The role of electron captures by nuclei in the shallow heating of magnetars is further investigated using both nuclear measurements and the theoretical atomic mass table HFB-27. Starting from the composition of the outer crust in full equilibrium, we have calculated the onset of electron captures and the heat released due to the slow decay of the magnetic field. Numerical results are found to be similar to those previously obtained with the HFB-24 atomic mass model and are consistent with neutron-star cooling data.info:eu-repo/semantics/publishe
Magnetars form a subclass of neutron stars characterized by magnetic fields of order 1014-1015 G at ...
Neutron stars cool down during their lifetime through the combination of neutrino emission from the ...
Aims. We study the efficiency of Joule heating in the crustal layers of young neutron stars. ...
International audienceThe role of electron captures by nuclei in the shallow heating of magnetars is...
The decay of the magnetic field in the interior of a magnetar may trigger electron captures by nucle...
International audienceThe persistent thermal luminosity of magnetars and their outbursts suggest the...
The persistent thermal luminosity of magnetars and their outbursts suggest the existence of some int...
The loss of magnetic pressure accompanying the decay of the magnetic field in a magnetar may trigger...
The loss of magnetic pressure accompanying the decay of the magnetic field in a magnetar may trigger...
The outer-crust structure and composition of a cold, non-accreting magnetar are studied. We model th...
We study thermal structure and evolution of magnetars as cooling neutron stars with a phenomenologic...
This computer code (written in C language) determines the internal constitution of the outer crust o...
Magnetars form a subclass of neutron stars characterized by magnetic fields of order 1014-1015 G at ...
Neutron stars cool down during their lifetime through the combination of neutrino emission from the ...
Aims. We study the efficiency of Joule heating in the crustal layers of young neutron stars. ...
International audienceThe role of electron captures by nuclei in the shallow heating of magnetars is...
The decay of the magnetic field in the interior of a magnetar may trigger electron captures by nucle...
International audienceThe persistent thermal luminosity of magnetars and their outbursts suggest the...
The persistent thermal luminosity of magnetars and their outbursts suggest the existence of some int...
The loss of magnetic pressure accompanying the decay of the magnetic field in a magnetar may trigger...
The loss of magnetic pressure accompanying the decay of the magnetic field in a magnetar may trigger...
The outer-crust structure and composition of a cold, non-accreting magnetar are studied. We model th...
We study thermal structure and evolution of magnetars as cooling neutron stars with a phenomenologic...
This computer code (written in C language) determines the internal constitution of the outer crust o...
Magnetars form a subclass of neutron stars characterized by magnetic fields of order 1014-1015 G at ...
Neutron stars cool down during their lifetime through the combination of neutrino emission from the ...
Aims. We study the efficiency of Joule heating in the crustal layers of young neutron stars. ...