Registry
Module Specifications
Archived Version 2023 - 2024
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Description Graduate astrophysics | |||||||||||||||||||||||||||||||||||||
Learning Outcomes 1. Appraise the use of a variety of models for the dynamics of plasmas in different astrophysical systems 2. Identify the key assumptions in deriving the shock relations in plasmas 3. Summarise the primary process by which non-thermal particles are accelerated. 4. Identify and describe radiative processes leading to the observed X-ray and gamma-ray emission. 5. Differentiate between the various radiative processes relevant to a variety of astrophysical systems | |||||||||||||||||||||||||||||||||||||
All module information is indicative and subject to change. For further information,students are advised to refer to the University's Marks and Standards and Programme Specific Regulations at: http://www.dcu.ie/registry/examinations/index.shtml |
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Indicative Content and
Learning Activities Plasma AstrophysicsIdeal MHD; non-ideal MHD; multi-fluid MHD; Generalised Ohm's LawShocks and astrophysical plasmasRankine-Hugoniot relations; ideal MHD; non-ideal MHD; multi-fluid MHD; numerical study of MHDAstrophysical shocksThe Rankine-Hugoniot relations; J-shocks; C-shocksShock accelerationThe Fermi process; Acceleration power-law distribution; Acceleration time-scalesRadiative ProcessesThermal radiation; radiative transfer; synchrotron emission; Thomson scattering; Synchrotron Emission, Inverce Compton Emission, Hadronic EmissionStar FormationJeans instability; Stages of gravitational contraction; accretion processes; | |||||||||||||||||||||||||||||||||||||
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Indicative Reading List
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Other Resources None | |||||||||||||||||||||||||||||||||||||
Programme or List of Programmes | |||||||||||||||||||||||||||||||||||||
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