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Saha Ionization Equation
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High Quality Content by WIKIPEDIA articles! The Saha ionization equation, also known as the Saha-Langmuir equation, was developed by the famous Indian astrophysicist Megh Nad Saha in 1920, and later (1923) by Irving Langmuir. One of the important applications of the equation was in explaining the spectral classification of stars. The equation is a result of combining ideas of quantum mechanics and statistical mechanics. For a gas at a high enough temperature, the thermal collisions of the atoms will ionize some of the atoms. One or more of the electrons that are normally bound to the atom in orbits around the atomic nucleus will be ejected from the atom and will form an electron gas that co-exists with the gas of atomic ions and neutral atoms. This state of matter is called a plasma.
Weitere Informationen
- Allgemeine Informationen
- GTIN 09786131431593
- Editor Lambert M. Surhone, Mariam T. Tennoe, Susan F. Henssonow
- Genre Physik & Astronomie
- EAN 9786131431593
- Titel Saha Ionization Equation
- Herausgeber Betascript Publishing
- Anzahl Seiten 100
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