平坦 FRW 宇宙相干挤压真空状态下非经典膨胀子的粒子生成与密度波动

Dhwani Gangal, Sudhava Yadav, K. K. Venkataratnam
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引用次数: 0

摘要

我们研究了在相干挤压真空态(CSVS)中的 FRW 宇宙中与这些半经典引力最小耦合的非经典流入子。我们确定了流入子的振荡相位、幂律膨胀、尺度因子、密度波动、量子波动和 CSVS 中粒子的产生。我们得到了 CSVS 中尺度因子与 t^{2/3}$ 成比例的估计领先解,它遵循物质主导宇宙中引力的半经典爱因斯坦方程(SCEE)所证明的类似多样化。我们还研究了 SCEE 在 CSVS 中的有效性。通过确定 CSVS 的量子波动,还计算了 FRW 宇宙不确定性关系的有效性。结果表明,量子波动并不依赖于相干参数$Upsilon$,因为不确定性关系并不受相空间中$Upsilon$位移的影响。我们研究了在平坦的 FRW 宇宙中,振荡的大质量膨胀子在 CSVS 中产生粒子的情况。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Particle Production and Density Fluctuations of Non-classical Inflaton in Coherent Squeezed Vacuum State of Flat FRW Universe
We study non-classical inflaton, which is minimally coupled to the semiclassical gravity in FRW universe in Coherent Squeezed Vacuum State (CSVS). We determined Oscillatory phase of inflaton, power-law expansion, scale factor, density fluctuations, quantum fluctuations and particle production for CSVS. We obtained an estimated leading solution of scale factor in CSVS proportional to $t^{2/3}$ follow similar diversification as demonstrated by Semiclassical Einstein Equation (SCEE) of gravity in matter dominated universe. We also studied the validity of SCEE in CSVS. By determining the quantum fluctuation for CSVS validity of uncertainty relation for FRW Universe also computed. The results shows that Quantum fluctuations doesn't depend on coherent parameter $\Upsilon$ as uncertainty relation doesn't effected by the displacement of $\Upsilon$ in phase space. We study the production of particles in CSVS for oscillating massive inflaton in flat FRW universe.
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