EXPERIMENTAL GRAVITATION

Course objectives

A - Knowledge and understanding OF 1) Starting from the experimental bases of gravitation, and the theoretical implications, the course focusses on gravitational wave detection. Two interlaces aspects will be illustrated, the experimental apparuses and data analysis technicques. OF 2) This will give students the necessary preparation for a rigorous application of the acquired notions, not only for the topics inherent to the course, but for the broadest and more general field of experimental physics of fundamental interactions. B - Application skills OF 3) The student will be able to correctly interpret the experimental issues and the avancement of the apparatuses. OF 4) The student will be able to apply techniques/metods of data analysis C - Autonomy of judgment OF 5) Thanks to the lesson attendance, and the persistent interaction with the lecturer, the student will develop an adequate autonomy of judgment and will critically analyze the acquired information. D - Communication skills OF 6) The acquisition of adequate skills and tools for communication will be verified both during the lessons and during the final exam, contributing to the development of clear communication skills by the student. E - Ability to learn OF 7) The student will have the ability to evaluate and solve a broad range of data analysis issues. OF 8) Ther student will be able to conceive and develop an experimental/theoretical project, starting from the data acquisition, through the analysis of the collected data and outlining some conclusions via the related post-processing.

Channel 1
ETTORE MAJORANA Lecturers' profile

Program - Frequency - Exams

Course program
Experimental bases of Gravitation ------------------------------------------------------- - Inertial mass and gravitational mass, the Newtonian theory of gravitation and the 1/r2 trend of the gravitational field. Experimental checks. Gravity and other forces of nature. Isotropy and homogeneity of space and time. Gravitational red shift. Principle of equivalence in General Relativity. Roll, Krotkov and Dicke experiment. Homogeneity of time. Translation invariance and gravitational red shift. Pound and Rebka experiment. Vessot experiment. Lorentz invariance: the measure of g-2. - Theoretical implications and experimental verifications of the constancy over time of G. Classical verifications of General Relativity. Precession of Mercury, light deflection, radar echo delay. - Parametrized Post-Newtonian (PPN) formalism. Physical meaning of the parameters and their values in General Relativity. PPN tests in the solar system based on light deviation, radar echo delay, interferometry on a large basis, precession of the perihelion of Mercury. Test based on the observation of binary systems. Upper limits on the validity of the strong equivalence principle and lunar ranging experiment. The gravito-magnetic effect and the experimental basis for its detection. Gravitational waves and their effect on matter ------------------------------------------------------- - Gravitational Waves (GWs) as solutions of the Einstein equations. Effect on test masses. Intensity and brightness of the source. Generation of GWs: bond with the mass quadrupole moment, oscillating quadrupole and rotating quadrupole. Reduction of the orbital period by GW emission: the emblematic case of the PSR1913 + 16 system and the new double systems.Notes on astrophysical sources of GWs: coalescence of binary systems, rotating neutron stars, stellar collapse. Astrophysical and cosmological GW background. GW Detectors - Noise in measuring instruments. Stochastic processes. Average, variance, correlation, autocorrelation. Harmonic process. Poisson process. Stochastic process transformations. Systems without memory. Linear transformations. - Power spectrum. Fluctuation-Dissipation Theorem. Thermal noise in the circuits. Thermal noise in a pendulum. Attenuation of the seismic noise and of the thermal noise: the suspension systems. Wideband optical detectors ------------------------------------------------------- - Michelson interferometer and Fabry-Perot cavity. Light recirculation. Opto-mechanical systems with feedback: Pound-Drever-Hall technique for Fabry-Perot cavity control. Shot and radiation pressure noise reduction. Power and Signal Recycling. The Newtonian noise. Quantum limit of gravitational detectors and strategies to bypass this issue. Space detectors and pulsar timing technique. ------------------------------------------------------- Data Analysis: Theory and Applications ------------------------------------------------------- Elements of probability and statistics. Signals (continuous and discrete) and noise; Fourier transform. Spectral estimation (periodogram, auto-regressive estimates, spectrograms). The signal-to-noise ratio and the linear data filtering problem. Filtering (Wiener filter, adapted filter, triangular filters). Detection theory. Procedure in non-stationary noise. Image analysis. GW signal extraction. Parameter estimation. GW sources. Analysis of the open data collected by the LIGO-Virgo interferometric detectors (https://www.gw openscience.org/).
Prerequisites
Basics Physics topics, matured through the standard courses during the three-year Bachelor in physics. Very useful also the knowledge of basic statistics tools and probability concepts. Tensor algebra is also used on some topics and is certainly quite useful.
Books
• L. Landau, E.Lifshitz, Teoria dei campi, Editori Riuniti • Ciufoli, J. A. Wheeler : Gravitation and Inertia, Princeton University Press, 1995 • A. Papoulis, S. Unnikrishna Pillai , Probability, Random Variables and Stochastic Processes, McGraw-Hill, 2002 • H. C. Ohanian, R. Ruffini Gravitazione e spazio-tempo, Zanichelli, 1997 • Clifford M. Will, Theory and Experiment in Gravitational Physics, Cambridge University Press • P. Saulson, Fundamentals of Interferometric Detection of Gravitational waves, World Scientific 1994 • C.Will, Was Einstein Right? Testing Relativity at the Centenary; gr-qc/0504086 • C.M.Will, The Confrontation between General Relativity and Experiment; gr-qc/0103036 • E.G. Adelberger, B.R. Heckel, and A.E. Nelson: Tests of the Gravitational Inverse- Square law; ArXiv:hep-ph/0307284 • G.Pizzella, Fisica Sperimentale del Campo Gravitazionale, Nuova Italia, 1993 • A.M.Nobili, Precise gravitation measurements on Earth and in space: Tests of the Equivalence Principle - http://eotvos.dm.unipi.it/nobili/murst/varenna2000/nobili2.pdf • Fulvio Ricci’s notes: https://sites.google.com/a/uniroma1.it/fulvio-ricci/didattica/gravitazione-sperimentale • Sergio Frasca’s notes: https://drive.google.com/drive/folders/1-GfrpXDVYO5wj0MjcQoJKdma8SXrt_XN
Frequency
optional but highly recommended
Exam mode
The exam consists of an oral dissertation on specific themes treated during the course and a dedicated in-depth presentation.
  • Lesson code1055363
  • Academic year2025/2026
  • CourseAstrophysics and Cosmology
  • CurriculumSingle curriculum
  • Year2nd year
  • Semester1st semester
  • SSDFIS/01
  • CFU6