45 citations · 70 across the 5 of their papers we have counts for
5 papers
Three-dimensional numerical simulations of neutron star cores in the two-fluid MHD approximation: simple configurations
Andrei Igoshev, Nicolás A. Moraga, Andreas Reisenegger +2
Magnetic field evolution in neutron star cores is not fully understood. We describe the field evolution both for one barotropic fluid as well as two collisionally coupled barotropi…
Magnetic field decay in normal radio pulsars
A. P. Igoshev, S. B. Popov
We analyse the origin of the magnetic field decay in normal radio pulsars found by us in a recent study. This decay has a typical time scale ~yrs, and operates…
Unifying neutron stars: getting to GUNS
A. P. Igoshev, S. B. Popov, R. Turolla
The variety of the observational appearance of young isolated neutron stars must find an explanation in the framework of some unifying approach. Nowadays it is believed that such s…
Gaussian mixture model and population synthesis of radio pulsars
A. P. Igoshev, S. B. Popov
Recently, Lee et al. used Gaussian mixture models (GMM) to study the radio pulsar population. In the distribution of normal pulsars in the P-dotP plane, they found four clusters. W…
Neutron stars initial spin period distribution
A. P. Igoshev, S. B. Popov
We analyze different possibilities to explain the wide initial spin period distribution of radio pulsars presented by Noutsos et al. (2013). With a population synthesis modeling we…