465f · inbound
Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.
Measuring neutrino mass in light of ACT DR6 and DESI DR2 Revisiting holographic dark energy after DESI 2024
Reference 125
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e1a39c2d-1073-475b-ba91-9a8d281d0578 · inbound
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 Revisiting holographic dark energy after DESI 2024
Reference 34
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation ac40267f-9caf-494e-b499-e499418dd0cd · 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 Revisiting holographic dark energy after DESI 2024
Reference 56
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation f0f49c5b-6e2f-4708-82d6-0a206422d943 · inbound
Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection cites this paper.
Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection Revisiting holographic dark energy after DESI 2024
Reference 50
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 0f259ac1-ff1f-49e6-b594-7e395d0e7de5 · inbound
Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays cites this paper.
Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays Revisiting holographic dark energy after DESI 2024
Reference 15
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 846ff88d-9484-40ea-a9c0-c4bd41148b5b · 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 Revisiting holographic dark energy after DESI 2024
Reference 30
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 95d0f56e-cfee-4eff-bf89-b02c2613f4ce · 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 Revisiting holographic dark energy after DESI 2024
Reference 75
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 13044591-f84f-4523-aa47-2b41fe8b86a3 · inbound
HIcosmo: a differentiable JAX-based framework for cosmology inference cites this paper.
HIcosmo: a differentiable JAX-based framework for cosmology inference Revisiting holographic dark energy after DESI 2024
Reference 66
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation e52bb9be-0490-432e-9531-28b9bcef1a20 · inbound
Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.
Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Revisiting holographic dark energy after DESI 2024
Reference 130
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 867f059f-6c89-4d73-b410-32337e597ef5 · 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 Revisiting holographic dark energy after DESI 2024
Reference 95
- Resolution
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Source-reported events for the cited work
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Observation 0ee9bd43-0e8b-45b7-85d9-d0784e923994 · inbound
Imprint of swampland-inspired coupled early dark energy cites this paper.
Imprint of swampland-inspired coupled early dark energy Revisiting holographic dark energy after DESI 2024
Reference 49
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.
Observation 92420f23-ddf4-4a24-9b39-5b8dea8a54d6 · inbound
Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent cites this paper.
Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent Revisiting holographic dark energy after DESI 2024
Reference 30
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.