Region of hadron-quark mixed phase in hybrid stars

Details Region of hadron-quark mixed phase in hybrid stars Region of hadron-quark mixed phase in hybrid stars

2011-05-12

arxiv.org/abs/1105.2445v1

Phys.Rev.C83:068801,2011

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

to be published in Physical Review C

Scientific paper

10.1103/PhysRevC.83.068801

Hadron--quark mixed phase is expected in a wide region of the inner structure of hybrid stars. However, we show that the hadron--quark mixed phase should be restricted to a narrower region to because of the charge screening effect. The narrow region of the mixed phase seems to explain physical phenomena of neutron stars such as the strong magnetic field and glitch phenomena, and it would give a new cooling curve for the neutron star.

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