Please use this identifier to cite or link to this item:
Title: Modelling Tidal Streams from Galactic Satellites
Authors: Hasanuddin
Supervisors: Dehnen, Walter
Wilkinson, Mark
Award date: 7-Aug-2019
Presented at: University of Leicester
Abstract: Astrophysical simulations are very useful for understanding the physical phenomena of the stellar systems. In this simulation, the computational cost is one of the main concern. To tackle this issue, a choice of the time-step criterion is crucial. In this thesis, I study the efficiency of the time-step depending on the tidal force. This quantity follows gauge invariance under adding a constant acceleration where this property is not owned by conventional time-step criteria. Time step function based on the tidal force is more efficient than other time-step criteria. The observed tidal streams are very important to constrain the Galactic potential and the distribution of sub-haloes structure in the Milky-Way. In this thesis, I present a restricted N-body model for tidal debris to simulate the formation of tidal streams from Galactic satellites. If the satellite orbits are close to a Galactic disc, the structures of tidal debris do not spread in one dimension like the conventional streams but form two dimensions structures like a ribbon. This phenomenon can be explained analytically by action-angle variables and Hamiltonian formalism. This restricted N-body method has fewer ad-hoc assumptions and is more accurate than the alternative (and popular) particle sprinkling techniques at only a modest increase of the computational expense.
Type: Thesis
Level: Doctoral
Qualification: PhD
Rights: Copyright © the author. All rights reserved.
Appears in Collections:Leicester Theses
Theses, Dept. of Physics and Astronomy

Files in This Item:
File Description SizeFormat 
2019HasanuddinPhD.pdfThesis12.9 MBAdobe PDFView/Open

Items in LRA are protected by copyright, with all rights reserved, unless otherwise indicated.