The Ginzburg-Landau equations for magnetic and gluomagnetic gauge fields of the semi-superfluid strings in the color superconducting core of the neutron star with diquark condensate in the color-flavor-locking (CFL) phase are derived. The simultaneous coupling of the CFL diquark condensate to the magnetic and gluomagnetic gauge fields is taken into account. The asymptotic values of these string energies are defined from quantization conditions. It is shown that a lattice of semi-superfluid strings with minimal quantum of circulation emerges in the superconducting quark core during rotation of the star. The magnetic field in the core of this string is of order of 10^18 G. The cluster of proton vortices appeared in the hadronic phase around e...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
We suggest a mechanism that may resolve a conflict between the precession of a neutron star and the...
The core region of a neutron star may feature quark matter in the color-flavor-locked (CFL) phase. T...
At very high densities, as for example in the core of a neutron star, matter may appear in the color...
We study, within Ginzburg-Landau theory, the responses of three-flavor superfluid quark-gluon plasma...
Color-flavor locked (CFL) quark matter expels color-magnetic fields due to the Meissner effect. One ...
Using a phenomenological Ginzburg–Landau model that includes entrainment, we identify the poss...
The behaviour of the magnetic ˇeld inside the superconducting quark matter core of a neutron star is...
It is expected that in the interior of compact stars a proton superconductor coexists with and coupl...
A microscopic, quantum mechanical model for neutron vortices in the crust of a neutron star is pres...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2007.Includes bibliographi...
In this thesis we investigate the role played by gauge elds in providing new observable signatures t...
We study a superconductor that is coupled to a superfluid via density and derivative couplings. Star...
We explore the effects of an external magnetic field in the structure and magnitude of the diquark c...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
We suggest a mechanism that may resolve a conflict between the precession of a neutron star and the...
The core region of a neutron star may feature quark matter in the color-flavor-locked (CFL) phase. T...
At very high densities, as for example in the core of a neutron star, matter may appear in the color...
We study, within Ginzburg-Landau theory, the responses of three-flavor superfluid quark-gluon plasma...
Color-flavor locked (CFL) quark matter expels color-magnetic fields due to the Meissner effect. One ...
Using a phenomenological Ginzburg–Landau model that includes entrainment, we identify the poss...
The behaviour of the magnetic ˇeld inside the superconducting quark matter core of a neutron star is...
It is expected that in the interior of compact stars a proton superconductor coexists with and coupl...
A microscopic, quantum mechanical model for neutron vortices in the crust of a neutron star is pres...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2007.Includes bibliographi...
In this thesis we investigate the role played by gauge elds in providing new observable signatures t...
We study a superconductor that is coupled to a superfluid via density and derivative couplings. Star...
We explore the effects of an external magnetic field in the structure and magnitude of the diquark c...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
Deconfinement phase transition and condensation of Goldstone bosons in neutron star matter are inves...
We suggest a mechanism that may resolve a conflict between the precession of a neutron star and the...