Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Kornet, Kacper"'
Autor:
Andrade, Tomas, Salo, Llibert Areste, Aurrekoetxea, Josu C., Bamber, Jamie, Clough, Katy, Croft, Robin, de Jong, Eloy, Drew, Amelia, Duran, Alejandro, Ferreira, Pedro G., Figueras, Pau, Finkel, Hal, França, Tiago, Ge, Bo-Xuan, Gu, Chenxia, Helfer, Thomas, Jäykkä, Juha, Joana, Cristian, Kunesch, Markus, Kornet, Kacper, Lim, Eugene A., Muia, Francesco, Nazari, Zainab, Radia, Miren, Ripley, Justin, Shellard, Paul, Sperhake, Ulrich, Traykova, Dina, Tunyasuvunakool, Saran, Wang, Zipeng, Widdicombe, James Y., Wong, Kaze
Publikováno v:
Journal of Open Source Software, 6(68), 3703, 2021
GRChombo is an open-source code for performing Numerical Relativity time evolutions, built on top of the publicly available Chombo software for the solution of PDEs. Whilst GRChombo uses standard techniques in NR, it focusses on applications in theor
Externí odkaz:
http://arxiv.org/abs/2201.03458
Autor:
Kornet, Kacper, Potherat, Alban
We present Direct Numerical Simulations of decaying Magnetohydrodynamic (MHD) turbulence at low magnetic Reynolds number. The domain considered is bounded by periodic boundary conditions in the two directions perpendicular to the magnetic field and b
Externí odkaz:
http://arxiv.org/abs/1502.07631
Autor:
Kornet, Kacper, Pothérat, Alban
We put forward a new type of spectral method for the direct numerical simulation of flows where anisotropy or very fine boundary layers are present. The mean idea is to take advantage of the fact that such structures are dissipative and that their pr
Externí odkaz:
http://arxiv.org/abs/1403.4129
We present a new multi-fluid, grid MHD code PIERNIK, which is based on the Relaxing TVD scheme (Jin and Xin, 1995). The original scheme (see Trac & Pen (2003) and Pen et al. (2003)) has been extended by an addition of dynamically independent, but int
Externí odkaz:
http://arxiv.org/abs/0812.2799
We examine the predictions of the core accretion - gas capture model concerning the efficiency of planet formation around stars with various masses. First, we follow the evolution of gas and solids from the moment when all solids are in the form of s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606094
Autor:
Kornet, Kacper, Wolf, Sebastian
We have investigated the problem of the distribution of both masses and orbital radii of planets resulting from the gas-accretion, gas-capture model. First we followed the evolution of gas and solids from the moment where all solids are in the form o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601209
Publikováno v:
Astron.Astrophys. 430 (2005) 1133-1138
We present the first results from simulations of processes leading to planet formation in protoplanetary disks with different metallicities. For a given metallicity, we construct a two-dimensional grid of disk models with different initial masses and
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410112
Publikováno v:
Astron.Astrophys. 417 (2004) 151-158
We have calculated an evolution of protoplanetary disk from an extensive set of initial conditions using a time-dependent model capable of simultaneously keeping track of the global evolution of gas and water-ice. A number of simplifications and idea
Externí odkaz:
http://arxiv.org/abs/astro-ph/0312471
Publikováno v:
Astron.Astrophys. 396 (2002) 977-986
Formation of planets in the 47 UMa system is followed in an evolving protoplanetary disk composed of gas and solids. The evolution of the disk is calculated from an early stage, when all solids, assumed to be high-temperature silicates, are in the du
Externí odkaz:
http://arxiv.org/abs/astro-ph/0209613
Autor:
Kornet, Kacper, Pothérat, Alban
Publikováno v:
In Journal of Computational Physics 1 October 2015 298:266-279
