CODE 61874 ACADEMIC YEAR 2021/2022 CREDITS 6 cfu anno 2 FISICA 9012 (LM-17) - GENOVA 6 cfu anno 1 FISICA 9012 (LM-17) - GENOVA SCIENTIFIC DISCIPLINARY SECTOR FIS/01 LANGUAGE Italian TEACHING LOCATION GENOVA SEMESTER 2° Semester PREREQUISITES Propedeuticità in ingresso Per sostenere l'esame di questo insegnamento è necessario aver sostenuto i seguenti esami: PHYSICS 9012 (coorte 2020/2021) NUCLEAR AND PARTICLE PHYSICS AND ASTROPHYSICS 2 61847 2020 THEORETICAL PHYSICS 61842 2020 MATTER PHYSICS 2 61844 2020 PHYSICS 9012 (coorte 2021/2022) NUCLEAR AND PARTICLE PHYSICS AND ASTROPHYSICS 2 61847 2021 THEORETICAL PHYSICS 61842 2021 MATTER PHYSICS 2 61844 2021 TEACHING MATERIALS AULAWEB OVERVIEW The course aims to provide a phenomenological introduction to modern astrophysics and cosmology in particular by showing the application to the context of the phenomena of the cosmos of different branches of classical and modern physics, in order to constitute a solid basis for students interested in a career in these disciplines, while providing knowledge of phenomena and methods for students interested in pursuing other areas of physics. AIMS AND CONTENT LEARNING OUTCOMES Broad knowledge of the most important phenomena of astrophysics and cosmology AIMS AND LEARNING OUTCOMES At the end of the course the student will have knowledge regarding: units of measurement and observables in use; mechanisms of production of electromagnetic waves of different energies in astrophysical phenomena; interaction and propagation of photons in the cosmos and their detection (with hints to other messengers); elements of observational astronomy; stellar physics (equilibrium and various phases of stellar evolution, multiple systems); planetary systems; interstellar medium; extra-galactic astrophysics; elements of general relativity and cosmology for the description of the evolution of the universe on a large scale. The students will acquire an understanding of the different astrophysical phenomena by applying the knowledge of the various branches of classical and modern physics (classical mechanics, thermodynamics, electromagnetism, optics, relativity, quantum mechanics, statistical physics, nuclear physics, particle physics) and will be informed on the lines of leading research of modern astrophysics and cosmology. TEACHING METHODS Classes with use of the black board and of slides (given in advance) SYLLABUS/CONTENT Observables and units of measurement of astrophysical / cosmological interest. Radiative transport. Electromagnetic radiation emission mechanisms from astrophysical sources and their detection (instrumentation and most relevant objects observable in the various bands) Stellar and galactic dynamics Star balance conditions in the various evolutionary stages Star systems Planetary systems Interstellar medium Types and structures of galaxies Dark matter Active galaxies and super massive black holes The universe on a large scale Introduction to general relativity Evolutionary scenarios of the universe Thermal history of the universe: the cosmic background radiation Dark energy To finish the course, if possible: activity (optional) with an optical telescope Planning of an observational campaign for one of the objects studied during the course and possible data acquisition RECOMMENDED READING/BIBLIOGRAPHY Astrophysics for Physicists" by Arnab Rai Choudhuri"; "Invitation to Astrophysics" by T. Padmanabhan "Modern Cosmology" di S. Dodelson TEACHERS AND EXAM BOARD SILVANO TOSI Ricevimento: Anytime, by previous request of appointment by email Exam Board SILVANO TOSI (President) CARLA BIGGIO MARCO PALLAVICINI ALESSANDRO PETROLINI MARCO RAVERI FLAVIO GATTI (President Substitute) LESSONS LESSONS START II semester Class schedule The timetable for this course is available here: Portale EasyAcademy EXAMS EXAM DESCRIPTION Oral exam. 2 possibilities: questions by the committee or description of a project (realized in small groups) ASSESSMENT METHODS Questions by the committee on the program and, in case, questions on the project. The exam lasts about 30 minutes per student.