Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks | Paper Citation Record

Observation e709455e-4e11-463f-b104-7b5162bd8965 · outbound

This paper cites Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant,

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This paper cites Measurements of Ω and Λ from 42 High-Redshift Supernovae,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Measurements of Ω and Λ from 42 High-Redshift Supernovae,

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Observation 36ee8f0a-0c8e-4309-b01c-26b0b5d56bb0 · outbound

This paper cites The Cosmological Constant Problem,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks The Cosmological Constant Problem,

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This paper cites The Cosmological Constant and Dark Energy,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks The Cosmological Constant and Dark Energy,

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Observation f2195674-216c-4773-843d-d287be3713bb · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Planck 2018 results. VI. Cosmological parameters,

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Observation 145b22cb-017c-48bf-b094-19f93cb8d687 · outbound

This paper cites Dynamics of Dark Energy,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Dynamics of Dark Energy,

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This paper cites Modified Gravity and Cosmology,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Modified Gravity and Cosmology,

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Observation 1d057033-ffb4-4a4b-b5a0-007abcc7ed13 · outbound

This paper cites Accelerating Universes with Scaling Dark Matter,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Accelerating Universes with Scaling Dark Matter,

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This paper cites Exploring the Expansion History of the Universe,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Exploring the Expansion History of the Universe,

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Observation b8b86326-c4fb-4fde-8693-a4ea59ed68c7 · outbound

This paper cites Exploring the Expanding Universe and Dark Energy Using the Statefinder Diagnostic,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Exploring the Expanding Universe and Dark Energy Using the Statefinder Diagnostic,

Reference 10

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Observation 84b8e718-f6d6-4df9-9ce6-b41090cd2f16 · outbound

This paper cites Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant,

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Observation 848c1f05-c62a-4287-94dd-faf0f63e7485 · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Tensions between the Early and the Late Universe,

Reference 12

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Observation 53c5b3a8-2786-4172-84fd-788aaa64144d · outbound

This paper cites In the Realm of the Hubble Tension—A Review of Solutions,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks In the Realm of the Hubble Tension—A Review of Solutions,

Reference 13

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Observation c2401f50-7573-4537-9dd3-14be2884ec0f · outbound

This paper cites Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck,

Reference 14

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Observation c35232e6-a4dd-4f4c-bbf5-cc9f1845fb28 · outbound

This paper cites KiDS-450: Cosmological Parameter Constraints from Tomographic Weak Gravitational Lensing,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks KiDS-450: Cosmological Parameter Constraints from Tomographic Weak Gravitational Lensing,

Reference 15

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This paper cites Tension and Constraints on Modified Gravity Parametrizations ofGeff (z) from Growth Rate and Planck Data,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Tension and Constraints on Modified Gravity Parametrizations ofGeff (z) from Growth Rate and Planck Data,

Reference 16

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Observation b747c2d3-07e0-4fab-bc73-07582c998147 · outbound

This paper cites Massive neutrinos and cosmology,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Massive neutrinos and cosmology,

Reference 17

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Observation f761f3e2-c28b-471d-b185-2f6e2babb6f0 · outbound

This paper cites Neutrino mass from cosmology,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Neutrino mass from cosmology,

Reference 18

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Observation 446b1f46-b1dc-4012-945c-187b53c72616 · outbound

This paper cites Unveilingνsecrets with cosmological data: Neutrino masses and mass hierarchy,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Unveilingνsecrets with cosmological data: Neutrino masses and mass hierarchy,

Reference 19

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Observation 92ac7aab-7536-47ff-a8d1-10f44135f39c · outbound

This paper cites Beyond six parameters: extending ΛCDM,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Beyond six parameters: extending ΛCDM,

Reference 20

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Observation 6d15e870-8e1a-4a17-be9a-27c77b901187 · outbound

This paper cites A CMB-based analysis of neutrino masses,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A CMB-based analysis of neutrino masses,

Reference 21

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Observation fcdfdfc7-c0b4-48b5-a2fd-afccbc5ba62b · outbound

This paper cites Physics–Informed Neural Networks: A Deep Learning Framework for Solving Forward and Inverse Problems Involving Nonlinear Partial Differential Equations,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Physics–Informed Neural Networks: A Deep Learning Framework for Solving Forward and Inverse Problems Involving Nonlinear Partial Differential Equations,

Reference 22

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This paper cites B–PINNs: Bayesian Physics–Informed Neural Networks for Forward and Inverse PDE Problems with Uncertainty Quantification,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks B–PINNs: Bayesian Physics–Informed Neural Networks for Forward and Inverse PDE Problems with Uncertainty Quantification,

Reference 23

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Observation c094ee06-e616-4d12-b92e-355b9b52c6a2 · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks The European Physical Journal C 83 (910 (2023))

Reference 24

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Observation f29c0e02-c69b-43dd-bdbe-1b03cf6af43b · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Communications in Theoretical Physics 75 - 055401(2023)

Reference 25

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This paper cites Scientific Machine Learning through Physics–Informed Neural Networks: Where we are and What’s next,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Scientific Machine Learning through Physics–Informed Neural Networks: Where we are and What’s next,

Reference 26

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Observation 9f38041a-6cdb-4d0b-95c9-5cfdcdbae71f · outbound

This paper cites Bayesian neural networks in cosmology: reconstruction and model comparison,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Bayesian neural networks in cosmology: reconstruction and model comparison,

Reference 27

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This paper cites Dropout as a Bayesian Approximation,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Dropout as a Bayesian Approximation,

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This paper cites Surrogate modeling for fluid flows,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Surrogate modeling for fluid flows,

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This paper cites The Pantheon+ Analysis: The Full Dataset and Cosmological Constraints,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks The Pantheon+ Analysis: The Full Dataset and Cosmological Constraints,

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Observation cb950bc2-3024-4d11-8c9a-284559d91d9d · outbound

This paper cites Measuring cosmic bulk flow with Pantheon catalogue in perturbed f(R) gravity,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Measuring cosmic bulk flow with Pantheon catalogue in perturbed f(R) gravity,

Reference 32

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This paper cites A Comparative Bayesian PINN–MCMC Analysis of Barrow–Tsallis Holographic Dark Energy with Neutrinos: Toward Resolving the Hubble Tension,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A Comparative Bayesian PINN–MCMC Analysis of Barrow–Tsallis Holographic Dark Energy with Neutrinos: Toward Resolving the Hubble Tension,

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This paper cites Cosmic Bulk Flow Analysis in Modified Gravity Theories: and Perturbed Models with Neutrino Coupling,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Cosmic Bulk Flow Analysis in Modified Gravity Theories: and Perturbed Models with Neutrino Coupling,

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Observation ffc2fb83-6f36-4e33-9a3b-7bc57e5e2406 · outbound

This paper cites A 2.4% Determination of the Local Value of the Hubble Constant,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A 2.4% Determination of the Local Value of the Hubble Constant,

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This paper cites A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s −1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s −1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team,

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Observation c217989e-16d2-4305-bb65-cb0e8ffa4d1e · outbound

This paper cites On the Hubble constant tension in the SNe Ia Pantheon sample.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks On the Hubble constant tension in the SNe Ia Pantheon sample

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Observation 73906ccf-1da0-45ce-a488-6e7ae43ef9b8 · outbound

This paper cites On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030

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Observation 594b1988-6fda-49fa-a081-4cff7031b8cb · outbound

This paper cites A New Master Supernovae Ia sample and the investigation of the $H_0$ tension.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A New Master Supernovae Ia sample and the investigation of the $H_0$ tension

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix

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Observation 13faf3b1-896e-4417-8cc0-ba56cac341b7 · 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.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Improved constraints on the expansion rate of the Universe up to z~1.1 from the spectroscopic evolution of cosmic chronometers

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Observation 1f13c63e-d3a1-4637-9c1c-1eb18183f3cf · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\sim$2

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks A 6% measurement of the Hubble parameter at $z\sim0.45$: direct evidence of the epoch of cosmic re-acceleration

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This paper cites Coupled non-canonical scalar field to neutrinos could alleviate the Hubble tension and cross the phantom barrier,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Coupled non-canonical scalar field to neutrinos could alleviate the Hubble tension and cross the phantom barrier,

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This paper cites Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Ten- sion,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Neutrino Interactions with perturbed Rastall Gravity: A Novel Approach to Reducing the Hubble Ten- sion,

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Observation 9424d2ab-fc90-4c07-8a85-9a18391d736a · outbound

This paper cites Generalized Logarithmic Modification of Barrow-Tsallis Entropy Can Alleviate the Hubble Tension,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Generalized Logarithmic Modification of Barrow-Tsallis Entropy Can Alleviate the Hubble Tension,

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This paper cites Beyond the Local Universe: Impacts of Scalar field Coupled to Non-Relativistic Neutrinos on Bulk Flow,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Beyond the Local Universe: Impacts of Scalar field Coupled to Non-Relativistic Neutrinos on Bulk Flow,

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Observation 3fe6cbcd-e28e-423e-b1cb-f2747228d47a · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements

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Observation d33db03d-751d-4ade-8981-7ff20b53aa5a · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope

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Observation b9248510-f26e-4854-95a0-086f5deb0aad · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks 2024, MNRAS,Pages 3055–3067, https://doi.org/10.1093/mnras/stae2257

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Observation 1f7e9c2e-af86-4b6a-8809-203dbddc09d6 · outbound

This paper cites Distance priors from Planck final release,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Distance priors from Planck final release,

Reference 54

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Observation 61875b5d-1f23-4d3d-b888-346085488b8b · outbound

This paper cites DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest

Reference 56

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Observation 828fe697-3995-4099-add0-cac87e28e024 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Planck 2018 results. V. CMB power spectra and likelihoods

Reference 57

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Observation cb718998-8d2b-4f39-af96-b8cd39f76b33 · outbound

This paper cites Astrophys.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Astrophys

Reference 58

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Observation 4fbc5cfe-09bd-4c9b-8a5f-515bcf026497 · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Eur.Phys.J.C 84 (2024) 4, 443

Reference 59

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Observation f5e29ee1-0b80-4a56-8541-8ea1a313b311 · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints

Reference 60

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Observation 5d27b911-033c-4bd4-ad7d-b19f74790cbc · outbound

This paper cites Dynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Dynamical Dark Energy in the Crosshairs: A Joint Analysis with DESI, Pantheon plus, and TDCOSMO Constraints,

Reference 61

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Observation 6db5ea7e-8bbe-4919-b194-3607123b0e45 · outbound

This paper cites How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks How Complex is Dark Energy? A Bayesian Analysis of CPL Extensions with Recent DESI BAO Measurements

Reference 62

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Observation 8034202c-60b6-46e3-8769-b6612315d42f · outbound

This paper cites Using non-DESI data to confirm and strengthen the DESI 2024 spatially flat w0waCDM cosmological parametrization result,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Using non-DESI data to confirm and strengthen the DESI 2024 spatially flat w0waCDM cosmological parametrization result,

Reference 63

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Observation ecfaab3a-c8f8-4e8a-a547-51484e63c0e0 · outbound

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Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Unresolved cited work

Reference 64

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Observation d17224e9-5e4c-4a7c-9dab-b2a8fd076e46 · outbound

This paper cites Yarahmadi et al.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Yarahmadi et al

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.546102Z

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Observation 96043510-a480-49fb-a734-1e9cd7c19a26 · outbound

This paper cites Cosmology with massive neutrinos coupled to dark energy.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Cosmology with massive neutrinos coupled to dark energy

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.654368Z

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Observation 09a690da-1a3d-4f20-9fb8-28776f9a2df3 · outbound

This paper cites Neutrinos in Cosmology,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Neutrinos in Cosmology,

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.724531Z

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Observation c4c54b0e-d928-419a-9d99-e05847bd5ad8 · outbound

This paper cites Status of neutrino properties and future prospects - Cosmological and astrophysical constraints.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Status of neutrino properties and future prospects - Cosmological and astrophysical constraints

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.787152Z

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Observation 33206306-36f3-43e6-a9da-11f6b0f936ba · outbound

This paper cites Effects of neutrino mass and asymmetry on cosmological structure formation.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Effects of neutrino mass and asymmetry on cosmological structure formation

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.859333Z

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Observation e1dd11d4-3bdf-4d85-91e9-444350575fff · outbound

This paper cites Can Chameleon fields be the source of both the dark energy dipole and the CMB dipole?.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Can Chameleon fields be the source of both the dark energy dipole and the CMB dipole?

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:12.937726Z

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Observation 071d19f2-ef0d-415f-b133-41edd3421260 · outbound

This paper cites Calibration of the Tip of the Red Giant Branch (TRGB).

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Calibration of the Tip of the Red Giant Branch (TRGB)

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.025763Z

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Observation 026bdabd-606e-4669-a165-6d0a6d295652 · outbound

This paper cites Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.104765Z

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Observation 917e55b8-2701-4f83-b757-07350f43b3c2 · outbound

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.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\sigma$ tension between early and late-Universe probes

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.143620Z

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Observation 6e404702-29cd-498e-8f6c-5f8ee76520fb · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Determining the Hubble Constant without the Sound Horizon Scale: Measurements from CMB Lensing

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.261530Z

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Observation 8117d398-f51d-49ce-bea9-a84cc908ce49 · outbound

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.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.347074Z

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Observation 71ab0465-1a86-48a5-858f-60184f9d4a3a · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Cosmology-independent Estimate of the Hubble Constant and Spatial Curvature Using Time-delay Lenses and Quasars

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.384090Z

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Observation 8318d296-da19-4c47-9a21-238f8764f98c · outbound

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

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Tensions between the Early and the Late Universe

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.484703Z

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Observation b6432fec-ff46-4211-8d4e-401624e1acb2 · outbound

This paper cites Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos,.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Towards a Machine Learning Solution for Hubble Tension: Physics-Informed Neural Network (PINN) Analysis of Tsallis Holographic Dark Energy in Presence of Neutrinos,

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.597278Z

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Observation 8b59b394-2265-4dd3-8e7b-4163f3ea6462 · outbound

This paper cites Can dark energy evolve to the Phantom?.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Can dark energy evolve to the Phantom?

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.676361Z

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Observation 53861522-8017-4d39-afbf-03b119549b27 · outbound

This paper cites Introduction to Modified Gravity and Gravitational Alternative for Dark Energy.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Introduction to Modified Gravity and Gravitational Alternative for Dark Energy

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.736617Z

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Observation 139b7f48-54f2-479c-97ae-219308a65ea4 · outbound

This paper cites Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.830681Z

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Observation f5503950-e7bd-4b5a-b1b5-27ee4291b022 · outbound

This paper cites Models of f(R) Cosmic Acceleration that Evade Solar-System Tests.

Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks Models of f(R) Cosmic Acceleration that Evade Solar-System Tests

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-03T13:11:13.966306Z

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