Add to ORKGA four-parameter class of exact asymptotically flat solutions of the Einstein-Maxwell equations involving only rational functions is presented. It is able to describe the exterior field of a slowly or rapidly rotating neutron star with poloidal magnetic field
RESUMEN Estudiamos el efecto de un modelo de crecimiento del campo magnético en los llamados Objetos...
The gravitational properties of astrophysical objects depend sensitively on their internal structure...
A new spectral code for constructing general-relativistic models of rapidly rotating stars with an u...
A new six-parametric, axisymmetric and asymptotically flat exact solution of Einstein-Maxwell field ...
The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO frame...
The potential enhancement of the cross section $\nu\bar\nu\to e^+e^-$ in the presence of a magnetic ...
Because of the tremendous densities that exist in the cores of neutron stars, a significant fraction...
Thesis (Ph. D.) University of KwaZulu-Natal, Westville, 2007.In this thesis we seek exact solutions ...
We calculate the amplitude of gravitational waves from a neutron star accreting symmetrically at its...
We present exact solutions to the Einstein-Maxwell system of equations with a specified form of the ...
Strongly asymmetric nuclear matter becomes unstable with respect to proton localization above a spec...
New expanding, axisymmetric pure-radiation solutions are found, exploiting the analogy with the Eule...
In the first part of our work, we formulated the equilibrium equa- tions for static neutron stars, t...
In the first part of our work, we formulated the equilibrium equa- tions for static neutron stars, ...
We consider bound states of fermions with an anomalous magnetic moments inthe field of charged cylin...
RESUMEN Estudiamos el efecto de un modelo de crecimiento del campo magnético en los llamados Objetos...
The gravitational properties of astrophysical objects depend sensitively on their internal structure...
A new spectral code for constructing general-relativistic models of rapidly rotating stars with an u...
A new six-parametric, axisymmetric and asymptotically flat exact solution of Einstein-Maxwell field ...
The second Maxwell’s relativistic equations of a rapidaly rotating neutron star, based on ZAMO frame...
The potential enhancement of the cross section $\nu\bar\nu\to e^+e^-$ in the presence of a magnetic ...
Because of the tremendous densities that exist in the cores of neutron stars, a significant fraction...
Thesis (Ph. D.) University of KwaZulu-Natal, Westville, 2007.In this thesis we seek exact solutions ...
We calculate the amplitude of gravitational waves from a neutron star accreting symmetrically at its...
We present exact solutions to the Einstein-Maxwell system of equations with a specified form of the ...
Strongly asymmetric nuclear matter becomes unstable with respect to proton localization above a spec...
New expanding, axisymmetric pure-radiation solutions are found, exploiting the analogy with the Eule...
In the first part of our work, we formulated the equilibrium equa- tions for static neutron stars, t...
In the first part of our work, we formulated the equilibrium equa- tions for static neutron stars, ...
We consider bound states of fermions with an anomalous magnetic moments inthe field of charged cylin...
RESUMEN Estudiamos el efecto de un modelo de crecimiento del campo magnético en los llamados Objetos...
The gravitational properties of astrophysical objects depend sensitively on their internal structure...
A new spectral code for constructing general-relativistic models of rapidly rotating stars with an u...