Phase transitions in rotating neutron stars cores: back bending,stability, corequakes, and pulsar timing

E-ISSN： 1432-0746|450|2|747-758

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.450, Iss.2, 2006-05, pp. : 747-758

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Related content

Hydromagnetic stability of differentially rotating neutron stars

Astronomy & Astrophysics, Vol. 410, Iss. 3, 2003-11 ,pp. : 975-981

Edp Sciences

Access to resources Recommend Favorite

Neutrino transport and hydrodynamic stability of rotating proto-neutron stars

Astronomy & Astrophysics, Vol. 469, Iss. 2, 2007-07 ,pp. : 639-644

Edp Sciences

Access to resources Recommend Favorite

New model of relativistic slowly rotating neutron stars with surface layer crust: application to giant glitches of Vela Pulsar

Journal of Physics: Conference Series , Vol. 314, Iss. 1, 2011-09 ,pp. : 552-555

IOP Publishing

Access to resources Recommend Favorite

Hyperons in neutron-star cores and a 2 M_⊙ pulsar

By Bednarek I. Haensel P. Zdunik J. L. Bejger M. Mańka R.

Astronomy & Astrophysics, Vol. 543, Iss. issue, 2012-07 ,pp. : A157-A157

Edp Sciences

Access to resources Recommend Favorite

Phase transitions in dense matter and the maximum mass of neutron stars

By Chamel N. Fantina A. F. Pearson J. M. Goriely S.

Astronomy & Astrophysics, Vol. 553, Iss. issue, 2013-04 ,pp. : A22-A22

Edp Sciences

Access to resources Recommend Favorite