Dynamical modelling of debris disks

Details Dynamical modelling of debris disks Dynamical modelling of debris disks

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..862r&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Computer Science

Performance

Scientific paper

I will present a new numerical method aimed at modelling the dynamical evolution of Poynting-Robertson drag dominated debris disks interacting with one or more planets. Unlike other approaches, our model employs the so-called Hermite scheme for particle integration, an algorithm widely used in the N-body community. I will discuss advantages and disadvantages of this integration scheme and compare it to other methods. Example runs will be shown to demonstrate the validity and performance of the model. Finally, I will discuss open issues and further developments of the code.

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