Parallel computing has turned out to be the enabling technology to solve complex physical systems. However, the transition from shared memory, vector computers to massively parallel, distributed memory systems and, recently, to hybrid systems poses new challenges to the scientist. We want to present a cook-book (with a very strong, personal bias) based on our experience with parallization of our existing codes. Some of the general tools and communication libraries are discussed. Our approach includes a mixture of algorithm, domain and physical module based parallization. The advantages, scalability and limitations of each are discussed at some examples. We want show that it becomes easier to write parallel code with increasing complexity of...
AbstractWe describe a scalable parallel algorithm for numerical simulations of turbulent, radiative,...
We present a highly scalable demonstration of a portable asynchronous many-task programming model an...
AbstractIn this paper we discuss numerical methods and algorithms for the solution of NLTE stellar a...
We describe an important addition to the parallel implementation of our generalized NLTE stellar atm...
This paper describes a parallel implementation of a grand challenge problem: global atmospheric mode...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
Multidimensional nucleosynthesis studies with hundreds of nuclei linked through thousands of nuclear...
High performance computing has been used in various fields of astrophysical research. But most of it...
We present a tree-code for integrating the equations of the motion of collisionless systems, which h...
We present a performance analysis of different parallelization schemes for direct codes used in the ...
We describe PTreeSPH, a gravity treecode combined with an SPH hydrodynamics code designed for massiv...
Parallel programming allows the speed of computations to be increased by using multiple processors o...
We present the new parallel version (pCRASH2) of the cosmological radiative transfer code CRASH2 for...
157-173A critical review is presented in this paper on parallel computing, including parallel algori...
Ever since computers were first used for scientific and numerical work, there has existed an "arms r...
AbstractWe describe a scalable parallel algorithm for numerical simulations of turbulent, radiative,...
We present a highly scalable demonstration of a portable asynchronous many-task programming model an...
AbstractIn this paper we discuss numerical methods and algorithms for the solution of NLTE stellar a...
We describe an important addition to the parallel implementation of our generalized NLTE stellar atm...
This paper describes a parallel implementation of a grand challenge problem: global atmospheric mode...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
Multidimensional nucleosynthesis studies with hundreds of nuclei linked through thousands of nuclear...
High performance computing has been used in various fields of astrophysical research. But most of it...
We present a tree-code for integrating the equations of the motion of collisionless systems, which h...
We present a performance analysis of different parallelization schemes for direct codes used in the ...
We describe PTreeSPH, a gravity treecode combined with an SPH hydrodynamics code designed for massiv...
Parallel programming allows the speed of computations to be increased by using multiple processors o...
We present the new parallel version (pCRASH2) of the cosmological radiative transfer code CRASH2 for...
157-173A critical review is presented in this paper on parallel computing, including parallel algori...
Ever since computers were first used for scientific and numerical work, there has existed an "arms r...
AbstractWe describe a scalable parallel algorithm for numerical simulations of turbulent, radiative,...
We present a highly scalable demonstration of a portable asynchronous many-task programming model an...
AbstractIn this paper we discuss numerical methods and algorithms for the solution of NLTE stellar a...