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Source: paper_references, paper_reference_links, observed 2026-08-12T13:51:30.715897Z
Paper Citation Record · LEDGER
General parametrization for energy density of quintessence field
As of 22 August 2026, this Paper Citation Record lists 73 of 73 outbound references and 11 inbound Pith citation observations for arXiv:2411.15892.
A citation records a reference. It does not transfer a finding from one paper to another.
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Source: paper_references, paper_reference_links, observed 2026-08-16T11:37:32.170844Z
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Source: pith, observed 2026-07-08T15:55:05.051740Z
Reference resolution
73 of 73 outbound references displayed
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External citation measurements
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Outbound references
Observation 87bb8ee6-1cf3-4b4b-9e60-6a18044c70f6 · outbound
This paper cites Planck 2013 results. XVI. Cosmological parameters.
General parametrization for energy density of quintessence field Planck 2013 results. XVI. Cosmological parameters
Reference 1
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Observation 14eacc21-c062-4e2a-9a92-3205230bfa96 · outbound
This paper cites Dynamics of dark energy.
General parametrization for energy density of quintessence field Dynamics of dark energy
Reference 2
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Observation bb2ea6e0-0d49-4994-8f48-711fa2a7b303 · outbound
This paper cites Dynamical systems applied to cosmology: dark energy and modified gravity.
General parametrization for energy density of quintessence field Dynamical systems applied to cosmology: dark energy and modified gravity
Reference 3
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Observation a185ad86-d237-4796-b64d-12add0965fdb · outbound
This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team.
General parametrization for energy density of quintessence field A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
Reference 4
- Resolution
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Observation 5738b904-2e3f-412f-aa68-d74b673c1933 · outbound
This paper cites Planck 2018 results. VI. Cosmological parameters.
General parametrization for energy density of quintessence field Planck 2018 results. VI. Cosmological parameters
Reference 5
- Resolution
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Observation 27b108e8-7c05-467d-839d-a3884367e88f · outbound
This paper cites The Hubble Tension and Early Dark Energy.
General parametrization for energy density of quintessence field The Hubble Tension and Early Dark Energy
Reference 6
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Observation 50a2c367-054a-46b1-abff-f157baf25610 · outbound
This paper cites Progress in Direct Measurements of the Hubble Constant.
General parametrization for energy density of quintessence field Progress in Direct Measurements of the Hubble Constant
Reference 7
- Resolution
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Observation c79a0fac-a7df-4618-abca-ef0faf965463 · outbound
This paper cites The trouble with $H_0$.
General parametrization for energy density of quintessence field The trouble with $H_0$
Reference 8
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Observation 56efff06-4bb1-4482-b231-1203541d0f42 · outbound
This paper cites The Hubble Hunter's Guide.
General parametrization for energy density of quintessence field The Hubble Hunter's Guide
Reference 9
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Observation cbd12adb-5fd7-48fa-8323-ef1d1ea5ada4 · outbound
This paper cites Challenges for $\Lambda$CDM: An update.
General parametrization for energy density of quintessence field Challenges for $\Lambda$CDM: An update
Reference 10
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Observation 06b6486e-d58b-47d5-85d5-bf9aad23cf26 · outbound
This paper cites DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys.
General parametrization for energy density of quintessence field DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
Reference 11
- Resolution
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Observation b72773a8-99bb-49a1-8413-eeaab8e68c9d · outbound
This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.
General parametrization for energy density of quintessence field DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
Reference 12
- Resolution
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Unavailable: canonical work link unavailable.
Observation 6a5db833-b4be-4af0-8498-bb64b74f1659 · outbound
This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.
General parametrization for energy density of quintessence field DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data
Reference 13
- Resolution
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Unavailable: canonical work link unavailable.
Observation 9287421a-7f07-4aa2-9f41-fa87b5f0321c · outbound
This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.
General parametrization for energy density of quintessence field DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data
Reference 14
- Resolution
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Unavailable: canonical work link unavailable.
Observation 0895ca74-f2dd-409c-83be-040742e07c61 · outbound
This paper cites Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements.
General parametrization for energy density of quintessence field Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
Reference 15
- Resolution
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Observation aede10a5-ca0f-4b55-a035-c2e3f5fa9502 · outbound
This paper cites Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements.
General parametrization for energy density of quintessence field Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements
Reference 16
- Resolution
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Observation 80ef6ee9-fc0e-42d8-a6ef-df84c8587866 · outbound
This paper cites Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing.
General parametrization for energy density of quintessence field Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing
Reference 17
- Resolution
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Observation c769b158-beb4-4c23-a5a4-b9088aa45a9a · outbound
This paper cites Dark energy in light of recent DESI BAO and Hubble tension.
General parametrization for energy density of quintessence field Dark energy in light of recent DESI BAO and Hubble tension
Reference 18
- Resolution
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Observation 1190e88e-d899-4e1c-b798-abfd4d8cca99 · outbound
This paper cites Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements.
General parametrization for energy density of quintessence field Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
Reference 19
- Resolution
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Observation 06eb4e65-eb78-40b3-84aa-a4bf3f336e6c · outbound
This paper cites Assessing observational constraints on dark energy.
General parametrization for energy density of quintessence field Assessing observational constraints on dark energy
Reference 20
- Resolution
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Observation cc0c5acf-fd16-4e9c-a4bc-7372dc97f372 · outbound
This paper cites Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements.
General parametrization for energy density of quintessence field Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements
Reference 21
- Resolution
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Observation b49bb3d9-81f3-4052-bc17-e0032c8dbaf3 · outbound
This paper cites DESI Constraints on Exponential Quintessence.
General parametrization for energy density of quintessence field DESI Constraints on Exponential Quintessence
Reference 22
- Resolution
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Observation a42774a6-c06c-4f47-bb3a-e30b9fa5b9e4 · outbound
This paper cites Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data.
General parametrization for energy density of quintessence field Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data
Reference 23
- Resolution
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Observation c75f7a37-693e-4358-b590-12d39fcf21ee · outbound
This paper cites Do Observations Prefer Thawing Quintessence?.
General parametrization for energy density of quintessence field Do Observations Prefer Thawing Quintessence?
Reference 24
- Resolution
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- no resolver link, observed 2026-08-12T13:51:30.445387Z
Source-reported events for the cited work
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Observation cbf343e4-267e-4bc6-86d1-814207519fdd · outbound
This paper cites Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology.
General parametrization for energy density of quintessence field Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $\Lambda$CDM cosmology
Reference 25
- Resolution
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Observation 6150f789-4830-4f09-885e-6b33238434a0 · outbound
This paper cites Underdetermination of dark energy.
General parametrization for energy density of quintessence field Underdetermination of dark energy
Reference 26
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Observation 94a85d11-bb18-4875-beaf-a859525ae220 · outbound
This paper cites Scant evidence for thawing quintessence.
General parametrization for energy density of quintessence field Scant evidence for thawing quintessence
Reference 27
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Observation d14a1f9f-5567-4342-8877-c4cfacde321b · outbound
This paper cites Matching current observational constraints with nonminimally coupled dark energy.
General parametrization for energy density of quintessence field Matching current observational constraints with nonminimally coupled dark energy
Reference 28
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Observation 67275906-fc36-4137-b2e8-54f84efdba12 · outbound
This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.
General parametrization for energy density of quintessence field Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result
Reference 29
- Resolution
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Observation ef9dabc4-3ea0-49db-8b37-87a3fec5afef · outbound
This paper cites Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?.
General parametrization for energy density of quintessence field Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?
Reference 30
- Resolution
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Unavailable: canonical work link unavailable.
Observation 098b1f72-6158-4f05-ad00-4de06dc85779 · outbound
This paper cites Does DESI 2024 Confirm $\Lambda$CDM?.
General parametrization for energy density of quintessence field Does DESI 2024 Confirm $\Lambda$CDM?
Reference 31
- Resolution
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Observation a990d5c9-1693-48e0-a14e-d871b8ca3646 · outbound
This paper cites Ratra and P.J.E.
General parametrization for energy density of quintessence field Ratra and P.J.E
Reference 32
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Observation bf79bca2-3fca-4c29-b563-b45d73f10ef3 · outbound
This paper cites Wetterich,Cosmologies With Variable Newton’s ’Constant’, Nucl.
General parametrization for energy density of quintessence field Wetterich,Cosmologies With Variable Newton’s ’Constant’, Nucl
Reference 33
- Resolution
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Observation 66109756-0668-4ada-a6c6-f5d3bf0713f6 · outbound
This paper cites Cosmology and the Fate of Dilatation Symmetry.
General parametrization for energy density of quintessence field Cosmology and the Fate of Dilatation Symmetry
Reference 34
- Resolution
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Observation 390f5207-ffa7-477e-b46e-eccccda10ae3 · outbound
This paper cites Exponential potentials and cosmological scaling solutions.
General parametrization for energy density of quintessence field Exponential potentials and cosmological scaling solutions
Reference 35
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Source-reported events for the cited work
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Observation d889244d-b2c4-4db5-a5df-fd77684e0945 · outbound
This paper cites Quintessence arising from exponential potentials.
General parametrization for energy density of quintessence field Quintessence arising from exponential potentials
Reference 36
- Resolution
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Observation c743ba6e-f909-4216-ad4d-cd33cb041e97 · outbound
This paper cites A New Cosmological Model of Quintessence and Dark Matter.
General parametrization for energy density of quintessence field A New Cosmological Model of Quintessence and Dark Matter
Reference 37
- Resolution
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Observation bb2005fb-1c05-4d32-ae83-42386f443dcd · outbound
This paper cites Cosmological Tracking Solutions.
General parametrization for energy density of quintessence field Cosmological Tracking Solutions
Reference 38
- Resolution
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Source-reported events for the cited work
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Observation ec3e909a-5071-4869-aa38-95ec8739473e · outbound
This paper cites Quintessence, Cosmic Coincidence, and the Cosmological Constant.
General parametrization for energy density of quintessence field Quintessence, Cosmic Coincidence, and the Cosmological Constant
Reference 39
- Resolution
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Observation 98f218f3-3a91-4d06-a1f9-ff7b9eede151 · outbound
This paper cites Thawing quintessence with a nearly flat potential.
General parametrization for energy density of quintessence field Thawing quintessence with a nearly flat potential
Reference 40
- Resolution
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Unavailable: canonical work link unavailable.
Observation 1d203e5f-5dab-4b98-8d1f-b1478c71f1fb · outbound
This paper cites A comparison between axion-like and power law potentials in cosmological background.
General parametrization for energy density of quintessence field A comparison between axion-like and power law potentials in cosmological background
Reference 41
- Resolution
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Observation 4de99c70-d801-451a-a301-695ed6e3787f · outbound
This paper cites Accelerating Universes with Scaling Dark Matter.
General parametrization for energy density of quintessence field Accelerating Universes with Scaling Dark Matter
Reference 42
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 68255b10-50d3-469d-a616-bea55d62d65c · outbound
This paper cites Exploring the Expansion History of the Universe.
General parametrization for energy density of quintessence field Exploring the Expansion History of the Universe
Reference 43
- Resolution
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Observation 69765275-2f10-48b0-abb5-5ac34a77b3bd · outbound
This paper cites Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies.
General parametrization for energy density of quintessence field Constraining the equation of state of the Universe from Distant Type Ia Supernovae and Cosmic Microwave Background Anisotropies
Reference 44
- Resolution
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Observation 6b7f0cc5-7d3a-4bfd-99cb-830ae116f505 · outbound
This paper cites Observational constraints on low redshift evolution of dark energy: How consistent are different observations?.
General parametrization for energy density of quintessence field Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
Reference 45
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1f28afd1-e22d-4ece-9ed0-915b1e0424bd · outbound
This paper cites A parametric model for dark energy.
General parametrization for energy density of quintessence field A parametric model for dark energy
Reference 46
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 40a28937-f8e4-46e7-887a-555ca7306fe4 · outbound
This paper cites The Limits of Quintessence.
General parametrization for energy density of quintessence field The Limits of Quintessence
Reference 47
- Resolution
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Source-reported events for the cited work
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Observation 6bfaeff7-e469-4fd8-a573-617562c08462 · outbound
This paper cites Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential.
General parametrization for energy density of quintessence field Phase Space Analysis of Quintessence Cosmologies with a Double Exponential Potential
Reference 48
- Resolution
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Observation b475a8cb-6d82-4f98-aa01-b8e93ae2373b · outbound
This paper cites Turner,Coherent Scalar Field Oscillations in an Expanding Universe, Phys.
General parametrization for energy density of quintessence field Turner,Coherent Scalar Field Oscillations in an Expanding Universe, Phys
Reference 49
- Resolution
- verified fuzzy
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Observation c500083f-1ba5-44c5-9a58-e76262108200 · outbound
This paper cites Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data.
General parametrization for energy density of quintessence field Tension and constraints on modified gravity parametrizations of $G_{\textrm{eff}}(z)$ from growth rate and Planck data
Reference 50
- Resolution
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Unavailable: canonical work link unavailable.
Observation c9a7648d-c81b-4779-8e8c-6c36a2653203 · outbound
This paper cites Axion Cosmology.
General parametrization for energy density of quintessence field Axion Cosmology
Reference 51
- Resolution
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Observation cfdc0712-b2c1-4b89-973a-5f724c19d75b · outbound
This paper cites Early Dark Energy Can Resolve The Hubble Tension.
General parametrization for energy density of quintessence field Early Dark Energy Can Resolve The Hubble Tension
Reference 52
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 872a187b-91d7-4a14-982d-789ad48dfd4d · outbound
This paper cites Cosmological implications of ultra-light axion-like fields.
General parametrization for energy density of quintessence field Cosmological implications of ultra-light axion-like fields
Reference 53
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a4308ffc-df41-449e-bbad-c6e7120054cd · outbound
This paper cites The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023.
General parametrization for energy density of quintessence field The Ups and Downs of Early Dark Energy solutions to the Hubble tension: a review of models, hints and constraints circa 2023
Reference 54
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 37fb4649-bd60-498c-93a1-cdb6e57bfb2b · outbound
This paper cites Oscillating scalar fields and the Hubble tension: a resolution with novel signatures.
General parametrization for energy density of quintessence field Oscillating scalar fields and the Hubble tension: a resolution with novel signatures
Reference 55
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6ff1e5b5-8b48-4653-91e7-2a00d686595a · outbound
This paper cites A search for ultra-light axions using precision cosmological data.
General parametrization for energy density of quintessence field A search for ultra-light axions using precision cosmological data
Reference 56
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a1ca1817-8435-4045-be8c-a3a1532a308c · outbound
This paper cites Akaike,A New Look at the Statistical Model Identification, IEEE Transactions on Automatic Control 19 (1974) 716.
General parametrization for energy density of quintessence field Akaike,A New Look at the Statistical Model Identification, IEEE Transactions on Automatic Control 19 (1974) 716
Reference 57
- Resolution
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- raw_fallback, observed 2026-08-12T13:51:31.896769Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 8f6c2812-e4a9-4ef9-bb75-c3e17ff27a69 · outbound
This paper cites Cosmological model selection.
General parametrization for energy density of quintessence field Cosmological model selection
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.616909Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation da501003-bd1e-40ce-9c34-24c15bbddf63 · outbound
This paper cites Bayesian Methods in Cosmology.
General parametrization for energy density of quintessence field Bayesian Methods in Cosmology
Reference 59
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.624256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3dd8d7a5-a1f9-4a9d-932b-f31cbaba65bc · outbound
This paper cites A comprehensive comparison of cosmological models from latest observational data.
General parametrization for energy density of quintessence field A comprehensive comparison of cosmological models from latest observational data
Reference 60
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.635384Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 577cb248-bc36-46b7-b2cc-4a92562fc55c · outbound
This paper cites emcee: The MCMC Hammer.
General parametrization for energy density of quintessence field emcee: The MCMC Hammer
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.642134Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e1c9b6a6-7f9b-4f06-a9b0-a7bd422f3b6f · outbound
This paper cites GetDist: a Python package for analysing Monte Carlo samples.
General parametrization for energy density of quintessence field GetDist: a Python package for analysing Monte Carlo samples
Reference 62
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.647891Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9d7c5321-d818-40c4-999d-e14baab4cd10 · outbound
This paper cites Gelman and D.B.
General parametrization for energy density of quintessence field Gelman and D.B
Reference 63
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-12T13:51:31.884139Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 849bb4de-ade9-4ca3-a13e-dfa280732ab7 · outbound
This paper cites Distance Priors from Planck Final Release.
General parametrization for energy density of quintessence field Distance Priors from Planck Final Release
Reference 64
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.661185Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 12ff97f3-9c41-4577-ab56-8d20d0b797ca · outbound
This paper cites DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars.
General parametrization for energy density of quintessence field DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
Reference 65
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.667645Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5c9ce665-e58a-4eba-9bbf-540f0ee5d805 · outbound
This paper cites DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest.
General parametrization for energy density of quintessence field DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
Reference 66
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.677185Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f05df5b8-8970-42b2-997d-70c043a253b5 · outbound
This paper cites The Pantheon+ Analysis: The Full Dataset and Light-Curve Release.
General parametrization for energy density of quintessence field The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
Reference 67
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.684443Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a01bf9c5-de31-4cd6-b888-5e5ccb1a54d1 · outbound
This paper cites The Pantheon+ Analysis: Cosmological Constraints.
General parametrization for energy density of quintessence field The Pantheon+ Analysis: Cosmological Constraints
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.690462Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2423588-a491-4061-a5ef-e3efb3da1699 · outbound
This paper cites $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method.
General parametrization for energy density of quintessence field $H_0$ from cosmic chronometers and Type Ia supernovae, with Gaussian Processes and the novel Weighted Polynomial Regression method
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.694934Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3e7950fb-5d40-411c-95d7-5e579461b60e · outbound
This paper cites Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches.
General parametrization for energy density of quintessence field Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches
Reference 70
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.700138Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 75498b07-107c-4f5c-9a9b-d0de9cedfa9e · outbound
This paper cites New physics in light of the $H_0$ tension: an alternative view.
General parametrization for energy density of quintessence field New physics in light of the $H_0$ tension: an alternative view
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.705481Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1a35d82b-4179-43d5-af37-0eb2a531a406 · outbound
This paper cites Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z) \geq -1$ are tighter than those obtained in $\Lambda$CDM.
General parametrization for energy density of quintessence field Constraints on the sum of the neutrino masses in dynamical dark energy models with $w(z) \geq -1$ are tighter than those obtained in $\Lambda$CDM
Reference 72
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.710559Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 47cb3ca9-c3b7-47b9-ba94-46818094e442 · outbound
This paper cites Constraining the dark-energy equation of state with cosmological data.
General parametrization for energy density of quintessence field Constraining the dark-energy equation of state with cosmological data
Reference 73
- Resolution
- unresolved
- no resolver link, observed 2026-08-12T13:51:30.715897Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
Observation 49cc3799-4ec1-4bc7-a57c-68571baab858 · 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? General parametrization for energy density of quintessence field
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:00:59.886169Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation deb75ad8-7ebc-4bdf-b17e-79ed6f5dccb5 · inbound
Dark energy and lensing anomaly in Planck CMB data cites this paper.
Dark energy and lensing anomaly in Planck CMB data General parametrization for energy density of quintessence field
Reference 52
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T22:04:59.521471Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6dcfd20e-0870-40eb-8e94-e2e186fb533f · inbound
Robustness of dark energy phenomenology across different parameterizations cites this paper.
Robustness of dark energy phenomenology across different parameterizations General parametrization for energy density of quintessence field
Reference 90
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T21:04:17.845726Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 57b0e5f3-6afd-4a44-b0df-cb10495c330d · inbound
Physical vs phantom dark energy after DESI: thawing quintessence in a curved background cites this paper.
Physical vs phantom dark energy after DESI: thawing quintessence in a curved background General parametrization for energy density of quintessence field
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T11:37:32.170844Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 50e099d8-c2d6-4a79-b092-d1e7a86a3b8d · 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? General parametrization for energy density of quintessence field
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T10:52:56.349433Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 83300037-19a7-4320-b816-1b7604246914 · inbound
Simple quintessence models in light of DESI-BAO observations cites this paper.
Simple quintessence models in light of DESI-BAO observations General parametrization for energy density of quintessence field
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T00:43:09.706256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f9b10b1-82a6-456c-a2bc-bc90b4456cf5 · 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 General parametrization for energy density of quintessence field
Reference 43
- Resolution
- verified exact
- arxiv_id, observed 2026-05-18T10:46:16.532829Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation f0b932aa-3c9e-4da3-b609-a33c3a96d555 · inbound
Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility cites this paper.
Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility General parametrization for energy density of quintessence field
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T21:18:32.697658Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 6d899b9c-61b7-47d6-bcab-8a23e1ee9fbd · 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 General parametrization for energy density of quintessence field
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T14:40:55.423143Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4ef7baf0-437e-4583-8236-83edac15427f · 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 General parametrization for energy density of quintessence field
Reference 80
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T14:27:03.493738Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
Observation 7e1c0b51-1d94-4048-a5d1-2e5395bfb3c8 · inbound
Imprint of swampland-inspired coupled early dark energy cites this paper.
Imprint of swampland-inspired coupled early dark energy General parametrization for energy density of quintessence field
Reference 52
- Resolution
- verified exact
- local_arxiv, observed 2026-07-08T15:55:05.053071Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.