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Quantum Black Holes

Chapter
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Part of the NATO ASI Series book series (volume 150)

Summary

The conventional way to set up a decent looking theory for interacting elementary particles is to take some set of classical fields, satisfying simple, polynomial field equations. These equations should be compatible with an extremum principle: they are taken to be the Euler-Lagrange equations generated by some Lagrange function L of the fields. One then “quantizes” the theory by replacing Poisson brackets by commutators.

Keywords

Black Hole Radiation Temperature High Order Interaction Extremum Principle Quantum Black Hole 
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

© Plenum Press, New York 1987

Authors and Affiliations

  1. 1.Institute for Theoretical PhysicsUtrechtThe Netherlands

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