坍縮 的英文怎麼說

中文拼音 [tānsuō]
坍縮 英文
collapse; pinch; flow down
  • 坍 : 動詞（倒塌） collapse; fall; tumble; crumble down
  • 縮 : 縮構詞成分。
  1. During collapse, the dark cloud "fragments" into a series of dense clumps.

    在坍縮過程中，暗雲「碎裂」為一批稠密的團塊。
  2. All black holes are formed from the gravitational collapse of a star, usually having a great, massive, core

    所有的黑洞都是因為恆星的引力坍縮而形成，這種恆星通常有一顆巨大而厚重的核心。
  3. A quantitative analysis of this idea led to the prediction that a star remaining about three times the mass of the sun at the end of its evolution ( usually as a neutron star ), will almost inevitably shrink to the critical size needed to undergo a gravitational collapse

    該想法的定量分析導致預言一顆恆星在終止它演化時候保持大約三倍太陽的質量（通常看做一顆中子星） ，將會幾乎不可避免收縮到臨界體積必須遭受引力坍塌。
  4. After the initial collapse and hydrodynamic phases, a young stellar object is still embedded deep within its progenitor.

    在初始坍縮和流體力學階段之後，一個年青星體仍然深深嵌在產生它的母體之中。
  5. Collapsing interstellar cloud reverses its gravitational infall and expands outward into the relatively quiescent interstellar environment.

    坍縮的星際雲克服向內的引力而向外膨脹到較寧靜的星際環境中去。
  6. The addition of matter over this critical value would lead to the collapse of the star without limit because of the ever-increasing gravitational forces.

    質量超過臨界值時，增加著的引力將造成恆星的無限坍縮。
  7. Two-and three-dimensional hydrodynamic computer codes have been applied to the study of the early phases of the collapse of a gas cloud.

    二維和三維流體力學計算機程序，已用於研究氣體雲的早期坍縮。
  8. Progressively, larger objects substantially increase the timescale for collapse over still longer wavelengths.

    進而言之，較大的天體，因要在更長的波長上坍縮，將大大增長時間尺度。
  9. Collapsed parenchymatous cell

    坍縮柔組織細胞
  10. A burnedout star could collapse to so small a radius as to make the effects of general relativity quite important near its surface.

    一個燃燒完的星球可能坍縮到如此之小的半徑，以致在其表面附近，廣義相對論效應相當重要。
  11. The collapse of the protostella is extremely non-homologous.

    原恆星雲的坍縮是極其不保形的。
  12. As soon as this occurred, the giant gas ball collapsed rapidly.

    一旦出現這種情況，這個龐大的氣體球便迅速坍縮。
  13. A star is formed when a cloud of gas collapses from the interstellar medium toward high density.

    一個氣體雲自星際物質中坍縮，密度達到很高時，即形成了一個恆星。
  14. The evolution of fixed star having something to do with nuclear reaction, the star generally loses partial mass in its final period and finally collapses into compact star ( white dwarf, neutron star or black hole )

    恆星的演化與核反應有關，演化到晚期的恆星一般要損失一部分質量，然後坍縮成緻密星（白矮星、中子星或黑洞） 。
  15. Colliding black holes, collapsing stars, and spinning compact celestial objects such as pulsars create ripples in the fabric of space and time that subtly distort the world around us

    黑洞碰撞、恆星坍縮以及自旋脈沖星所激起的時空結構波動，微妙的扭曲了我們周圍的世界。
  16. If the universe is closed, omega is greater than unity, and the universe will eventually stop its expansion and recollapse back upon itself

    如果宇宙是封閉的，歐米加大於平均數，而且宇宙最終會停止它的膨脹及重新往回坍縮自己。
  17. And we conswt the mp cormbon prowties of several oboles of two quhas pare pe nd produced ty dfor collape under the m conditions. bed on the logic ta of harde wi we hav proved. by mere conche tabo focal hidden vahables thcory cannt give the same ed as tbe - - inecws does

    運用cabello的邏輯方法論證兩個自旋1 2粒子系統的非定域關聯性質，考察了不同情況下兩個量子位純態的不同態坍縮效應所導致的各個可觀測量之間的量子關聯幾率。
  18. Post - core - collapse cluster

    核心坍縮后星團
  19. After the process of matter ejection stellar body will continue collapsing into black hole if the mass of the nuclear - energy - exhausted star is more than 3 mq

    星體經過物質拋射后，核能耗盡的恆星質量超過3m _ ，則此星體將繼續坍縮成黑洞。
  20. Fourthlk using the wtmechimow inequality we investigated the classhal cormbon and quantuin correlaion of two classes of pely pe entangleineni : ghz stat and w the, dri are - - nt under local o ~ ns and classhal commforations ( locc ). we calculated the wt cormlation probabtheies of two states in the way agdri some hare [ 681

    用clauser - horne - shimony - holt不等式我們考察了兩種三體量子位糾纏態： ghz態和w態在不同的態坍縮條件下經典關聯和量子關聯性質，用不同於文獻[ 68 ] ，但更細致的方法計算了態關聯幾率及構成的chsh不等式。
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