史瓦西解 的英文怎麼說
中文拼音 [shǐwǎxījiě]
史瓦西解
英文
schwarzschild metric-
The meso - cenozoic evolution of bachu fault - uplift is closely related to its south and north subsiding foredeep. under the background of indian plate subducting under asia - europe plate, bachu forebulge was greatly affected by the development of southwest depression and awati depression. almost all of its structure reversed, and as a result of it, both of its south and north boundary migrated. according to its evolution history and its feature, the authors tentatively use both - side migration model to interpret the evolution of compound forebulge. since triassic, almost all the spheres above lithosphere synchronously became flexure. because transpressional stress field became increasingly strong, bachu forebulge continued uplifting and big faults formed. then, bachu uplift, as a whole, slipped upward along those big faults and showed migrating toward thrust zone in plane. in tectonic tranquility, the lithosphere bounded back and in consequence of it, bachu uplift slipped down and showed migration toward craton, at that moment negative inversion structures developed. while the forebulge migrated toward its south and north foredeep, it was very possible that locally extensional stress appeared in the forebulge
在印度板塊向歐亞板塊俯沖的大背景下，巴楚前緣斷隆受西南坳陷和阿瓦提凹陷的影響，新生代時構造體制發生反轉，邊界向南北遷移。根據其發育過程特徵，作者用復合前緣隆起兩端遷移模式對復合前緣隆起獨特的構造發育史進行了解釋：即三疊紀以來巖石圈各圈層同步撓曲變形。隨著擠壓應力場的增大，巴楚隆起在撓曲基礎上不斷抬升，形成幾條大型斷裂帶。A few months later, karl schwarzschild gave the solution for the gravitational field of a point mass, showing that something we now call a black hole could theoretically exist
幾個月之後，卡爾?史瓦西給出了點質量引力場解決方法，表明我們現在稱做黑洞某物理論上可以存在。Soon after einstein published his general theory of relativity in the beginning of 20th century, karl schwarzschild found a mathematical solution of the theory to describe the spacetime structure of such object with spherical symmetry. that was the prelude to the study of black holes
愛因斯坦在二十世紀初發表了廣義相對論后不久，史瓦西便利用廣義相對論方程求得一個描述球對稱天體附近時空結構的解，為黑洞的研究展開了序幕。The schwarzschild solution 1916
史瓦西解The schwarzschild radius is now known to be the radius of a non - rotating black hole, but was not well understood at that time
史瓦西半徑就是現在知道的非旋轉黑洞半徑，但是在那時不是很好理解。分享友人