
Lecture Description
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- The CosmoLearning Team
- The CosmoLearning Team
Course Index
- Brief Overview of the Course
- Measurement of Nuclear Sizes
- Measurement of Nuclear Sizes II
- Measurement of Nuclear Sizes III
- Semi-empirical Mass Formula
- Semi-empirical Mass Formula II
- Semi-empirical Mass Formula III
- Semi-empirical Mass Formula IV
- Semi-empirical Mass Formula V
- How Neutron Stars Bound
- Deuteron
- Deuteron II
- Deuteron III
- Scattering of Nucleons
- Low Energy n-p Scattering
- Theories of Nuclear Forces
- Shell Model
- Shell Model II
- Shell Model III
- Shell Model IV
- Shell Model V
- Collective Models
- Vibrational and Rotational Levels
- Radioactivity, Alpha Decay
- Alpha Decay II
- Beta Decay
- Beta Decay II
- Beta Decay III
- Gamma Decay
- Nuclear Reactions
- Nuclear Reactions II
- Nuclear Reactions III
- Nuclear Fission Basics
- Nuclear Fission of Uranium
- Nuclear Fission Reactor
- Nuclear Energy Programme of India
- Nuclear Fusion
- Nuclear Fusion II
- Thermonuclear Fusion Reactors
- Fusion Reactions in Stars and Stellar Neutrinos
- Nucleosynthesis of Elements in Stars
- Mössbauer Spectroscopy
- RBS, PIXE, NAA, Summary of the Course
Course Description
This basic course on Nuclear physics will give an introductory but still rigorous description of both experimental and theoretical aspects of the present understanding of nuclei and their interaction. Nuclear Physics originated with Geiger and Marsden bombarding alpha particles on metal foils including gold, hundred years ago sometime in the year 1909. The hundred year journey of Nuclear physics has been very exciting, both in terms of developing experimental techniques to probe at the length scale of femtometers and also developing right kind of theoretical models to understand the vigorous activities going on inside a nucleus. On one side it interfaces with Atomic Physics and on the other side with Particle Physics. (Source: nptel.ac.in)
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