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NCERT Solutions for Class 12 Physics

Chapter 11: Dual Nature of Radiation and Matter

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Complete NCERT Solution PDF for Chapter 11: Dual Nature of Radiation and Matter

NCERT Solutions For Class 12 Physics Chapter 11 Dual Nature of Radiation and Matter helps students explore the dual behaviour of matter and radiation at the microscopic level. The page provides detailed NCERT Solutions that explain concepts such as photoelectric effect, Einstein’s photoelectric equation, wave-particle duality, and de Broglie wavelength. NCERT Solutions For Class 12 Physics simplify these modern Physics concepts through clear explanations and solved numerical problems. The chapter introduces important ideas that connect classical Physics with quantum concepts. These solutions help students understand theoretical principles and improve their problem-solving abilities. Students can access the chapter PDF for revision, practice, and examination preparation. The detailed explanations make quantum Physics concepts easier to understand.

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Examples 11.1-11.3

Example 11.1 Monochromatic light of frequency $$6.0 \times 10^{14} \, \mathrm{Hz}$$ is produced by a laser. The power emitted is $$2.0 \times 10^{-3} \, \mathrm{W}$$. (a) What is the energy of a photon in the light beam? (b) How many photons per second, on an average, are emitted by the source?

Solution

Each photon in a monochromatic beam of frequency $$\nu$$ carries an energy $$E = h\nu$$, where $$h = 6.63 \times 10^{-34}\,\mathrm{J\,s}$$ is Planck's constant.

(a) Energy of a photon.

$$E = h\nu = (6.63 \times 10^{-34}\,\mathrm{J\,s}) \times (6.0 \times 10^{14}\,\mathrm{Hz})$$

$$E = 3.98 \times 10^{-19}\,\mathrm{J}$$

Converting to electron volts by dividing by $$1.6 \times 10^{-19}\,\mathrm{J/eV}$$:

$$E = \frac{3.98 \times 10^{-19}}{1.6 \times 10^{-19}}\,\mathrm{eV} = 2.49\,\mathrm{eV}$$

(b) Number of photons emitted per second.

If the source emits $$N$$ photons per second, each carrying energy $$E$$, then the power (energy radiated per second) is $$P = NE$$. Therefore

$$N = \frac{P}{E} = \frac{2.0 \times 10^{-3}\,\mathrm{W}}{3.98 \times 10^{-19}\,\mathrm{J}}$$

$$N \approx 5.0 \times 10^{15}\ \text{photons per second}$$

Answer

(a) $$E = 3.98 \times 10^{-19}\,\mathrm{J} = 2.49\,\mathrm{eV}$$; (b) $$N \approx 5.0 \times 10^{15}$$ photons per second.

Example 11.2 The work function of caesium is $$2.14 \, \mathrm{eV}$$. Find (a) the threshold frequency for caesium, and (b) the wavelength of the incident light if the photocurrent is brought to zero by a stopping potential of $$0.60 \, \mathrm{V}$$.

Solution

For a photosensitive metal of work function $$\phi_0$$, the threshold frequency $$\nu_0$$ is the minimum frequency of incident light that just frees an electron, defined by $$h\nu_0 = \phi_0$$.

(a) Threshold frequency.

First express the work function in joules:

$$\phi_0 = 2.14\,\mathrm{eV} = 2.14 \times 1.6 \times 10^{-19}\,\mathrm{J} = 3.42 \times 10^{-19}\,\mathrm{J}$$

$$\nu_0 = \frac{\phi_0}{h} = \frac{3.42 \times 10^{-19}\,\mathrm{J}}{6.63 \times 10^{-34}\,\mathrm{J\,s}}$$

$$\nu_0 = 5.16 \times 10^{14}\,\mathrm{Hz}$$

(b) Wavelength of the incident light.

A stopping potential $$V_0 = 0.60\,\mathrm{V}$$ means the maximum kinetic energy of the photoelectrons is $$K_{\max} = eV_0 = 0.60\,\mathrm{eV}$$. Einstein's photoelectric equation gives

$$h\nu = \phi_0 + eV_0$$

so the energy of an incident photon is

$$h\nu = (2.14 + 0.60)\,\mathrm{eV} = 2.74\,\mathrm{eV} = 2.74 \times 1.6 \times 10^{-19}\,\mathrm{J} = 4.38 \times 10^{-19}\,\mathrm{J}$$

The incident frequency is

$$\nu = \frac{4.38 \times 10^{-19}}{6.63 \times 10^{-34}} = 6.61 \times 10^{14}\,\mathrm{Hz}$$

and the corresponding wavelength is

$$\lambda = \frac{c}{\nu} = \frac{3.0 \times 10^{8}\,\mathrm{m/s}}{6.61 \times 10^{14}\,\mathrm{Hz}} = 4.54 \times 10^{-7}\,\mathrm{m} \approx 454\,\mathrm{nm}$$

Answer

(a) $$\nu_0 = 5.16 \times 10^{14}\,\mathrm{Hz}$$; (b) $$\lambda \approx 454\,\mathrm{nm}$$ (incident frequency $$6.61 \times 10^{14}\,\mathrm{Hz}$$).

Example 11.3 What is the de Broglie wavelength associated with (a) an electron moving with a speed of $$5.4 \times 10^{6} \, \mathrm{m/s}$$, and (b) a ball of mass $$150 \, \mathrm{g}$$ travelling at $$30.0 \, \mathrm{m/s}$$?

Solution

The de Broglie wavelength of a particle of mass $$m$$ moving with speed $$v$$ (momentum $$p = mv$$) is

$$\lambda = \frac{h}{p} = \frac{h}{mv}$$

(a) Electron. With $$m_e = 9.11 \times 10^{-31}\,\mathrm{kg}$$ and $$v = 5.4 \times 10^{6}\,\mathrm{m/s}$$, the momentum is

$$p = m_e v = (9.11 \times 10^{-31}\,\mathrm{kg}) \times (5.4 \times 10^{6}\,\mathrm{m/s}) = 4.92 \times 10^{-24}\,\mathrm{kg\,m/s}$$

$$\lambda = \frac{h}{p} = \frac{6.63 \times 10^{-34}\,\mathrm{J\,s}}{4.92 \times 10^{-24}\,\mathrm{kg\,m/s}} = 1.35 \times 10^{-10}\,\mathrm{m} = 0.135\,\mathrm{nm}$$

This is comparable to atomic dimensions, which is why electrons of this speed display pronounced wave (diffraction) effects.

(b) Ball. With $$m = 150\,\mathrm{g} = 0.150\,\mathrm{kg}$$ and $$v = 30.0\,\mathrm{m/s}$$,

$$p = mv = 0.150 \times 30.0 = 4.50\,\mathrm{kg\,m/s}$$

$$\lambda = \frac{h}{p} = \frac{6.63 \times 10^{-34}}{4.50} = 1.47 \times 10^{-34}\,\mathrm{m}$$

This wavelength is so vanishingly small (far smaller than any atomic or nuclear size) that the wave nature of an everyday object such as a ball can never be detected.

Answer

(a) $$\lambda \approx 1.35 \times 10^{-10}\,\mathrm{m} = 0.135\,\mathrm{nm}$$; (b) $$\lambda \approx 1.47 \times 10^{-34}\,\mathrm{m}$$.

Exercises

11.1 Find the
(a) maximum frequency, and
(b) minimum wavelength of X-rays produced by $$30 \, \mathrm{kV}$$ electrons.

(a) maximum frequency, and

Solution

When electrons accelerated through a potential difference $$V$$ strike a target, they produce X-rays. Each electron acquires kinetic energy $$K = eV$$, and the X-ray photon of highest frequency (and hence shortest wavelength) is produced when an electron loses all of its kinetic energy in a single collision, converting it entirely into one photon.

(a) Maximum frequency.

$$h\nu_{\max} = eV \quad\Rightarrow\quad \nu_{\max} = \frac{eV}{h}$$

With $$V = 30\,\mathrm{kV} = 30 \times 10^{3}\,\mathrm{V}$$:

$$\nu_{\max} = \frac{(1.6 \times 10^{-19}\,\mathrm{C}) \times (30 \times 10^{3}\,\mathrm{V})}{6.63 \times 10^{-34}\,\mathrm{J\,s}} = \frac{4.8 \times 10^{-15}}{6.63 \times 10^{-34}}$$

$$\nu_{\max} \approx 7.24 \times 10^{18}\,\mathrm{Hz}$$

(b) Minimum wavelength. The shortest wavelength corresponds to this maximum frequency, since $$\lambda = c/\nu$$:

$$\lambda_{\min} = \frac{c}{\nu_{\max}} = \frac{3.0 \times 10^{8}\,\mathrm{m/s}}{7.24 \times 10^{18}\,\mathrm{Hz}} \approx 4.14 \times 10^{-11}\,\mathrm{m} \approx 0.041\,\mathrm{nm}$$

Equivalently, one may write $$\lambda_{\min} = \dfrac{hc}{eV}$$ to obtain the same result directly. This very short wavelength (a few hundredths of a nanometre) lies in the X-ray region of the electromagnetic spectrum.

Answer

(a) $$\nu_{\max} \approx 7.24 \times 10^{18}\,\mathrm{Hz}$$; (b) $$\lambda_{\min} \approx 4.14 \times 10^{-11}\,\mathrm{m} \approx 0.041\,\mathrm{nm}$$

(b) minimum wavelength of X-rays produced by $$30 \, \mathrm{kV}$$ electrons.

Solution

The minimum wavelength corresponds to the maximum frequency found in part (a), since $$\lambda = c/\nu$$.

$$\lambda_{\min} = \frac{c}{\nu_{\max}} = \frac{3.0 \times 10^{8}\,\mathrm{m/s}}{7.24 \times 10^{18}\,\mathrm{Hz}}$$

$$\lambda_{\min} = 4.14 \times 10^{-11}\,\mathrm{m} \approx 0.041\,\mathrm{nm}$$

Equivalently, one can write $$\lambda_{\min} = \dfrac{hc}{eV}$$ directly. This very short wavelength (a few hundredths of a nanometre) lies in the X-ray region of the electromagnetic spectrum.

Answer

$$\lambda_{\min} \approx 4.14 \times 10^{-11}\,\mathrm{m} \approx 0.041\,\mathrm{nm}$$

11.2 The work function of caesium metal is $$2.14 \, \mathrm{eV}$$. When light of frequency $$6 \times 10^{14} \, \mathrm{Hz}$$ is incident on the metal surface, photoemission of electrons occurs. What is the

(a) maximum kinetic energy of the emitted electrons,

Solution

By Einstein's photoelectric equation, the maximum kinetic energy of the emitted electrons is

$$K_{\max} = h\nu - \phi_0$$

Energy of an incident photon:

$$h\nu = (6.63 \times 10^{-34}\,\mathrm{J\,s}) \times (6 \times 10^{14}\,\mathrm{Hz}) = 3.98 \times 10^{-19}\,\mathrm{J}$$

Work function in joules:

$$\phi_0 = 2.14\,\mathrm{eV} = 2.14 \times 1.6 \times 10^{-19}\,\mathrm{J} = 3.42 \times 10^{-19}\,\mathrm{J}$$

Maximum kinetic energy:

$$K_{\max} = 3.98 \times 10^{-19}\,\mathrm{J} - 3.42 \times 10^{-19}\,\mathrm{J} = 5.5 \times 10^{-20}\,\mathrm{J}$$

$$K_{\max} = \frac{5.5 \times 10^{-20}}{1.6 \times 10^{-19}}\,\mathrm{eV} \approx 0.34\,\mathrm{eV}$$

Answer

$$K_{\max} \approx 0.34\,\mathrm{eV}\;(\approx 5.5 \times 10^{-20}\,\mathrm{J})$$

(b) Stopping potential, and

Solution

The stopping potential $$V_0$$ is the retarding voltage that just reduces the photocurrent to zero. It is related to the maximum kinetic energy of the photoelectrons by

$$eV_0 = K_{\max}$$

Using $$K_{\max} \approx 0.34\,\mathrm{eV}$$ from part (a):

$$V_0 = \frac{K_{\max}}{e} = \frac{0.34\,\mathrm{eV}}{e} = 0.34\,\mathrm{V}$$

(Since $$K_{\max}$$ is expressed in electron volts, dividing by the electronic charge $$e$$ gives the numerically equal value in volts.)

Answer

$$V_0 \approx 0.34\,\mathrm{V}$$

(c) maximum speed of the emitted photoelectrons?

Solution

The maximum speed $$v_{\max}$$ corresponds to the maximum kinetic energy:

$$K_{\max} = \frac{1}{2} m v_{\max}^2 \quad\Rightarrow\quad v_{\max} = \sqrt{\frac{2K_{\max}}{m}}$$

Using $$K_{\max} = 5.5 \times 10^{-20}\,\mathrm{J}$$ from part (a) and the electron mass $$m = 9.11 \times 10^{-31}\,\mathrm{kg}$$:

$$v_{\max} = \sqrt{\frac{2 \times (5.5 \times 10^{-20})}{9.11 \times 10^{-31}}}$$

$$v_{\max} = \sqrt{1.21 \times 10^{11}} = 3.5 \times 10^{5}\,\mathrm{m/s}$$

So the photoelectrons are emitted with a maximum speed of about $$3.5 \times 10^{5}\,\mathrm{m/s}$$, i.e. roughly $$3.5 \times 10^{2}\,\mathrm{km/s}$$.

Answer

$$v_{\max} \approx 3.5 \times 10^{5}\,\mathrm{m/s}$$

11.3 The photoelectric cut-off voltage in a certain experiment is $$1.5 \, \mathrm{V}$$. What is the maximum kinetic energy of photoelectrons emitted?

Solution

The cut-off (stopping) voltage $$V_0$$ is the potential needed to stop the most energetic photoelectrons. The work done by this retarding potential in stopping an electron equals the electron's maximum kinetic energy:

$$K_{\max} = eV_0$$

With $$V_0 = 1.5\,\mathrm{V}$$ and $$e = 1.6 \times 10^{-19}\,\mathrm{C}$$:

$$K_{\max} = (1.6 \times 10^{-19}\,\mathrm{C}) \times (1.5\,\mathrm{V})$$

$$K_{\max} = 2.4 \times 10^{-19}\,\mathrm{J}$$

Equivalently, expressed in electron volts, $$K_{\max} = eV_0 = 1.5\,\mathrm{eV}$$.

Answer

$$K_{\max} = 2.4 \times 10^{-19}\,\mathrm{J} = 1.5\,\mathrm{eV}$$

11.4 Monochromatic light of wavelength $$632.8 \, \mathrm{nm}$$ is produced by a helium-neon laser. The power emitted is $$9.42 \, \mathrm{mW}$$.

(a) Find the energy and momentum of each photon in the light beam,

Solution

Energy of each photon. For light of wavelength $$\lambda$$, a photon carries energy

$$E = h\nu = \frac{hc}{\lambda}$$

With $$\lambda = 632.8\,\mathrm{nm} = 632.8 \times 10^{-9}\,\mathrm{m}$$:

$$E = \frac{(6.63 \times 10^{-34}\,\mathrm{J\,s}) \times (3.0 \times 10^{8}\,\mathrm{m/s})}{632.8 \times 10^{-9}\,\mathrm{m}}$$

$$E = \frac{1.989 \times 10^{-25}}{6.328 \times 10^{-7}} = 3.14 \times 10^{-19}\,\mathrm{J}$$

In electron volts, $$E = \dfrac{3.14 \times 10^{-19}}{1.6 \times 10^{-19}} \approx 1.96\,\mathrm{eV}$$.

Momentum of each photon. A photon's momentum is related to its energy by $$p = E/c$$ (equivalently $$p = h/\lambda$$):

$$p = \frac{E}{c} = \frac{3.14 \times 10^{-19}\,\mathrm{J}}{3.0 \times 10^{8}\,\mathrm{m/s}}$$

$$p = 1.05 \times 10^{-27}\,\mathrm{kg\,m/s}$$

Answer

$$E \approx 3.14 \times 10^{-19}\,\mathrm{J}\;(\approx 1.96\,\mathrm{eV})$$; $$p \approx 1.05 \times 10^{-27}\,\mathrm{kg\,m/s}$$.

(b) How many photons per second, on the average, arrive at a target irradiated by this beam? (Assume the beam to have uniform cross-section which is less than the target area), and

Solution

Let $$N$$ be the number of photons arriving at the target per second. Since the whole beam falls on the target (its cross-section is smaller than the target area), the power delivered equals the energy carried by all those photons:

$$P = NE \quad\Rightarrow\quad N = \frac{P}{E}$$

With $$P = 9.42\,\mathrm{mW} = 9.42 \times 10^{-3}\,\mathrm{W}$$ and $$E = 3.14 \times 10^{-19}\,\mathrm{J}$$ from part (a):

$$N = \frac{9.42 \times 10^{-3}\,\mathrm{W}}{3.14 \times 10^{-19}\,\mathrm{J}}$$

$$N \approx 3.0 \times 10^{16}\ \text{photons per second}$$

Answer

$$N \approx 3.0 \times 10^{16}$$ photons per second.

(c) How fast does a hydrogen atom have to travel in order to have the same momentum as that of the photon?

Solution

We need the speed of a hydrogen atom whose momentum equals the photon momentum $$p = 1.05 \times 10^{-27}\,\mathrm{kg\,m/s}$$ found in part (a).

For the (non-relativistic) atom, $$p = m_H v$$, so

$$v = \frac{p}{m_H}$$

The mass of a hydrogen atom is $$m_H = 1.66 \times 10^{-27}\,\mathrm{kg}$$. Hence

$$v = \frac{1.05 \times 10^{-27}\,\mathrm{kg\,m/s}}{1.66 \times 10^{-27}\,\mathrm{kg}}$$

$$v \approx 0.63\,\mathrm{m/s}$$

So a hydrogen atom moving at only about $$0.63\,\mathrm{m/s}$$ has the same momentum as a single photon of this laser light.

Answer

$$v \approx 0.63\,\mathrm{m/s}$$

11.5 In an experiment on photoelectric effect, the slope of the cut-off voltage versus frequency of incident light is found to be $$4.12 \times 10^{-15} \, \mathrm{V \, s}$$. Calculate the value of Planck's constant.

Solution

According to Einstein's photoelectric equation, the cut-off (stopping) potential $$V_0$$ is related to the frequency $$\nu$$ of the incident light by

$$eV_0 = h\nu - \phi_0 \quad\Rightarrow\quad V_0 = \left(\frac{h}{e}\right)\nu - \frac{\phi_0}{e}$$

This is the equation of a straight line of $$V_0$$ against $$\nu$$, whose slope is $$\dfrac{h}{e}$$. Therefore

$$\text{slope} = \frac{h}{e} \quad\Rightarrow\quad h = e \times \text{slope}$$

$$h = (1.6 \times 10^{-19}\,\mathrm{C}) \times (4.12 \times 10^{-15}\,\mathrm{V\,s})$$

$$h = 6.59 \times 10^{-34}\,\mathrm{J\,s}$$

This is in excellent agreement with the accepted value $$h = 6.63 \times 10^{-34}\,\mathrm{J\,s}$$.

Answer

$$h \approx 6.59 \times 10^{-34}\,\mathrm{J\,s}$$

11.6 The threshold frequency for a certain metal is $$3.3 \times 10^{14} \, \mathrm{Hz}$$. If light of frequency $$8.2 \times 10^{14} \, \mathrm{Hz}$$ is incident on the metal, predict the cut-off voltage for the photoelectric emission.

Solution

Einstein's photoelectric equation can be written in terms of the threshold frequency $$\nu_0$$, since the work function is $$\phi_0 = h\nu_0$$:

$$eV_0 = h\nu - h\nu_0 = h(\nu - \nu_0)$$

Hence the cut-off potential is

$$V_0 = \frac{h(\nu - \nu_0)}{e}$$

Substituting $$\nu = 8.2 \times 10^{14}\,\mathrm{Hz}$$ and $$\nu_0 = 3.3 \times 10^{14}\,\mathrm{Hz}$$:

$$\nu - \nu_0 = (8.2 - 3.3) \times 10^{14}\,\mathrm{Hz} = 4.9 \times 10^{14}\,\mathrm{Hz}$$

$$V_0 = \frac{(6.63 \times 10^{-34}\,\mathrm{J\,s}) \times (4.9 \times 10^{14}\,\mathrm{Hz})}{1.6 \times 10^{-19}\,\mathrm{C}}$$

$$V_0 = \frac{3.25 \times 10^{-19}}{1.6 \times 10^{-19}} \approx 2.0\,\mathrm{V}$$

Answer

$$V_0 \approx 2.0\,\mathrm{V}$$

11.7 The work function for a certain metal is $$4.2 \, \mathrm{eV}$$. Will this metal give photoelectric emission for incident radiation of wavelength $$330 \, \mathrm{nm}$$?

Solution

Photoelectric emission occurs only if the energy of an incident photon is at least equal to the work function $$\phi_0$$ of the metal. Equivalently, the incident wavelength must not exceed the threshold wavelength $$\lambda_0$$.

Energy of an incident photon of wavelength $$\lambda = 330\,\mathrm{nm} = 330 \times 10^{-9}\,\mathrm{m}$$:

$$E = \frac{hc}{\lambda} = \frac{(6.63 \times 10^{-34}) \times (3.0 \times 10^{8})}{330 \times 10^{-9}}$$

$$E = \frac{1.989 \times 10^{-25}}{3.30 \times 10^{-7}} = 6.03 \times 10^{-19}\,\mathrm{J}$$

$$E = \frac{6.03 \times 10^{-19}}{1.6 \times 10^{-19}}\,\mathrm{eV} \approx 3.77\,\mathrm{eV}$$

Comparison. The work function is $$\phi_0 = 4.2\,\mathrm{eV}$$. Since the photon energy is less than the work function,

$$E = 3.77\,\mathrm{eV} \;<\; \phi_0 = 4.2\,\mathrm{eV},$$

each photon carries less energy than is needed to liberate an electron, so no photoelectric emission takes place.

As a check, the threshold wavelength of the metal is

$$\lambda_0 = \frac{hc}{\phi_0} = \frac{1.989 \times 10^{-25}}{4.2 \times 1.6 \times 10^{-19}} \approx 2.96 \times 10^{-7}\,\mathrm{m} \approx 296\,\mathrm{nm}$$

Since the incident wavelength $$330\,\mathrm{nm}$$ is greater than $$\lambda_0 \approx 296\,\mathrm{nm}$$, emission cannot occur — confirming the conclusion.

Answer

No. The photon energy ($$\approx 3.77\,\mathrm{eV}$$) is less than the work function ($$4.2\,\mathrm{eV}$$), so the metal gives no photoelectric emission for $$330\,\mathrm{nm}$$ light.

11.8 Light of frequency $$7.21 \times 10^{14} \, \mathrm{Hz}$$ is incident on a metal surface. Electrons with a maximum speed of $$6.0 \times 10^{5} \, \mathrm{m/s}$$ are ejected from the surface. What is the threshold frequency for photoemission of electrons?

Solution

The maximum kinetic energy of the ejected electrons is

$$K_{\max} = \frac{1}{2} m v_{\max}^2$$

With $$m = 9.11 \times 10^{-31}\,\mathrm{kg}$$ and $$v_{\max} = 6.0 \times 10^{5}\,\mathrm{m/s}$$:

$$K_{\max} = \frac{1}{2} \times (9.11 \times 10^{-31}) \times (6.0 \times 10^{5})^2$$

$$K_{\max} = \frac{1}{2} \times (9.11 \times 10^{-31}) \times (3.6 \times 10^{11}) = 1.64 \times 10^{-19}\,\mathrm{J}$$

By Einstein's photoelectric equation, $$h\nu = h\nu_0 + K_{\max}$$, so the threshold frequency is

$$\nu_0 = \nu - \frac{K_{\max}}{h}$$

$$\frac{K_{\max}}{h} = \frac{1.64 \times 10^{-19}}{6.63 \times 10^{-34}} = 2.47 \times 10^{14}\,\mathrm{Hz}$$

$$\nu_0 = 7.21 \times 10^{14}\,\mathrm{Hz} - 2.47 \times 10^{14}\,\mathrm{Hz}$$

$$\nu_0 \approx 4.74 \times 10^{14}\,\mathrm{Hz}$$

Answer

$$\nu_0 \approx 4.7 \times 10^{14}\,\mathrm{Hz}$$

11.9 Light of wavelength $$488 \, \mathrm{nm}$$ is produced by an argon laser which is used in the photoelectric effect. When light from this spectral line is incident on the emitter, the stopping (cut-off) potential of photoelectrons is $$0.38 \, \mathrm{V}$$. Find the work function of the material from which the emitter is made.

Solution

The energy of a photon of the incident light ($$\lambda = 488\,\mathrm{nm} = 488 \times 10^{-9}\,\mathrm{m}$$) is

$$E = \frac{hc}{\lambda} = \frac{(6.63 \times 10^{-34}) \times (3.0 \times 10^{8})}{488 \times 10^{-9}}$$

$$E = \frac{1.989 \times 10^{-25}}{4.88 \times 10^{-7}} = 4.08 \times 10^{-19}\,\mathrm{J}$$

$$E = \frac{4.08 \times 10^{-19}}{1.6 \times 10^{-19}}\,\mathrm{eV} \approx 2.55\,\mathrm{eV}$$

By Einstein's photoelectric equation, the photon energy is shared between the work function and the maximum kinetic energy of the photoelectrons, the latter equal to $$eV_0$$:

$$E = \phi_0 + eV_0 \quad\Rightarrow\quad \phi_0 = E - eV_0$$

With a stopping potential $$V_0 = 0.38\,\mathrm{V}$$, we have $$eV_0 = 0.38\,\mathrm{eV}$$, so

$$\phi_0 = 2.55\,\mathrm{eV} - 0.38\,\mathrm{eV} = 2.17\,\mathrm{eV}$$

Answer

$$\phi_0 \approx 2.17\,\mathrm{eV}$$

11.10 What is the de Broglie wavelength of

(a) a bullet of mass $$0.040 \, \mathrm{kg}$$ travelling at the speed of $$1.0 \, \mathrm{km/s}$$,

Solution

The de Broglie wavelength of a particle of mass $$m$$ moving with speed $$v$$ is

$$\lambda = \frac{h}{mv}$$

For the bullet, $$m = 0.040\,\mathrm{kg}$$ and $$v = 1.0\,\mathrm{km/s} = 1.0 \times 10^{3}\,\mathrm{m/s}$$, so its momentum is

$$mv = 0.040 \times (1.0 \times 10^{3}) = 40\,\mathrm{kg\,m/s}$$

$$\lambda = \frac{6.63 \times 10^{-34}\,\mathrm{J\,s}}{40\,\mathrm{kg\,m/s}} = 1.7 \times 10^{-35}\,\mathrm{m}$$

Answer

$$\lambda \approx 1.7 \times 10^{-35}\,\mathrm{m}$$

(b) a ball of mass $$0.060 \, \mathrm{kg}$$ moving at a speed of $$1.0 \, \mathrm{m/s}$$, and

Solution

Using $$\lambda = \dfrac{h}{mv}$$ for the ball, with $$m = 0.060\,\mathrm{kg}$$ and $$v = 1.0\,\mathrm{m/s}$$:

$$mv = 0.060 \times 1.0 = 0.060\,\mathrm{kg\,m/s}$$

$$\lambda = \frac{6.63 \times 10^{-34}\,\mathrm{J\,s}}{0.060\,\mathrm{kg\,m/s}} = 1.1 \times 10^{-32}\,\mathrm{m}$$

Answer

$$\lambda \approx 1.1 \times 10^{-32}\,\mathrm{m}$$

(c) a dust particle of mass $$1.0 \times 10^{-9} \, \mathrm{kg}$$ drifting with a speed of $$2.2 \, \mathrm{m/s}$$?

Solution

Using $$\lambda = \dfrac{h}{mv}$$ for the dust particle, with $$m = 1.0 \times 10^{-9}\,\mathrm{kg}$$ and $$v = 2.2\,\mathrm{m/s}$$:

$$mv = (1.0 \times 10^{-9}) \times 2.2 = 2.2 \times 10^{-9}\,\mathrm{kg\,m/s}$$

$$\lambda = \frac{6.63 \times 10^{-34}\,\mathrm{J\,s}}{2.2 \times 10^{-9}\,\mathrm{kg\,m/s}} = 3.0 \times 10^{-25}\,\mathrm{m}$$

In every case (a)-(c) the de Broglie wavelength is far smaller than any measurable length, which is why the wave nature of ordinary macroscopic objects is never observed.

Answer

$$\lambda \approx 3.0 \times 10^{-25}\,\mathrm{m}$$

11.11 Show that the wavelength of electromagnetic radiation is equal to the de Broglie wavelength of its quantum (photon).

Solution

Consider electromagnetic radiation of wavelength $$\lambda$$. Since it travels at speed $$c$$, its frequency is $$\nu = c/\lambda$$.

Energy of its quantum (photon). By Planck's relation,

$$E = h\nu = \frac{hc}{\lambda}$$

Momentum of the photon. A photon is massless and travels at speed $$c$$; from relativity its energy and momentum are related by $$E = pc$$. Hence

$$p = \frac{E}{c} = \frac{hc/\lambda}{c} = \frac{h}{\lambda}$$

de Broglie wavelength of the photon. The de Broglie wavelength of any particle carrying momentum $$p$$ is $$\lambda_{dB} = h/p$$. Substituting the photon momentum found above,

$$\lambda_{dB} = \frac{h}{p} = \frac{h}{\,h/\lambda\,} = \lambda$$

Thus the de Broglie wavelength of a photon is exactly equal to the wavelength of the electromagnetic radiation of which it is the quantum.

$$\lambda_{dB} = \frac{h}{p} = \lambda$$

Answer

Proved: the de Broglie wavelength of a photon, $$\lambda_{dB} = h/p$$, equals the wavelength $$\lambda$$ of the electromagnetic radiation, because the photon's momentum is $$p = h/\lambda$$.
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