Note: This is an archived Handbook entry from 2010.
|Dates & Locations:|| |
This subject has the following teaching availabilities in 2010:Semester 2, Parkville - Taught on campus.
Timetable can be viewed here. For information about these dates, click here.
|Time Commitment:||Contact Hours: 36 hours comprising 3 one-hour lectures/week |
Total Time Commitment:
|Prerequisites:||This subject will assume a general familiarity with Physics at third year level.|
|Recommended Background Knowledge:||None.|
|Non Allowed Subjects:||None.|
|Core Participation Requirements:||
It is University policy to take all reasonable steps to minimise the impact of disability upon academic study and reasonable steps will be made to enhance a student's participation in the University's programs. Students who feel their disability may impact upon their participation are encouraged to discuss this with the subject coordinator and the Disability Liaison Unit.
CoordinatorDr Nicole Bell
|Subject Overview:||This subject provides an advanced introduction to physical cosmology. Specific topics may include the isotropic homogeneous Universe, the Robertson Walker metric, the Friedmann equations, baryogenesis, inflation, big-bang nucleosynthesis, the recombination era, density fluctuations as the origin of galaxies, the cosmic microwave background, linear and non-linear growth of structure, the Press-Schechter mass function, reionization of the IGM and gravitational lensing. Examples are drawn from past and current cosmological observations.|
The objectives of this subject are:
|Assessment:||Three assignments totalling up to 36 pages (20%), spaced equally throughout the semester, plus one end-of-semester oral examination lasting up to an hour or one end-of-semester written examination lasting up to four hours (80%).|
|Breadth Options:|| |
This subject is not available as a breadth subject.
|Fees Information:||Subject EFTSL, Level, Discipline & Census Date|
At the completion of this subject, students should have gained skills in:
Master of Science (Physics) |
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