逢甲學報, Ausgaben 6-7逢甲大學, 1973 |
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... energy gap , it is difficult to conduct until it breakd- owns . The breakdown excitation is about 6ev . It is also difficult to raise the electron in valence band up to the conduction band by thermal excitation in an intrinsic ...
... energy gap , it is difficult to conduct until it breakd- owns . The breakdown excitation is about 6ev . It is also difficult to raise the electron in valence band up to the conduction band by thermal excitation in an intrinsic ...
Seite
... energy gap . However , there certainly exist some gapless superconductors , then the treatment given in sections II an III does not hold . For a comprehensive discussion for gapless superconductor , the readers are refered to the paper ...
... energy gap . However , there certainly exist some gapless superconductors , then the treatment given in sections II an III does not hold . For a comprehensive discussion for gapless superconductor , the readers are refered to the paper ...
Seite
... energy cosmic ray electron ( 8 , 9 ) . So that the high energy electron , especially ultrarelativistic electron ( for an electron energy E > mc2 ) , may be considered as a clue to the solution of the origin of cosmic rays . In this ...
... energy cosmic ray electron ( 8 , 9 ) . So that the high energy electron , especially ultrarelativistic electron ( for an electron energy E > mc2 ) , may be considered as a clue to the solution of the origin of cosmic rays . In this ...