1990
DOI: 10.1016/0375-9601(90)90684-g
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Lorentz-squeezed hadrons and hadronic temperature

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Cited by 25 publications
(22 citation statements)
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“…There are also models of current interest in which one of the variables is not observed, including thermo-field dynamics [23], two-mode squeezed states [11,12], the hadronic temperature [24], and entropy increase caused by Lorentz boosts [25], and the Barnet-Phoenix version of information theory [26]. They are indeed the examples of Feynman's rest of universe.…”
Section: Physical Modelsmentioning
confidence: 99%
“…There are also models of current interest in which one of the variables is not observed, including thermo-field dynamics [23], two-mode squeezed states [11,12], the hadronic temperature [24], and entropy increase caused by Lorentz boosts [25], and the Barnet-Phoenix version of information theory [26]. They are indeed the examples of Feynman's rest of universe.…”
Section: Physical Modelsmentioning
confidence: 99%
“…In the meantime, let us study what happens when the matrix G 3 is introduced into the set of matrices given in Eq. (20) and Eq. (21).…”
Section: Non-canonical Transformations In Classical Mechanicsmentioning
confidence: 99%
“…This Wigner function is of the form given in Eq. (32) for the thermal excitation, if we identify the squeeze parameter η as [20] cosh(2η) = 1 tanh(1/2T ) .…”
Section: Canonical Approachmentioning
confidence: 99%
“…The width of the distribution becomes √ cosh η, and becomes wide-spread as the hadronic speed increases. Likewise, the momentum distribution becomes wide-spread [5,29]. This simultaneous increase in the momentum and position distribution widths is called the parton phenomenon in high-energy physics [13,14].…”
Section: Time-separation Variable In Feynman's Rest Of the Universementioning
confidence: 99%
“…Likewise, the momentum distribution becomes wide-spread [5,29]. This simultaneous increase in the momentum and position distribution widths is called the parton phenomenon in high-energy physics [13,14].…”
Section: Time-separation Variable In Feynman's Rest Of the Universementioning
confidence: 99%