Planet-Disk Interaction revisited

We present results on our investigations of planet–disk interaction in protoplanetary disks. For the hydrodynamic simulations we use a second order semi–discrete total variation diminishing (TVD) scheme for systems of hyperbolic conservation laws on curvilinear grids. Our previously used method...

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Main Authors: Illenseer T. F., Jung Manuel, Duschl W. J.
Format: Article
Language:English
Published: EDP Sciences 2013-04-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20134607006
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author Illenseer T. F.
Jung Manuel
Duschl W. J.
author_facet Illenseer T. F.
Jung Manuel
Duschl W. J.
author_sort Illenseer T. F.
collection DOAJ
description We present results on our investigations of planet–disk interaction in protoplanetary disks. For the hydrodynamic simulations we use a second order semi–discrete total variation diminishing (TVD) scheme for systems of hyperbolic conservation laws on curvilinear grids. Our previously used method conserves the momentum in two dimensional systems with rotational symmetry. Additionally, we modified our simulation techniques for inertial angular momentum conservation even in two dimensional rotating polar coordinate systems. The basic numerical practices are outlined briefly. In addition we present the results of a common planet–disk interaction setup.
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spelling doaj.art-ba9119609b1d494d91899e34ae9177752022-12-22T04:08:29ZengEDP SciencesEPJ Web of Conferences2100-014X2013-04-01460700610.1051/epjconf/20134607006Planet-Disk Interaction revisitedIllenseer T. F.Jung ManuelDuschl W. J.We present results on our investigations of planet–disk interaction in protoplanetary disks. For the hydrodynamic simulations we use a second order semi–discrete total variation diminishing (TVD) scheme for systems of hyperbolic conservation laws on curvilinear grids. Our previously used method conserves the momentum in two dimensional systems with rotational symmetry. Additionally, we modified our simulation techniques for inertial angular momentum conservation even in two dimensional rotating polar coordinate systems. The basic numerical practices are outlined briefly. In addition we present the results of a common planet–disk interaction setup.http://dx.doi.org/10.1051/epjconf/20134607006
spellingShingle Illenseer T. F.
Jung Manuel
Duschl W. J.
Planet-Disk Interaction revisited
EPJ Web of Conferences
title Planet-Disk Interaction revisited
title_full Planet-Disk Interaction revisited
title_fullStr Planet-Disk Interaction revisited
title_full_unstemmed Planet-Disk Interaction revisited
title_short Planet-Disk Interaction revisited
title_sort planet disk interaction revisited
url http://dx.doi.org/10.1051/epjconf/20134607006
work_keys_str_mv AT illenseertf planetdiskinteractionrevisited
AT jungmanuel planetdiskinteractionrevisited
AT duschlwj planetdiskinteractionrevisited