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Nuclear Processes in the Space - NJSF112

Title:	Jaderné procesy ve vesmíru
Guaranteed by:	Institute of Particle and Nuclear Physics (32-UCJF)
Faculty:	Faculty of Mathematics and Physics
Actual:	from 2022
Semester:	winter
E-Credits:	3
Hours per week, examination:	winter s.:2/0, Ex [HT]
Capacity:	unlimited
Min. number of students:	unlimited
4EU+:	no
Virtual mobility / capacity:	no
State of the course:	not taught
Language:	Czech
Teaching methods:	full-time
Teaching methods:	full-time
Additional information:	http://www-ucjf.troja.mff.cuni.cz/~nosek/Nosek_NPU.html

Guarantor:	doc. RNDr. Dalibor Nosek, Dr.

Opinion survey results Examination dates Schedule Noticeboard

Annotation -

Last update: doc. RNDr. Dalibor Nosek, Dr. (22.04.2013)

Nuclear processes in the Universe and stars. Composition of the Universe, relic radiation, dark matter, dark energy. Friedmann evolution of the Universe. Observational Cosmology. The thermal history of the Universe, primordial nucleosynthesis and neutrinos, wimps, baryogenesis. Particle physics in stars and galaxies.

Course completion requirements - Czech

Last update: doc. RNDr. Dalibor Nosek, Dr. (10.06.2019)

Ústní zkouška

Literature -

Last update: doc. RNDr. Dalibor Nosek, Dr. (22.04.2013)

J.Rich: Fundamentals of Cosmology, Springer-Verlag Berlin Heidelberg 2001, Kapitoly 1,2,5,6.

D.H.Perkins, Particle Astrophysics, Oxford University Press, 2003.

G.Börner, The Early Universe, Springer-Verlag, 1988

Requirements to the exam - Czech

Last update: doc. RNDr. Dalibor Nosek, Dr. (12.10.2017)

Ústní zkouška a diskuze nad domácími úkoly.

Syllabus -

Last update: doc. RNDr. Dalibor Nosek, Dr. (31.05.2013)

1. Basic ideas on Universe development.

2. Composition of the Universe, dark matter, dark energy.

3. Thermodynamics of the early Universe - radiation and matter epoch. Relic radiation. Primordial nucleosynthesis. Synthesis of heavy elements.

4. Problems of the Friedmann Universe. Inflation.

5. Nuclear processes in stars. Thermodynamics of self-gravitating objects. Supernova explosions. Neutron star formation and evolution. Supernova neutrinos.