Module Specifications.
Current Academic Year 2024 - 2025
All Module information is indicative, and this portal is an interim interface pending the full upgrade of Coursebuilder and subsequent integration to the new DCU Student Information System (DCU Key).
As such, this is a point in time view of data which will be refreshed periodically. Some fields/data may not yet be available pending the completion of the full Coursebuilder upgrade and integration project. We will post status updates as they become available. Thank you for your patience and understanding.
Date posted: September 2024
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Repeat examination |
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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 | |||||||||||||||||||||||||||||||||||||||||||