Modelling the evolution of pulsar wind nebulae / Michael Johannes Vorster

Modelling the evolution of pulsar wind nebulae / Michael Johannes Vorster

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This study focusses on modelling important aspects of the evolution of pulsar wind nebulae using two different approaches. The first uses a hydrodynamic model to simulate the morphological evolution of a spherically-symmetric composite supernova remnant that is expanding into a homogeneous interstel...

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Bibliographic Details
Main Author: Vorster, Michael Johannes
Language:en
Published: 2014
Subjects:
Composite supernova remnants
Morphological evolution
Hydrodynamic
Kinematic magnetic field
Pulsar wind nebulae
Particle evolution models
Fokker-Planck transport equation
Spherically-symmetric
Axisymmetric
Diffusion
Drift
Energy losses
Saamgestelde supernova-oorblyfsels
Morfologiese evolusie
Hidrodinamiese
Kinematiese magneetveld
Pulsarwindnewels
Deeltjie evolusiemodelle
Fokker-Planck transport vergelyking
Sferies-simmetries
Aksiaal-simmetries
Diffusie
Dryf
Energie verliese
Online Access:http://hdl.handle.net/10394/10861

Internet

http://hdl.handle.net/10394/10861

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