scholarly journals Charge screening effect on hadron-quark mixed phase in compact stars

2006 ◽  
Author(s):  
Tomoki Endo ◽  
Toshiki Maruyama ◽  
Satoshi Chiba ◽  
Toshitaka Tatsumi
Keyword(s):  
Mixed Phase ◽  
Compact Stars ◽  
Screening Effect ◽  
Charge Screening

scholarly journals Charge Screening Effect in the Hadron-Quark Mixed Phase

2006 ◽  
Vol 115 (2) ◽  
pp. 337-353 ◽  
Author(s):  
T. Endo ◽  
T. Maruyama ◽  
S. Chiba ◽  
T. Tatsumi
Keyword(s):  
Mixed Phase ◽  
Screening Effect ◽  
Charge Screening

scholarly journals Properties of a hyperon–quark mixed phase in compact stars

2008 ◽  
Vol 35 (10) ◽  
pp. 104076 ◽  
Author(s):  
Toshiki Maruyama ◽  
Satoshi Chiba ◽  
Hans-Josef Schulze ◽  
Toshitaka Tatsumi
Keyword(s):  
Mixed Phase ◽  
Compact Stars

scholarly journals COOLING OF COMPACT STARS WITH COLOR SUPERCONDUCTING PHASE IN QUARK-HADRON MIXED PHASE

2013 ◽  
Vol 765 (1) ◽  
pp. 1 ◽  
Author(s):  
Tsuneo Noda ◽  
Masa-aki Hashimoto ◽  
Nobutoshi Yasutake ◽  
Toshiki Maruyama ◽  
Toshitaka Tatsumi ◽  
...  
Keyword(s):  
Superconducting Phase ◽  
Mixed Phase ◽  
Compact Stars

scholarly journals Charge screening in hadron–quark mixed phase

2002 ◽  
Vol 541 (1-2) ◽  
pp. 93-100 ◽  
Author(s):  
D.N. Voskresensky ◽  
M. Yasuhira ◽  
T. Tatsumi
Keyword(s):  
Mixed Phase ◽  
Charge Screening

scholarly journals Electric charge screening effect in single-W production with the KoralW Monte Carlo

2003 ◽  
Vol 27 (1) ◽  
pp. 19-32 ◽  
Author(s):  
S. Jadach ◽  
W. Placzek ◽  
M. Skrzypek ◽  
B.F.L. Ward ◽  
Z. Was
Keyword(s):  
Monte Carlo ◽  
Electric Charge ◽  
Screening Effect ◽  
Charge Screening

scholarly journals Charge screening at first order phase transitions and hadron–quark mixed phase

2003 ◽  
Vol 723 (1-2) ◽  
pp. 291-339 ◽  
Author(s):  
D.N. Voskresensky ◽  
M. Yasuhira ◽  
T. Tatsumi
Keyword(s):  
Phase Transitions ◽  
Mixed Phase ◽  
First Order ◽  
Charge Screening ◽  
First Order Phase

scholarly journals MIXED PHASE IN COMPACT STARS: M–R RELATIONS AND RADIAL OSCILLATIONS

2004 ◽  
Vol 13 (07) ◽  
pp. 1197-1205
Author(s):  
ASHOK GOYAL
Keyword(s):  
Neutron Stars ◽  
Recent Observation ◽  
Accurate Determination ◽  
Mixed Phase ◽  
Compact Stars ◽  
Quark Stars ◽  
Physical Laboratory ◽  
Low Mass ◽  
Relationship Of

It is believed that quark stars or neutron stars with mixed phase in the core have smaller radii compared to ordinary compact stars. With the recent observation of several low radius objects, typically a radius of <10 km for star of mass <1 M⊙ in low mass X-ray binaries (LMXB), it has become very important to understand the nature of these objects. An accurate determination of the mass–radius relationship of these objects provide us with a physical laboratory to study the composition of high density matter and the nature of phase transition. We study the effect of quark and nuclear matter mixed phase on the mass radius relationship and radial oscillations of neutron stars. We find that the effect of the mixed phase is to decrease the maximum mass of a stable neutron star and to decrease the radial frequencies.

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