degenerate electron pressure 中文意思是什麼
degenerate electron pressure
解釋
簡並電子壓力- 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...
- electron : n. 【物理學】電子。 the electron beam 電子束。 the electron theory 電子（學）說。
- pressure : n 1 壓；按；擠；榨。2 【物理學】壓力，壓強；大氣壓力；電壓。3 精神壓力，政治[經濟、輿論等]壓力。4...
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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。 -
Electron degenerate pressure
電子簡並壓力 -
Stops it from further contracting. an extremely simplified, but not totally correct, picture is that the electron degenerate pressure develops when the electrons are touching each others
雖然過于簡略和不準確，但電子簡並壓力可勉強看成是來自電子擠至互相觸碰時所造成的抵抗力成為了抵抗恆星進一步塌縮的主要力量。 -
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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