Mandel's Q parameter for squeezed number and coherent squeezed number inflaton states in a flat FRW universe is found to be positive, which the paper interprets as super-Poissonian nonclassical behavior.
Density fluctuations for Squeezed Number State and Coherent Squeezed Number State in Flat FRW Universe
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abstract
We study the density fluctuations for Coherent Squeezed Number State (CSNS) and Squeezed Number States (SNS) formalism in Semiclassical theory of grav ity in flat FRW universe. We used Number state evolution of oscillatory phase of inflaton for coherent squeezed number state and squeezed number states for malisms. We analyzed that density fluctuations for SNS depends upon squeezing parameter and number state while for CSNS density fluctuations depends upon squeezing parameter, number state and coherent state parameter. These param eters plays an important role for quantum consideration of SNS and CSNS. The results of the analysis shows that increase in density fluctuations for both SNS and CSNS, demonstrate quantum behavior of SCEE as well as production of various kind of particles in these states.
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Investigation of Super-Poissonian Nonclassical Nature of Inflaton Field in Flat FRW Universe through Cosmological Mandels $Q$ Parameter
Mandel's Q parameter for squeezed number and coherent squeezed number inflaton states in a flat FRW universe is found to be positive, which the paper interprets as super-Poissonian nonclassical behavior.