A closer look at the Yukawa's interaction from a symmetry group perspective
arXiv:2305.19388 · doi:10.1093/ptep/ptad129
Abstract
I investigate the use of the SU(3) Clebsch-Gordan coefficients in light of the relations of completeness and closure. I show that in the case of 1, there is an additional interaction: the exchange of a meson between a and a hyperon that only affects the symmetric coupling. I then calculate these additional coupling constants and show that this recovers the completeness and closure of the SU(3) Clebsch-Gordan coefficients for all values of . Besides, it increases the symmetry of the theory, once now we can group the baryon octet into four doublets. Finally, I add the new coupling constants to study numerical results in the hyperon onset in dense nuclear matter assuming as a free parameter.
arXiv comment16 pages, published version
References in corpus (33)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- A Massive Pulsar in a Compact Relativistic Binary
- GW170817: Measurements of Neutron Star Radii and Equation of State
- PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
- A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
- A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy
- Gravitational-wave constraints on the neutron-star-matter Equation of State
- Implications of PREX-II on the equation of state of neutron-rich matter
- Hyperon-rich Matter in Neutron Stars
- Hyperons and massive neutron stars: vector repulsion and SU(3) symmetry
- Relativistic effective interaction for nuclei, giant resonances, and neutron stars
- Hyperons and massive neutron stars: the role of hyperon potentials
- Multi-messenger Bayesian parameter inference of a binary neutron-star merger
- Properties of Strange Hadronic Matter in Bulk and in Finite Systems
- K-proton scattering and the in dense matter
- Equation of state for neutron stars in SU(3) flavor symmetry
- Neutron star properties in the quark-meson coupling model
- Heavy Baryons in Compact Stars
- The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
- Hyperons in neutron stars and supernova cores
- Physics input for modelling superfluid neutron stars with hyperon cores
- Hypernuclear stars from relativistic Hartree-Fock density functional theory
- Broken SU(6) symmetry and massive hybrid stars
- The baryon coupling scheme in an unified SU(3) and SU(6) symmetry formalism
- Constraining the nuclear symmetry energy and properties of neutron star from GW170817 by Bayesian analysis
- Heavy Magnetic Neutron Stars
- Role of vector channel in different classes of (non) magnetized neutron stars
- Phase transition towards strange matter
- Examination of strangeness instabilities and effects of strange meson couplings in dense strange hadronic matter and compact stars
- Liquid-gas phase transition in strange hadronic matter with relativistic models
- Massive relativistic compact stars from SU(3) symmetric quark models
- The system
- Phase transitions and latent heat in magnetized matter
Cited by in corpus (5)
- XTE J1814-338 as a dark matter admixed neutron star
- Correlation between the symmetry energy slope and the deconfinement phase transition
- Role of local anisotropy in hybrid stars
- Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry
- An Undergraduate Approach to the Quantum Hadrodynamics and the Physics of Neutron Stars Part II: Neutron Stars' Exotic Content