Implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field model

Abstract

In this dissertation, we have studied the implications of nuclear interaction for nuclear structure and astrophysics within the relativistic mean-field (RMF) model.

arXiv commentThesis based on the papers Phys. Rev. C 2015, 92, 054314; Int. J. Mod. Phys. E 2016, 25, 1650062; Phys. Rev. C 2017, 95, 015801; Phys. Rev. C 2017, 96, 034623; Nucl. Phys. A 2017, 966, 197; Phys. Rev. C 2018, 97, 045806; arXiv:1701.00731; and Lecture on Tides in binary stars by T. Hinderer

References in corpus (94)

• Observation of Gravitational Waves from a Binary Black Hole Merger
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• A New Parameterization for the Lagrangian Density of Relativistic Mean Field Theory
• Nuclear ground-state masses and deformations: FRDM(2012)
• Testing General Relativity with Present and Future Astrophysical Observations
• Determination of the Equation of State of Dense Matter
• Neutron Star Observations: Prognosis for Equation of State Constraints
• Tidal Love numbers of neutron stars
• Constraining neutron star tidal Love numbers with gravitational wave detectors
• Gravitational-wave constraints on the neutron-star-matter Equation of State
• Relativistic tidal properties of neutron stars
• Constraints on a phenomenologically parameterized neutron-star equation of state
• Recent Progress in Quantum Hadrodynamics
• Relativistic theory of tidal Love numbers
• Constraints on the symmetry energy and neutron skins from experiments and theory
• Neutron-Rich Nuclei in Heaven and Earth
• Constraints on the density dependence of the symmetry energy
• Skyrme Interaction and Nuclear Matter Constraints
• Mean-field description of ground-state properties of drip-line nuclei: Pairing and continuum effects
• Nuclear symmetry energy probed by neutron skin thickness of nuclei
• Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering
• Relativistic Mean-Field Theory and the High-Density Nuclear Equation of State
• Neutron skins and neutron stars in the multi-messenger era
• Measurability of the tidal polarizability of neutron stars in late-inspiral gravitational-wave signals
• The Skyrme Interaction in finite nuclei and nuclear matter
• Neutron skin of 208Pb, nuclear symmetry energy, and the parity radius experiment
• Astrophysical Measurement of the Equation of State of Neutron Star Matter
• Gravitationally redshifted absorption lines in the X-ray burst spectra of a neutron star
• Superheavy nuclei in selfconsistent nuclear calculations
• The effective force NL3 revisited
• Unexpectedly large charge radii of neutron-rich calcium isotopes
• Parity Violating Measurements of Neutron Densities
• Systematic parameter errors in inspiraling neutron star binaries
• Constraining the neutron-proton effective mass splitting using empirical constraints on the density dependence of nuclear symmetry energy around normal density
• Post-1-Newtonian tidal effects in the gravitational waveform from binary inspirals
• Hyperon stars in the Brueckner-Bethe-Goldstone theory
• Matter effects on binary neutron star waveforms
• Symmetry Energy II: Isobaric Analog States
• Hyperons and massive neutron stars: the role of hyperon potentials
• Electric dipole polarizability and the neutron skin
• Effective One Body description of tidal effects in inspiralling compact binaries
• Systematic and statistical errors in a bayesian approach to the estimation of the neutron-star equation of state using advanced gravitational wave detectors
• Connecting Neutron Star Observations to Three-Body Forces in Neutron Matter and to the Nuclear Symmetry Energy
• Results of the ASY-EOS experiment at GSI: The symmetry energy at suprasaturation density
• Determination of the parameters of a Skyrme type effective interaction using the simulated annealing approach
• The neutron skin thickness from the measured electric dipole polarizability in ${}^{68}$Ni, ${}^{120}$Sn, and ${}^{208}$Pb
• Low-density neutron matter
• Higher-order effects on the incompressibility of isospin asymmetric nuclear matter
• Incompressibility in finite nuclei and nuclear matter
• Relativistic mean field interaction with density dependent meson-nucleon vertices based on microscopical calculations
• Nuclear Matter in Relativistic Mean Field Theory with Isovector Scalar Meson
• Potential Energy Surfaces of Actinide Nuclei from a Multi-dimensional Constraint Covariant Density Functional Theory: Barrier Heights and Saddle Point Shapes
• Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
• Extracting equation of state parameters from black hole-neutron star mergers. I. Nonspinning black holes
• Constraining the High-Density Behavior of Nuclear Symmetry Energy with the Tidal Polarizability of Neutron Stars
• Extracting equation of state parameters from black hole-neutron star mergers: aligned-spin black holes and a preliminary waveform model
• Analytic modelling of tidal effects in the relativistic inspiral of binary neutron stars
• Isoscalar giant resonances in the Sn nuclei and implications for the asymmetry term in the nuclear-matter incompressibility
• Equation of state constraints for the cold dense matter inside neutron stars using the cooling tail method
• Accurate numerical simulations of inspiralling binary neutron stars and their comparison with effective-one-body analytical models
• Will black hole-neutron star binary inspirals tell us about the neutron star equation of state?
• A survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crust
• The fission barriers in Actinides and superheavy nuclei in covariant density functional theory
• First-post-Newtonian quadrupole tidal interactions in binary systems
• On the Progenitor of Binary Neutron Star Merger GW170817
• Density dependence of the symmetry energy from neutron skin thickness in finite nuclei
• Hypernuclear matter in a complete SU(3) symmetry group
• Equation of state of superfluid neutron matter and the calculation of ${}^1{S}_0$ pairing gap
• Tidal Stabilization of Rigidly Rotating, Fully Relativistic Neutron Stars
• The Giant Monopole Resonance in the Sn Isotopes: Why is Tin so "Fluffy"?
• Ground-state properties of deformed proton emitters in the relativistic Hartree-Bogoliubov model
• Aspects of particle production in isospin asymmetric matter
• New parameterization of the effective field theory motivated relativistic mean field model
• A new microscopic nucleon-nucleon interaction derived from relativistic mean field theory
• Tidal deformability of neutron and hyperon star with relativistic mean field equations of state
• Post-1-Newtonian equations of motion for systems of arbitrarily structured bodies
• Generic Constraints on the Relativistic Mean-Field and Skyrme-Hartree-Fock Models from the Pure Neutron Matter Equation of State
• Symmetry Energy Constraints from Giant Resonances: A Theoretical Overview
• Effects of $\omega$ meson self-coupling on the properties of finite nuclei and neutron stars
• Relativistic theory of surficial Love numbers
• Sensitivity of elements of the symmetry energy of nuclear matter to the properties of neutron-rich systems
• Phase transition and properties of compact star
• Breathing-mode measurements in Sn isotopes and isospin dependence of nuclear incompressibility
• Direct Evidence of Washing out of Nuclear Shell Effects
• The effect of isoscalar-isovector coupling in infinite nuclear matter
• Neutron density distributions for atomic parity nonconservation experiments
• Shape co-existence and parity doublet in Zr isotopes
• Exotic fission properties of highly neutron-rich Uranium isotopes
• Symmetry Energy
• Ternary fission within the temperature dependent relativistic mean field approach
• Stability of Strutinsky Shell Correction Energy in Relativistic Mean Field Theory
• Quark-Pauli effects in three octet-baryons