For the 2P → 1S transition in the hydrogen atom calculate ω. Assuming the
spontaneous emission lifetime of the 2P state to be 1.6 ns, calculate the Einstein B
coefficient. Assume n0 ≈1.
We know that energy of the photon during "2p\\rightarrow1s" transition "\\hbar\\omega =\\frac{E_o}{4}-E_o"
"\\Rightarrow \\hbar\\omega =\\frac{-3E_o}{4}"
"\\Rightarrow \\hbar\\omega =10.2eV"
"\\Rightarrow \\omega=\\frac{10.2\\times 1.6\\times 10^{-19}}{6.6\\times 10^{-34}}J\/J.s"
"\\Rightarrow \\omega =2.47\\times 10^{15} rev\/s"
"B=\\frac{\\pi e^2}{\\epsilon_o \\hbar}=\\frac{3.14\\times 1.6\\times 1.6\\times10^{-38}}{8.85\\times 6.6\\times 10^{-46}}" T
"=0.137\\times 10^{8}T"
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