Cosmology and the Large-scale Structure of the Universe
150 Hours
One Semester or equivalent
Hawthorn
Available to incoming Study Abroad and Exchange students
Overview
This Unit aims to provide an introduction to cosmology, including the physics of the early Universe, dark matter and dark energy, and the evolution of the observed large-scale structure.
Requisites
Prerequisites
AST10001
Discovering the UniversePHY10004 Electronics and Electromagnetism
AND
150 credit points
Assumed Knowledge
A foundation of conceptual astronomy
Teaching periods
Location
Start and end dates
Last self-enrolment date
Census date
Last withdraw without fail date
Results released date
Study Period 1
Location
Hawthorn
Start and end dates
03-March-2025
01-June-2025
01-June-2025
Last self-enrolment date
16-March-2025
Census date
24-March-2025
Last withdraw without fail date
02-May-2025
Results released date
24-June-2025
Learning outcomes
Students who successfully complete this unit will be able to:
- Appraise and state a conceptual knowledge of space-time and how it has evolved, its observational and theoretical basis
- Explain and apply advanced cosmology concepts such as the big bang model and cosmic inflation, dark matter and dark energy, with the ability to use them in a technical way
- Distinguish and summarise the major unresolved questions in cosmology
- Appraise, apply and explain the tools with which we probe the large-scale structure of the universe, including large galaxy surveys and supercomputer simulations in technical manner understandable to a specialist audience
- Use problem solving skills to explain and synthesise solutions to problems in cosmology
- Design and create a research project on an astronomy topic, assessing and critiquing current knowledge, using credible sources of astronomical information, data and research articles
Teaching methods
Hawthorn
Type | Hours per week | Number of weeks | Total (number of hours) |
---|---|---|---|
Online Learning Activities |
3.00 | 12 weeks | 36 |
On-Campus Class |
2.00 | 6 weeks | 12 |
Unspecified Activities Independent Learning |
8.50 | 12 weeks | 102 |
TOTAL | 150 |
Assessment
Type | Task | Weighting | ULO's |
---|---|---|---|
Newsgroups | Individual | 20 - 40% | 1,2,3,4 |
Online Quizzes | Individual | 15 - 25% | 1,2,3,4,5 |
Project | Individual | 40 - 60% | 6 |
Content
- Cosmology: special and general relativity; the hot “big bang” cosmology and alternative cosmologies; the different ‘flavours’ of dark matter and dark energy
- Modern cosmological observations, redshift, Hubble’s Law, standard candles and standard rods
- The Early Universe: inflation; early universe particle physics; origin and physics of the cosmic microwave background radiation; nucleosynthesis.
- Basic demographic properties of galaxies in the local universe: morphology/mass/size/stellar populations/scaling relations
- The earliest galaxies, galaxies formation and growth, galaxy dynamics
- Cosmology: special and general relativity; the hot “big bang” cosmology and alternative cosmologies; the different ‘flavours’ of dark matter and dark energy
- Modern cosmological observations, redshift, Hubble’s Law, standard candles and standard rods
- The Early Universe: inflation; early universe particle physics; origin and physics of the cosmic microwave background radiation; nucleosynthesis.
- Basic demographic properties of galaxies in the local universe: morphology/mass/size/stellar populations/scaling relations
- The earliest galaxies, galaxies formation and growth, galaxy dynamics.
- Large-scale Structure: structure formation and evolution; observational cosmology; using supercomputers to build synthetic Universes; the ultimate fate of the Universe
Study resources
Reading materials
A list of reading materials and/or required textbooks will be available in the Unit Outline on Canvas.