Curriculum
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.Mutuazione: 20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 R BIANCHI STEFANO
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.Mutuazione: 20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 R BIANCHI STEFANO
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.Mutuazione: 20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 R BIANCHI STEFANO
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.Mutuazione: 20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 R BIANCHI STEFANO
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.Mutuazione: 20402146 ASTROFISICA DELLE ALTE ENERGIE in Fisica LM-17 R BIANCHI STEFANO
Programma
COMPACT OBJECTS: WHITE DWARFS, NEUTRON STARS, THE CHANDRASEKHAR LIMIT, PULSARS, BLACK HOLESACCRETION: 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
Testi Adottati
(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]
Modalità Erogazione
Slideshow lectures, with in-depth discussions, followed by questions/answers.Modalità Frequenza
attendance is not mandatory but strongly recommendedModalità Valutazione
Oral exam about the course's content, with an in-depth discussion aided by formulae and plots, as needed.