Nucleonic models at finite temperature with in-medium effective fields
Fuente:
arXiv
Guardado en:
| Autores principales: | Lourenço, Odilon, Dutra, Mariana, Margueron, Jérôme |
|---|---|
| Formato: | Preprint |
| Publicado: |
2023
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Surface and curvature tensions of relativistic models
por: Dutra, Mariana, et al.
Publicado: (2024)
por: Dutra, Mariana, et al.
Publicado: (2024)
Effects of dilute neutron matter on the neutron star crust equation of state
por: Grams, Guilherme, et al.
Publicado: (2024)
por: Grams, Guilherme, et al.
Publicado: (2024)
NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration
por: Pradhan, Bikram Keshari, et al.
Publicado: (2025)
por: Pradhan, Bikram Keshari, et al.
Publicado: (2025)
Nuclear Matter Equation of State in the Brueckner-Hartree-Fock Approach and Standard Skyrme Energy-Density Functionals
por: Vidaña, Isaac, et al.
Publicado: (2024)
por: Vidaña, Isaac, et al.
Publicado: (2024)
Dark energy effects on realistic neutron stars
por: Pretel, Juan M. Z., et al.
Publicado: (2024)
por: Pretel, Juan M. Z., et al.
Publicado: (2024)
Non-Radial Oscillation Modes in Hybrid Stars with Hyperons and Delta Baryons
por: Rather, Ishfaq Ahmad, et al.
Publicado: (2024)
por: Rather, Ishfaq Ahmad, et al.
Publicado: (2024)
Equation of state at neutron-star densities and beyond from perturbative QCD
por: Komoltsev, Oleg, et al.
Publicado: (2023)
por: Komoltsev, Oleg, et al.
Publicado: (2023)
Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
por: Li, Jia-Jie, et al.
Publicado: (2025)
por: Li, Jia-Jie, et al.
Publicado: (2025)
$\textit{Ab initio}$ Exact Calculation of Strongly-Correlated Nucleonic Matter
por: Hu, Rongzhe, et al.
Publicado: (2025)
por: Hu, Rongzhe, et al.
Publicado: (2025)
Constraining a relativistic mean field model using neutron star mass-radius measurements I: Nucleonic models
por: Huang, Chun, et al.
Publicado: (2023)
por: Huang, Chun, et al.
Publicado: (2023)
Many-body effects on dense matter with hyperons at finite temperature
por: Jacobsen, Rafael Bán, et al.
Publicado: (2026)
por: Jacobsen, Rafael Bán, et al.
Publicado: (2026)
Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter
por: Cai, Bao-Jun, et al.
Publicado: (2025)
por: Cai, Bao-Jun, et al.
Publicado: (2025)
Compiled Properties of Nucleonic Matter and Nuclear and Neutron Star Models from Non-Relativistic and Relativistic Interactions
por: Sun, Boyang, et al.
Publicado: (2023)
por: Sun, Boyang, et al.
Publicado: (2023)
Modified Urca neutrino emissivity at finite temperature
por: Suleiman, Lami, et al.
Publicado: (2023)
por: Suleiman, Lami, et al.
Publicado: (2023)
Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature
por: Constantinou, Constantinos, et al.
Publicado: (2025)
por: Constantinou, Constantinos, et al.
Publicado: (2025)
Role of the symmetry energy on hybrid stars
por: Güven, H., et al.
Publicado: (2026)
por: Güven, H., et al.
Publicado: (2026)
Resonant shattering flares as asteroseismic tests of chiral effective field theory
por: Neill, Duncan, et al.
Publicado: (2024)
por: Neill, Duncan, et al.
Publicado: (2024)
Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties
por: Mendes, Melissa, et al.
Publicado: (2026)
por: Mendes, Melissa, et al.
Publicado: (2026)
Constraining Hamiltonians from chiral effective field theory with neutron-star data
por: Armstrong, Cassandra L., et al.
Publicado: (2026)
por: Armstrong, Cassandra L., et al.
Publicado: (2026)
Symmetry energy and neutron star properties constrained by chiral effective field theory calculations
por: Lim, Yeunhwan, et al.
Publicado: (2023)
por: Lim, Yeunhwan, et al.
Publicado: (2023)
Neutron matter from local chiral effective field theory interactions at large cutoffs
por: Tews, I., et al.
Publicado: (2024)
por: Tews, I., et al.
Publicado: (2024)
Equation of state and Fermi liquid properties of dense matter based on chiral effective field theory interactions
por: Alp, Faruk, et al.
Publicado: (2025)
por: Alp, Faruk, et al.
Publicado: (2025)
Density-dependent quark mean-field model for nuclear matter and neutron stars
por: Huang, Kaixuan, et al.
Publicado: (2024)
por: Huang, Kaixuan, et al.
Publicado: (2024)
Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties
por: Göttling, H., et al.
Publicado: (2025)
por: Göttling, H., et al.
Publicado: (2025)
Investigations on the equation of state of neutron star matter with density-dependent relativistic mean-field model
por: Huang, Kaixuan, et al.
Publicado: (2024)
por: Huang, Kaixuan, et al.
Publicado: (2024)
Isentropic hybrid stars in the Nambu-Jona-Lasinio model: effects of neutrino trapping
por: Sabatucci, Andrea, et al.
Publicado: (2026)
por: Sabatucci, Andrea, et al.
Publicado: (2026)
Neutron Star Equation of State with Nucleon Short-Range Correlations: A Concise Review and Open Issues
por: Cai, Bao-Jun, et al.
Publicado: (2025)
por: Cai, Bao-Jun, et al.
Publicado: (2025)
Self-consistent thermodynamical treatment for quark matter in quasi-particle model at finite temperature
por: Pal, Suman, et al.
Publicado: (2024)
por: Pal, Suman, et al.
Publicado: (2024)
Enhanced Neutrino Cooling from Parity-Doubled Nucleons in Neutron Star Cooling Simulations
por: Negreiros, Rodrigo, et al.
Publicado: (2026)
por: Negreiros, Rodrigo, et al.
Publicado: (2026)
Composition of scalar mesons and their effects on nuclear matter properties in an extended linear sigma model
por: Ma, Yao, et al.
Publicado: (2025)
por: Ma, Yao, et al.
Publicado: (2025)
Evolutions of in-medium baryon-baryon scattering cross sections and stiffness of dense nuclear matter from Bayesian analyses of FOPI proton flow excitation functions
por: Li, Bao-An, et al.
Publicado: (2025)
por: Li, Bao-An, 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)
por: Miyatsu, Tsuyoshi, et al.
Publicado: (2025)
Unraveling the global behavior of equation of state by explicit finite nuclei constraints
por: Venneti, Anagh, et al.
Publicado: (2024)
por: Venneti, Anagh, et al.
Publicado: (2024)
Delayed Thermal Relaxation of Rapidly Cooling Neutron Stars: Nucleon Superfluidity and Non-nucleon Particles
por: Tu, Zhonghao, et al.
Publicado: (2025)
por: Tu, Zhonghao, et al.
Publicado: (2025)
Dynamical scheme for computing the mass parameter of a system in a medium
por: Zdanowicz, Agata, et al.
Publicado: (2025)
por: Zdanowicz, Agata, et al.
Publicado: (2025)
NucleiML: A machine learning framework of ground-state properties of finite nuclei for accelerated Bayesian exploration
por: Venneti, Anagh, et al.
Publicado: (2025)
por: Venneti, Anagh, et al.
Publicado: (2025)
Modeling direct and pre-equilibrium processes of neutron-induced reactions with noniterative finite amplitude method and distorted-wave Born approximation
por: Sasaki, Hirokazu, et al.
Publicado: (2025)
por: Sasaki, Hirokazu, et al.
Publicado: (2025)
Relativistic mean-field models of neutron-rich matter
por: Piekarewicz, J.
Publicado: (2026)
por: Piekarewicz, J.
Publicado: (2026)
Validity of a finite temperature expansion for dense nuclear matter
por: Mroczek, Debora, et al.
Publicado: (2024)
por: Mroczek, Debora, et al.
Publicado: (2024)
Extended Skyrme effective interactions for transport model and neutron stars
por: Wang, Si-Pei, et al.
Publicado: (2023)
por: Wang, Si-Pei, et al.
Publicado: (2023)
Ejemplares similares
-
Surface and curvature tensions of relativistic models
por: Dutra, Mariana, et al.
Publicado: (2024) -
Effects of dilute neutron matter on the neutron star crust equation of state
por: Grams, Guilherme, et al.
Publicado: (2024) -
NJL-Chiral Soliton and the Nucleon Equation of State at supra-saturation density: Impact of Chiral Symmetry Restoration
por: Pradhan, Bikram Keshari, et al.
Publicado: (2025) -
Nuclear Matter Equation of State in the Brueckner-Hartree-Fock Approach and Standard Skyrme Energy-Density Functionals
por: Vidaña, Isaac, et al.
Publicado: (2024) -
Dark energy effects on realistic neutron stars
por: Pretel, Juan M. Z., et al.
Publicado: (2024)