Lecture 1 - Historical Background, Observational Astronomy, Properties of Sun and of Stars
Lecture 2 - Properties of Galaxies and Universe
Lecture 3 - Background of elemental abundance curve
Lecture 4 - Evidences of Nucleosynthesis - I
Lecture 5 - Evidences of Nucleosynthesis - II
Lecture 6 - Evidences of Nucleosynthesis - III and Mass gaps
Lecture 7 - H-R Diagram
Lecture 8 - M-L relation, Hubble’s Law and Echo of Big Bang
Lecture 9 - Thermonuclear reactions and Reaction cross-section
Lecture 10 - Reaction rate
Lecture 11 - Reaction rate and Neutron induced reactions
Lecture 12 - Gamma induced reactions and Inverse reactions
Lecture 13 - Inverse reactions
Lecture 14 - Inverse reactions and Mean life time of a nuclei
Lecture 15 - Mean life time of a nuclei and Time dependent abundance evolution
Lecture 16 - Non-resonant charged particle induced reactions
Lecture 17 - Astrophysical S-factor and Non-resonant charged particle induced reactions
Lecture 18 - Gamow peak and Electron screening effect
Lecture 19 - Resonant reactions
Lecture 20 - Resonant reactions
Lecture 21 - Neutron induced non-resonant reactions
Lecture 22 - Burning stages of stars and Hydrogen burning
Lecture 23 - pp chain
Lecture 24 - pp chain and CN cycle
Lecture 25 - CNO cycle, Shell model and Gamma decay
Lecture 26 - Formation of 12C
Lecture 27 - Survival of 12C
Lecture 28 - Carbon, Neon, Oxygen and Silicon burning
Lecture 29 - Nucleosynthesis beyond Iron
Lecture 30 - s-, r- and p-process
Lecture 31 - Charged particle and Neutron beams
Lecture 32 - Accelerators and Targets
Lecture 33 - Backing materials and Target preparation
Lecture 34 - Contaminants and Radiation sources
Lecture 35 - Detectors - I
Lecture 36 - Detectors - II
Lecture 37 - Activity method
Lecture 38 - Kinematics - I
Lecture 39 - Kinematics - II
Lecture 40 - Time of flight method and Indirect methods
