Module: Advanced GR 1: Gravitational Waves

Module Specifications..

Current Academic Year 2023 - 2024

Please note that this information is subject to change.

Module Title	Advanced GR 1: Gravitational Waves
Module Code	MS539
School	School of Mathematical Sciences
Module Co-ordinator	Semester 1: Abraham Harte Semester 2: Abraham Harte Autumn: Abraham Harte
Module Teachers	Abraham Harte
NFQ level	9	Credit Rating	7.5
Pre-requisite	None
Co-requisite	None
Compatibles	None
Incompatibles	None

Repeat examination

Description

This module develops the physics of gravitational waves in general relativity, from their generation and propagation to their observable consequences.

Learning Outcomes

1. Predict gravitational waveforms in novel physical systems using the quadrupole formula and identify when such results are reliable.
2. Predict the physical effects of gravitational waves in novel situations, using this to analyze and propose potential detection strategies.
3. Compute and contrast the effects of different background geometries on the propagation of gravitational waves.
4. Translate between exact, linearized, and high-frequency models of gravitational waves, identifying their limitations and applying them to make predictions about novel physical systems.

*Type*	*Hours*	*Description*
Workload	Full-time hours per semester
Lecture	24	No Description
Tutorial	12	No Description
Independent Study	89	No Description
Total Workload: 125

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

Indicative Content and Learning Activities

Gravitational waves as linear perturbations
Linearized Einstein equation in flat and curved backgrounds, TT gauge, quadrupole formula, Green functions and tails

Geometric optics for gravitational waves
High-frequency limits as tools to convert PDEs to ODEs, separating gravitational waves and backgrounds, effective stress-energy tensors

Exact models for gravitational waves
Exact plane wave solutions, relation with TT-gauge perturbation theory, features not captured by linearized theory, wave-wave interaction

Gravitational wave observables
Connection with geodesic deviation, effects on pulsar timing, interferometers, and star positions, memory effects

Gravitational wave sources and their detection
Sources, frequency bands, implications for detection. Ground and space-based gravitational wave detectors.

Assessment Breakdown
Continuous Assessment	20%	Examination Weight	80%

Type	Description	% of total	Assessment Date
Course Work Breakdown
Assignment	Homework problems	5%	Week 5
Assignment	Homework problems	5%	Week 12
Written Exam	In-class exam	10%	Week 9

Reassessment Requirement Type
Resit arrangements are explained by the following categories; 1 = A resit is available for all components of the module 2 = No resit is available for 100% continuous assessment module 3 = No resit is available for the continuous assessment component
This module is category 1

Indicative Reading List

KS Thorne and RD Blandford: 0, Modern classical physics,
M Maggiore: 0, Gravitational waves volume I,

Other Resources

None

Programme or List of Programmes

MSAR	MSc in Astrophysics and Relativity

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