Kaon condensation in hyperonic matter and properties of neutron stars

2005 ◽  
Vol 754 ◽  
pp. 350-355 ◽  
Author(s):  
Takumi Muto
2007 ◽  
Vol 76 (6) ◽  
Author(s):  
Guo-hua Wang ◽  
Wei-jie Fu ◽  
Yu-xin Liu

1998 ◽  
Vol 81 (21) ◽  
pp. 4564-4567 ◽  
Author(s):  
Norman K. Glendenning ◽  
Jürgen Schaffner-Bielich

2000 ◽  
Vol 50 (1) ◽  
pp. 481-524 ◽  
Author(s):  
Henning Heiselberg ◽  
Vijay Pandharipande

▪ Abstract  We review recent progress in the theory of neutron stars and compare its predictions with the observational data on masses, radii, and temperatures. The theory of neutron stars made up of neutrons, protons, and leptons is discussed in detail along with recent models of nuclear forces and modern many-body techniques. The possibilities of pion and kaon condensation in dense neutron star matter are considered, as is the possible occurrence of strange hyperons and quark-matter drops in the stellar core. The structure of mixed-phase matter in neutron stars, as well as the probable effect of phase transitions on the spin down of pulsars, is also discussed.


2014 ◽  
Vol 89 (5) ◽  
Author(s):  
Yeunhwan Lim ◽  
Kyujin Kwak ◽  
Chang Ho Hyun ◽  
Chang-Hwan Lee

1994 ◽  
Vol 571 (4) ◽  
pp. 758-783 ◽  
Author(s):  
Fujii Hirotsugu ◽  
Muto Takumi ◽  
Tatsumi Toshitaka ◽  
Tamagaki Ryozo

2008 ◽  
Vol 17 (09) ◽  
pp. 1635-1647 ◽  
Author(s):  
A. LI ◽  
G. F. BURGIO ◽  
U. LOMBARDO ◽  
G. X. PENG

The appearance of exotic phases in neutron stars is studied. The possible transition from hadron to quark phase is studied within the density dependent mass quark model, and the kaon condensation within the Nelson and Kaplan model. In both cases a microscopic approach is adopted for dense hadron matter. From the study of the possible coexistence between the two phases it is found that the hybrid phase may strongly hinder the onset of kaon condensation.


Sign in / Sign up

Export Citation Format

Share Document