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chandrasekhar limit การใช้

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ประโยคมือถือ
  • The Chandrasekhar limit doesn't exist because of some other process taking over.
  • In which case, the article Chandrasekhar limit will be useful.
  • In an infamous encounter in 1935, Eddington publicly ridiculed the concept of the Chandrasekhar limit.
  • He is also known for his discovery of the Chandrasekhar limit before S . Chandrasekhar.
  • The Chandrasekhar limit is surpassed from the infalling matter.
  • When the Chandrasekhar limit is reached, that indicates that electron capture has become a feasible process.
  • Subgiants more than about reach the Sch鰊berg Chandrasekhar limit relatively quickly before the core becomes degenerate.
  • That limit is today called the Chandrasekhar Limit.
  • This iron core is pushed towards the Chandrasekhar limit till it surpasses it and therefore collapses.
  • Eventually, the white dwarf could explode as a Type Ia supernova if it approaches the Chandrasekhar limit.
  • The Chandrasekhar limit is named after him.
  • Mass transfer in a binary system may cause an initially stable white dwarf to surpass the Chandrasekhar limit.
  • The limit of neutron degeneracy pressure, analogous to the Chandrasekhar limit, is known as the Tolman Oppenheimer Volkoff limit.
  • If white dwarfs were an ideal Fermi gas, they would collapse into a black hole at the Chandrasekhar limit.
  • As the white dwarf gains matter, eventually it reaches its Chandrasekhar Limit of 1.4 M _ { \ odot }.
  • The same happens when two white dwarfs collide and the mass of the remnant is also over the Chandrasekhar limit.
  • All this star talk reminds me that there are still essentials of white dwarf and Chandrasekhar limit that I don't understand.
  • The helium core mass is below the Sch鰊berg Chandrasekhar limit and it remains in thermal equilibrium with the fusing hydrogen shell.
  • When the white dwarf approaches the Chandrasekhar limit of 1.4 solar masses ( ), it may explode as a Type Ia supernova.
  • He showed that the mass of a white dwarf could not exceed 1.44 times that of the Sun  the Chandrasekhar limit.
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