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- + diff --git a/academic/physics/ipho-formulas-jpn/11.html b/academic/physics/ipho-formulas-jpn/11.html index 67b5f45d..b6254f71 100644 --- a/academic/physics/ipho-formulas-jpn/11.html +++ b/academic/physics/ipho-formulas-jpn/11.html @@ -8,7 +8,7 @@ - + @@ -40,10 +40,10 @@ s-271.3,567,-271.3,567c-38.7,80.7,-84,175,-136,283c-52,108,-89.167,185.3,-111.5, c-22.3,46.7,-33.8,70.3,-34.5,71c-4.7,4.7,-12.3,7,-23,7s-12,-1,-12,-1 s-109,-253,-109,-253c-72.7,-168,-109.3,-252,-110,-252c-10.7,8,-22,16.7,-34,26 c-22,17.3,-33.3,26,-34,26s-26,-26,-26,-26s76,-59,76,-59s76,-60,76,-60z -M1001 80h400000v40h-400000z">) であれば容易に透過する.

11.7: Bohr モデル

  1. Bohr モデル : En1/n2E_n \propto-1 / n^2. (古典的に計算される) 円軌道では, 軌道の長さが波長 λ=h/mv\lambda=h / m v の整数倍.

11.8: Compton 効果

  1. Compton 効果: 光子が電子から散乱されると, 光子の Δλ=λC(1cosθ)\Delta \lambda=\lambda_C(1-\cos \theta)

11.9: 光電効果

  1. 光電効果: W+mvmax2/2=hνW+m v_{\max }^2 / 2=h \nu ( WW は仕事関数 )). IVI-V グラフ:光電流は阻止電圧 V=(hνW)/eV=-(h \nu-W) / e で始まり, 正方向に電圧が大きくなると緩和する.

11.10: Stefan-Boltzmann の法則

  1. Stefan-Boltzmann の法則 : P=σAT4P=\sigma A T^4