First cycle
degree courses
Second cycle
degree courses
Single cycle
degree courses
School of Science
PHYSICS
Course unit
GRAVITATIONAL PHYSICS
SCP7081719, A.A. 2017/18

Information concerning the students who enrolled in A.Y. 2017/18

Information on the course unit
Degree course Second cycle degree in
PHYSICS
SC2382, Degree course structure A.Y. 2017/18, A.Y. 2017/18
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Degree course track PHYSICS OF THE UNIVERSE [003PD]
Number of ECTS credits allocated 6.0
Type of assessment Mark
Course unit English denomination GRAVITATIONAL PHYSICS
Website of the academic structure http://fisica.scienze.unipd.it/2017/laurea_magistrale
Department of reference Department of Physics and Astronomy
Mandatory attendance No
Language of instruction English
Branch PADOVA
Single Course unit The Course unit can be attended under the option Single Course unit attendance
Optional Course unit The Course unit can be chosen as Optional Course unit

Lecturers
Teacher in charge GIACOMO CIANI FIS/01

ECTS: details
Type Scientific-Disciplinary Sector Credits allocated
Educational activities in elective or integrative disciplines FIS/01 Experimental Physics 3.0
Educational activities in elective or integrative disciplines FIS/05 Astronomy and Astrophysics 3.0

Mode of delivery (when and how)
Period Second semester
Year 1st Year
Teaching method frontal

Organisation of didactics
Type of hours Credits Hours of
teaching
Hours of
Individual study
Shifts
Lecture 6.0 48 102.0 No turn

Calendar
Start of activities 26/02/2018
End of activities 01/06/2018

Examination board
Examination board not defined

Syllabus
Prerequisites: General Relativity is recommended
Target skills and knowledge: Fundamentals of general relativity and gravitational waves (GW) theory.
GW generation mechanisms and astrophysical sources.
Understanding of the working principles, main limitations and future prospects of GW detectors.
Overview of the current state of the field of GW astronomy.
Examination methods: Oral examination aimed at verifying the conceptual understanding of the topics presented and the ability to correctly approach and analyze specific problems related to GW theory and detection.
Assessment criteria: The students must demonstrate the comprehension and the ability to critically evaluate the concepts, mechanisms and problems related to the generation and detection of gravitational radiation.
Course unit contents: Elements of general relativity. Gravitational waves (GW) in linearized theory; TT-gauge; interaction with matter.

Generation of GW. Quadrupole and post-newtonian approximations. Examples of GW sources: stable and coalescing binary systems, rotating rigid bodies, extreme mass-ratio inspirals.

GW detection. Hulse-Taylor system. Fundamentals of stochastic signals and noise theory. Resonant bars detectors. Modern GW interferometers: basic principle, noise sources, fundamental and technical limitations. Future GW experiments. Elements of data analysis.

Astronomy and science with gravitational waves. Current observations of black hole and neutron star mergers. Tests of general relativity. Astrophysical implications. Multimessenger astronomy.
Planned learning activities and teaching methods: Frontal lessons with exercises and examples
Additional notes about suggested reading: Lessons may be complemented by slides, which will be made available in advance to the students.

Useful excerpts from other written resources will be indicated as they become useful for specific sections of the course.
Textbooks (and optional supplementary readings)
  • Maggiore, Michele, Gravitational wavesMichele Maggiore. Oxford: Oxford University Press, 2008.