In this paper, we report on the improvements implemented in the cosmological radiative transfer code CRASH. In particular, we present a new multi-frequency algorithm for spectra sampling which makes use of coloured photon packets: we discuss the need for the multi-frequency approach, describe its implementation and present the improved CRASH performance in reproducing the effects of ionizing radiation with an arbitrary spectrum. We further discuss minor changes in the code implementation which allow for more efficient performance and an increased precision
Dust has been recognized as a crucial component of galaxies that strongly influences Interstellar Me...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
This is the Python source code for the software GAmma-Ray Monte-carlo Radiative transfer (GARMR). Th...
Abstract Here we introduce CRASH4 [6], the fourth release of the cosmological radiative transfer c...
We present the new parallel version (PCRASH2) of the cosmological radiative transfer code CRASH2 for...
We introduce CRASH-AMR, a new version of the cosmological radiative transfer (RT) code CRASH, enable...
Here we introduce CRASH3, the latest release of the 3D radiative transfer code CRASH. In its current...
MetalCRASH is a new variant of the cosmological radiative transfer code CRASH[1 -4] . MetalCRASH ex...
We describe the Center for Radiative Shock Hydrodynamics (CRASH) code, a block-adaptive-mesh code fo...
We present a new dust extension to the Monte Carlo radiative transfer code CRASH, which enables it t...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
Particle-in-cell (PIC) simulations of relativistic shocks are in principle capable of predicting the...
We present a new dust extension to the Monte Carlo radiative transfer code CRASH, which enables it t...
This thesis consider the improvement of the simulation tools used to describe high energy particle c...
International audienceContext. Star formation begins with the gravitational collapse of a d...
Dust has been recognized as a crucial component of galaxies that strongly influences Interstellar Me...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
This is the Python source code for the software GAmma-Ray Monte-carlo Radiative transfer (GARMR). Th...
Abstract Here we introduce CRASH4 [6], the fourth release of the cosmological radiative transfer c...
We present the new parallel version (PCRASH2) of the cosmological radiative transfer code CRASH2 for...
We introduce CRASH-AMR, a new version of the cosmological radiative transfer (RT) code CRASH, enable...
Here we introduce CRASH3, the latest release of the 3D radiative transfer code CRASH. In its current...
MetalCRASH is a new variant of the cosmological radiative transfer code CRASH[1 -4] . MetalCRASH ex...
We describe the Center for Radiative Shock Hydrodynamics (CRASH) code, a block-adaptive-mesh code fo...
We present a new dust extension to the Monte Carlo radiative transfer code CRASH, which enables it t...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
Particle-in-cell (PIC) simulations of relativistic shocks are in principle capable of predicting the...
We present a new dust extension to the Monte Carlo radiative transfer code CRASH, which enables it t...
This thesis consider the improvement of the simulation tools used to describe high energy particle c...
International audienceContext. Star formation begins with the gravitational collapse of a d...
Dust has been recognized as a crucial component of galaxies that strongly influences Interstellar Me...
We describe the 2017 release of the spectral synthesis code Cloudy, summarizing the many improvement...
This is the Python source code for the software GAmma-Ray Monte-carlo Radiative transfer (GARMR). Th...