May 13, 2024
3 minute read
Nuclear fusion is the process of combining two or more atomic nuclei to form a single, heavier nucleus. This process releases a great amount of energy, which can be used to generate electricity. Nuclear fusion is the process that powers the sun and other stars.
How Does Nuclear Fusion Work?
Nuclear fusion occurs when two atomic nuclei are brought close enough together to overcome the electrostatic repulsion between them. This requires a great deal of energy, but once the nuclei are close enough together, they can fuse to form a single, heavier nucleus. The mass of the new nucleus is less than the mass of the two original nuclei, and the difference in mass is released as energy.
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Find a path to becoming a Nuclear Fusion. Learn more at:
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Reading list
We've selected 11 books
that we think will supplement your
learning. Use these to
develop background knowledge, enrich your coursework, and gain a
deeper understanding of the topics covered in
Nuclear Fusion.
Provides a comprehensive and advanced treatment of plasma physics and fusion energy. It is suitable for graduate students and researchers in the field.
Covers both plasma physics and inertial confinement fusion. It is suitable for advanced undergraduates and graduate students in relevant fields, as well as researchers and industry professionals.
Provides a non-technical overview of nuclear fusion and its potential as a source of energy. Bodansky leading expert in nuclear fusion history and policy.
Provides a comprehensive overview of plasma theory and applications. It is suitable for advanced undergraduates, graduate students, and researchers in the field.
Provides a comprehensive overview of plasma physics, which is essential for understanding nuclear fusion. Bittencourt leading expert in plasma physics and has written extensively on the subject.
Provides an accessible and comprehensive overview of nuclear fusion, covering the basic principles and the latest developments in the field. Fitzpatrick leading expert in nuclear fusion and has written extensively on the subject.
Provides a comprehensive overview of the principles of stellar evolution and nucleosynthesis, including the role of nuclear fusion in the formation of heavy elements.
Provides an overview of the physics of the Sun, including nuclear fusion reactions that power the Sun. Prialnik leading expert in solar physics and has written extensively on the subject.
Provides a comprehensive overview of the fundamental concepts of high energy physics, including nuclear fusion reactions.
Provides an overview of the fundamental concepts of astrophysical fluid dynamics, including the role of nuclear fusion in the evolution of stars.
Includes a chapter on nuclear fusion (chapter 10) that provides a good introduction to the topic, suitable for undergraduate students. The book is written clearly and concisely and is well-suited for self-study.
For more information about how these books relate to this course, visit:
OpenCourser.com/topic/raifwp/nuclear
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