球對稱的 的英文怎麼說
中文拼音 [qiúduìchènde]
球對稱的
英文
spherically symmetric-
A central force is one derived from a potential-energy function that is spherically symmetric.
中心力是由球對稱的勢能函數而來的力。Planck absolue entropy of charged evaporative black hole with general spherical symmetry
廣義球對稱帶電蒸發黑洞的普朗克絕對熵Einstein s original cosmological model, introduced by him in 1917, was a static, homogeneous model with spherical geometry
愛恩斯坦在1917年發表的宇宙模型是一個靜態均勻及具有球狀對稱的宇宙。In addition, it was the sign of the initial amplitude growth rate, not the manner of the interface motion that determined whether the amplitude could increase. at weakly nonlinear stage, mode - coupling equations were derived in cylindrical and spherical geometries. it showed that the nonlinear terms were inversely proportional to the position of the interface in cylindrical and spherical geometries
在弱非線性階段,推導了柱和球幾何中模耦合方程,結果表明:非線性作用項反比于界面的位置,界面的位置越小,非線性作用越強,反之越弱;同時柱幾何中模耦合方程的解表明,在收縮幾何中,擾動在界面兩側的發展是不對稱的,在弱非線性階段,不穩定性向內發展的部分受到慣性力的擠壓,而向外發展的部分受到慣性力的拉伸。Hence a full subshell has zero angular momentum and is spherically symmetric.
於是,一個已經填滿的支殼層的角動量為零,並且是球面對稱的。Three non - spherical symmetry dibaryon chiral soliton in skyrme model
模型的3個非球對稱雙重子手征孤子Entropy of a general spherically symmetric and charged evaporating black hole
一般球對稱帶電蒸發黑洞的熵The statistical entropy of spherically symmetric evaporating black hole with charge
帶電球對稱蒸發黑洞的統計熵On the basis of that, according to basic theory of spherical symmetry grin optics and the rigorous computation of light tracking, its effect on retro - reflection was estimated. finally, by optimized computation the best technical parameters were obtained and the direction of improve its retro - reflection effect was determined
在此基礎上,根據球對稱梯度折射率光學的基本理論和光線追跡的嚴格計算,估算了用其製作回歸反射材料能夠達到的性能指標,並通過優化計算尋找到最佳技術參數,為提高回歸反射材料的性能指明了方向。The main origin of the perpendicular magnetic anisotropy in tbco amorphous films is the static interaction between the aspheric distribution charges of non - s tb ions and the aberrant crystal field produced in sputtering and deposition process. the magnetic dipole interaction is in a secondary cause
對于tbco非晶垂直磁化膜而言,具有非球對稱電荷分佈的非s態離子tb與濺射沉積薄膜過程中產生的畸變晶格場之間的靜電相互作用構成了tbco非晶薄膜垂直磁各向異性的主要部分, tbco薄膜內的磁偶極相互作用構成了其次要部分。In chapter 4, the influences of the earth ' s models on the elastic green ' s function, as well as on the atmospheric loading effects, are discussed using the numerical techniques. the attraction green ' s function is solved out based on the state equations of the ideal gas and the hydrostatic equilibrium equation. the influences of various factors upon the gravity and tilt green ' s functions, as well as upon the gravity and tilt, are considered in detail
第四章:採用數值計算方法,研究了地球模型對彈性項格林函數及其對大氣負荷響應的影響;利用理想氣體方程和流體靜力學平衡方程解算了吸引項格林函數,討論各種因素對大氣重力和傾斜格林函數及其對重力和傾斜的影響;基於球對稱地球模型,給出了武昌站臺站依賴的大氣重力、傾斜格林函數For some non - symmetric homogeneous domains, we can also get the explicit formulas of their bergman kernel functions by hua method [ xu4 ] [ gi ]. we know the complete orthonormal system of the bounded reinhardt domain made up of monomials, and complex ellipsoid domain is the bounded reinhardt domain, so the explicit formulas of the bergman kernel functions are obtained by summing an infinite series in some cases ( called method of summing series )
對於一些非對稱的齊性域,也可以用華羅庚方法得到它們的bergman核函數的顯表達式我們知道,有界reinhardt域的完備標準正交系由單項式組成,而復橢球域是包含原點且以原點為中心的有界reinhardt域,於是可以通過無窮級數求和函數的方法,計算其bergman核函數的顯表達式,這種求bergman核函數的顯表達式的方法稱為級數法。Statistical entropy of spherically symmetric dilatonic black hole
球對稱膨脹黑洞的統計熵Entropy of a generalized non - stationary spherically symmetric black hole with charge
動態廣義球對稱含荷黑洞的統計熵( 3 ) the most principal factors that influence the supersonic atomization process include the flow ratio of the gas - liquid metal ( gmr ) value, the flow of atomizing of gas and the range of the inverse vortex taper. the more of the value of three factors, the more advantage they are for the atomization and the more fine the powders are. ( 4 ) the produced powders are the best in efficient atomization efficiency, particle diameter, particle shape and dispersion when the solder alloy is zhl63a, atomizing medium is n2, the protrusion h = 6. 0mm, atomizing gas pressure p = 100mpa, over - heat temperature t = 167 ( t = 350 )
研究結果表明: ( 1 )超音速霧化器的氣體流場在導液管下端形成一個倒渦流錐,在二維空間上呈軸對稱的雙峰分佈,負壓形成於這個倒渦流錐內; ( 2 )修正後的霧化氣體速度公式可以滿足超音速霧化的要求; ( 3 )影響超音速霧化工藝最根本的因素有氣液質量流率比( gmr )的大小、霧化氣體流量和倒渦流錐范圍,三個因素的值越大,對形成細粉越有利; ( 4 )在焊錫合金為zhl63a ,霧化介質微n _ 2 ,導液管突出高度取h = 6 . 0mm ,霧化氣體壓力取p = 1 . 0mpa ,合金過熱度取t = 167 ( t = 350 )時,所制得的粉末在有效霧化率、顆粒球形度、粒度及其離散度三個方面綜合性能最好。On the base of the character of hemisphere continuously vibrating, the method of actuation and measuring, the asymmetry compensating process and the measuring limit were studied, the control loop and the parameter design were introduced, which will be prepared for the future circuit design and the automobile security application
本論文主要是在半球連續振動特性的基礎上,對陀螺儀的驅動及感測方法、非軸對稱的補償方法及感測極限進行研究,並詳細介紹其控制迴路與其參數的設計,為以後電路設計和面向汽車安全的應用打下了堅實的理論基礎。The usga only requires that the golfball ' s dimple pattern be spherically symmetric
美國高爾夫球協會只要求高爾夫球酒窩式樣必須是球面對稱的。Quantum entropy of the general non - stationary black hole with charges
動態廣義球對稱含荷黑洞的量子熵A entire study of the spacetime metric and entropy of the system containing a blackhole
中心黑洞體系球對稱度規及熵的整體研究First, we concisely recall the formation and development of bose - einstein condensa - tion ' s theory and it ' s experimentation. secondly, we briefly intro - duce some properties of weakly interactive bose gases, and derive the nonlinear gross - pitaevskii equation that is the condensate macroscopic wave function ' s equation. thirdly, we give a exam - pie, an approximation analytical solution of the gross - pitaevskii equation in a spherical symmetric harmonic trap is derived by a perturbation theory approach, this solution is consistent with that numerically obtained
全文共分為四章:第一章首先簡要的介紹和回顧了玻色-愛因斯坦凝聚理論的產生和發展,以及其實驗研究的過程,然後著重介紹了弱相互作用的玻色氣體的一些性質,並推導出了凝聚體宏觀波函數滿足非線性的gp方程,還以球對稱的諧振子勢為例,用標準的微擾方法求出了定態的gp方程近似解,發現其與已知的數值結果符合得很好。分享友人