Optional group:
SCELTA DA 12 CFU - (show)
|
12
|
|
|
|
|
|
|
|
20401070 -
DATA ACQUISITION AND CONTROL OF EXPERIMENTS
(objectives)
To provide the student with the basic knowledge on how the construction of a nuclear physics experiment is structured in relation to the collection of data from the detector, the control of the equipment and the experiment, the monitoring of the good functioning of the apparatus and the quality of data acquired
-
RUGGIERI FEDERICO
( syllabus)
The aim of the course is to provide the student with the general cognitive elements underlying the acquisition, control and monitoring systems of Nuclear and Subnuclear Physics experiments. The course is divided into the following topics: -Introduction to DAQ-Parallelism and Pipelining systems -Derandomization-DAQ and Trigger-Data Transmission -Front End Electronics-Trigger-Architecture Computing Systems-Real Time Systems-Real Time Operating Systems -C Language-TCP / IP Network Protocols-DAQ-Architecture Building -VME Bus-Run Control-Farming-Data Archiving During the course, laboratory exercises will take place with the execution of simple examples of: - reading and data transfer systems through pipe mechanisms with concurrent processes; - signal-based trigger simulation programs; - Run Control program for activation and termination of processes; - configuration and reading of data from board on VME bus.
( reference books)
Lecture notes prepared by the teacher on the basis of the slides presented and available on the Moodle server: https://matematicafisica.el.uniroma3.it
|
6
|
FIS/04
|
60
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402146 -
HIGH ENERGY ASTROPHYSICS
(objectives)
Provide the student with an overview of the main phenomena in the field of High Energy Astrophysics, with particular attention to growth phenomena on compact objects (white dwarfs, neutron stars and black holes) and to particle acceleration phenomena
-
Derived from
20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 N0 BIANCHI STEFANO
( syllabus)
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLES ACCRETION: THEORY, EDDINGTON LIMIT, ACCRETION DISKS X-RAY BINARIES: CLASSIFICATION AND PHENOMENOLOGY, CATACLYSMIC VARIABLES, LOW-MASS AND HIGH-MASS X-RAY BINARIES, BLACK HOLE CANDIDATES ACTIVE GALACTIC NUCLEI: CLASSIFICATION AND PHENOMENOLOGY, X-RAY AND GAMMA-RAY EMISSION, JETS, SUPERLUMINAL MOTIONS GAMMA RAY BURSTS: PHENOMENOLOGY, ORIGIN, EMISSION MECHANISMS CLUSTER OF GALAXIES: EMISSION FROM THE INTERGALACTIC MEDIUM, COOLING FLOWS COSMIC RAYS: COMPOSITION, SPECTRUM AND ORIGIN, SUPERNOVA REMNANTS, ULTRA HIGH ENERGY COSMIC RAYS
( reference books)
(LONGAIR MALCOM S. ) HIGH ENERGY ASTROPHYSICS 3RD ED. [CAMBRIDGE 2011] (KIPPENHAHN R., WEIGERT A.) STELLAR STRUCTURE AND EVOLUTION [SPRINGER 1994] (G.B. RYBICKI, A.P. LIGHTMAN) RADIATIVE PROCESSES IN ASTRIPHYSICS [WILEY] (VIETRI M.) ASTROFISICA DELLE ALTE ENERGIE [BORINGHIERI] (SHAPIRO S.L, TEUKOLSKY S.A.) BLACK HOLES, WHITE DWARFS AND NEUTRON STARS [WILEY]
|
6
|
FIS/05
|
60
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410506 -
COSMOLOGY
(objectives)
The course aims to explore in detail some aspects of Modern Cosmology which are just as many topics of high interest both from the point of view of the physical phenomena involved and from the point of view of the methodologies used. Particular attention is paid to the comparison between observations and theory, that is to the relation between the Cosmology and the Astrophysical Astrophysics.
-
Derived from
20402143 COSMOLOGIA in Fisica LM-17 N0 BRANCHINI ENZO FRANCO
( syllabus)
This course discusses in detail the key issues in Modern Cosmology, including outstanding problems. The goal is to provide an overview of the subject and to illustrate the main techniques, theoretical and observational alike, commonly used in this field. The main topics are: - Density fluctuation in a cosmological scenario: generation and growth. Gravitational Instability. Newtonian limit and the Jeans Theory. Linear theory. - Cosmic Microwave Background temperature fluctuation. Acoustic peaks. The Sachs-Wolfe effect. Secondary effects. - - Cosmic backgrounds in different energy bands: Radio, X-ray and gamma-ray - Secondary anisotropies. The Gunn-Peterson effect, cosmic reionization, Ly-alpha forest and Sunayev-Zel'dovich effect. - The intergalactic medium at low redshift and the missing baryons problem. - Large scale structures. Statistical analysis of the galaxy distribution in space. Correlation functions and power spectra. - Luminous vs. dark matter. Galaxy bias. - Nonlinear growth of density fluctuations. The Zel'dovich approximation. The spherical collapse model. The halo model. Press-Schechter theory and its extension. - Peculiar velocities, distance indicators and their calibrations. - Gravitational lensing: Theory and observations. Micro-lensing. Strong lensing. Weak lensing.
( reference books)
Peacock J. Physical Cosmology. Cambridge Univ.Press Longair M. Galaxy Formation [A&A Library ] Coles P., Lucchin F. Cosmology [Wiley 2000] Vari articoli di rivista forniti dal docente durante il corso.
|
6
|
FIS/05
|
54
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410580 -
Education & Outreach, the communication of science
(objectives)
To provide the student with the basic concepts of communication, such as techniques for public speaking and for the preparation of presentation materials and scientific communication texts. To acquire skills on the design and implementation of communication products (images, audio, video) and on the Communication Plan (plan to organize the communication of an event or scientific project).
-
BERNIERI ENRICO
( syllabus)
This course is based on the use of case studies, intersting examples of science communication that will be presented and analysed during the lessons.
On the examples of these case studies, communication laboratories and practical activities will be organized. Students will work in team, guided by researchers and professional communicators, to plan and produce specific communication tools (articles, websites, blogs, audio/video etc).
The course will also take in account the technological aspects related to communication, introducing and examining selected open source software.
The program
The course is 52 hours long, including 40 ore of lessons and 12 hours of lab activities. 12 hours are in common with the “Communcating Science” PhD course.
Introduction to science communication • The postulates of communication: from body language to the communication plan • About science communication: why should we communicate science? • Different types of communication, including in the academic & research world • Planning an event for the public: the 5 steps strategy • Visual communication and science
Speaking to the public about science • Introduction to verbal communication: from public talks to press conferences • The basics of public speaking in science • Slides, audio/video and multimedia tools
Writing about science • Introducing science journalism • Differences between a scientific article, a press release and outreach articles • Writing for video: the storyboard
Visual communication of science • How to communicate science with images • How to plan and produce an image
Communicating science on web • How is science communicated on the web • Science and web 2.0 • How to plan and produce a website
Organization of a public event • The communication plan of a public event • Organizing an astronomical observation event
( reference books)
"The hands-on guide for science communicators: a step.by-step approach to public outreach" di Lars Lindberg Christensen https://play.google.com/store/books/details?id=GI_fpb4xFX4C&rdid=book-GI_fpb4xFX4C&rdot=1&source=gbs_vpt_read&pcampaignid=books_booksearch_viewport
-
GIACOMINI Livia
( syllabus)
This course is based on the use of case studies, intersting examples of science communication that will be presented and analysed during the lessons.
On the examples of these case studies, communication laboratories and practical activities will be organized. Students will work in team, guided by researchers and professional communicators, to plan and produce specific communication tools (articles, websites, blogs, audio/video etc).
The course will also take in account the technological aspects related to communication, introducing and examining selected open source software.
The program
The course is 52 hours long, including 40 ore of lessons and 12 hours of lab activities. 12 hours are in common with the “Communcating Science” PhD course.
Introduction to science communication • The postulates of communication: from body language to the communication plan • About science communication: why should we communicate science? • Different types of communication, including in the academic & research world • Planning an event for the public: the 5 steps strategy • Visual communication and science
Speaking to the public about science • Introduction to verbal communication: from public talks to press conferences • The basics of public speaking in science • Slides, audio/video and multimedia tools
Writing about science • Introducing science journalism • Differences between a scientific article, a press release and outreach articles • Writing for video: the storyboard
Visual communication of science • How to communicate science with images • How to plan and produce an image
Communicating science on web • How is science communicated on the web • Science and web 2.0 • How to plan and produce a website
Organization of a public event • The communication plan of a public event • Organizing an astronomical observation event
-
DE ANGELIS ILARIA
( syllabus)
This course is based on the use of case studies, intersting examples of science communication that will be presented and analysed during the lessons.
On the examples of these case studies, communication laboratories and practical activities will be organized. Students will work in team, guided by researchers and professional communicators, to plan and produce specific communication tools (articles, websites, blogs, audio/video etc).
The course will also take in account the technological aspects related to communication, introducing and examining selected open source software.
The program
The course is 52 hours long, including 40 ore of lessons and 12 hours of lab activities. 12 hours are in common with the “Communcating Science” PhD course.
Introduction to science communication • The postulates of communication: from body language to the communication plan • About science communication: why should we communicate science? • Different types of communication, including in the academic & research world • Planning an event for the public: the 5 steps strategy • Visual communication and science
Speaking to the public about science • Introduction to verbal communication: from public talks to press conferences • The basics of public speaking in science • Slides, audio/video and multimedia tools
Writing about science • Introducing science journalism • Differences between a scientific article, a press release and outreach articles • Writing for video: the storyboard
Visual communication of science • How to communicate science with images • How to plan and produce an image
Communicating science on web • How is science communicated on the web • Science and web 2.0 • How to plan and produce a website
Organization of a public event • The communication plan of a public event • Organizing an astronomical observation event
( reference books)
The hands-on guide for science communicators: a step.by-step approach to public outreach" di Lars Lindberg Christensen https://play.google.com/store/books/details?id=GI_fpb4xFX4C&rdid=book-GI_fpb4xFX4C&rdot=1&source=gbs_vpt_read&pcampaignid=books_booksearch_viewport
|
6
|
FIS/08
|
40
|
-
|
12
|
-
|
Elective activities
|
ITA |
20410505 -
ASTROPARTICLE PHYSICS
(objectives)
To introduce the student to research activities on problems in common between Elementary Particle Physics and Astrophysics. The different research themes that are the object of study by the international scientific community will be discussed within a single framework, with particular attention to the phenomenological interpretation and to the proposals for the realization of new experimental apparatus
-
BUSSINO SEVERINO ANGELO MARIA
( syllabus)
Phenomenological and Experimental topics in Astroparticle Physics. Common problems in particle physics, astrophysics and cosmology.Dark Matter. Cosmic Rays. Cosmic Rays Acceleration. Neutrino Masses and Neutrino Oscillation. Lepton Number non-conservation and double beta decay. Baryon Number non-conservation and proton decay. CP violation and the matter-antimatter asymmetry.
( reference books)
K. Thomas Gaisser Cosmic rays and particle physics Cambridge 1990 Malcom S. Longair High energy astrophysics Cambridge 1992 H. V. Klapdor - Kleingrothaus and A. Staudt Non - Accelerator particle physics Bristol 1995 Donald H. Perkins Particle Astrophysics, second edition Oxford 2009
-
MARI STEFANO MARIA
( syllabus)
Experimental Astroparticle Physics: detectors for Cosmic Ray measurement, Dark Matter search by direct approach, neutrino oscillation parameter measurement, Gravitational Wave measurement.
( reference books)
K. THOMAS GAISSER COSMIC RAYS AND PARTICLE PHYSICS CAMBRIDGE 1990 MALCOM S. LONGAIR HIGH ENERGY ASTROPHYSICS CAMBRIDGE 1992 H. V. KLAPDOR - KLEINGROTHAUS AND A. STAUDT NON - ACCELERATOR PARTICLE PHYSICS BRISTOL 1995 DONALD H. PERKINS PARTICLE ASTROPHYSICS, SECOND EDITION OXFORD 2009
|
6
|
FIS/04
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402259 -
PHYSICS OF CLIMATE
(objectives)
To provide the fundamental theoretical and experimental knowledge in the field of Climate Physics and Climate Change
-
Pasini Antonello
( syllabus)
first part
Definition of climate (climatology and meteorology). The climate system (atmosphere, biosphere, cryosphere, geosphere, hydrosphere, Sun). The solar radiation and the energy balance of the Earth (solar physics calls, laws of radiation, absorption of solar radiation in the atmosphere). Atmosphere and Climate (recalls of composition, structure and circulation of the atmosphere). Clouds and aerosols (calls processes of condensation and cloud formation). Ocean and climate (recalls composition, structure and ocean circulation). Radiative transfer (calls of absorption, emission and radiative transfer of the atmosphere). The greenhouse effect (the atmosphere as greenhouse gas emissions, the calculation of the energy balance, greenhouse models). The ozone layer (ultraviolet radiation in the atmosphere, photochemical production of ozone, ozone measurements, "hole" ozone). Climate observation with remote sensing (measurements from land, satellite measurements, infrared instruments, tools "limb viewing", applications of remote sensing to studies climate). Climate sensitivity and climate change (changes astronomical, solar, atmospheric, oceanic and temperature fluctuations). Atmosphere of other planets. Climate and society. Multidecadal variability of sea surface temperature (seminar Dr. Salvatore Marullo). Lidar measurement of greenhouse gases (visit to the ENEA Frascati Research Center).
second part
Introduction to climate models. The conceptual path from observations to simulations. Dynamic and statistical approaches. Hierarchy of climate models and their components, types of models, the concept of parameter. Models Power Budget (EBM). General structure of an EBM, EBM 0-dimensional, one-dimensional EBM, parameter in EBM, applications. Radiative-convective models (RC) and models Intermediate Complexity (EMIC). Radiative-convective and radiative balance in climate models and implementation at intermediate complexity. Global Climate Models (GCMs). Structure of a GCM, components and interactions, fundamental equations and their modeling. Activities and results of attribution. Validation of climate models. Elements of regional climate modeling and downscaling techniques. Scenarios and climate projections for the XXI century. Analyze the climate and its changes from another point of view: neural network models and analysis of Granger causality. Details on techniques and results of attribution. Downscaling with neural network models.
( reference books)
F. W. Taylor (2005), Elementary Climate Physics, Oxford. K. McGuffie & A. Henderson-Sellers (2014), The Climate Modelling Primer, 4th Edition, Wiley.
|
6
|
FIS/06
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402026 -
PHYSICS OF THE IONOSPHERE AND PHYSICS OF THE MAGNETOSPHERE
(objectives)
Electromagnetic and corpuscular radiation of solar origin gives rise to complex interactions affecting the magnetosphere and the Earth's ionosphere. The magnetic fields of the Sun and the Earth play a fundamental role in these interactions, in a space characterized by the presence of partially ionized plasma (weakly ionized gas): here the physics of the propagation of radio waves is very interesting.
The aim of the course is to present a selection of the most relevant physical phenomena that unfold in this complex environment, where man deploys sophisticated technological systems, on whose functioning the structures of contemporary society are increasingly dependent. Space Weather deals with problems resulting from disturbances in the circumterrestrial environment, in particular consequent to the deterioration of the radiopropagative conditions of the ionosphere.
The ultimate goal is to bring the student closer to the physics of phenomena, stimulating his interest in research in the sector and projecting him towards contemporary challenges to be met.
-
SCOTTO Carlo
( syllabus)
Program of the course of "Physics of the Ionosphere and Magnetosphere" prof. Carlo Scotto Most of the topics are dealt in the book by G.W. Prölss ("Physics of the Earth's Space Environment", ed. Springer). Reference is made to the paragraphs of this book. The remaining topics are reported in the distributed Lesson Notes. The relevant detailed bibliography is shown in them. Introduction: purpose of the course and presentation of the topics covered.
1. Notions of magneto-ionospheric plasma physics Plasma frequency, Debye distance and Debye-Hückel potential, plasma conditions, free mean path, phase refraction index for radio waves in a plasma without collisions and in the absence of magnetic field, cold plasma (Lesson notes). (P. 232, § 7.3.1, § 7.3.2, § 7.3.3). Energy of the electromagnetic field (Lesson notes). Motion of electric charges in a magnetic field: gyration motion, the magnetic moment as an adiabatic invariant, motion where grad(B) is parallel to B, bounce motion (§ 5.3.1, § 5.3.2, pp. 220-228), gradient drift motion (§ 5.3.2, pp. 228-229), neutral shift drift, drift E x B and plasma conductivity in the absence of collisions, drift under the action of external forces (§ 5.3.1, § 5.3.2, § 5.3.3 pp. 219-233).
2. The interplanetary medium. The solar corona and the solar wind (§ 6.1 and 6.1.1, pp. 278-282, including all the references). Large-scale solar wind structure and on the ecliptic plane (§ 6.1.6). The interplanetary magnetic field: observations and physical characteristics (§ 6.2.1, pp. 300-304). The heliosferic current sheet (§ 6.2.4). Segment structure of the polar component of B (§ 6.2.5). Alfven's theorem (Appendix A.14, pp.484-487).
3. Magnetosphere The geomagnetic field near the Earth (§ 5.2). Curvature drift (p. 233). Total drift (p. 234-235). Composed motion of charge carriers (§ 5.3.4). Particle populations in the internal magnetosphere: radiation belts, ring current, plasmashere (§ 5.4). The distant geomagnetic field: configuration and classification, currents on the diurnal side of the magnetopause, reflection of the particles and formation of the current, system of currents in the geomagnetic tail (§ 5.5). Particle population in the external magnetosphere: magnetotail plasma sheet, magnetotail lobe plasma, magnetospheric boundary layer (§ 5.6). Formation of bow shock and the magnetosheat (§ 6.4 introduction and § 6.4.1, pp. 325-328).
4. Ionosphere Absorption processes, gas radiation attenuation, energy deposition in the upper atmosphere: Chapman function. Earth ionosphere: historical outline, vertical profile of electron density, ionospheric temperature, production and disappearance of ionization, ionospheric regions, electronic equilibrium, vertical profile of electron density in E region and in region F2 region (§ 3.2; introduction of chap 4, § 4.1, § 4.2, § 4.3). Ionosphere morphology: the cusps on the ionogram trace and the ionospheric regions (Lesson notes). Regular variations of the ionosphere: layers E and F1 (Lesson notes). Irregular variations of the ionosphere: F2 layer (Lesson notes). Sporadic E layer(Lesson notes). Simplified photochemical model for regions E and F: F1 layer (Lesson notes). Simplified photochemical model for region D (Lesson notes). Refraction index for radio waves with collisions and in the absence of a magnetic field; interpretation of the imaginary part of the refractive index: absorption ( Lesson notes). Solar flares and short waves fadeout (Lesson notes). Additional notes on the F1 layer (Lesson notes). Additional notes on layer E (Lesson notes).
5. Magnetoionic theory Introduction. Constitutive equations for a cold plasma with collisions and in the presence of a magnetic field (Lesson notes). Refractive index for radio waves in the ionosphere, neglecting collisions and considering the Earth's magnetic field: Appleton-Hartree equation (Lesson notes). Continuity of nf in X = 1. The zeros of the collisionless Appleton-Hartree equation: longitudinal, transverse and general propagation case (Lesson notes). Polarization: continuity in X = 1 in the general case and in the case of longitudinal propagation. Polarization in case of longitudinal propagation: dependence on the sign of YL. Polarization in general conditions, for X = 1 (Lesson Notes). Refractive index for radio waves in the ionosphere, considering collisions and the earth's magnetic field. Mention upon the polarization in the collisional case. Curves of mi(X) with collisions: importance of the Booker rule (Lesson notes). Conditions of reflection and ionograms, ordinary, extraordinary trace. Ray Z (Lesson Notes). Examples of ionograms (Lesson notes). As indicated in the lesson notes, the material of this teaching unit can be found at: Ratcliffe, J. A. (1959), The magneto-Ionic Theory and its Applications to the Ionosphere, Cambridge University Press.
6. Absorption and dissipation of solar wind energy Topology of the high polar atmosphere (§ 7.1). Electric fields, and plasma convection (§ 7.2). Conductivity and currents in the polar ionosphere (§ 7.3). Polar auroras: energy dissipation of the auroral particles, origin of the auroral particles, diffuse and discrete aurora(§ 7. 4). Solar Wind Dynamo (§ 7.6.1), open magnetosphere (§ 7.6.2), plasma convection in the open magnetosphere (§ 7.6.3), open magnetosphere with tail (§ 7.6.4), mention upon the reconnection (part of § 7.6. 5) Birkeland currents in regions 1 and 2 (§ 7.6.6).
7. Geospheric storms Magnetic storms: regular variation, equatorial electroject, magnetic activity at low, high and medium latitudes, geomagnetic indexes (§ 8.1). Magnetic substorms: growth and expansion phase, Alvfèn waves and their role (§ 8.3). Ionospheric storms: negative and positive storms (§ 8.5).
( reference books)
1) G.W. Prölss "Physics of the Earth's Space Environment" 2) Lecture Notes
|
6
|
FIS/06
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410050 -
FISICA DELLE NANOSTRUTTURE
(objectives)
Give the student an in-depth understanding of the physical properties of low-dimensional systems, with nanometric characteristic dimensions. Illustrate the principles of implementation methodologies and nanotechnologies
-
Derived from
20410050 FISICA DELLE NANOSTRUTTURE in Fisica LM-17 DI GASPARE LUCIANA
( syllabus)
HETEROJUNCTIONS AND HETEROSTRUCTURES. 2, 1, -0 DIMENSIONAL SYSTEMS: ELECTRONIC STATES AND DENSITY OF STATES. 2DIMENSIONAL ELECTRON GASES. CHARACTERISTICS LENGTHS FOR THE ELECTRICAL TRANSPORT IN LOW DIMENSIONAL SYSTEMS. T-MATRICES AN RESONANT TUNNELLING. INTERFERENCE OF WAVE FUNCTIONS. AHARONOV-BOHM EFFECT. BALISTIC TRANSPORT AND CONDUCTANCE QUANTIZATION IN 1D SYSTEMS. MAGNETOTRANSPORT: SHUBNIKOV-DE HAAS OSCILLATIONS AND QUANTUM HALL EFFECT. SINGLE ELECTRON TUNNELING AND COULOMB BLOCKAFDE EFFECTS. SINGLE ELECTRON TRANSISTOR. GRAPHENE: STRUCTURAL AND ELECTRONIC PROPERTIES. OPTICAL PROPERTIES OF NANOSTRUCTURES: INTERBAND TRANSITIONS IN QUANTUM WELLS; EXCITONS IN 2D SYSTEMS; INTERSUBBANDTRANSITIONS. LIGHT-EMITTERS: GAIN COEFFICIENT; DIODE LASERS, HETEROSTRUCTURE LASERS, QUANTUM CASCADE LASERS (BRIEF).
( reference books)
DATTA S.: ELECTRONIC TRANSPORT IN MESOSCOPIC SYSTEMS [CAMBRIDGE UNIVERSITY PRESS ] FERRY D.K. AND GOODNICK S.M.: TRANSPORT IN NANOSTRUCTURES [CAMBRIDGE UNIVERSITY PRESS ] DAVIES J. H. : THE PHYSICS OF LOW DIMENSIONAL SEMICONDUCTORS [CAMBRIDGE UNIVERSITY PRESS)
|
6
|
FIS/03
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410051 -
FISICA DELLE SUPERFICI E INTERFACCE
(objectives)
Introduce the student to the fundamental knowledge on properties, preparation and characterization of surfaces and interfaces
-
Derived from
20410051 FISICA DELLE SUPERFICI E INTERFACCE in Fisica LM-17 OFFI FRANCESCO
( syllabus)
- Surface of a solid and solid/solid interface: general notions, historical development and applications
- Thermodynamics, crystallography and structure: two-dimensional lattices and superstructures; reciprocal lattice and Brillouin azone - surface tension and crystals shape; structural defects; relaxation and reconstruction; solid/solid interfaces; nucleation and thin film growth, low energy electron diffraction to investigate surface structure
- Electronic properties: surface electronic states; three-dimensional bands; band mapping with the photoemission technique; image states and core level shift; electronic states in semiconductors; the work function; surface and adsorbed vibrations; surface phonon observation methods; surface plasmons and polaritons
- Adsorption and desorption: physisorption and chemisorption; dissociative adsorption; adsorption and work function; interactions between adsorbed species; bi-dimensional phase transitions; adsorption kinetics; desorption. SUrface diffusion: Flick laws, mechanisms and anisotropy of diffusion, atomic and cluster diffusion
- Experimental techniques: general concepts of ultra high vacuum; pumping systems; vacuum components; preparation of a clean surface; vacuum deposition techniques
- Surface magnetism: electronic structure and anisotropy in ferromagnetic materials; magnetization and magnetic surface anisotropy; spin-polarized photoemission; magnetic dichroism; photoemission electron microscope for detecting magnetic domains
- Microscopy: scanning and transmission electron microscope; probe scanning microscopy: scanning tunneling microscope and atomic force microscope
( reference books)
- Philip Hofmann, Surface Physics
- Hans Lüth, Solid Surfaces, Interfaces and Thin Films (Springer-Verlag, 2010)
- K. Oura, et al., Surface Science, An Introduction (Springer-Verlag, 2003)
- Andrew Zangwill, Physics at Surfaces (Cambridge University press, 1992)
- Gabor A. Somorjai, Introduction to surface chemistry and catalysis (Wiley, 2010)
|
6
|
FIS/03
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410585 -
PHYSICS OF LIQUIDS AND SOFT MATTER
(objectives)
To offer an introduction to the modern physics of liquids, understood as the study of the phenomenology of fluids starting from interatomic force laws. We will study the theoretical methods based on integral equations that allow us to describe the structure of the liquid. Computer numerical simulation methods applied to the physics of liquids will be introduced. Then we will study the correlation functions and the theory of linear response with applications to the study of the dynamics of liquids in the hydrodynamic limit and in the visco-elastic limit. The memory functions will be introduced. The physics of supercooled liquids and the study of the glass transition will be discussed
-
Derived from
20410585 FISICA DEI LIQUIDI E DELLA MATERIA SOFFICE in Fisica LM-17 GALLO PAOLA
( syllabus)
1 - Review of Thermodynamics and Statistical Mechanics. Extensive and intensive thermodynamic functions. Conditions of equilibrium. Legendre transforms and thermodynamic potentials. Phase stability conditions. Phase transitions and their classification. Van der Waals equation. Review of the theory of statistical ensembles. Fluctuations.
2 - Forces between atoms and short-range order. Characterization of the liquid state of matter. Characterization of soft materials. Forces between atoms and effective potentials. Distribution functions in the canon and the grand canon. Radial distribution function and relationship with thermodynamics. The static structure factor. Measurement of the structure of a liquid with X-ray and neutron scattering techniques. Structure factors and radial distribution functions of liquid and liquid molecular mixtures. Classic density functional theory. Ornstein-Zernike equation. Closing relations for the density functional.
3 - Numerical simulation of liquid and soft material
Stochastic and deterministic simulation methods. Molecular Dynamics Method. Verlet-style algorithms. Molecular dynamics at constant temperature and pressure. The Monte Carlo simulation method. Monte Carlo simulation in different ensembles. Phase equilibrium simulation methods. Application of Monte Carlo and Molecular Dynamics methods to complex liquids and soft materials.
4 - Dynamics of liquids and soft matter Time-dependent correlation functions. Inelastic diffusion of neutrons and measurement of the dynamic structure factor. Van Hove correlation functions. Principle of the detailed budget. Linear response theory. Answer function. Fluctuation-dissipation theorem. Diffusion of particles. Diffusion coefficient. Speed correlation function. Hydrodynamics and collective modes. Scattering Brillouin. Memory functions.
5 - Metastable states, subcooled liquids and glass transition for liquids and soft materials.
Stability and metastability. Spinodal curve from the Van der Waals equation. Fluctuations and trends of correlation functions near the critical point. Subcooled liquids and glass transition. Angell diagram. Configurational entropy and Kauzmann temperature. The slow dynamics of subcooled liquids and soft matter and the theory of Mode Coupling.
( reference books)
J.P. Hansen and I.R. McDonald, Theory of Simple Liquids, seconda edizione, Academic Press. N. H. March and M. P. Tosi, Introduction to Liquid State Physics, World Scientific. P. G. Debenedetti, Metastable Liquids, Princeton University Press.
|
6
|
FIS/03
|
60
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410098 -
FISICA DEI PIANETI DEL SISTEMA SOLARE ED ESOPIANETI
(objectives)
Provide adequate knowledge about the physics of the planets of the solar system and the exoplanets, the techniques of investigation of atmospheres, surfaces and sub-surfaces of planets and introduce the astrophysical problem of the search for life.
Group:
1
-
CLAUDI Riccardo
( syllabus)
1 Solar System Part - Overall description of the Solar System, mass and angular momentum distribution, astrophysical variables. - Overall description of planets, their main characteristics ; description of planetary satellites systems and of minor bodies of the Solar System. - Terrestrial planets: main characteristics and evolutive processes of planetary surfaces. - Terrestrial planets: thermal history, impact cratering processes, volcanism, tectonics.Comparative planetology. - Meteorites and minor bodies; radiometric dating and clues for the formation of the Solar System. - Giant planets - Planetary satellites - Internal structure of planets, different evolution of terrestrial and giant planets. - Planetary atmospheres 2 Extrasolar Planets Part - Historical Introduction - Exo planets Indirect discovery methods - Exo planets Direct discovery methods - Exo Planets Characteristics - Physics of extrasolar Planets - Characterization and results - Which Life? - Habitability and Habitable Zone - The search for life 3 Common Part - Introduction to the Planetary formation Theory
( reference books)
- There is no official text of the course. A suggested text is the following: Imke de Pater and Jack J. Lissauer, Planetary Sciences, Cambridge University Press. During the course several scientific review papers will be suggested by the lecturers.
Material
- Course slides - Scientific papers
-
TOSI Federico
( syllabus)
1 Solar System Part - Overall description of the Solar System, mass and angular momentum distribution, astrophysical variables. - Overall description of planets, their main characteristics ; description of planetary satellites systems and of minor bodies of the Solar System. - Terrestrial planets: main characteristics and evolutive processes of planetary surfaces. - Terrestrial planets: thermal history, impact cratering processes, volcanism, tectonics.Comparative planetology. - Meteorites and minor bodies; radiometric dating and clues for the formation of the Solar System. - Giant planets - Planetary satellites - Internal structure of planets, different evolution of terrestrial and giant planets. - Planetary atmospheres 2 Extrasolar Planets Part - Historical Introduction - Exo planets Indirect discovery methods - Exo planets Direct discovery methods - Exo Planets Characteristics - Physics of extrasolar Planets - Characterization and results - Which Life? - Habitability and Habitable Zone - The search for life 3 Common Part - Introduction to the Planetary formation Theory
( reference books)
- There is no official text of the course. A suggested text is the following: Imke de Pater and Jack J. Lissauer, Planetary Sciences, Cambridge University Press. During the course several scientific review papers will be suggested by the lecturers.
Material
- Course slides - Scientific papers
|
6
|
FIS/05
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410097 -
FOTONICA QUANTISTICA
(objectives)
Acquire knowledge of the physics of laser systems and the description of the electromagnetic field in second quantization, with particular emphasis on phenomenological aspects.
-
BARBIERI MARCO
( syllabus)
The physics of laser: blackbody radiation, Einstein equation, interaction of light with a two-level atom, gain and attenuation. Optical transitions in semiconductors. CW and pulsed operation of a laser.
Optical coherence and quantisation of the e.m. field: classical theory of fluctuations, first- and second-order coherence. E.m. field as a harmonic oscillator, quantisation and quantum theory of optical coherence. Number states, coherent states, and thermal states. Interaction picture: beam splitter and squeezing hamiltonians. Homodyne detection and photon counting. Quasi-probability distributions.
( reference books)
R. Loudon, The quantum theory of light. Capp. 1, 2, 3, 4, 5, 6 O. Svelto, Principles of lasers. Capp. 1, 2, 3, 4, 5, 6, 7, 8, 9 R. Boyd, Nonlinear optics. Capp. 1, 2, 7 J.S. Bell, Speakable and unspeakable in quantum mechanics. Cap 2
|
6
|
FIS/03
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20401858 -
INTRODUCTION TO MEDICAL PHYSICS
(objectives)
Introduce the student to the study of the effects of ionizing and non-ionizing radiation on living matter. Lay the foundations of the principles of radiation protection and the therapeutic use of ionizing and non-ionizing radiation
-
ARAGNO DANILO
( syllabus)
The development of the program will mainly take place using the field study methodology with a guided internship in a Health Physics Unit of a Hospital Company. Basic topics. Physical quantities and units of measurement; Typical detectors for diagnostics and therapy with ionizing radiation; Diagnostic and therapy equipment; Principles of dosimetry of radiation beams, calculation and measurement of the dose; notes on the planning of therapeutic treatment plans; Radioactive decays and main radionuclides of medical use and; General principles of radioprotection, the role of images and information systems in the diagnostic and therapeutic fields; Health effects and physical risks in Magnetic Resonance STAGE program SECTOR: Physics in Radiotherapy 1) Dosimetry: Dose concept and its measurement. 2) Instrumentation for relative dosimetry: point detectors and bidimensional detectors. 3) Examples of dose measurements in photon beams with different devices. 4) Vision of the Linear Accelerator installations of the Radiotherapy Unit. Description and outline of the principles of operation of a linear accelerator. Vision of the TC installation dedicated to the centering of RT patients. 5) Vision of the systems for treatment plans (TPS) supplied. Illustration of the general principles of a TPS: structure and functions. 6) Realization of a simple treatment plan with an illustration of the fundamental criteria necessary for its setting. SECTOR: Physics in Diagnostic Imaging 7) Vision Radiiagnostics equipment, examples and illustrations. Description and overview of operating principles. 8) Vision and illustration of the instrumentation and the phantoms used for Quality Controls. 9) Examples of image analysis for the purpose of Quality Controls in MRI and Radiodiagnostics. SECTOR: Physics in Nuclear Medicine 10) Vision of Nuclear Medicine equipment. Description and overview of operating principles. 11) Mink and illustration of the instrumentation and puppets used for Quality Controls in MN. 12) Examples of image analysis for Quality Control in Nuclear Medicine. SECTOR: Radiation Protection and Security 13) Vision of an RM SITE: description and outline of the operating principles of an RM system. Safety issues of patients and operators. 14) Instrumentation and dosimetry of personnel exposed to ionizing radiation
( reference books)
- FONDAMENTI DI DOSIMETRIA DELLE RADIAZIONI IONIZZANTI ( IV Edizione) Raffaele Fedele Laitano ENEA http://www.enea.it/it/seguici/pubblicazioni/pdf-volumi/FondamentidosimetriaradiazioniionizzantiIV.pdf - Altro materiale didattico fornito dal docente
|
6
|
FIS/07
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402354 -
STATISTICAL MECHANICS
(objectives)
The course aims to give an overview of modern developments in statistical mechanics. In particular, starting from the theory of phase transitions and critical phenomena, we want to show how the concepts underlying the method of the re-normalization group emerged. This method is now widely used in various fields of statistical mechanics. The critical phenomena constitute the classical application of the method, which is illustrated in detail in the first 6 credits of the course. These first 6 credits can therefore be used by multiple addresses. The remaining 2 credits focus on more recent applications of the method in the field of matter physics.
-
Derived from
20401425 MECCANICA STATISTICA in Fisica LM-17 N0 LUPI LAURA
( syllabus)
1st module program (6 credits)
Introduction to thermodynamics. Thermodynamic potentials. Phase transitions and Van der Waals equation. Fluctuations and stability. Phase transitions and thermodynamic limit. Microscopic derivation of the Van der Waals equation. Critical point behavior of the Van der Waals equation. Curie-Weiss theory of ferromagnetism. Landau theory of second species transitions. Ginzburg criterion for the validity of the middle field theory. The role of symmetry and dimensionality: the theorem of Mermin-Wagner. Renormalization team. Kadanoff-Wilson transformation. Calculation of fixed points for the Landau-Wilson model and development in epsilon.
( reference books)
Statistical Mechanics and Applications in Condensed Matter by Carlo Di Castro and Roberto Raimondi Cambridge University Press 2015 ISBN: 9781107039407
|
6
|
FIS/02
|
60
|
-
|
-
|
-
|
Elective activities
|
ITA |
20410173 -
Numerical Methods for Differential Equations
(objectives)
To study and implement more advanced numerical approximation techniques, in particular relating to optimization problems and the approximate solution of Ordinary Differential Equations
-
Derived from
20410420 AN420 - ANALISI NUMERICA 2 in Scienze Computazionali LM-40 CACACE SIMONE
( syllabus)
Ordinary Differential Equations Finite difference approximation for ordinary differential equations: Euler's method. Consistency, stability, absolute stability. Second order Runge-Kutta methods. Single step implicit methods: backward Euler and Crank-Nicolson methods. Convergence of single step methods. Multi-step methods: general structure, complexity, absolute stability. Stability and consistency of multi-step methods. Adams methods, BDF methods, Predictor-Corrector methods. (Reference: Chapter 7 of curse notes "Appunti del corso di Analisi Numerica")
Partial Differential Equations Finite difference approximation for partial differential equations. Semi-discrete approximations and convergence. The Lax-Richtmeyer theorem. Transport equation: the method of characteristics. The "Upwind" (semi-discrete and fully-discrete) scheme, consistency and stability. Heat equation: Fourier approximation. Finite difference scheme, consistency and stability. Poisson equation: Fourier approximation. Finite difference scheme, convergence. (Reference: notes by R. LeVeque, "Finite Difference methods for differential equations", selected chapters 1, 2, 3, 12, 13)
( reference books)
Roberto Ferretti, "Appunti del corso di Analisi Numerica", in pdf at http://www.mat.uniroma3.it/users/ferretti/corso.pdf
Roberto Ferretti, "Esercizi d'esame di Analisi Numerica", in pdf at http://www.mat.uniroma3.it/users/ferretti/Esercizi.pdf
Lecture slides in pdf at http://www.mat.uniroma3.it/users/ferretti/bacheca.html
Additional notes given by the teacher
|
6
|
MAT/08
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402155 -
MEASUREMENTS IN ASTROPHYSICS
(objectives)
Make the student able to analyze, independently and critically, various types of astrophysical data
-
LA FRANCA FABIO
( syllabus)
Part I: Astrophysics Problem:
Active Galactic Nuclei and Galaxies 1. Definition and classification: BH paradigm, growth, AGN Radio Loud / Radio quiet, Unified Model 2. AGN astrophysics: X-band AGN-RQ properties, emission models: Comptonization, absorption properties and outflows 3. AGN astrophysics: reflection components in the X-band spectrum, observation of relativistic effects in the X-band spectrum 4. Spectra of AGN and Galaxies in the optical and NIR band
Part II: Introduction to X-band and optical detectors and telescopes 1. optical telescopes. Basic principles and techniques of detection 2. X-band detectors: basic principles and detection techniques 3. solid state detectors, Charged Coupled Devices (CCD) 4. collimated and focused optical systems 5. X telescope features: efficiency, sensitivity, energy resolution, angular resolution, effective area 6. The ESA / XMM-Newton, NASA / Chandra and NASA / NuStar space telescopes
Part III: Data Analysis
1. investigation tools: study of energy distribution (emission spectrum), study of temporal behavior (light curve), study of variability (power spectrum and reverberation) 2. statistical errors and systematic errors 3. background 4. S / N signal to noise ratio 5. observation and maximization of the S / N
Part IV: Data analysis tutorial
- XMM-epic session 1. search for archived data 2. Image analysis: DS9 3. spectrum analysis: xspec 4. Temporal analysis: xronos
Part V - data analysis in optical and NIR band
( reference books)
handouts by the course teacher
-
DE ROSA Alessandra
( syllabus)
Part I: Astrophysics Problem:
Active Galactic Nuclei and Galaxies 1. Definition and classification: BH paradigm, growth, AGN Radio Loud / Radio quiet, Unified Model 2. AGN astrophysics: X-band AGN-RQ properties, emission models: Comptonization, absorption properties and outflows 3. AGN astrophysics: reflection components in the X-band spectrum, observation of relativistic effects in the X-band spectrum 4. Spectra of AGN and Galaxies in the optical and NIR band
Part II: Introduction to X-band and optical detectors and telescopes 1. optical telescopes. Basic principles and techniques of detection 2. X-band detectors: basic principles and detection techniques 3. solid state detectors, Charged Coupled Devices (CCD) 4. collimated and focused optical systems 5. X telescope features: efficiency, sensitivity, energy resolution, angular resolution, effective area 6. The ESA / XMM-Newton, NASA / Chandra and NASA / NuStar space telescopes
Part III: Data Analysis
1. investigation tools: study of energy distribution (emission spectrum), study of temporal behavior (light curve), study of variability (power spectrum and reverberation) 2. statistical errors and systematic errors 3. background 4. S / N signal to noise ratio 5. observation and maximization of the S / N
Part IV: Data analysis tutorial
- XMM-epic session 1. search for archived data 2. Image analysis: DS9 3. spectrum analysis: xspec 4. Temporal analysis: xronos
Part V - data analysis in optical and NIR band
( reference books)
handouts by the course teacher
|
6
|
FIS/05
|
60
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402380 -
ENVIRONMENTAL RADIOACTIVITY
(objectives)
The course is designed to provide basic knowledge, both theoretical and experimental, in the field of Physics Ionizing Radiation and radiometric methods in Physics of the Earth and the Environment
-
PLASTINO WOLFANGO
( syllabus)
Atoms, Nuclides, and Radionuclides
Radiation sources. Radiation interactions. Counting Statistics.
Geochemistry of Radiogenic Isotopes
Mixing Theory. Origin of Igneous Rock. Water and Sediment. The Oceans.
Thermonuclear Radionuclides
Fission Products of Transuranium Elements. 90Sr in the Environment. 137Cs in the Environment. The 90Sr/137Cs, 239,240Pu, and 241Am in the Arctic Ocean.
General Properties of Radiation Detectors
Ionizing chambers. Proportional and Geiger-Mueller counters. Scintillation Detectors. Germanium Gamma-Ray Detectors.
Geochronometry
The Rb-Sr Method. The K-Ar Method. The 40Ar/39Ar Method. The Sm-Nd Method. The U-Pb, Th-Pb, and Pb-Pb Methods. The 14C Method. The 3H/3He Method.
Application of Tracer Technology to the Environment
Atmospheric Transport Modeling. Groundwater dynamics. Nuclear non-proliferation.
( reference books)
Knoll G.F. - Radiation Detection and Measurement. John Wiley & Sons, 2010 - ISBN:9780470649725
Faure G. and Mensing T.M - Isotopes-Principles and Applications. John Wiley & Sons, 2004 - ISBN:9780471384373
|
6
|
FIS/07
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20401000 -
PHYSICAL INSTRUMENTS IN BIOLOGY AND MEDICINE
(objectives)
Provide the student with the fundamentals of modern diagnostic imaging techniques supplemented by some laboratory exercises that allow him to further deepen the topics covered and enter this field subject to advanced research as well as fundamental clinical applications
-
FABBRI ANDREA
( syllabus)
1. Interaction of photons and charged particles with matter. 2. Nuclear Medicine principles 3. SPECT and PET techniques. 4. Radiology Principles and Instrumentation. 5. Computed Tomography. 6. Nuclear Magnetic Resonance. 8. Ultrasound Principles and Instrumentation. 9. Radioteraphy and Adroteraphy Principles. 10. Dosimetry Principles.
|
6
|
FIS/04
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
20402258 -
RELATIVITY THEORY
(objectives)
(English) To make the student familiar with the conceptual assumptions of the Theory of General Relativity, both as a geometric theory of space-time and by emphasizing analogies and differences with field theories based on local symmetries that describe the interactions between elementary particles. Illustrate the essential elements of differential geometry necessary to formalize the proposed concepts. Introduce the student to extensions of the theory of interest for current theoretical research.
-
Derived from
20402258 TEORIA DELLA RELATIVITA' in Fisica LM-17 FRANCIA DARIO
( syllabus)
Introductory notions Recap of Special Relativity. Lorentz transformations in Minkowski’s space. Vectors in Minkowski’s space. Basis of the tangent space. Cotangents space and dual vectors in Minkowski’s space. Basis of cotangent space. Lorentz transformations of vectors and dual vectors. Tensors in Minkowski’s space. Properties of vectors, dual vectors and tensors in Minkowski’s space. Definition of symmetric and antisymmetric tensor. Symmetrization and antisymmetrization of a generic tensor. Metric in Minkowski’s space: definition and properties. Operations related to the metric: scalar products, rising and lowering indices of a tensor, contractions and trace of a tensor. Equivalence between inertial and gravitational mass. Weak Equivalence Principle (WEP), Einstein’s equivalence Principle (EEP).
Basic notions of differential geometry Introduction to the notion of manifold. Definition and properties of maps. Injective and suriective maps (some examples included). Composition of charts. Invertible charts. Definition of diffeomorphism. Definition of chart (or coordinate system). Definition of atlas. Definition of manifold. Product of manifolds. Formal coordinate independent definition of vector. Demonstration that the dimension of the tangent space coincides with the one of the corresponding manifold. Basis (or coordinate system) of the tangent space. Coordinate transformations. Coordinate transformations of the components of a vector. Definition and properties of the tangent field. Definition of one parameter group of diffeomorphisms. Definition of integral curves. Commutator of two vectors. Coordinate independent definition of dual vector (one-form). Cotangent space and corresponding basis. Coordinate transformation of the components of a one-form. Coordinate independent definition of tensor. Demonstration that the partial derivative of a tensor is not a tensor. Metric: signature and canonical form. Tensor densities. Differential forms. Wedge product. Exterior derivative. Closed and exact form. Poincarre Lemma (statement only). Hodge duality. Maxwell equations expressed in term of exterior derivative and hodge duality (only small reference). Integration over a manifold: volume element in terms of the determinant of the metric. Maps between manifold: pullback and pushforward. Pullback and pushforward associated to diffeomorphisms. Equivalence between diffeomorphisms and coordinate transformations. Vector field associated to diffeomorphisms. Lie Derivative: definition and general properties. Action of Lie’s derivative on scalars, vectors, one-forms and tensors. General Relativity as diffeomorphism invariant theory. Analogy between gauge transformations and diffeomorphisms.
Symmetries. Notion of submanifold. Immersed and embedded submanifolds. Notion of hypersurface and boundary of a manifold. Integration on manifolds again: differential form as generic volume element. Orientation and orientable manifold. Covering of the manifold through partition of unity. Integration of p-forms over submanifold. Demonstrations that the volume element can be expressed in terms of the determinant of the metric. Stokes theorem (no demonstration).
Connection, Covariant Derivative, Curvature Lie’s Algebra and Lie’s group. Action from the right and from the left. Left- and right-invariant vectors. Structure constants. Examples of Lie groups. Maurer-Cartan forms. Maurer-Cartan’s equations. Action of Lie Groups on manifolds. Definition of free, effective and transitive action. Orbit and stabilizer. Algebric definition of connection and covariant derivative. General properties of covariant derivatives. Action of coordinate transformations on the connection. Demonstration that the difference of Christoffel coefficients associated to two different connections transforms as a tensor; torsion tensor, torsion-free and metric connection. Demonstrations that for any given metric exists a connection (metric connections) for which the covariant derivative of the metric is zero. Formal construction of the covariant derivative from the notion of parallel transport (qualitative introduction). Fiber bundle. Trivial and locally trivializable bundles. Local trivilizations. Maps between fiber bundles (notions). Defintion of bundle atlas, G-atlas, G-structure. Fiber Bundle with structure group G. Definition of Principal Bundle. Definition of section of a bundle. Vector bundle and bundle of basis, definition and general properties. Relation between principle bundle, vectorbundle and bundle of frames (definition of associated vector bundle to a principal bundle. Construction of the covariante derivative on a vectorbundle (only the knowledge of the fundamental logical steps is required for the exam). Curvature tensor as 2-form on a fiber bundle. Geometrical interpretation of the curvature. Bianchi identity. Fiber metric. Ortogonal basis. Connections and gauge theories: electromagnetism as simple example. Soldering form. Choice of the gauge. Ortonormal and metric gauge. Levi-Civita connection; Riemann’s tensor : definition and properties. Ricci’s tensor and scalar, Weyl’s tensor. Globally and locally inertial coordinates.
Einstein’s theory of gravity
Minimal coupling. Particle in a gravitational field: affine parameter, self-parallel curves. Geodesic’s equations. Geodesic deviation. Derivation of the Einstein’s equations from Newton’s limit. Lagrangian derivations of Einstein’s equations. General considerations on the structure of Einstein’s equations. Choice of the gauge. Energy conditions. Symmetries and Killing vectors: version of Noether’s theorem from general relativity. Maximal number of linearly independent Killing vectors on a manifold. Homogenous and isotropic manifold. Spaces at constant curvature. Metric in spaces at constant curvature.
Notable solutions of Einstein’s equations
Static spherically symmetric spacetimes. Determination of Schwarzschild’s metric. Cosmological solution. Spatially homogeneous and isotropic spacetime. Frieman’s Robertson-Walker metric. Friedman’s equations. Coordinate singularities. Case of study: Schwarzschild radius. Rindler metric. Kruskal coordinates. Black hole solution. Perturbation around a background metric. Case of study:perturbation of flat metric. Degrees of freedom. Linearized Einstein’s equations. Choice of the gauge. Linearized Einstein’s equations in vacuum: gravitational waves. Solutions in presence of the source (only few words).
Advanced concepts Conformal transformations. Cotton’s tensor. Conformally flat metric. Demonstration of the theorem: a metric is conformally flat if and only if Weyl (Cotton) tensor is null. Conformal group. Conformal Killing vectors. Alternative theories of gravity. Scalar-tensor theories. Jordan and Einstein’s frames.
( reference books)
Testi consigliati : 1. S. Carrol Space time and Geometry: An Introduction to General Relativity (Addison Wesley, 2004); 2. R. Wald General Relativity (The Chicago Press, 1984); 3. B. Schutz A First Course in General Relativity (Cambridge Press) 4. B. Schutz Geometrical Methods of Mathematical Physics (Cambridge Press) 5. S. Weinberg Gravitation and Cosmology-principles and application of the general theory of relativity (John Weiley & Sons, 1972); 6. people.sissa.it/~percacci/lectures/general/index.html
|
6
|
FIS/02
|
48
|
-
|
-
|
-
|
Elective activities
|
ITA |
|