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Curricular information is subject to change
- Learn the Kerr solution
- Understand how gravitational waves are generated and detected.
- Be able to reformulate the field equation in terms of the spin coefficients
- Solve the resulting ODEs
- FRW solution
- Kerr metric
- Gravitational wave solution to the field equation
- Sources of gravitational waves
- Newman Penrose formalism
Student Effort Type | Hours |
---|---|
Lectures | 30 |
Tutorial | 4 |
Specified Learning Activities | 20 |
Autonomous Student Learning | 60 |
Total | 114 |
Not applicable to this module.
Remediation Type | Remediation Timing |
---|---|
In-Module Resit | Prior to relevant Programme Exam Board |
• Group/class feedback, post-assessment
Not yet recorded.
Lecture | Offering 1 | Week(s) - 20, 21, 22, 23, 24, 25, 26, 29, 30, 31, 32, 33 | Mon 11:00 - 11:50 |
Lecture | Offering 1 | Week(s) - 20, 21, 22, 23, 24, 25, 26, 29, 30, 31, 32, 33 | Tues 16:00 - 16:50 |
Lecture | Offering 1 | Week(s) - 20, 21, 22, 23, 24, 25, 26, 29, 30, 31, 32, 33 | Wed 11:00 - 11:50 |