Copertina

Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Li, Shuying, Pang, Junbo, Shen, Hong, Hu, Jinniu, Sumiyoshi, Kohsuke
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Nuclear Theory High Energy Astrophysical Phenomena
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Nuclear pasta in hot neutron-star matter and proto-neutron stars
di: Zhou, Jian, et al.
Pubblicazione: (2026)

Investigations on the equation of state of neutron star matter with density-dependent relativistic mean-field model
di: Huang, Kaixuan, et al.
Pubblicazione: (2024)

The first-order phase transition in the neutron star from the deep neural network
di: Zhou, Wenjie, et al.
Pubblicazione: (2024)

Density-dependent quark mean-field model for nuclear matter and neutron stars
di: Huang, Kaixuan, et al.
Pubblicazione: (2024)

Role of symmetry energy at subnuclear densities in protoneutron star crusts
di: Nakazato, Ken'ichiro, et al.
Pubblicazione: (2025)

Probing spherical outbursts of neutron star mergers from an equation of state with composite nucleons
di: Soni, Vikram
Pubblicazione: (2023)

Impact of crust-core connection procedures on the tidal deformability of neutron stars
di: Pang, Junbo, et al.
Pubblicazione: (2026)

Neutrino flavor instabilities in a binary neutron star merger remnant: Roles of a long-lived hypermassive neutron star
di: Nagakura, Hiroki, et al.
Pubblicazione: (2025)

New {\em ab initio} constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: I. Subsaturation density domain
di: Raduta, Adriana R., et al.
Pubblicazione: (2025)

Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. V. Improved parametrization of the nucleon density distributions
di: Shchechilin, N. N., et al.
Pubblicazione: (2024)

Hyperonic uncertainties in neutron stars, mergers and supernovae
di: Kochankovski, Hristijan, et al.
Pubblicazione: (2023)

New ab initio constrained extended Skyrme equations of state for simulations of neutron stars, supernovae and binary mergers: II. Thermal response in the suprasaturation density domain
di: Raduta, Adriana R., et al.
Pubblicazione: (2025)

Bayesian Inference of Dense-Matter Equations of State from Small-Radius Compact Stars with Twin-Star Scenarios
di: Dong, Xieyuan, et al.
Pubblicazione: (2026)

A three-parameter characterization of neutron stars' mass-radius relation and equation of state
di: Ofengeim, Dmitry D., et al.
Pubblicazione: (2024)

Effects of dilute neutron matter on the neutron star crust equation of state
di: Grams, Guilherme, et al.
Pubblicazione: (2024)

Determining the minimal mass of a proto-neutron star with chirally constrained nuclear equations of state
di: Kunkel, Selina, et al.
Pubblicazione: (2024)

Insights into neutron star equation of state by machine learning
di: Guo, Ling-Jun, et al.
Pubblicazione: (2023)

Implication of neutron star observations to the origin of nucleon mass
di: Gao, Bikai, et al.
Pubblicazione: (2025)

Thermal x-ray studies of neutron stars and the equation of state
di: Miao, Zhiqiang, et al.
Pubblicazione: (2024)

Unified QMF equation of state for neutron star matter: Static and dynamic properties
di: Tu, Zhonghao, et al.
Pubblicazione: (2025)

Spin effects in superfluidity, neutron matter and neutron stars
di: Sedrakian, Armen, et al.
Pubblicazione: (2026)

Parity-doubled nucleons can rapidly cool neutron stars
di: Brodie, Liam, et al.
Pubblicazione: (2025)

Inference of neutron-star properties with unified crust-core equations of state for parameter estimation
di: Davis, P. J., et al.
Pubblicazione: (2024)

Illuminating dark matter admixed in neutron stars with simultaneous mass-radius constraints
di: Zhang, Nai-Bo, et al.
Pubblicazione: (2025)

General predictions of neutron star properties using unified relativistic mean-field equations of state
di: Scurto, Luigi, et al.
Pubblicazione: (2024)

Maximal mass of neutron stars constrained by neutron star observations
di: Kasza, Gábor, et al.
Pubblicazione: (2026)

Limits on dark matter existence in neutron stars from recent astrophysical observations and mass correlation analysis
di: Hu, Jing Fu, et al.
Pubblicazione: (2025)

Neutrino opacities in magnetic fields for binary neutron star merger simulations
di: Kumamoto, Mia, et al.
Pubblicazione: (2026)

Dark matter effects on the properties of hybrid neutron stars
di: Wei, Jin-Biao, et al.
Pubblicazione: (2026)

Inverse-mapped density-dependent relativistic mean-field inference of the neutron-star equation of state with multi-messenger constraints
di: Xie, Wen-Jie, et al.
Pubblicazione: (2026)

Constraining the nuclear equation of state from terrestrial experiments and neutron star observations using relativistic mean-field models
di: Miyatsu, Tsuyoshi, et al.
Pubblicazione: (2025)

Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry
di: Miyatsu, Tsuyoshi, et al.
Pubblicazione: (2025)

Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations
di: Sotani, Hajime, et al.
Pubblicazione: (2026)

Regulator-independent equations of state for neutron stars generated from first principles
di: Alarcón, J. M., et al.
Pubblicazione: (2024)

Quarkyonic equation of state with a momentum dependent interaction and neutron star structure
di: Folias, K., et al.
Pubblicazione: (2024)

Constrained Gaussian-process bridge prior for neutron-star equation-of-state inference
di: Gorda, Tyler, et al.
Pubblicazione: (2025)

Masking equation of state effects in binary neutron star mergers
di: Tsokaros, Antonios, et al.
Pubblicazione: (2024)

Vortex creep heating in neutron star cooling with direct Urca processes in heavy neutron stars
di: Nam, Yoonhak, et al.
Pubblicazione: (2025)

Thermodynamically consistent accreted crust of neutron stars: The role of proton shell effects
di: Gusakov, Mikhail E., et al.
Pubblicazione: (2024)

Constraining Hamiltonians from chiral effective field theory with neutron-star data
di: Armstrong, Cassandra L., et al.
Pubblicazione: (2026)