暴漲宇宙 的英文怎麼說

中文拼音 [bàozhǎngyǔzhòu]
暴漲宇宙 英文
inflationary universe
  • 暴 : Ⅰ形容詞1 （突然而且猛烈） sudden and violent 2 （兇狠; 殘酷） harsh and tyrannical; cruel; fierce...
  • 漲 : 漲動詞1 （體積增大） swell up 2 （充血） （of the head） be swelled by a rush of blood 3 （多出; ...
  • 宇 : 名詞1. （房檐） eaves2. （房屋） house 3. （上下四方, 所有的空間; 世界） space; universe; world 4. （姓氏） a surname
  • 宙 : 名詞（指古往今來的時間） time （conceived as past, present and future）
  • 暴漲 : rise suddenly and sharply; boom
  • 宇宙 : [天文學] universe; cosmos
  1. Firstly, in order to make a theoretical preparation for tachyon cosmology and d - star, we briefly review the standard hot big bang cosmology with inflation

    在這個模型中，快子場作為暴漲場，即由born - infeld標量場導致宇宙暴漲。
  2. Then, based on above review, we propose an analytical tachyon inflation model driven by scalar field with bom - infeld - type lagrangian. we find it ' s an analytical model if we choose an exponential potential. we compute it ' s power spectrum and find that it can explain the evolution of universe

    如果將勢選擇為指數勢，模型變成精確可解的，本文找到了一個精確解析的宇宙暴漲解並利用該解計算了cmb譜，發現這個解可以用來解釋宇宙的演化。
  3. In this master dissertation, under the fundamental frame of general relativity, we study the tachyon inflation, d - stars in the spacetime with a nonzero cosmological constant and it ' s observable effects by using some modern mathematical methods such as differential equation and qualitative analysis

    本文以廣義相對論作為基本理論框架，使用微分方程及其定性理論，研究了宇宙演化和結構中的兩個問題，其中包括了快子暴漲，非零宇宙常數時空中的d星以及它的種種可觀測效應。
  4. The thesis gives the background acknowledges and the developing procedure of the cosmological theory, summarizes the viewpoints in the standard cosmological model and the confirmations from observing experiments. and the thesis sums the problems in the standard cosmological model and the inflation theory that can solve these problems. the thesis also discusses the origin of the universe and the theory of quantum cosmology

    =本文綜述了宇宙學的提出過程及其背景知識，概述了目前的主要的宇宙學模型? ?標準宇宙學模型的主要觀點和觀測證據，並總結了標準宇宙學模型中存在問題及為解決這些問題而提出的暴漲宇宙學理論。
  5. We find that the cosmic scale factor has the form of exponent inflation if the cosmological constant contributes to the positive material density, and the factor is composite function of cosine if the cosmological constant contributes to the negative material, furthermore, we gain the new formality of the pressure and the temperature in the procedure of cosmological evolution

    首次發現當宇宙學常數對物質密度的貢獻大於零時有指數復合函數的型得一般暴漲，當宇宙學常數對密度的貢獻小於零時宇宙有餘弦形式的演化。通過對宇宙中壓強和溫度的計算，得到新的壓強表達式和暴漲宇宙模型中溫度隨時間演化的表達式。
  6. The exact solution of the einstein field equation is gained under the popular conditions when ， the new general expression of the density function is deduced. ， the new solution of the cosmic scale factor is further derived out under different evolution model

    求解了當時一般情況下標準宇宙模型方程，通過一般地求解不同密度物質情況下的暴漲宇宙演化方程，得到了的一般物質密度的表達式，解出了表徵宇宙標度因子不同演化的一般新解，並通過對不同情況下標準宇宙方程的求解，證明參數的正負取值直接影響宇宙尺度因子的表達形式。
  7. Much of his work bears on the concept of parallel universes : evaluating evidence for infinite space and cosmological inflation ; developing insights into quantum decoherence ; and studying the possibility that the amplitude of microwave background fluctuations, the dimensionality of spacetime and the fundamental laws of physics can vary from place to place

    許多他的工作都含有平行宇宙的概念：評估無限大空間與宇宙暴脹的證據，發展對量子去相干現象的洞察，以及研究諸如微波背景輻射漲落的振幅、時空的維度以及物理的基本定律可隨位置而變化的可能性。
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