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Bibliografski detalji
Glavni autori:	Semposki, A. C., Drischler, C., Furnstahl, R. J., Phillips, D. R.
Format:	Preprint
Izdano:	2025
Teme:	Nuclear Theory High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
Online pristup:	https://arxiv.org/abs/2505.18921
Oznake:	Dodaj oznaku Bez oznaka, Budi prvi tko označuje ovaj zapis!

Slični predmeti

From chiral EFT to perturbative QCD: a Bayesian model mixing approach to symmetric nuclear matter
od: Semposki, A. C., i dr.
Izdano: (2024)

Quarkyonic equation of state with a momentum dependent interaction and neutron star structure
od: Folias, K., i dr.
Izdano: (2024)

Bayesian analysis of hybrid neutron star EOS constraints within an instantaneous nonlocal chiral quark matter model
od: Ayriyan, Alexander, i dr.
Izdano: (2024)

Hybrid star within the framework of a lowest-order constraint variational method
od: Khanmohamadi, S., i dr.
Izdano: (2019)

Reexamining constraints on neutron star properties from perturbative QCD
od: Zhou, Dake
Izdano: (2023)

Regulator-independent equations of state for neutron stars generated from first principles
od: Alarcón, J. M., i dr.
Izdano: (2024)

Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference
od: Gorda, Tyler, i dr.
Izdano: (2025)

Impact of QCD sum rules coupling constants on neutron stars structure
od: Jangal, F. Moradi, i dr.
Izdano: (2025)

Constraining the neutron star equation of state by including the isoscalar-vector and isovector-vector coupling using the Bayesian analysis
od: Kumar, Deepak, i dr.
Izdano: (2025)

Conditional variational autoencoder inference of neutron star equation of state from astrophysical observations
od: Ferreira, Márcio, i dr.
Izdano: (2024)

Uncertainty quantification in the machine-learning inference from neutron star probability distribution to the equation of state
od: Fujimoto, Yuki, i dr.
Izdano: (2024)

Bulk viscosity from neutron decays to dark baryons in neutron star matter
od: Harris, Steven P., i dr.
Izdano: (2025)

Bayesian inference favors quark matter in neutron star interiors
od: Ayriyan, Alexander, i dr.
Izdano: (2025)

Maximal mass of neutron stars constrained by neutron star observations
od: Kasza, Gábor, i dr.
Izdano: (2026)

Hybrid stars within the framework of the Sigma-Omega-Rho model combined with the MIT and NJL models
od: Karimi, Reza, i dr.
Izdano: (2022)

Equation of state at neutron-star densities and beyond from perturbative QCD
od: Komoltsev, Oleg, i dr.
Izdano: (2023)

Extended Skyrme effective interactions for transport model and neutron stars
od: Wang, Si-Pei, i dr.
Izdano: (2023)

Extended momentum-dependent interaction for transport models and neutron stars
od: Wang, Si-Pei, i dr.
Izdano: (2025)

Constraints on the dense matter equation of state from young and cold isolated neutron stars
od: Marino, Alessio, i dr.
Izdano: (2024)

Strong model-agnostic constraints for twin-star solutions
od: Blomqvist, Sofia, i dr.
Izdano: (2025)

Pi in the Sky: Neutron Stars with Exceptionally Light QCD Axions
od: Kumamoto, Mia, i dr.
Izdano: (2024)

Astrophysical constraints on the cold equation of state of the strongly interacting matter
od: Kasza, Gábor, i dr.
Izdano: (2025)

Parity-doubled nucleons can rapidly cool neutron stars
od: Brodie, Liam, i dr.
Izdano: (2025)

Probing the nonstrange quark star equation of state with compact stars and gravitational waves
od: Wang, Shu-Peng, i dr.
Izdano: (2025)

Constraints on maximum neutron star mass from proto-neutron star evolution
od: Kumar, Deepak, i dr.
Izdano: (2025)

Properties of neutron stars and strangeness-mixed stars from a pion mean-field approach
od: Ghim, Nam-Yong, i dr.
Izdano: (2024)

Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars
od: Wang, Si-Pei, i dr.
Izdano: (2024)

Nuclear chiral density wave in neutron stars?
od: Papadopoulos, Orestis, i dr.
Izdano: (2025)

Particle-theory input for neutron-star physics
od: Vuorinen, Aleksi
Izdano: (2024)

Curvature of the energy per particle in neutron stars
od: Marczenko, Michał, i dr.
Izdano: (2023)

Neutron star equation of state: identifying hadronic matter characteristics
od: Providência, Constança, i dr.
Izdano: (2023)

Quark stars in $D_3$-$D_7$ holographic model
od: Aleixo, M., i dr.
Izdano: (2023)

Implications of the recent neutron decay measurements on the properties of compact objects -- a dark star with nucleonic shell ?
od: Veselský, M., i dr.
Izdano: (2025)

Constraining free parameters of a color superconducting non-local Nambu-Jona-Lasinio model using Bayesian analysis of neutron stars mass and radius measurements
od: Shahrbaf, Mahboubeh, i dr.
Izdano: (2021)

Structure and tidal deformability of a hybrid star within the framework of the field correlator method
od: Khanmohamadi, S., i dr.
Izdano: (2020)

First-order phase transitions in the cores of neutron stars
od: Komoltsev, Oleg
Izdano: (2024)

Effect of color superconductivity on the mass of hybrid neutron stars in an effective model with pQCD asymptotics
od: Blaschke, David, i dr.
Izdano: (2022)

Thermal twin stars within a hybrid equation of state based on a nonlocal chiral quark model compatible with modern astrophysical observations
od: Carlomagno, J. P., i dr.
Izdano: (2023)

Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers
od: Sokołowski, Kamil, i dr.
Izdano: (2026)

Detecting Hyperons in neutron stars -- a machine learning approach
od: Carvalho, Valéria, i dr.
Izdano: (2024)