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The deBroglie wavelength, associated with electrons, accelerated through a potential V, equals λB . The threshold wavelength, for a given photosensitive surface is λB (n > 1) . If this photosensitive surface is irradiated with monochromatic radiation of wavelength (λB/n), the stopping potential needed is VS

The relation, between VS and V, can be expressed as

(1) \(V_s=\left[\frac{(n^2-1)c}{n}\sqrt{\frac{2m}{e}}\right]\sqrt{V}\)

(2) \(V=\left[\frac{nc}{(n^2-1)}\sqrt{\frac{2m}{e}}\right]\sqrt{V}\)

(3) \(V_s=\left[\frac{nc}{(n^2-1)}\sqrt{\frac{2m}{e}}\right]\sqrt{V}\)

(4) \(V=\left[\frac{(n^2-1)c}{n}\sqrt{\frac{2m}{e}}\right]\sqrt{V_s}\)

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 (1) \(V_s=\left[\frac{(n^2-1)c}{n}\sqrt{\frac{2m}{e}}\right]\sqrt{V}\)

The work function, of the photosensitive surface = energy of a photon of its ‘threshold wavelength’ radiation = hc/nλB

Energy of a photon of the incident radiation

∴ As per Einstein’s photoelectric equation, 

we have 

This is the required relation between VS and V.

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