CODE  94844 

ACADEMIC YEAR  2022/2023 
CREDITS 

SCIENTIFIC DISCIPLINARY SECTOR  FIS/01 
LANGUAGE  Italian 
TEACHING LOCATION 

SEMESTER  2° Semester 
TEACHING MATERIALS  AULAWEB 
The experimental activities concerning gravitation contribute significantly to the increase of our knowledge and complete the picture of our understanding of the fundamental interactions. In this context, the recent observations of gravitational waves by the LIGO and VIRGO interferometers represent an essential contribution. In the field of experimental gravitational wave research, the most important initiative, in Italy and Europe, at the moment, is linked to the VIRGO interferometer. The course is taught by researchers from the National Institute of Nuclear Physics and the University of Genoa who participate in VIRGO and contribute in various sectors of this experiment.
The course presents the physics of gravitational waves, framing it in the context of the theory of general relativity, describing the experimental and data analysis techniques used for their observation and discussing their contribution in the field of astroparticle physics, astrophysics, cosmology and fundamental physics.
The course aims to provide students with adequate knowledge on the theoretical foundations, experimental techniques and data analysis strategies, necessary to understand the scientific literature on the observations of gravitational waves and their implications in the field of astronomy, astrophysics, cosmology and fundamental physics.
The course is aimed at students interested in the particular scientific topic of gravitational wave research, as well as those interested in a path in the field of astroparticle physics, astrophysics and cosmology. The course content is also a useful complement for students interested in the physics of fundamental interactions, as it concerns gravity physics issues not always covered in the curricular pathways. The elements of astrophysics, cosmology, classical optics, quantum optics and the data analysis techniques covered in the lessons provide a useful knowledge base also for the study of disciplines other than that covered by the course.
To achieve its objective, the course  of 48 hours in total  is structured in three modules of 16 hours each:
 Elements of general relativity and gravitational wave sources
The objective of this module is to provide students with the fundamental elements of the theory of general relativity, necessary for the study of the physics of gravitational waves. In addition to acquiring the fundamental concepts and tools of the theory, students will be able to understand the mechanisms underlying the generation of gravitational waves, useful for deepening the study of astrophysical sources, as well as the mechanisms of interaction of a gravitational wave with test masses, an essential prerequisite for understanding interferometric detection techniques.
 Interferometric detectors of gravitational waves and advanced detection techniques
The aim of this module is to provide students with a realistic description of the interferometric detection techniques of gravitational waves, starting from elements of classical optics, up to the study of advanced detection strategies based on on quantum optics techniques. Furthermore, the module deals with the study of the main noise sources that limit the sensitivity of the interferometer and the mitigation strategies adopted, with references to statistical physics (fluctuationdissipation theorem) and the theory of quantum fluctuations (quantum noise). At the end of the module students will be able to read and deepen independently the technical/scientific literature on the subject.
 Elements of analysis of stochastic processes and data analysis strategies
The objective of this module is to provide students with the elements necessary to understand the advanced data analysis techniques used in experiments dedicated to the observation of gravitational waves. Starting from elements of probability and statistics, the course deals with the study of techniques used in the analysis of time series dominated by noise (Bayesian inference, adaptive filters, machine learning) to arrive at the discussion of the significance of the observed events. At the end of the module, students will be able to read and deepen the scientific literature on the subject independently.
Threeyear fundamental physics courses. Special relativity theory and tensor algebra in Minkowski space. Elements of probability and statistics covered in the threeyear courses. Knowledge of elements of classical optics would be useful, but it is not considered an essential prerequisite.
Theoretical frontal lessons. During the lessons, if possible, a visit to the Virgo interferometer will be organized.
 Elements of general relativity
Principle of equivalence. Tensor algebra. Tensorial equations. Geodesic curves. Covariant derivative. Geodesic deviation and curvature. Riemann tensor. Energymomentum tensor. Einstein's equation. Weak field limit.
 Linear approximation and gravitational waves
Gravitational waves as solutions of Einstein's equations. Expression in TransverseTraceless gauge and in the laboratory system. Effect on test masses. Generation of gravitational waves in linear approximation; quadrupole formula. Intensity and brightness of a gravitational wave source.
 Elements of gravitational astrophysics
Gravitational waves generated by compact binary systems in linear approximation. Backaction of the gravitational wave on the orbital dynamics of the system. Binary systems at cosmological distances. Standard candles and elements of gravitational cosmology.
 Interferometric gravitational wave detectors
A simple Michelson interferometer. Interferometers with FabryPérot cavity. Power recycling. Virgo's optical scheme. Modes of propagation of laser beams, stability criteria for optical cavities. Thermal aberrations and mitigation methods. Noise sources and mitigation strategies (quantum noise; fluctuationdissipation theorem and thermal noise; seismic noise; Newtonian noise). Interferometer control strategies: PoundDreverHall technique, control of longitudinal degrees of freedom, control of angular degrees of freedom, locking. DC readout. Elements of quantum optics, signal recycling, squeezing.
 Elements of analysis of stochastic processes
Introduction to data analysis; elements of probability; estimators. Bayes' theorem. Definition and properties of Power Spectral Density. Stochastic processes and their characterization; Gaussian processes. Linear systems. Hypothesis test. Matched filtering in linear systems and in general. Detection theory: parameter estimation; templates; checking the consistency of the waveforms; coherent analysis of two detectors. False alarm rate. Sampling in the parameter space. Notes on calculation problems. Location of the source; overview on sources and alternative methods to the matched filter. "First Detection". Population of events and merge rates. Elements of postNewtonian formalism; tests of General Relativity. Deformability measurements for Neutron Stars and Equation of State limits through GW measurements. Notes on multimessenger astronomy.
T.A. Moore, A General Relativity Workbook, University Science Books (2013)
M. Maggiore, Gravitational Waves. Volume 1: Theory and Experiments, Oxford University Press (2008)
PR Saulson, Fundamentals of Interferometric Gravitational WaveDetectors, World Scientific (1994)
M. Bassan (Ed.), Advanced Interferometers and the Search forGravitational Waves, Springer (2014)
J. D. E. Creighton, W. G. Anderson, GravitationalWave Physics and Astronomy: An Introduction to Theory, Experiment and Data Analysis, Wiley (2011)
Second semester AY 2021/2022
Interview on the topics covered in the course starting from a topic chosen by the student.
Oral exam starting from a topic chosen by the student and questions on the topics covered in the course. During the interview, the commission tries to stimulate the student to elaborate links between the topics and the information acquired during the course (and in the threeyear courses) to evaluate the degree of learning, the synthesis ability and the clarity of the exposition.
The students can agree on the reception hours by contacting the teachers by email.
GEMME GIANLUCA
gianluca.gemme@ge.infn.it
CHINCARINI ANDREA
andrea.chincarini@ge.infn.it
SORRENTINO FIODOR
fiodor.sorrentino@ge.infn.it