Paper Citation Record · LEDGER

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

As of 19 August 2026, this Paper Citation Record lists 52 of 52 outbound references and 12 inbound Pith citation observations for arXiv:2504.15190.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2504.15190 v3

Coverage vector

measured 52 of 52 reference resolution

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:27:54.447261Z

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Source: arxiv_reference, observed 2026-05-22T20:55:08.595760Z

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External citation measurements

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Outbound references

Observation 8ea1cf11-130a-4b44-8d27-49355a82cd25 · outbound

This paper cites DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations

Reference 1

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Observation eb842551-23ab-4b2e-8ef0-1d4119694b6e · outbound

This paper cites DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data

Reference 2

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Observation 96a3742b-4488-40e6-9fa0-f1a2657cd03f · outbound

This paper cites DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data

Reference 3

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Observation 29234a6f-9545-45bf-a58a-2df477d18a22 · outbound

This paper cites DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 4

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Observation 79d96d37-d09d-45e3-9b24-4774efe7063a · outbound

This paper cites Extended Dark Energy analysis using DESI DR2 BAO measurements.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Extended Dark Energy analysis using DESI DR2 BAO measurements

Reference 5

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Observation 87037580-206f-4251-93e8-4fec5c075b9e · outbound

This paper cites Assessing cosmological evidence for non-minimal coupling.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Assessing cosmological evidence for non-minimal coupling

Reference 6

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Observation e97785f9-c077-4d2c-a521-73ede3d4d68d · outbound

This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result

Reference 7

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Observation 5ece4cd2-4c17-4541-84c6-3f9e6d58ff6d · 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?.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background 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 8

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Observation 2f54c8f7-6b4f-4a16-90e8-1d19c3ffef1e · outbound

This paper cites Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?

Reference 9

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Unresolved cited work

Reference 10

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Observation d1c44285-bcec-4905-98b8-c3b0d5347909 · outbound

This paper cites Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension

Reference 11

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Observation 46446daf-6afd-4f90-aa4e-54bb262ffe9e · outbound

This paper cites an unresolved cited work.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Unresolved cited work

Reference 12

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Observation 6501fee1-772b-45f6-b91a-f812cfeae6d9 · outbound

This paper cites Chakraborty , author P.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Chakraborty , author P

Reference 13

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Observation e42ae125-1b58-42c9-9c04-7c1022721f2a · outbound

This paper cites Improved null tests of $\Lambda$CDM and FLRW in light of DESI DR2.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Improved null tests of $\Lambda$CDM and FLRW in light of DESI DR2

Reference 14

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Observation 1d39559b-bf7a-4733-8227-52992b0ff6aa · outbound

This paper cites Model-agnostic assessment of dark energy after DESI DR1 BAO.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Model-agnostic assessment of dark energy after DESI DR1 BAO

Reference 15

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Observation 8db021c7-4760-463b-af16-480eab2c2861 · outbound

This paper cites A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data

Reference 16

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Observation 3ef09265-729d-4e8a-a699-4c7fe84d58fa · outbound

This paper cites Large-scale instability in interacting dark energy and dark matter fluids.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Large-scale instability in interacting dark energy and dark matter fluids

Reference 17

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Observation 14ff1d70-10fd-43e1-be37-0e52a3b869b5 · outbound

This paper cites Modified Gravity and Cosmology.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Modified Gravity and Cosmology

Reference 18

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Observation 66d464b6-75ab-42c8-b4c8-a9be718c44a6 · outbound

This paper cites The Dynamics of Quintessence, The Quintessence of Dynamics.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background The Dynamics of Quintessence, The Quintessence of Dynamics

Reference 19

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Observation 2242ae9f-6334-40f7-9cfd-6ae449b98981 · outbound

This paper cites Quintessence's Last Stand?.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Quintessence's Last Stand?

Reference 20

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Observation 563b67a8-e2dc-4873-bb4e-ccfe9c0fdb2f · outbound

This paper cites The Limits of Quintessence.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background The Limits of Quintessence

Reference 21

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Observation 658f7285-6127-43e8-a337-53ad24a81038 · outbound

This paper cites Quintessence: A Review.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Quintessence: A Review

Reference 22

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Observation 863177bd-a5ef-4a44-ab47-c43a813d3de6 · outbound

This paper cites Cosmological Imprint of an Energy Component with General Equation of State.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Cosmological Imprint of an Energy Component with General Equation of State

Reference 23

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Observation e444b273-82e6-428a-ac44-80a1c5c2b32e · outbound

This paper cites Scalar-field-dominated cosmology with a transient accelerating phase.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Scalar-field-dominated cosmology with a transient accelerating phase

Reference 24

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This paper cites Optimal parameterizations for observational constraints on thawing dark energy.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Optimal parameterizations for observational constraints on thawing dark energy

Reference 25

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This paper cites DESI Dark Secrets.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI Dark Secrets

Reference 26

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background General parametrization for energy density of quintessence field

Reference 27

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Observation 2247c1e6-75a2-4ad5-91cf-ec20ca2c025b · outbound

This paper cites In the Realm of the Hubble tension $-$ a Review of Solutions.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 28

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This paper cites Cosmic expansion parametrization: Implication for curvature and $\text{H}_{0}$ tension.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Cosmic expansion parametrization: Implication for curvature and $\text{H}_{0}$ tension

Reference 29

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This paper cites Is Local $H_0$ At Odds With Dark Energy EFT?.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Is Local $H_0$ At Odds With Dark Energy EFT?

Reference 30

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This paper cites Has DESI detected exponential quintessence?.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Has DESI detected exponential quintessence?

Reference 31

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Bounded Dark Energy

Reference 32

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Scalar field dark energy models: Current and forecast constraints

Reference 33

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This paper cites Robustness of dark energy phenomenology across different parameterizations.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Robustness of dark energy phenomenology across different parameterizations

Reference 34

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Dubey , author S

Reference 35

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This paper cites Quintessential interpretation of the evolving dark energy in light of DESI.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Quintessential interpretation of the evolving dark energy in light of DESI

Reference 36

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background DESI Constraints on Exponential Quintessence

Reference 37

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Observation 3bb7edb6-5e9b-4f3c-a0cb-ca36f67154dd · outbound

This paper cites Scant evidence for thawing quintessence.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Scant evidence for thawing quintessence

Reference 38

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This paper cites Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Beyond dark energy Fisher forecasts: how DESI will constrain LCDM and quintessence models

Reference 40

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Do Observations Prefer Thawing Quintessence?

Reference 41

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Aspects of the cosmological "coincidence problem"

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Dark Energy Constraints and Joint Cosmological Inference from Mutually Inconsistent Observations

Reference 43

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This paper cites Probing dark energy using convergence power spectrum and bi-spectrum.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Probing dark energy using convergence power spectrum and bi-spectrum

Reference 45

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Cosmological constraints on curved quintessence

Reference 46

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Exponential Quintessence: curved, steep and stringy?

Reference 47

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Thawing quintessence with a nearly flat potential

Reference 48

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This paper cites Observational Constraints on Quintessence: Thawing, Tracker, and Scaling models.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Observational Constraints on Quintessence: Thawing, Tracker, and Scaling models

Reference 49

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This paper cites Imprint of thawing scalar fields on large scale galaxy overdensity.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Imprint of thawing scalar fields on large scale galaxy overdensity

Reference 50

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Quintessence, Cosmic Coincidence, and the Cosmological Constant

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Physical vs phantom dark energy after DESI: thawing quintessence in a curved background The Case for a Positive Cosmological Lambda-term

Reference 52

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Pith citing papers

Observation 2d5d9161-ed9c-4d8e-ac10-2af9d8e04bae · inbound

Hubble tension and small-scale inhomogeneities on light propagation cites this paper.

Hubble tension and small-scale inhomogeneities on light propagation Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 12

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Observation b641a23a-1ee6-4466-b6af-0d28c4ccc4e6 · inbound

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition cites this paper.

Challenging $\Lambda$CDM: 5$\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 96

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf30cc7f-2ff3-4c91-83ca-6d69bff434e5 · inbound

It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2 cites this paper.

It's All ${\tt Ok}$: Curvature in Light of BAO from DESI DR2 Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-16T04:44:34.628303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85ddcbee-ea72-4bbe-9617-9864825f92bb · inbound

Examining Quintessence Models with DESI Data cites this paper.

Examining Quintessence Models with DESI Data Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T14:30:35.453275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0b6ebbdf-c3fb-4a80-bc16-475cd66343f3 · inbound

Topological defects as effective dynamical dark energy cites this paper.

Topological defects as effective dynamical dark energy Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T04:41:33.603337Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5d07604-d1ba-4821-9aef-e75c6281d46a · inbound

Implications for dark energy of cosmic transparency in light of DESI data cites this paper.

Implications for dark energy of cosmic transparency in light of DESI data Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-06T22:08:48.898139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 25963578-5f72-498f-8bf2-62c38bc7bbe4 · inbound

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data cites this paper.

Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-05-18T15:51:35.039937Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 3bc148c4-8718-4b58-9e61-62ef38d03383 · inbound

Cosmological constraints on Galileon dark energy with broken shift symmetry cites this paper.

Cosmological constraints on Galileon dark energy with broken shift symmetry Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-15T15:54:51.038744Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7dd5088-71aa-4763-998d-9d868f39d1bc · inbound

Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide cites this paper.

Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 51

Resolution: verified exact; arxiv_id, observed 2026-05-11T07:21:00.237359Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation dcb673cb-c282-4be8-9b35-58019415f8b0 · 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 Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 236

Resolution: unresolved; no resolver link, observed 2026-08-02T14:29:38.520413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 013b9b2a-60a7-40a6-9751-c9103d87050f · inbound

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison cites this paper.

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison Physical vs phantom dark energy after DESI: thawing quintessence in a curved background

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-14T19:12:51.496555Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation da033328-070d-484d-841b-2da05ffc0ceb · inbound

No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison cites this paper.

Reference 41

Resolution: verified exact; arxiv_id, observed 2026-05-21T08:19:52.311888Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.