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Radius of a beam of radiation of wavelength \(5000 \AA\) is $10^{-3} \mathrm{~m}\(. Power of the beam is \)10^{-3} \mathrm{~W}$. This beam is normally incident on a metal of work function \(1.9 \mathrm{eV}\). The charge emitted by the metal per unit area in unit time is \(\ldots \ldots \ldots\) Assume that each incident photon emits one electron. $\left(\mathrm{h}=6.625 \times 10^{-34} \mathrm{~J} . \mathrm{s}\right)$ (A) \(1.282 \mathrm{C}\) (B) \(12.82 \mathrm{C}\) (C) \(128.2 \mathrm{C}\) (D) \(1282 \mathrm{C}\)

Short Answer

Expert verified
The correct answer is: \(Q = 128.2 \mathrm{C}\) (Option C)

Step by step solution

01

Calculate the energy of each photon

The energy of a photon can be calculated using the formula \(E = \cfrac{hc}{\lambda}\), where \(E\) is the energy, \(h\) is Planck's constant, \(c\) is the speed of light, and \(\lambda\) is the wavelength. Given that the wavelength of the beam is \(5000 \AA\), we first need to convert it to meters. \(1 \AA = 10^{-10} \mathrm{m}\) Therefore, the wavelength of the beam in meters is: \(\lambda = 5000 \times 10^{-10} \mathrm{m}\) Now, using the values of \(h = 6.625 \times 10^{-34} \mathrm{J \cdot s}\) and \(c = 3 \times 10^8 \mathrm{m/s}\), we can calculate the energy of one photon: \(E = \cfrac{(6.625 \times 10^{-34} \mathrm{J \cdot s})(3 \times 10^8 \mathrm{m/s})}{(5000 \times 10^{-10} \mathrm{m})}\)
02

Calculate the number of incident photons per second

We are given the power of the beam as \(10^{-3} \mathrm{W}\). Since power is the energy per unit time, we can find the number of photons incident per second by dividing the power by the energy of one photon: \(N = \cfrac{10^{-3} \mathrm{W}}{E}\)
03

Calculate the charge emitted per unit area in unit time

Since we are given the radius of the beam, we can find the area of the beam using the formula for the area of a circle: \(A = \pi r^2\). The radius of the beam is \(10^{-3} \mathrm{m}\), thus: \(A = \pi (10^{-3} \mathrm{m})^2\) We are told to assume that each incident photon emits one electron. Therefore, the charge emitted by the metal per unit area in unit time can be calculated as: \(Q = \cfrac{Ne}{A}\) Where \(N\) is the number of incident photons per second, \(e\) is the elementary charge (\(1.6 \times 10^{-19} \mathrm{C}\)), and \(A\) is the area of the beam. Plug in the values calculated in the previous steps to find the charge emitted per unit area in unit time: \(Q = \cfrac{Ne}{A}\) Now, compare the calculated value of \(Q\) with the given options to find the correct answer.

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Most popular questions from this chapter

A star which can be seen with naked eye from Earth has intensity $1.6 \times 10^{-9} \mathrm{Wm}^{-2}\( on Earth. If the corresponding wavelength is \)560 \mathrm{~nm}\(, and the radius of the human eye is \)2.5 \times 10^{-3} \mathrm{~m}\(, the number of photons entering in our in \)1 \mathrm{~s}$ is..... (A) \(7.8 \times 10^{4} \mathrm{~s}^{-1}\) (B) \(8.85 \times 10^{4} \mathrm{~s}^{-1}\) (C) \(7.85 \times 10^{5} \mathrm{~s}^{-1}\) (D) \(8.85 \times 10^{5} \mathrm{~s}^{-1}\)

In which of the following phenomena the photon picture is required? (A) Energy distribution in black body radiation (B) Compton scattering (C) Photoelectric effect (D) all of the above

An electron moving with velocity \(0.6 \mathrm{c}\), then de-brogly wavelength associated with is \(\ldots \ldots \ldots\) (rest mars of electron, \(\mathrm{m}_{0}=9.1 \times 10^{-31}(\mathrm{k} / \mathrm{s})\) \(\mathrm{h}=6.63 \times 10^{-34} \mathrm{Js}\) (A) \(3.24 \times 10^{-12} \mathrm{~m}\) (B) \(32.4 \times 10^{-12} \mathrm{~m}\) (C) \(320 \times 10^{-12} \mathrm{~m}\) (D) \(3.29 \times 10^{-14} \mathrm{~m}\)

de-Broglie wavelength of atom at T \(\mathrm{K}\) absolute temperature will be \(\ldots \ldots \ldots\) (A) \([\mathrm{h} /\\{\mathrm{mkT}\\}]\) (B) \([\mathrm{h} /\\{\sqrt{3} \mathrm{mKT}\\}]\) (C) \([\\{\sqrt{2} \mathrm{mKT}\\} / \mathrm{h}]\) (D) \(\sqrt{(2 \mathrm{mKT})}\)

According to Einstein's photoelectric equation, graph of kinetic energy of emitted photo electrons from metal versus frequency of incident radiation is linear. Its slope.......... (A) depends on type of metal used (B) depends on intensity of radiation (C) depends on both metal used and intensity of radiation. (D) is same for all metals and free from intensity of radiation.

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