Paper Citation Record · LEDGER

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension

As of 8 August 2026, this Paper Citation Record lists 100 of 100 outbound references and 3 inbound Pith citation observations for arXiv:2506.02235.

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

pith.paper-citation-record.v1
2506.02235 v1

Coverage vector

measured 100 of 100 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:35:05.415106Z

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One-hop event checks from named stored sources.

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measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T11:25:06.228942Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T08:19:44.111735Z

Reference resolution

100 of 100 outbound references displayed

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External citation measurements

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Outbound references

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This paper cites We assume that baryonic matter and cold dark matter are pressureless, i.e., pb = pc = 0.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension We assume that baryonic matter and cold dark matter are pressureless, i.e., pb = pc = 0

Reference 1

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This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 2

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This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 3

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This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 4

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 5

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 6

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This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 7

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 8

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This paper cites Uncertainty Quantification.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Uncertainty Quantification

Reference 9

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This paper cites Baryshev, AIP.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Baryshev, AIP

Reference 10

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Observation 3593c4c5-d61c-459b-91d7-b3c62b605fa3 · outbound

This paper cites Lusso, E.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Lusso, E

Reference 11

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Observation 6a74e6cf-9c17-494f-9268-11b2fc579aa5 · outbound

This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 12

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 13

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Observation 7b1e832f-f3f3-4c46-a28c-9307d4f93a7e · outbound

This paper cites Padmanabhan, Understanding Our Universe: Current Status and Open Issues, 100 years of Relativity (Cambridge University Press, 2005), pp.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Padmanabhan, Understanding Our Universe: Current Status and Open Issues, 100 years of Relativity (Cambridge University Press, 2005), pp

Reference 14

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 15

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 16

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Ratra, J

Reference 17

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This paper cites Caldwell, Phys.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Caldwell, Phys

Reference 18

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This paper cites Feng et al., Phys.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Feng et al., Phys

Reference 19

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Sahni, Class

Reference 20

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 21

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Observation 2ba6e75c-0a65-4d6d-8c3f-4b6e790e5b43 · outbound

This paper cites Susskind, J.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Susskind, J

Reference 22

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This paper cites Bousso, Rev.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Bousso, Rev

Reference 23

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Observation 343f005e-3e41-4dcc-be9b-358f847dc058 · outbound

This paper cites Holography and Cosmology.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Holography and Cosmology

Reference 24

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Jamil, M.U

Reference 25

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Li, Phys

Reference 26

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Sheykhi, Class

Reference 27

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Sheykhi, Phys

Reference 28

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Tsallis, L

Reference 32

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Renyi, Proceedings of the Fourth Berkeley Symposium on Mathematics, Statistics and Probability, University of Cali- 31 fornia Press (1960), pp 547-561

Reference 33

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Sayahian Jahromi, S

Reference 34

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Majhi, Phys

Reference 35

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Kaniadakis, Phys

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Raissi, P

Reference 38

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Zhang, H

Reference 40

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Reference 41

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Tsallis, ”Possible Generalization of Boltzmann-Gibbs Statistics,” J

Reference 43

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Calibration of the Tip of the Red Giant Branch (TRGB)

Reference 45

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant

Reference 46

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This paper cites H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Reference 47

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This paper cites Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing

Reference 48

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This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 49

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Observation 8f57ce4b-0cfd-4e92-9023-92b8368d1544 · outbound

This paper cites Cosmology-independent Estimate of the Hubble Constant and Spatial Curvature Using Time-delay Lenses and Quasars.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Cosmology-independent Estimate of the Hubble Constant and Spatial Curvature Using Time-delay Lenses and Quasars

Reference 50

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This paper cites Tensions between the Early and the Late Universe.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Tensions between the Early and the Late Universe

Reference 51

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This paper cites Physics Letters B, 2020.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Physics Letters B, 2020

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.362628Z

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Observation 989d76f7-c745-4f12-ae6f-2187c8588923 · outbound

This paper cites Physical Review D, 2020.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Physical Review D, 2020

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.344581Z

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Observation 7696c20e-fada-448a-801f-502ef2d05408 · outbound

This paper cites Basilakos, and E.N.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Basilakos, and E.N

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.323003Z

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Observation 346261bf-82e4-4a17-81f9-6cb3ffa9fcb5 · outbound

This paper cites Modified cosmology through spacetime thermodynamics and Barrow horizon entropy.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Modified cosmology through spacetime thermodynamics and Barrow horizon entropy

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.055281Z

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Observation bdd6f242-b863-4d8c-8292-95478f48ad4b · outbound

This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 56

Resolution: unresolved; raw_fallback, observed 2026-08-07T11:35:07.294863Z

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Observation e445de61-dc7c-4d5e-9446-0588d0fddcf1 · outbound

This paper cites Neto, and E.M.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Neto, and E.M

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.269812Z

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Observation b9ed96aa-6347-4353-a83c-d0341c44c713 · outbound

This paper cites Barrow HDE model for Statefinder diagnostic in FLRW Universe.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Barrow HDE model for Statefinder diagnostic in FLRW Universe

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-08-07T11:35:06.497716Z

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Observation 80cbe951-bfaf-4d96-90fe-95d69f462f09 · 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.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension 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 60

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This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 61

Resolution: unresolved; raw_fallback, observed 2026-08-07T11:35:07.246594Z

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Observation 394750ee-e205-4e4f-9474-686add052210 · outbound

This paper cites Barrow and Tsallis entropies in the framework of thermodynamics: A comparative study,.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Barrow and Tsallis entropies in the framework of thermodynamics: A comparative study,

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.227927Z

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Observation 857d58ec-87d9-4d3f-97b2-af4838df4e4b · outbound

This paper cites Modified theories of gravity from nonadditive entropies: Barrow and Tsallis entropies from Verlinde’s scenario,.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Modified theories of gravity from nonadditive entropies: Barrow and Tsallis entropies from Verlinde’s scenario,

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.206891Z

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Observation 452caa63-4219-42fa-9ae1-168c7049bbd8 · outbound

This paper cites Eur.Phys.J.C 84 (2024) 4, 443.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Eur.Phys.J.C 84 (2024) 4, 443

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.184547Z

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Observation d29e1622-939e-4188-a271-ed070c872cd8 · outbound

This paper cites 2024, MNRAS,Pages 3055–3067, https://doi.org/10.1093/mnras/stae2257.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension 2024, MNRAS,Pages 3055–3067, https://doi.org/10.1093/mnras/stae2257

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.121844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 946ba83b-7db9-43b9-b1cc-4e5eacecff85 · outbound

This paper cites an unresolved cited work.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 66

Resolution: metadata mismatch; raw_fallback, observed 2026-08-07T11:35:06.439287Z

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Observation f22eb674-ecde-4608-9330-e865d287dc8a · outbound

This paper cites Yarahmadi et al.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Yarahmadi et al

Reference 67

Resolution: metadata mismatch; raw_fallback, observed 2026-08-07T11:35:06.319402Z

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Observation b4040bcb-c799-4b94-bbac-11528fc23492 · outbound

This paper cites The European Physical Journal C 83 (910 (2023)).

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension The European Physical Journal C 83 (910 (2023))

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.164139Z

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Observation 9ae78425-4151-4094-8831-f9130ef1030b · outbound

This paper cites Communications in Theoretical Physics 75 - 055401(2023).

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Communications in Theoretical Physics 75 - 055401(2023)

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.144495Z

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Observation d95a1e6b-ebbd-4be4-9726-74356c1fa253 · outbound

This paper cites Mohseni Sadjadi, V.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Mohseni Sadjadi, V

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.121203Z

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Observation 53dfc543-56ba-42ca-a464-0c0d9f936cc5 · outbound

This paper cites Mohseni Sadjadi, V.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Mohseni Sadjadi, V

Reference 71

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.093216Z

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Observation 7176dbce-2f26-4766-b62a-dd7a7fbae181 · outbound

This paper cites Anari, H.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Anari, H

Reference 72

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.073746Z

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Observation 09a46f2d-776a-4045-b504-7eedbd781a85 · outbound

This paper cites Mohseni Sadjadi, V.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Mohseni Sadjadi, V

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.055151Z

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Observation 14ffd7b2-2803-4d7c-abea-7c51507fb3ca · outbound

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 74

Resolution: unresolved; raw_fallback, observed 2026-08-07T11:35:07.034460Z

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Observation 6868209d-d5f9-4569-993a-8e6bdca18218 · outbound

This paper cites Casas, V.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Casas, V

Reference 75

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:07.009997Z

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Observation eea61394-f571-436e-bb95-895b024c5fdd · outbound

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 76

Resolution: unresolved; raw_fallback, observed 2026-08-07T11:35:06.988128Z

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Observation 850018e5-5257-4ad6-9bf1-b7b2375ae13d · outbound

This paper cites Dropout as a Bayesian Approximation: Representing Model Uncertainty in Deep Learning,.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Dropout as a Bayesian Approximation: Representing Model Uncertainty in Deep Learning,

Reference 77

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.969209Z

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Observation 08c6a7c6-8406-4ff7-87ff-315007800bfb · outbound

This paper cites Power-law entropy corrected holographic dark energy in non-flat universe,.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Power-law entropy corrected holographic dark energy in non-flat universe,

Reference 78

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.950815Z

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Observation c8557b93-455a-4a65-a921-e082c60dd082 · outbound

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A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Unresolved cited work

Reference 79

Resolution: unresolved; raw_fallback, observed 2026-08-07T11:35:06.929220Z

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Observation fd88255e-18b8-46c4-b02a-d26a46a9c44c · outbound

This paper cites Sheykhi, ”Tsallis Holographic Dark Energy with IR Cutoff,” Phys.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Sheykhi, ”Tsallis Holographic Dark Energy with IR Cutoff,” Phys

Reference 80

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.908635Z

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Observation d4f83672-ebe8-4284-9f4c-5a15fd398423 · outbound

This paper cites Moradpour et al., ”Tsallis Holographic Dark Energy in Modified Gravity,” Eur.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Moradpour et al., ”Tsallis Holographic Dark Energy in Modified Gravity,” Eur

Reference 81

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.886652Z

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Observation 1444c510-781a-4fb0-8a63-3e7d26b2c0f5 · outbound

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

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Planck 2018 results. VI. Cosmological parameters

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.232509Z

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Observation 90a5bfa9-7842-4c80-a2f4-a7048fd22c6d · outbound

This paper cites Astrophys.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Astrophys

Reference 83

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.860935Z

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Observation a71fd679-d217-4ac1-a554-91c38c02d921 · outbound

This paper cites Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Low Redshift Baryon Acoustic Oscillation Measurement from the Reconstructed 6-degree Field Galaxy Survey

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.242417Z

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Observation 7f41a469-36e9-4e6f-941c-a57fb9ca0db4 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.247258Z

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Observation 8ec8ca27-f971-4222-ba09-481937259a11 · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1.

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.253059Z

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Observation f0255f89-3289-4446-a816-64f7532f100f · outbound

This paper cites Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Dark Energy Survey Year 3 Results: A 2.7% measurement of Baryon Acoustic Oscillation distance scale at redshift 0.835

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.258218Z

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Observation 0128a5f5-efb8-47f7-ac10-da42c0e20d58 · outbound

This paper cites Neveux, E.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Neveux, E

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.264075Z

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Observation 98e44318-3e51-4ff4-9337-8de8cf5ad36c · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.270666Z

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Observation de198d3f-bd5f-42d4-8fd3-ad395a1af19c · outbound

This paper cites The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\alpha$ forests

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.278223Z

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Observation e4ea219a-e006-4503-8b7c-3570a688dbf5 · outbound

This paper cites f(R) Cosmology revisited.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension f(R) Cosmology revisited

Reference 91

Resolution: metadata mismatch; local_arxiv, observed 2026-08-07T11:35:05.484748Z

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Observation 9fb1651f-9a45-4bf4-81af-3f38246fbc30 · outbound

This paper cites et al., ApJ, Volume 938, Number 2 (2022).

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension et al., ApJ, Volume 938, Number 2 (2022)

Reference 92

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T11:35:06.843268Z

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Observation a45ed7f4-18a6-4ae8-b786-68d4c8c1e750 · outbound

This paper cites Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.311023Z

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Observation f0434743-cde1-4e1a-81c4-fc655651188f · outbound

This paper cites Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.320223Z

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Observation c6ca1088-b8bc-4c03-b7f5-cbc2df4fe11e · outbound

This paper cites A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.329541Z

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Unavailable: canonical work link unavailable.

Observation fdfbf44a-eff1-4400-aa61-016a6ba118b2 · outbound

This paper cites Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.347174Z

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Unavailable: canonical work link unavailable.

Observation dc662403-9102-49c2-a783-e907b46a565a · outbound

This paper cites Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.354869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b15d720d-3f2f-4e77-9fa4-ea0181c4c20a · outbound

This paper cites Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.375582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1bf9d6c6-55d8-4f7c-886d-168dff713645 · outbound

This paper cites Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.381491Z

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Unavailable: canonical work link unavailable.

Observation afc426b1-b4ce-4bcc-bc17-9543f1a84367 · outbound

This paper cites Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.386379Z

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Observation 24a714d5-bad6-4fbe-84d9-a74b74dcc4b4 · outbound

This paper cites MontePython 3: boosted MCMC sampler and other features.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension MontePython 3: boosted MCMC sampler and other features

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.402721Z

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Observation 06f79c28-5437-4be9-9ad7-c24c0d49ba10 · outbound

This paper cites The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes.

A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-07T11:35:05.415106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 66ce9f9a-38b2-4d85-8565-1fbf6e087a6c · inbound

Mass Varying Neutrino Oscillation in Teleparallel Gravity cites this paper.

Mass Varying Neutrino Oscillation in Teleparallel Gravity A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension

Reference 17

Resolution: verified exact; arxiv_id, observed 2026-07-03T14:58:33.031143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation e3ba6946-2918-4bfb-8734-2b9dd74b4be0 · inbound

Beyond Data-Driven: How Physics-Informed Neural Networks are Reshaping Multi-Physics Design and Discovery cites this paper.

Beyond Data-Driven: How Physics-Informed Neural Networks are Reshaping Multi-Physics Design and Discovery A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension

Reference 199

Resolution: verified exact; arxiv_id, observed 2026-07-04T08:19:44.113202Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation 5c7fd857-033b-41c2-88a4-35762d00c530 · inbound

QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia cites this paper.

QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia A Bayesian PINN Framework for Barrow-Tsallis Holographic Dark Energy with Neutrinos: Toward a Resolution of the Hubble Tension

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T11:25:06.228942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.