KVL / Klausuren / MAP 1.HS: 16.10  2.HS: 11.12  Zw.Sem.: 19.02  Beginn SS: 14.04

4020235138 Neutrino physics and astrophysics (theory) (Zw.Sem.)      VVZ  

VL wöch. Walter Winter
UE wöch. Walter Winter

Präsenzkurs

Unterrichtssprache
EN
Lern- und Qualifikationsziele
Basic principles of theoretical neutrino physics and astrophysics with connection to current research. The teaching language will be English.
Voraussetzungen
Astroparticle physics (desirable), introduction to the Standard Model (recommended)
Gliederung / Themen / Inhalte
Neutrino oscillations
Solar neutrinos, MSW effect
Neutrino masses and mixings
Neutrinos meet the Standard Model
Multi-messenger astroparticle physics
Radiation models for astrophysical sources
Hadronic interactions in astrophysical sources
Baryogenesis/Leptogenesis
Zugeordnete Module
P25.1.a
Umfang, Studienpunkte; Modulabschlussprüfung / Leistungsnachweis
3 SWS, 6 SP/ECTS (Arbeitsanteil im Modul für diese Lehrveranstaltung, nicht verbindlich)
Oral examination, participation in tutorials (50% points), reading assignment with short presentation
Sonstiges
This lecture is planned as a joint teaching project with the University of Oxford, financially supported by the Oxford Berlin Research partnership. The actual lecture and tutorials will be delivered as block courses, one week in Oxford (March 18-22, 2024) and one week in Berlin (April 8-12, 2024), with assignments in between. Students from HUB are expected to travel to Oxford and live in a college in the first week, whereas students from Oxford visit us in the second week. For details and updates, see webpage.
Ansprechpartner
Walter Winter, 1'410 (HUB) 2R01 (DESY Zeuthen)
Literatur
M. S. Athar, ..., W. Winter, et al. Status and perspectives of neutrino physics. Prog. Part. Nucl. Phys. 124 (2022) 103947
Carlo Giunti and Chung Kim. Fundamental of neutrino physics and astrophysics. Oxford
Gaisser, Engel and Resconi. Cosmic rays and particle physics. Cambridge
Siehe auch:
http://www.zeuthen.desy.de/~wwinter/Teach/Neutrinos/neutrinos24.html
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