Rotating Neutron Stars in a Chiral SU(3) Model
S. Schramm, D. Zschiesche
Abstract
We study the properties of rotating neutron stars within a generalized chiral SU(3)-flavor model. The influence of the rotation on the inner structure and the hyperon matter content of the star is discussed. We calculate the Kepler frequency and moments of inertia of the neutron star sequences. An estimate for the braking index of the associated pulsars is given.
Create a lesson
Related papers
Pionization experiments in light nuclei
Slawomir Wycech, Guillaume Hupin, Jaume Carbonell
Deep Learning for Longitudinal Asymmetry in Heavy-Ion Collisions at RHIC Energies
Anup Kumar Sikdar, Sanchari Thakur, Pingal Dasgupta et al.
Non-uniqueness of the amplitude reconstruction in the inverse scattering problem and a refinement of Hoehler's resonance clustering
A. Švarc
Modeling fragmentation of 20Ne nuclei at the LHC
Aleksandr Svetlichnyi, Savva Savenkov, Igor Pshenichnov
Parametrization of unitary matrices, parametrizing the symmetric S matrix and the NN S matrix above the inelastic threshold
N. A. Khokhlov
Thermofractal Dynamics in the Multisource Thermal Model: A Unified Approach to Multiparticle Production
Airton Deppman, Trambak Bhattacharyya, Maciej Rybczyński et al.