Imagen de Portada

Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Passarella, Luca, Margueron, Jerome, Pagliara, Giuseppe
Formato:	Preprint
Publicado:	2025
Materias:	Nuclear Theory
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

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

Relativistic mean-field models of neutron-rich matter
por: Piekarewicz, J.
Publicado: (2026)

Conformal prediction for uncertainties in the neutron star equation of state
por: Dezdarani, Habib Yousefi, et al.
Publicado: (2026)

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

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

Effect of the equation of state for dilute neutron matter on the composition of the inner crust of neutron stars
por: Gupta, Sunny Kumar, et al.
Publicado: (2023)

Relativistic mean-field study of the neutron star inner crust using the asymmetric finite difference method
por: Zhang, Jinzhe, et al.
Publicado: (2026)

Thermal fluctuations of matter composition and quark nucleation in compact stars
por: Guerrini, Mirco, et al.
Publicado: (2024)

Equation of state at neutron-star densities and beyond from perturbative QCD
por: Komoltsev, Oleg, et al.
Publicado: (2023)

How well known is the compressibility of nuclear matter?
por: Margueron, J., et al.
Publicado: (2026)

Assessing the joint effect of temperature and magnetic field on the neutron star equation of state
por: Scurto, Luigi, et al.
Publicado: (2024)

Realizing the potential of deep neural network for analyzing neutron star observables and dense matter equation of state
por: Thete, Ameya, et al.
Publicado: (2022)

Nucleonic models at finite temperature with in-medium effective fields
por: Lourenço, Odilon, et al.
Publicado: (2023)

Unified neutron star equations of state calibrated to nuclear properties
por: Malik, Tuhin, et al.
Publicado: (2024)

Implication of multimessenger observations on the relativistic mean-field equation of state of dense nuclear matter and skin thickness of nuclei
por: Kumar, Rahul, et al.
Publicado: (2025)

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

$Λ$ and $Σ$ potentials in dense matter based on chiral EFT: Bridging heavy-ion collisions, hypernuclei, and neutron stars
por: Jinno, Asanosuke, et al.
Publicado: (2025)

Constraints on the dense matter equation of state from young and cold isolated neutron stars
por: Marino, Alessio, et al.
Publicado: (2024)

Freeze-out model of light nuclei formation in heavy-ion collision transport
por: Savchuk, Oleh, et al.
Publicado: (2026)

Radial oscillations of neutron stars within density-dependent relativistic-mean field model
por: Geng, Xuesong, et al.
Publicado: (2025)

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

The equation of state for neutron stars with speed of sound constraints via Bayesian inference
por: Dong, Xieyuan, et al.
Publicado: (2025)

Bayesian inference of the dense matter equation of state built upon extended Skyrme interactions
por: Beznogov, Mikhail V., et al.
Publicado: (2024)

From existing and new nuclear and astrophysical constraints to stringent limits on the equation of state of neutron-rich dense matter
por: Koehn, Hauke, et al.
Publicado: (2024)

Kaon-meson coupling from SU(3) flavour symmetry and application to antikaon condensed dense matter in neutron star
por: S., Athira, et al.
Publicado: (2025)

Neutrino emission from neutron star matter
por: Benhar, Omar, et al.
Publicado: (2025)

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

Role of thermal fluctuations in nucleation of three-flavor quark matter
por: Guerrini, Mirco, et al.
Publicado: (2025)

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

Shedding light on the pion production in heavy-ion collisions and application into the neutron star matter properties
por: Liu, Heng-Jin, et al.
Publicado: (2023)

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

The mean-field theory of superfluid-superconducting vortex states in the outer core of neutron stars
por: Kobyakov, Dmitry
Publicado: (2026)

Nucleon-quark mixed matter and neutron star EOS
por: Yamamoto, Y., et al.
Publicado: (2024)

Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state
por: Seif, W. M., et al.
Publicado: (2025)

The Effects of Multi-$Λ$ Hyperons on Collective Modes in Nuclei
por: Suleymanli, Bahruz, et al.
Publicado: (2026)

Effects of Finite Temperature and Pairing Correlations in Multi-$Λ$ Hypernuclei
por: Suleymanli, Bahruz, et al.
Publicado: (2024)

Nuclear structure within the relativistic mean field approach including chiral symmetry and quark confinement effects
por: Chamseddine, M., et al.
Publicado: (2026)

Dark matter effects on the properties of neutron stars: optical radii
por: Liu, Hong-Ming, et al.
Publicado: (2023)

Explainable autoencoder for neutron star dense matter parameter estimation
por: Di Clemente, Francesco, et al.
Publicado: (2025)

Is the compact object associated with HESS J1731-347 a strange quark star?
por: Di Clemente, Francesco, et al.
Publicado: (2022)