Answer
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Hint: When a photon hits a metal, the metal will eject photoelectron. This is called a photoelectric effect. The incident energy of the photon is equal to the algebraic sum of the kinetic energy of the ejected photon and the work function to eject the photoelectron from the metal. By using the given relation between the kinetic energy of the photoelectron in two cases, the correct answer can be calculated.
Formula used:
De Broglie wavelength, $\lambda = \dfrac{h}{p}$
Where $h$ is the Planck’s constant and $p$ is the momentum of the particle.
The kinetic energy of the particle, $T = \dfrac{1}{2}m{v^2}$
Where $m$ is the mass of the particle and $v$ is the velocity of the particle.
Complete step by step solution:
Given: Energy of photon in case one, ${E_A} = 4.25\;eV$
Energy of photon in case two, ${E_B} = 4.70\;eV$
Given relations are ${T_B} = \left( {{T_A} - 1.50} \right)\;eV$ and ${\lambda _B} = 2{\lambda _A}$.
In the metal A, the de Broglie wavelength, ${\lambda _A} = \dfrac{h}{{{p_A}}}$
By rearranging, we get
${p_A} = \dfrac{h}{{{\lambda _A}}}$
The kinetic energy of the photoelectron emitted from metal A, ${T_A} = \dfrac{1}{2}m{v_A}^2$
Since, the momentum of moving particle is ${p_A} = m{v_A}$
Squaring on both sides, we get ${p_A}^2 = {m^2}{v_A}^2\; \Rightarrow m{v_A}^2 = \dfrac{{{p_A}^2}}{m}$
Substituting the above value on the equation of ${T_A}$, we get
${T_A} = \dfrac{{{p_A}^2}}{{2m}}$
Substitute the value of ${p_A}$ in above equation, we get
${T_A} = \dfrac{{{h^2}}}{{2m \times {\lambda _A}^2}}\;................................................\left( 1 \right)$
In the metal B, the de Broglie wavelength, ${\lambda _B} = \dfrac{h}{{{p_B}}}$
By rearranging, we get
${p_B} = \dfrac{h}{{{\lambda _B}}}$
The kinetic energy of the photoelectron emitted from metal B, ${T_B} = \dfrac{1}{2}m{v_B}^2$
Since, the momentum of moving particle is ${p_B} = m{v_B}$
Squaring on both sides, we get ${p_B}^2 = {m^2}{v_B}^2\; \Rightarrow m{v_B}^2 = \dfrac{{{p_B}^2}}{m}$
Substituting the above value on the equation of ${T_B}$, we get
${T_B} = \dfrac{{{p_B}^2}}{{2m}}$
Substitute the value of ${p_B}$ in above equation, we get
${T_B} = \dfrac{{{h^2}}}{{2m \times {\lambda _B}^2}}\;................................................\left( 2 \right)$
By dividing equation (1) by (2), we get
$\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{\left( {\dfrac{{{h^2}}}{{2m \times {\lambda _A}^2}}} \right)}}{{\left( {\dfrac{{{h^2}}}{{2m \times {\lambda _B}^2}}} \right)}}$
Since the Planck’s constant and the mass of the photoelectron are the same in both cases.
$
\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{\left( {\dfrac{1}{{{\lambda _A}^2}}} \right)}}{{\left( {\dfrac{1}{{{\lambda _B}^2}}} \right)}} \\
\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{{\lambda _B}^2}}{{{\lambda _A}^2}}\;............................................\left( 3 \right) \\
$
From the question, ${\lambda _B} = 2{\lambda _A}$. Thus, by rearranging we get $\dfrac{{{\lambda _B}}}{{{\lambda _A}}} = 2$
By substituting the above relation in equation (3), we get
$\dfrac{{{T_A}}}{{{T_B}}} = {2^2} = 4$
Hence, by rearranging we get ${T_A} = 4 \times {T_B}$
From the question, ${T_B} = \left( {{T_A} - 1.50} \right)\;eV$
Substitute the value of ${T_A}$ in above relation, we get
$
{T_B} = \left( {4{T_B} - 1.50} \right)\;eV \\
1.5 = 4{T_B} - {T_B} \\
$
By rearranging, we get
$
3{T_B} = 1.5 \\
{T_B} = \dfrac{{1.5}}{3} \\
{T_B} = 0.5\;eV \\
$
Substitute the value of ${T_B}$ in the equation of ${T_A}$, we get
$
{T_A} = 4 \times 0.5\;eV \\
{T_A} = 2\;eV \\
$
By the law of conservation of energy in the first case, the energy of the photon is equal to the sum of the kinetic energy of the photoelectron emitted and the work function tends the photoelectron to emit.
Hence, ${E_A} = {T_A} + {W_A}$
Substitute the given values in the above equation, we get
$
4.25\;eV = 2\;eV + {W_A} \\
{W_A} = 4.25 - 2 \\
{W_A} = 2.25\;eV \\
$
By the law of conservation of energy in the second case, the energy of a photon is equal to the sum of the kinetic energy of the photoelectron emitted and the work function tends the photoelectron to emit.
Hence, ${E_B} = {T_B} + {W_B}$
Substitute the given values in the above equation, we get
$
4.70\;eV = 0.5\;eV + {W_B} \\
{W_B} = 4.70 - 0.5 \\
{W_B} = 4.2\;eV \\
$
$\therefore$ Hence, the options (A), (B) and (C) are correct.
Note:
When a photon hits the metal surface, due to the photoelectric effect, the photoelectrons are emitted from the metal. It requires some energy of the incident photon to eject an electron. That energy is called the work function of the photoelectric effect. The work function will vary based on the attraction force between the nucleus and the valence electron.
Formula used:
De Broglie wavelength, $\lambda = \dfrac{h}{p}$
Where $h$ is the Planck’s constant and $p$ is the momentum of the particle.
The kinetic energy of the particle, $T = \dfrac{1}{2}m{v^2}$
Where $m$ is the mass of the particle and $v$ is the velocity of the particle.
Complete step by step solution:
Given: Energy of photon in case one, ${E_A} = 4.25\;eV$
Energy of photon in case two, ${E_B} = 4.70\;eV$
Given relations are ${T_B} = \left( {{T_A} - 1.50} \right)\;eV$ and ${\lambda _B} = 2{\lambda _A}$.
In the metal A, the de Broglie wavelength, ${\lambda _A} = \dfrac{h}{{{p_A}}}$
By rearranging, we get
${p_A} = \dfrac{h}{{{\lambda _A}}}$
The kinetic energy of the photoelectron emitted from metal A, ${T_A} = \dfrac{1}{2}m{v_A}^2$
Since, the momentum of moving particle is ${p_A} = m{v_A}$
Squaring on both sides, we get ${p_A}^2 = {m^2}{v_A}^2\; \Rightarrow m{v_A}^2 = \dfrac{{{p_A}^2}}{m}$
Substituting the above value on the equation of ${T_A}$, we get
${T_A} = \dfrac{{{p_A}^2}}{{2m}}$
Substitute the value of ${p_A}$ in above equation, we get
${T_A} = \dfrac{{{h^2}}}{{2m \times {\lambda _A}^2}}\;................................................\left( 1 \right)$
In the metal B, the de Broglie wavelength, ${\lambda _B} = \dfrac{h}{{{p_B}}}$
By rearranging, we get
${p_B} = \dfrac{h}{{{\lambda _B}}}$
The kinetic energy of the photoelectron emitted from metal B, ${T_B} = \dfrac{1}{2}m{v_B}^2$
Since, the momentum of moving particle is ${p_B} = m{v_B}$
Squaring on both sides, we get ${p_B}^2 = {m^2}{v_B}^2\; \Rightarrow m{v_B}^2 = \dfrac{{{p_B}^2}}{m}$
Substituting the above value on the equation of ${T_B}$, we get
${T_B} = \dfrac{{{p_B}^2}}{{2m}}$
Substitute the value of ${p_B}$ in above equation, we get
${T_B} = \dfrac{{{h^2}}}{{2m \times {\lambda _B}^2}}\;................................................\left( 2 \right)$
By dividing equation (1) by (2), we get
$\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{\left( {\dfrac{{{h^2}}}{{2m \times {\lambda _A}^2}}} \right)}}{{\left( {\dfrac{{{h^2}}}{{2m \times {\lambda _B}^2}}} \right)}}$
Since the Planck’s constant and the mass of the photoelectron are the same in both cases.
$
\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{\left( {\dfrac{1}{{{\lambda _A}^2}}} \right)}}{{\left( {\dfrac{1}{{{\lambda _B}^2}}} \right)}} \\
\dfrac{{{T_A}}}{{{T_B}}} = \dfrac{{{\lambda _B}^2}}{{{\lambda _A}^2}}\;............................................\left( 3 \right) \\
$
From the question, ${\lambda _B} = 2{\lambda _A}$. Thus, by rearranging we get $\dfrac{{{\lambda _B}}}{{{\lambda _A}}} = 2$
By substituting the above relation in equation (3), we get
$\dfrac{{{T_A}}}{{{T_B}}} = {2^2} = 4$
Hence, by rearranging we get ${T_A} = 4 \times {T_B}$
From the question, ${T_B} = \left( {{T_A} - 1.50} \right)\;eV$
Substitute the value of ${T_A}$ in above relation, we get
$
{T_B} = \left( {4{T_B} - 1.50} \right)\;eV \\
1.5 = 4{T_B} - {T_B} \\
$
By rearranging, we get
$
3{T_B} = 1.5 \\
{T_B} = \dfrac{{1.5}}{3} \\
{T_B} = 0.5\;eV \\
$
Substitute the value of ${T_B}$ in the equation of ${T_A}$, we get
$
{T_A} = 4 \times 0.5\;eV \\
{T_A} = 2\;eV \\
$
By the law of conservation of energy in the first case, the energy of the photon is equal to the sum of the kinetic energy of the photoelectron emitted and the work function tends the photoelectron to emit.
Hence, ${E_A} = {T_A} + {W_A}$
Substitute the given values in the above equation, we get
$
4.25\;eV = 2\;eV + {W_A} \\
{W_A} = 4.25 - 2 \\
{W_A} = 2.25\;eV \\
$
By the law of conservation of energy in the second case, the energy of a photon is equal to the sum of the kinetic energy of the photoelectron emitted and the work function tends the photoelectron to emit.
Hence, ${E_B} = {T_B} + {W_B}$
Substitute the given values in the above equation, we get
$
4.70\;eV = 0.5\;eV + {W_B} \\
{W_B} = 4.70 - 0.5 \\
{W_B} = 4.2\;eV \\
$
$\therefore$ Hence, the options (A), (B) and (C) are correct.
Note:
When a photon hits the metal surface, due to the photoelectric effect, the photoelectrons are emitted from the metal. It requires some energy of the incident photon to eject an electron. That energy is called the work function of the photoelectric effect. The work function will vary based on the attraction force between the nucleus and the valence electron.
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