Amanote Research

Amanote Research

    RegisterSign In

Equation of State for Neutron Stars: Hyperon Mixing in SU(3) Flavor Symmetry

doi 10.7566/jpscp.1.013080
Full Text
Open PDF
Abstract

Available in full text

Date

March 19, 2014

Authors
Tsuyoshi MiyatsuMyung-Ki CheounKoichi Saito
Publisher

Journal of the Physical Society of Japan


Related search

Strong Hyperon-Nucleon Pairing in Neutron Stars

Physical Review Letters
AstronomyPhysics
2005English

Exotic Matter in Neutron Stars and the Equation of State

2019English

How Neutron Stars Constrain the Nuclear Equation of State

EPJ Web of Conferences
AstronomyPhysics
2014English

Neutron Anomaly inγN→ηNand the Flavour SU(3) Symmetry

EPJ Web of Conferences
AstronomyPhysics
2017English

Charmed Baryon Weak Decays With Decuplet Baryon and SU(3) Flavor Symmetry

Physical Review D
AstronomyPhysics
2019English

Extracting Information on the Equation of State From Binary Neutron Stars

Springer proceedings in physics
High Energy PhysicsNuclear
2015English

Structures of Rotating Traditional Neutron Stars and Hyperon Stars in the Relativistic $\Sigma-\Omega$ Model

European Physical Journal A
High Energy PhysicsNuclear
2004English

Akmal-Pandharipande-Ravenhall Equation of State for Simulations of Supernovae, Neutron Stars, and Binary Mergers

Physical Review C
High Energy PhysicsNuclear
2019English

SU(3) Breaking in Hyperon Transition Vector Form Factors

Physical Review D
2015English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2026 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy