We currently have a coherent model that tracks the growth of subtle density fluctuations laid down in the early universe to the present richness of the night sky 現(xiàn)在我們擁有一致的理論模型,能夠描述早期宇宙密度的細(xì)微起伏,一路上是如何成長,而成為現(xiàn)在夜空中的豐富結(jié)構(gòu)。
We employ largest lyapunov exponent to explore the relation between the chaos and phase transition . then , we study the mechanic ( spinodal ) instability of these nuclear systems with the density fluctuation 我們通過改變基態(tài)核的溫度(激發(fā)能) ,來研究核體系隨溫度(激發(fā)能)的改變而發(fā)生的相變。
And the incompressible navier - stokes equations are exactly derived from this incompressible lbgk model , thus the compressible effect due to the density fluctuation is theoretically eliminated 其中密度保持為常數(shù),使得從格子bgk方程能夠?qū)С龊暧^不可壓ns方程,理論上消除了因密度變化導(dǎo)致的壓縮誤差。
Cosmologists assume that our universe , with an almost uniform distribution of matter and initial density fluctuations of one part in 100 , 000 , is a fairly typical one ( at least among those that contain observers ) 宇宙學(xué)家假設(shè),我們的宇宙是一個相當(dāng)?shù)湫偷挠钪?,具有幾乎均勻的物質(zhì)分布,與十萬分之一的初始密度漲落。
Making use of the wigner transform of the one - body density matrix , the coherent density fluctuation model ( cdfm ) is introduced into semiclassical distorted wave ( scdw ) model . the new model is applied to the analyses of multistep direct processes of ( p , p ' x ) reactions to continuum 本文利用單體密度矩陣的wigner變換,將相干密度漲落模型( cdfm )引入半經(jīng)典扭曲波( scdw )模型,并將新的scdw模型應(yīng)用于分析預(yù)平衡反應(yīng)( p , p ' x )中散射到連續(xù)態(tài)的多步直接過程。