Squeezed states, time-energy uncertainty relation, and Feynman's rest of the universe

Details Squeezed states, time-energy uncertainty relation, and Feynman's rest of the universe Squeezed states, time-energy uncertainty relation, and Feynman's rest of the universe

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ssur.work..269h&link_type=abstract

In its Workshop on Squeezed States and Uncertainty Relations p 269-282 (SEE N92-22045 12-74)

Statistics

Covariance, Hadrons, Oscillators, Quantum Statistics, Quark Models, Quarks, Relativistic Particles, Squeezed States (Quantum Theory), Universe, Entropy, Lorentz Transformations, Partons, Symmetry, Wave Functions

Scientific paper

Two illustrative examples are given for Feynman's rest of the universe. The first example is the two-mode squeezed state of light where no measurement is taken for one of the modes. The second example is the relativistic quark model where no measurement is possible for the time-like separation fo quarks confined in a hadron. It is possible to illustrate these examples using the covariant oscillator formalism. It is shown that the lack of symmetry between the position-momentum and time-energy uncertainty relations leads to an increase in entropy when the system is different Lorentz frames.

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