中子星 的英文怎麼說

中文拼音 [zhōngzixīng]
中子星 英文
netutron star
  • 子 : 子Ⅰ名詞1 （兒子） son 2 （人的通稱） person 3 （古代特指有學問的男人） ancient title of respect f...
  • 星 : 名詞1 （夜晚天空中閃爍發光的天體） star 2 [天文學] （宇宙間能發射光或反射光的天體） heavenly body...
  1. The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.

    在中子星或黑洞伴星上發生吸積的模型，仍應看成是一個有價值的假說。
  2. In the april 14 physical review letters, investigators at the university of basel in switzerland and their colleagues suggest antineutrinos streaming in huge numbers from the neutron star could irradiate the protons and turn some into neutrons, which build stable, heavy isotopes

    在4月14日的《物理評論通訊》中，瑞士巴塞爾大學的研究人員與合作伴提出，從中子星大量湧出的反微中子會照射質子，並使部份質子轉變為中子，以形成穩定的重同位素。
  3. The results show that the chiral symmetry is restored partially when the strange matter density increases and 2 plays a very important role in the strange matter which may approach the constituents of the neutron stars. in additions, we can find that the strange matter density where the - condensate emerges is led to the ratio of the nucleon number to baryon number. and the occurrence of - condensate is only in certain density and gradually increases for higher density, so we guess that - field may be necessary to carefully consider for studying the neutron stars

    （ 3 ） -凝聚出現時所對應的奇異物質密度值與核子在奇異物質中的比例有關。另外，雖然本文對夸克凝聚的討論是在低密度的奇異物質中進行的，但是-凝聚的出現卻需達到一定的密度值並且隨密度的增大而遞增，所以我們推測場可能對于仔細研究中子星是一必要因素。
  4. This requires even more detectors because these waves are even weaker than the waves from binary stars and neutron stars

    這將需要更多的探測器，因為與雙星和中子星產生的引力波相比，這些引力波還要更弱。
  5. There is a positive observational and theoretical basis for believing that neutron stars and black holes follow as a result of supernovae.

    中子星和黑洞則是超新星的產物，觀測上和理論上的依據使我們相信這一點。
  6. Does a neutron star represent the ultimate in compression ?

    中子星是壓縮的最終產物嗎？
  7. Neutron stars are the second exhibit in the gallery of stellar corpses.

    中子星是死之恆星陳列館內第二類樣品。
  8. In the first seconds after a supernova, a region rich in protons emerges around the dead star ' s core, which has most likely collapsed into a neutron star

    在發生超新星爆炸后的最初幾秒內，這個死亡恆星的核心（最可能塌縮形成中子星的地方）周圍，會產生一個富含質子的區域。
  9. X - ray flashes had previously been detected from some neutron stars, but they never exceeded the eddington limit by very much

    以往天文學家就曾觀測到過從中子星發出來的x射線閃光，但其亮度從來不會超過艾丁頓上限太多。
  10. For example, if there is a planet orbiting around the neutron star, it will wobble a little and the pulses will come a little early or late. we can then deduce the mass and the radius of the orbit of the planet from the arrival time of the pulses. this is how the first extrasolar planet is discovered

    例如假若有一顆行星圍繞一顆中子星運行，它會令中子星出現搖動，引致脈沖的間隔變長或短，由此我們根據脈沖周期的變化，可推斷出行星的質量和軌道半徑，這亦是天文學家找出第一顆地外行星時所用的方法。
  11. 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。
  12. The strong gravitational field of a neutron star provides the answer

    中子星的超強引力提供了最佳的解答。
  13. The results show that - condensate appears at some baryon densities and makes great effect to the curve of state equation of neutron star ; hyperons - and a exist in neutron star matter at high desities

    結果表明， ~ -凝聚將出現在一定的重子密度區間，並對中子星狀態方程曲線有重要的影響；超子~ -和在較高密度也會出現。
  14. In this model, the resulting implosion and ensuing explosion would blow off the outer envelope of the star and leave behind the core as a neutron star.

    按此模型，引起的突然壓縮和隨后的爆發會把恆量的外部包層吹跑，留下的核成為一顆中子星。
  15. But only a handful of neutron stars are paired up with other neutron stars that are close enough to show the indirect evidence of gravitational waves

    但是只有少量的中子星是和其它中子星靠得足夠近並顯示出引力波存在的證據。
  16. Finally, due to the rapid rotation of the neutron star, or the evolution of the companion, the infall of matter stops, the x - ray emission declines, and the neutron star emerges as a radio - emitting millisecond pulsar

    最後，由於中子星疾速的自轉，或是伴星自身的演化，物質的流入停止， x射線輻射減弱，這顆中子星就呈現出了毫秒脈沖星的面目。
  17. When electrons move in spirals around magnetic lines of force, radio waves are produced and radiated out along the two magnetic poles of the star. usually, the rotational axis of the neutron star does not align with the magnetic axis. the radiation beams will sweep around and create the

    通常恆星的自轉軸和磁軸並不一致，中子星亦不例外，所以沿著磁軸向外發射的無線電波束，在中子星自轉的帶動下，便會如燈塔般向宇宙掃射，這便是著名的
  18. Are some known neutron stars actually strange stars

    一些已知的中子星會否就是奇異星？
  19. Study of the gravitational energy in neutron stars

    中子星內引力能的研究
  20. Structure of a pulsar ? a rotating magnetic neutron star

    脈沖星的結構。一顆旋轉磁中子星。
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