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Quantum Processes in Astrophysics

  • Martin Harwit
Part of the Astronomy and Astrophysics Library book series (AAL)

Abstract

In Chapter 6, we considered the means by which particles could absorb or emit radiation. But we restricted ourselves to processes in which the Maxwell field equations of classical electrodynamics could be applied. These equations break down on the scale of atomic systems. The electron bound to a positively charged nucleus does not lose energy because of its accelerated motion, although the classical theory of radiation predicts that it should. Instead, the ground state of hydrogen, or any atom, is stable for an indefinitely long period. Moreover, when energy is actually radiated from excited states, and the atomic ground energy state is finally reached, we always find that only discrete amounts of energy have been given off in each transition. Again, this is at variance with classical predictions.

Keywords

Angular Momentum Absorption Cross Section Atomic System Equivalent Width Principal Quantum Number 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media New York 1998

Authors and Affiliations

  • Martin Harwit
    • 1
  1. 1.Department of Astronomy, Space Sciences BuildingCornell UniversityIthacaUSA

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