degenerate star 中文意思是什麼
degenerate star
解釋
簡並星- degenerate : vi 1 腐化，墮落，頹廢。2 衰敗；【生物學】退化 （to）；【生理】 變質。adj n 1 腐化的，墮落的，頹廢...
- star : n 1 星；【天文學】恆星 （opp planet）。2 星狀物，星（形勛）章。3 【印刷】星形號〈 〉。4 【占星術...
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The electron degenerate pressure does not come from the burning of any nuclear fuel and can therefore support the star from further gravitational contraction forever
電子簡並壓力並非來自任何核反應所以它能永遠抵抗恆星的引力。 -
Can stop the star from further collapsing. note : again, neutron degenerate pressure does not come from nuclear burning. it can support a neutron star from further gravitational contraction forever
則足以防止恆星進一步收縮同電子簡並壓力一樣中子簡並壓力並非來自核子反應它可永遠?抗恆星的引力收縮。 -
Nature of the universe - chapter seventeen if the remnant of a supernova explosion is heavier than two or three solar masses, the neutron degenerate pressure is not strong enough to support the star. there does not exist stronger force up to our knowledge and we believe the remnant will collapse to a black hole
在超新星爆發后，如果恆星剩餘質量超過二或三個太陽質量，中子簡並壓力亦不足以抵抗向內的引力，這時在已知的物理理論裏面，再沒有更強的力能足以與引力一決雌雄，恆星只可以不斷塌縮，成為黑洞。 -
If the mass of the core after a supernova explosion is more than 1. 4 but less than about 3 solar masses, then electron degenerate pressure is not strong enough to support the star. the star will contract to a size even smaller than the white dwarf. the electrons are squeezed into the nuclei and are combined with the protons to form neutrons
假若在超新星爆發后，剩餘核心質量介乎太陽質量的1 . 4至3倍，那麼核心中的電子簡並壓力便再不足以抵抗強大的引力，恆星會進一步收縮，直至電子亦被擠壓至原子核內，和質子結合成為中子。
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