Paper Citation Record · LEDGER

Exploring parametrized dark energy models in interacting scenario

As of 8 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 4 inbound Pith citation observations for arXiv:2505.16438.

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

pith.paper-citation-record.v1
2505.16438 v1

Coverage vector

measured 40 of 40 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-07T15:07:16.440283Z

measured 44 of 44 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:36:59.514284Z

measured 0 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-15T13:15:50.209661Z

Reference resolution

40 of 40 outbound references displayed

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External citation measurements

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Outbound references

Observation 21806e0f-e213-4f5a-8c25-0253b36c8f22 · outbound

This paper cites an unresolved cited work.

Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 1

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Observation 7447b1be-7bb3-43aa-b660-db7b798c44c7 · outbound

This paper cites Perlmutter, G.

Exploring parametrized dark energy models in interacting scenario Perlmutter, G

Reference 2

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Observation 373de35b-e6a5-46e3-85f2-00856b988c8e · outbound

This paper cites Arnaud, M.

Exploring parametrized dark energy models in interacting scenario Arnaud, M

Reference 3

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This paper cites an unresolved cited work.

Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 4

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Observation e67f1ea1-6123-45b6-9a66-450d939a8e78 · outbound

This paper cites Jarosik, C.

Exploring parametrized dark energy models in interacting scenario Jarosik, C

Reference 5

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Observation a5ec755e-3ac2-48f9-a698-53f91e4caff1 · outbound

This paper cites Ratra, P.

Exploring parametrized dark energy models in interacting scenario Ratra, P

Reference 6

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Observation fed2dcb8-4dbf-4d56-8ad2-4721bba9df62 · outbound

This paper cites an unresolved cited work.

Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 7

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Observation 47fc3d6d-2de5-4b35-82db-0e977406c2f9 · outbound

This paper cites Caldwell, A phantom menace? cosmological consequences of a dark energy component with super-negative equation of state, Physics Letters B 545 (1–2) (2002) 23–29.

Exploring parametrized dark energy models in interacting scenario Caldwell, A phantom menace? cosmological consequences of a dark energy component with super-negative equation of state, Physics Letters B 545 (1–2) (2002) 23–29

Reference 8

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 9

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 10

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Observation df8fddc7-3972-49ec-8ef3-571606d1926d · outbound

This paper cites Bousso, The holographic principle, Reviews of Modern Physics 74 (3) (2002) 825–874.

Exploring parametrized dark energy models in interacting scenario Bousso, The holographic principle, Reviews of Modern Physics 74 (3) (2002) 825–874

Reference 11

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Observation f41886af-04d6-46f1-b7b7-d7d02dd2d132 · outbound

This paper cites Holography and Cosmology.

Exploring parametrized dark energy models in interacting scenario Holography and Cosmology

Reference 12

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Observation 62146bbb-b466-4633-af7c-6989c743125b · outbound

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

Exploring parametrized dark energy models in interacting scenario In the Realm of the Hubble tension $-$ a Review of Solutions

Reference 13

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Observation b3e6514b-a0b1-4ce0-a6d5-53aa8e874fa8 · outbound

This paper cites Zimdahl, D.

Exploring parametrized dark energy models in interacting scenario Zimdahl, D

Reference 14

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Observation f04f40c8-ff9c-44cb-b410-060944f7d6cb · outbound

This paper cites Models of Interacting Dark Energy.

Exploring parametrized dark energy models in interacting scenario Models of Interacting Dark Energy

Reference 15

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Observation 490f0658-6c05-4c28-b05e-ab172e1a5369 · outbound

This paper cites Del Campo, R.

Exploring parametrized dark energy models in interacting scenario Del Campo, R

Reference 16

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Observation 0c575312-0560-4dbd-86a0-04d9bc5d8d18 · outbound

This paper cites Olivares, F.

Exploring parametrized dark energy models in interacting scenario Olivares, F

Reference 17

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Observation 45171475-7554-47ad-b92b-01f451336dc8 · outbound

This paper cites Sinha, M.

Exploring parametrized dark energy models in interacting scenario Sinha, M

Reference 18

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Observation 7dc29041-b6a8-4763-91f2-523ae95a3506 · outbound

This paper cites an unresolved cited work.

Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 19

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Observation d5d7def0-6d7c-46c1-8ff0-6f9bb11d7ebc · outbound

This paper cites Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae.

Exploring parametrized dark energy models in interacting scenario Testing the phenomenological interacting dark energy model with gamma-ray bursts and Pantheon+ type Ia supernovae

Reference 20

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Observation 19e3de20-e3e9-4630-9f2d-87fec0cbb063 · outbound

This paper cites Brout, D.

Exploring parametrized dark energy models in interacting scenario Brout, D

Reference 21

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 22

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Observation 55c34b6f-f2ca-41d2-aec1-700b005c41ed · outbound

This paper cites Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity.

Exploring parametrized dark energy models in interacting scenario Cosmic acceleration with bulk viscosity in modified $f(Q)$ gravity

Reference 23

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Observation bd27f4e3-3803-4a54-b1b3-c35e1448c200 · outbound

This paper cites New parametrization of the dark-energy equation of state with a single parameter.

Exploring parametrized dark energy models in interacting scenario New parametrization of the dark-energy equation of state with a single parameter

Reference 24

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 25

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Observation 5e01231f-ebf9-48ff-bf6f-4dc010743f4e · outbound

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 26

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Observation 6f7cbe68-dded-4066-9767-0bcf99dcd1fc · outbound

This paper cites emcee v3: A Python ensemble sampling toolkit for affine-invariant MCMC.

Exploring parametrized dark energy models in interacting scenario emcee v3: A Python ensemble sampling toolkit for affine-invariant MCMC

Reference 27

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This paper cites GetDist: a Python package for analysing Monte Carlo samples.

Exploring parametrized dark energy models in interacting scenario GetDist: a Python package for analysing Monte Carlo samples

Reference 28

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This paper cites The Pantheon Sample Analysis of Cosmological Constraints under New Models.

Exploring parametrized dark energy models in interacting scenario The Pantheon Sample Analysis of Cosmological Constraints under New Models

Reference 29

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 30

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 31

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Observation 936170bc-f696-4b57-9165-3cf379291708 · outbound

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Exploring parametrized dark energy models in interacting scenario Goswami, S

Reference 32

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Exploring parametrized dark energy models in interacting scenario Unresolved cited work

Reference 33

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Observation 7f423890-7a20-4882-b4fe-8395fb535dd8 · outbound

This paper cites Mandal, S.

Exploring parametrized dark energy models in interacting scenario Mandal, S

Reference 34

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This paper cites The impact of the cosmic variance on $H_0$ on cosmological analyses.

Exploring parametrized dark energy models in interacting scenario The impact of the cosmic variance on $H_0$ on cosmological analyses

Reference 35

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This paper cites Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\Lambda$CDM Model.

Exploring parametrized dark energy models in interacting scenario Exploring the Possibility of Interacting Quintessence Model as an Alternative to the $\Lambda$CDM Model

Reference 36

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

Exploring parametrized dark energy models in interacting scenario Planck 2018 results. VI. Cosmological parameters

Reference 37

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Exploring parametrized dark energy models in interacting scenario Sahni, A

Reference 38

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Exploring parametrized dark energy models in interacting scenario Pav ´on, B

Reference 39

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Observation fcabd56b-c216-4e42-8c88-c59cfd6beed8 · outbound

This paper cites Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data.

Exploring parametrized dark energy models in interacting scenario Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data

Reference 40

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Pith citing papers

Observation 67bc321b-a70d-4b2e-9b42-6fa0f763c410 · 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 Exploring parametrized dark energy models in interacting scenario

Reference 45

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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 Exploring parametrized dark energy models in interacting scenario

Reference 32

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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 Exploring parametrized dark energy models in interacting scenario

Reference 129

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Observation eb2ed846-6baa-4efe-b9e3-51c1a2ed183d · 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 Exploring parametrized dark energy models in interacting scenario

Reference 45

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