This paper describes an explicit multidimensional numerical scheme for special relativistic two-fluid magnetohydrodynamics of electron-positron plasma and a suit of test problems. The scheme utilizes Cartesian grid and the third-order weighted essentially non-oscillatory interpolation. Time integration is carried out using the third-order total variation diminishing method of Runge-Kutta type, thus ensuring overall third-order accuracy on smooth solutions. The magnetic field is kept near divergence-free by means of the method of generalized Lagrange multiplier. The test simulations, which include linear and non-linear continuous plasma waves, shock waves, strong explosions and the tearing instability, show that the scheme is sufficiently ro...
A new code and methodology are introduced for solving the fully general relativistic magnetohydrodyn...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
Abstract. A third order shock-capturing numerical scheme for three-dimensional special relativistic ...
The paper describes an explicit multi-dimensional numerical scheme for Special Relativistic Two-Flui...
Multidimensional shock-capturing numerical schemes for special relativistic hydrodynamics (RHD) are ...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code, RAI...
A third order shock-capturing numerical scheme for three-dimensional special relativistic magnetohy...
We present a new numerical implementation of the general-relativistic resistive magnetohydrodynamics...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
The 5-moment two-fluid plasma model uses Euler equations to describe the ion and electron fluids, an...
Many astrophysical processes involving magnetic fields and quasi-stationary processes are well descr...
ABSTRACT We describe a conservative, shock-capturing scheme for evolving the equations of general re...
The stability of current sheets in collisionless relativistic pair plasma was studied via two-dimens...
In this paper an approach to multidimensional magnetohydrodynamics (MI-ID) which correctly handles s...
In this paper we propose the first better than second order accurate method in space and time for th...
A new code and methodology are introduced for solving the fully general relativistic magnetohydrodyn...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
Abstract. A third order shock-capturing numerical scheme for three-dimensional special relativistic ...
The paper describes an explicit multi-dimensional numerical scheme for Special Relativistic Two-Flui...
Multidimensional shock-capturing numerical schemes for special relativistic hydrodynamics (RHD) are ...
We have developed a new three-dimensional general relativistic magnetohydrodynamic (GRMHD) code, RAI...
A third order shock-capturing numerical scheme for three-dimensional special relativistic magnetohy...
We present a new numerical implementation of the general-relativistic resistive magnetohydrodynamics...
A robust second order, shock-capturing numerical scheme for multidimensional special relativistic ma...
The 5-moment two-fluid plasma model uses Euler equations to describe the ion and electron fluids, an...
Many astrophysical processes involving magnetic fields and quasi-stationary processes are well descr...
ABSTRACT We describe a conservative, shock-capturing scheme for evolving the equations of general re...
The stability of current sheets in collisionless relativistic pair plasma was studied via two-dimens...
In this paper an approach to multidimensional magnetohydrodynamics (MI-ID) which correctly handles s...
In this paper we propose the first better than second order accurate method in space and time for th...
A new code and methodology are introduced for solving the fully general relativistic magnetohydrodyn...
Aims. We describe a newly-developed magnetohydrodynamic (MHD) code with the capacity to simulate the...
Abstract. A third order shock-capturing numerical scheme for three-dimensional special relativistic ...