Paper Citation Record · LEDGER

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis

As of 21 August 2026, this Paper Citation Record lists 100 of 114 outbound references and 4 inbound Pith citation observations for arXiv:2501.15810.

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2501.15810 v2

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Observation 6d2f91c0-1831-49b4-af1c-0619fea68513 · outbound

This paper cites an unresolved cited work.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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This paper cites Note that the change in the inverse sound speed squared is given by κs(ξ) → κs(ξ) + d∆ε(ξ) P dξ δε, correspondingly.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Note that the change in the inverse sound speed squared is given by κs(ξ) → κs(ξ) + d∆ε(ξ) P dξ δε, correspondingly

Reference 2

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis observational values

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This paper cites Dense Nuclear Matter Equation of State from Heavy-Ion Collisions.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Dense Nuclear Matter Equation of State from Heavy-Ion Collisions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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This paper cites In MCMC, the parameter ensemble is sampled one after another as a chain.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis In MCMC, the parameter ensemble is sampled one after another as a chain

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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This paper cites It should be noted that the overall posterior is normalized, 1 = R P(ϑ)dN −2 ˆϑ dξPT d∆ε, so that the marginal one is also normalized, R P(ξPT, ∆ε) dξPT d∆ε.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis It should be noted that the overall posterior is normalized, 1 = R P(ϑ)dN −2 ˆϑ dξPT d∆ε, so that the marginal one is also normalized, R P(ξPT, ∆ε) dξPT d∆ε

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This paper cites Introductory lectures on lattice QCD at nonzero baryon number.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Introductory lectures on lattice QCD at nonzero baryon number

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Simulating QCD at finite density

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This paper cites Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Future Physics Perspectives on the Equation of State from Heavy Ion Collisions to Neutron Stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Little-Bang and Femto-Nova in Nucleus-Nucleus Collisions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

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This paper cites The Nuclear Equation of State and Neutron Star Masses.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis The Nuclear Equation of State and Neutron Star Masses

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This paper cites From hadrons to quarks in neutron stars: a review.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis From hadrons to quarks in neutron stars: a review

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis GW170817: Measurements of Neutron Star Radii and Equation of State

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Correlations between the Neutron Star Mass-Radius Relation and the Equation of State of Dense Matter

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis The Radius of PSR J0740+6620 from NICER and XMM-Newton Data

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Gravitational-Wave and X-ray Probes of the Neutron Star Equation of State

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Lindblom, Astrophys

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Maximal Mass Neutron Star as a Key to Superdense Matter Physics

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Compiled Properties of Nucleonic Matter and Nuclear and Neutron Star Models from Non-Relativistic and Relativistic Interactions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis New equations of state constrained by nuclear physics, observations, and QCD calculations of high-density nuclear matter

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Constraining Neutron-Star Matter with Microscopic and Macroscopic Collisions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Chatziioannou, H

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Combining Electromagnetic and Gravitational-Wave Constraints on Neutron-Star Masses and Radii

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Baym and C

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis A unified equation of state of dense matter and neutron star structure

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Hypernuclear Physics for Neutron Stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Vida˜ na, Nucl

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Phase Transition to Hyperon Matter in Neutron Stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis QCD phase diagram: an overview

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Evidence for quark-matter cores in massive neutron stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Mapping the Phases of Quantum Chromodynamics with Beam Energy Scan

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Strongly interacting matter exhibits deconfined behavior in massive neutron stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Indication of Sharp and Strong Phase-Transitions from NICER Observations

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Neural network reconstruction of the dense matter equation of state from neutron star observables

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Reconstructing the neutron star equation of state from observational data via automatic differentiation

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Reconstructing parton distribution functions from Ioffe time data: from Bayesian methods to Neural Networks

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis An open-source machine learning framework for global analyses of parton distributions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Continuum-extrapolated NNLO Valence PDF of Pion at the Physical Point

Reference 54

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Heavy quark potential in quark-gluon Plasma: Deep neural network meets lattice quantum chromodynamics

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Reconstructing spectral functions via automatic differentiation

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Rethinking the ill-posedness of the spectral function reconstruction -- why is it fundamentally hard and how Artificial Neural Networks can help

Reference 57

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Deep-learning quasi-particle masses from QCD equation of state

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Nuclear equation of state at finite $\mu_B$ using deep learning assisted quasi-parton model

Reference 59

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Neural Network Modeling of Heavy-Quark Potential from Holography

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Building Hadron Potentials from Lattice QCD with Deep Neural Networks

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Deep learning for exploring hadron-hadron interactions

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Learning Hadron Emitting Sources with Deep Neural Networks

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Exploring QCD matter in extreme conditions with Machine Learning

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Aarts, K

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

Reference 66

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis ¨Ozel and P

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Applying Bayesian parameter estimation to relativistic heavy-ion collisions: simultaneous characterization of the initial state and quark-gluon plasma medium

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Unresolved cited work

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This paper cites Phenomenological constraints on the transport properties of QCD matter with data-driven model averaging.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Phenomenological constraints on the transport properties of QCD matter with data-driven model averaging

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Multi-system Bayesian constraints on the transport coefficients of QCD matter

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Determining the jet transport coefficient $\hat{q}$ from inclusive hadron suppression measurements using Bayesian parameter estimation

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Early-times Yang-Mills dynamics and the characterization of strongly interacting matter with statistical learning

Reference 73

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Bayesian quantification of strongly-interacting matter with color glass condensate initial conditions

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This paper cites Andrieu, N.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Andrieu, N

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Keplerian frequency of uniformly rotating neutron stars and quark stars

Reference 76

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Rotating neutron stars with exotic cores: masses, radii, stability

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Observational appearance of rapidly rotating neutron stars: X-ray bursts, cooling tail method, and radius determination

Reference 78

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This paper cites Do we need dense matter equation of state in curved spacetime for neutron stars?.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Do we need dense matter equation of state in curved spacetime for neutron stars?

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Constraining neutron star tidal Love numbers with gravitational wave detectors

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Relativistic tidal properties of neutron stars

Reference 81

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Tidal Love numbers of neutron stars

Reference 82

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Tidal Love Numbers of Neutron and Self-Bound Quark Stars

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Comment on "Tidal Love numbers of neutron and self-bound quark stars"

Reference 84

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Core-collapse supernova equations of state based on neutron star observations

Reference 85

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Adam: A Method for Stochastic Optimization

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis A high-bias, low-variance introduction to Machine Learning for physicists

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Kahn and A

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Leshno and S

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Kratsios, Annals of Mathematics and Artificial In- telligence (2021), 10.1007/s10472-020-09723-1

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This paper cites LeCun, Y.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis LeCun, Y

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Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis An equation-of-state-meter for CBM using PointNet

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