1. | \(\dfrac{h \omega_{1}}{2 \pi}\) or \(\dfrac{h \omega_{2}}{2 \pi}\) | Either
2. | \(\left(\dfrac{h \omega_{1}}{2 \pi}-h \nu_{0}\right)\) or \(\left(\dfrac{h \omega}{2 \pi}-h \nu_{0}\right)\) | Either
3. | \(\dfrac{h\left(\omega_{1}+\omega_{2}\right)}{2 \pi}-h \nu_{0}\) |
4. | Both \(\dfrac{h\left(\omega_{1}+\omega_{2}\right)}{2 \pi}-h \nu_{0}\) and \(\dfrac{h\left |\omega_{1}-\omega_{2}\right|}{2 \pi}-h \nu_{0}\) |
The stopping potential for electrons emitted from a photosensitive surface illuminated with light of wavelength \(491~\text{nm}\) is \(0.710~\text{V}.\) When the wavelength of the incident light changes, the stopping potential increases to \(1.43~\text{V}.\) The new wavelength is approximately:
1. \(329~\text{nm}\)
2. \(309~\text{nm}\)
3. \(382~\text{nm}\)
4. \(400~\text{nm}\)
1. | \(1\) V | 2. | \(1.5\) V |
3. | \(2\) V | 4. | \(5.2\) V |
1. | \(K_1>\dfrac{K_2}{3} \) | 2. | \({K}_1<\dfrac{{K}_2}{3} \) |
3. | \({K}_1=\dfrac{{K}_2}{3} \) | 4. | \({K}_2=\dfrac{{K}_1}{3}\) |
1. | does not depend on \(v\) |
2. | increases as \(v\) increases |
3. | decreases as \(v\) increases |
4. | first increases and then decreases as \(v\) is increased |