| 1. | \(13.6~\text{eV}+2.2~\text{eV}\) |
| 2. | \((10.2+2.2)~\text{eV}\) |
| 3. | \((3.4+2.2)~\text{eV}\) |
| 4. | \((1.89+2.2)~\text{eV}\) |
| 1. | \(\lambda = \lambda_0\) |
| 2. | \(\lambda < \lambda_0\) |
| 3. | \(\lambda > \lambda_0\) |
| 4. | data is not sufficient to reach a conclusion |
Two metals, \(A\) and \(B,\) have threshold frequencies of \(1.8\times 10^{14}\ ~\text{Hz}\) and \(2.2\times 10^{14}~~\text{Hz;}\) respectively. If identical photons of energy \(2.2~\text{eV}\) are incident on both metals, photoelectrons will be emitted from: (take \(h=6.6\times 10^{-34}~\text{J-s}\))
1. Metal \(B\) only
2. Metal \(A\) only
3. Neither metal \(A\) nor metal \(B\)
4. Both metals \(A\) and \(B\)
| 1. | be tripled | 2. | be more than tripled |
| 3. | be less than tripled | 4. | become one-third |
| 1. | \(\dfrac{\lambda{P}}{h c} f\) | 2. | \(\dfrac{2\lambda{P}}{h c} f\) |
| 3. | \(\dfrac{\lambda{P}}{h c} f e\) | 4. | \(\dfrac{2\lambda{P}}{h c} f e\) |
In the case of the photoelectric effect:
| 1. | Since photons are absorbed as single (discrete) units, there is no significant time delay in the emission of photoelectrons. |
| 2. | According to Einstein, the critical frequency \(\nu_{0} =\dfrac{e\phi }{h},\) where \(\phi\) is the work function and \(h\) is Planck’s constant. When light with this frequency \((\nu_0)\) hits the material, it causes electrons to be ejected with the maximum possible kinetic energy. |
| 3. | Only a small fraction of the incident photons succeed in ejecting photoelectrons, while the majority are absorbed by the system as a whole and generate thermal energy. |
| 4. | The maximum kinetic energy of the electrons depends on the intensity of the radiation. |
| 1. | \(1.95~\text{eV}\) | 2. | \(2.12~\text{eV}\) |
| 3. | \(1.82~\text{eV}\) | 4. | \(1.66~\text{eV}\) |