首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >DENSITY FLUCTUATIONS IN THE OSCILLATORY PHASE OF A NONCLASSICAL INFLATON IN THE FRW UNIVERSE
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DENSITY FLUCTUATIONS IN THE OSCILLATORY PHASE OF A NONCLASSICAL INFLATON IN THE FRW UNIVERSE

机译:FRW宇宙中非经典浮子振荡阶段的密度波动

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摘要

The use of the coherent and squeezed state formalisms of quantum optics for a minimally coupled nonclassical inflation in the FRW metric is studied, in the semiclassical theory of gravity. The leading order solutions to the semiclassical Einstein equations in the coherent, squeezed and squeezed vacuum states are obtained perturbatively and exhibit power law expansion behavior. The validity of the semiclassical theory is examined in the squeezed vacuum state in the oscillatory phase of the inflaton. The semiclassical theory in the oscillatory phase of the nonclassical inflaton holds only if the associated squeezing parameter is much smaller than unity. Quantum fluctuations of the inflaton are also examined in the coherent and squeezed state formalisms.
机译:在重力的半经典理论中,研究了量子光学的相干态和压缩态形式论在FRW度量中用于最小耦合非经典膨胀的研究。相干,压缩和压缩真空状态下的半经典爱因斯坦方程的前导解是扰动地获得的,并表现出幂律展开行为。在充气子振荡阶段的压缩真空状态下检验了半经典理论的有效性。仅当相关的压缩参数远小于1时,非经典充气的振荡阶段中的半经典理论才成立。在连贯和压缩的状态形式主义中,还检查了充气子的量子涨落。

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