Angelos K
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Hello!
My textbook quotes the probability W of a transition between the levels 1 and 2 of a laser that appears in the rate equations. For
E_2 = E_1 +h\nu
it is supposed to be given by:
W = \frac{1}{\tau VD(\nu)\Delta\nu}
where \tau is the lifetime of the level 2 (probably for the case of spontaneous emission making the only important contribution), D(\nu)d\nu is the number of modes of the field in the intervall (\nu,\nu+d\nu) per unit volume of the laser substance and \Delta\nu is the broadness of the spectral line corresponding to transitions between states 2 and 1.
There are no comments on how to prove this. I would appreciate help, since many important conclusions are driven from that formula.
I have also discovered the attached document, which derives a more complex formula:
W = g(\nu) \frac{A_{21}c^{2}I(\nu)}{8\pi h {\nu}^3}
containing the Einstein coefficient for spontaneous emission, the radiation Intensity I(\nu) and the line shape g(\nu). The formulas are fairly similar if we remember the equalities:
A_{21} = \frac{1}{\tau}
and
D(\nu) = \frac{8\pi{\nu}^2}{c^3}
It would be sufficient if you could explain how to go from the second expression for W to the first one. It is the \Delta\nu in particular that I do not see how to obtain!
Thanks for any help,
Angelos
My textbook quotes the probability W of a transition between the levels 1 and 2 of a laser that appears in the rate equations. For
E_2 = E_1 +h\nu
it is supposed to be given by:
W = \frac{1}{\tau VD(\nu)\Delta\nu}
where \tau is the lifetime of the level 2 (probably for the case of spontaneous emission making the only important contribution), D(\nu)d\nu is the number of modes of the field in the intervall (\nu,\nu+d\nu) per unit volume of the laser substance and \Delta\nu is the broadness of the spectral line corresponding to transitions between states 2 and 1.
There are no comments on how to prove this. I would appreciate help, since many important conclusions are driven from that formula.
I have also discovered the attached document, which derives a more complex formula:
W = g(\nu) \frac{A_{21}c^{2}I(\nu)}{8\pi h {\nu}^3}
containing the Einstein coefficient for spontaneous emission, the radiation Intensity I(\nu) and the line shape g(\nu). The formulas are fairly similar if we remember the equalities:
A_{21} = \frac{1}{\tau}
and
D(\nu) = \frac{8\pi{\nu}^2}{c^3}
It would be sufficient if you could explain how to go from the second expression for W to the first one. It is the \Delta\nu in particular that I do not see how to obtain!
Thanks for any help,
Angelos
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