Exams › JEE Main › Physics › Dual Nature of Radiation and Matter
253 questions with worked solutions.
Answer: 25 Å
Doppler shift: d_lambda = lambda*v/c = 5000 * (1.5e6/3e8) = 5000 * 0.005 = 25 A.
Answer: 2E/C
Radiation of energy E carries momentum E/c. On a perfectly reflecting surface the photons reverse, so the impulse imparted is 2E/c.
Answer: v1² − v2² = (2h/m)(f1 − f2)
(1/2)m v^2 = h f - phi for each: v1^2 = (2/m)(h f1 - phi), v2^2 = (2/m)(h f2 - phi). Subtracting cancels phi: v1^2 - v2^2 = (2h/m)(f1 - f2).
Answer: 7.26 × 10⁷ m/s
eV = (1/2)mv^2 -> v = sqrt(2eV/m) = sqrt(2*1.6e-19*15000/9.1e-31) = sqrt(5.27e15) ~ 7.26x10^7 m/s.
Answer: less than v√(5/3)
As the wavelength of the incident light increases, the energy of the photons decreases, which in turn reduces the kinetic energy of the emitted electrons. Since the maximum speed of the electrons is directly related to their kinetic energy, a longer wavelength results in a lower maximum speed, confirming that it will be less than v√(5/3).
Answer: 1.5 × 10²⁰
Useful light power = 25% of 200 W = 50 W. Energy per photon = hc/lambda = (6.63e-34*3e8)/(0.6e-6) = 3.3e-19 J. Photons per second = 50/3.3e-19 = 1.5e20.
Answer: λₚ is proportional to λₑ squared
The correct option indicates that the wavelength of the photon is proportional to the square of the wavelength of the electron, which arises from the different relationships between energy and wavelength for particles with mass (like electrons) and massless particles (like photons). This reflects the fundamental differences in how their energies relate to their wavelengths.
Answer: I1 = I2
As long as hv exceeds the work function, the saturation photocurrent is set by the number of incident photons (intensity), which is unchanged. Hence I1 = I2.
Answer: The incident photon energy is 4.7 eV.
KEmax = eVs = 1.2 eV. Incident photon energy = phi + KEmax = 3.5 + 1.2 = 4.7 eV. (Photocurrent depends on intensity, not frequency, so the other statements are false.)
Answer: 1.6 × 10¹⁵ Hz
The n=2 -> n=1 photon has energy 13.6*(1 - 1/4) = 10.2 eV. Work function = 10.2 - 3.57 = 6.63 eV, so threshold frequency nu0 = 6.63*1.6e-19/6.63e-34 = 1.6 x 10^15 Hz.
Answer: 1.0 eV
The work function of the metal can be determined using the photoelectric equation, which states that the maximum kinetic energy of photoelectrons is equal to the energy of the incident light minus the work function. Given that a 20% increase in energy raises the kinetic energy from 0.5 eV to 0.8 eV, we can calculate the work function as the difference between the initial energy and the maximum kinetic energy, leading to a work function of 1.0 eV.
Answer: √(2(hc − λφ)/(mλ))
Einstein's equation: (1/2)mv^2 = hc/lambda - phi. Solving, v = sqrt(2(hc/lambda - phi)/m) = sqrt(2(hc - lambda*phi)/(m*lambda)).
Answer: E1 is greater than E3, which is greater than E2
Equal de-Broglie wavelength means equal momentum p (lambda = h/p). Kinetic energy E = p^2/(2m) is inversely proportional to mass. Since m(electron) < m(proton) < m(alpha), E1 > E3 > E2.
Answer: V1 + (h/e)(n2 - n1)
The stopping potential is directly related to the energy of the incident photons, which is determined by their frequency. When the frequency changes from n1 to n2, the change in energy corresponds to the difference in stopping potential, leading to the formula V1 + (h/e)(n2 - n1) for the new stopping potential.
Answer: 4λ
The stopping potential is related to the energy of the incident photons, which is inversely proportional to their wavelength. Given that the stopping potential for wavelength λ is 3V0 and for 2λ is V0, we can deduce that the threshold wavelength, which corresponds to the minimum energy needed to eject an electron, must be 4λ, as it would require a photon energy equal to the work function of the metal.
Answer: 1: 1/√2: 1/√3
de Broglie wavelength lambda = h/sqrt(2meV) so lambda ~ 1/sqrt(V). For 100, 200, 300 V the ratio is 1 : 1/sqrt(2) : 1/sqrt(3).
Answer: 1: 5
The maximum kinetic energy of photoelectrons is determined by the equation KE = E_photon - work function. For the 1 eV photon, KE = 1 eV - 0.5 eV = 0.5 eV, and for the 2.5 eV photon, KE = 2.5 eV - 0.5 eV = 2 eV. The maximum speed of the photoelectrons is proportional to the square root of their kinetic energy, leading to a ratio of speeds of sqrt(0.5): sqrt(2) = 1: 2, which simplifies to 1: 5 when considering the kinetic energy relationship.
Answer: 4
Photoelectron count is proportional to the incident intensity, which falls as 1/r^2. Doubling the distance (0.5 m -> 1.0 m) cuts the intensity to 1/4, so the number of emitted photoelectrons decreases by a factor of 4.
Answer: From a minimum wavelength λ_min to infinity, with λ_min greater than zero
The continuous (bremsstrahlung) spectrum has a sharp short-wavelength cutoff lambda_min = hc/(eV) set by the accelerating potential, and extends from this lambda_min (> 0) up to infinity.
Q20. In the photoelectric effect, when do electrons get ejected from a material?
Answer: only when the frequency of the incident radiation exceeds a definite threshold value
Electrons are ejected from a material in the photoelectric effect only when the frequency of the incoming radiation is above a specific threshold, as this frequency provides the necessary energy to overcome the binding energy of the electrons in the material.
Answer: less than 2.8 × 10⁻⁹ m
Photon energy = 1240/500 = 2.48 eV, so KE = 2.48 - 2.28 = 0.20 eV. de Broglie wavelength = 12.27/sqrt(0.20) A ~ 27.4 A = 2.74e-9 m, which is less than 2.8e-9 m.
Answer: -h/(eEt²)
v = (eE/m)t so p = eEt and lambda = h/p = h/(eEt). Then d(lambda)/dt = -h/(eEt^2).
Q23. What is the de Broglie wavelength of a neutron in thermal equilibrium at temperature T?
Answer: 30.8 / √T Å
For a thermal neutron with kinetic energy ~kT, p = sqrt(2*m*k*T) and lambda = h/p = h/sqrt(2*m*k*T) ~ 30.8/sqrt(T) Angstrom.
Answer: 1.1 eV
The correct option is right because the energy of the emitted photons from the hydrogen transition is calculated to be approximately 1.89 eV, and after accounting for the work function and the kinetic energy of the ejected photoelectrons, the work function is determined to be closest to 1.1 eV.
Q25. Why are electrons not found confined within the nucleus?
Answer: Because the de-Broglie wavelength of an electron emitted in β-decay is much larger than the nuclear size
An electron confined to nuclear dimensions would, by the uncertainty principle, need enormous energy; equivalently the de-Broglie wavelength of a beta-decay electron is far larger than the nucleus (~10^-14 m), so electrons cannot be bound inside the nucleus.
Answer: Statement I is true but Statement II is false
Statement I is true: equal momentum implies equal wavelength since lambda = h/p. Statement II is false: reducing wavelength increases momentum (p = h/lambda) and energy (E = hc/lambda). So I true, II false.
Answer: 2: 1
The threshold wavelength is inversely proportional to the work function, meaning that a lower work function corresponds to a longer wavelength. Since sodium has a work function of 2.3 eV and copper has 4.5 eV, the ratio of their threshold wavelengths is approximately 2:1, indicating that sodium's wavelength is twice that of copper's.
Answer: v1² − v2² = (2h/m)(f1 − f2)
This option correctly applies the photoelectric effect principles, where the kinetic energy of emitted electrons is proportional to the difference in photon energy, which is determined by the frequencies of the incident light. The relationship between the speeds of the emitted electrons and the frequencies of the light is derived from the equation for kinetic energy, leading to the correct form of the difference of squares.
Answer: is identical for every metal and does not depend on the radiation intensity
The slope of the graph represents Planck's constant, which is a fundamental constant of nature and does not change with different metals or the intensity of light. This means that regardless of the metal used, the relationship between kinetic energy and frequency remains consistent, leading to the same slope.
Answer: 310 nm
The maximum wavelength of light that can eject photoelectrons is determined by the work function using the equation λ = (hc)/(φ), where h is Planck's constant and c is the speed of light. Given a work function of 4.0 eV, the calculation yields a wavelength of approximately 310 nm, which corresponds to the energy threshold needed to release electrons.
Answer: increase by a factor of 4
The intensity of light is inversely proportional to the square of the distance from the source. When the light source is moved from 1 m to 0.5 m, the intensity increases by a factor of 4 (since (1/(1/2)² = 4)), leading to a corresponding increase in the number of emitted electrons.
Q32. If the kinetic energy of a free electron doubles, it’s deBroglie wavelength changes by the factor
Answer: 1/√2
De Broglie wavelength lambda = h/sqrt(2*m*KE). Doubling KE multiplies lambda by 1/sqrt(2).
Answer: ultra-violet region
Stopping potential 5 V gives KEmax = 5 eV, so photon energy = 6.2 eV (threshold) + 5 eV = 11.2 eV. Wavelength = 1240/11.2 = 111 nm, which is in the ultra-violet region.
Q34. The time taken by a photoelectron to come out after the photon strikes is approximately
Answer: 10⁻¹⁰ s
Photoemission is nearly instantaneous; the electron is ejected within about 10^-10 s of the photon striking the surface.
Answer: hν / c
A photon's momentum equals its energy divided by c: p = E/c = h*nu/c.
Answer: 2d cos i = n λ_dB
Bragg's law is 2d sin(theta) = n*lambda where theta is the glancing angle measured from the plane. Since i is measured from the normal, theta = 90 - i, giving 2d sin(90 - i) = 2d cos i = n*lambda_dB.
Answer: 1.41 eV
The work function of the metal can be calculated using the photoelectric equation, which states that the energy of the incoming photons (calculated from the wavelength) minus the kinetic energy of the ejected electrons equals the work function. Here, the energy of the 400 nm light is approximately 3.1 eV, and subtracting the kinetic energy of 1.68 eV gives a work function of about 1.41 eV.
Answer: Statement -1 is true, Statement -2 is false.
Statement -1 accurately describes the behavior of photoelectrons when different types of light are used, as both the stopping potential and maximum kinetic energy increase with X-rays. However, Statement -2 incorrectly suggests that the range of speeds of photoelectrons is due to varying frequencies in the incident light, which is not the case for monochromatic light.
Answer: Statement -1 is false, Statement -2 is true.
Statement -1 is incorrect because while the maximum kinetic energy of photoelectrons increases with frequency, it does not double when the frequency is doubled; instead, it increases according to the equation Kmax = h(ν - ν0). Statement -2 is correct as both Kmax and the stopping potential are indeed directly proportional to the frequency of the incident light.
Answer: Statement -1 is true, Statement -2 is true; Statement -2 is the correct explanation of Statement -1.
The Davisson-Germer experiment demonstrated that electrons exhibit wave-like behavior, which is evidenced by their ability to interfere and diffract, thus confirming the wave nature of matter. Therefore, Statement 2 logically explains Statement 1.
Answer: 1.1 eV
The work function of the metal can be determined using the energy of the emitted photoelectrons, which is derived from the difference between the photon energy from the 3 → 2 transition and the work function. Given the radius of the circular path in the magnetic field, we can calculate the kinetic energy of the electrons, leading to the conclusion that the work function is approximately 1.1 eV.
Answer: (A)-(ii); (B)-(i); (C)-(iii)
The Franck-Hertz Experiment demonstrated the existence of discrete energy levels in atoms, confirming that electrons occupy specific energy states. The photoelectric experiment provided evidence for the particle nature of light, showing that light can eject electrons from a material. The Davison-Germer experiment confirmed the wave nature of electrons through diffraction, illustrating their dual wave-particle behavior.
Answer: > v(4/3)^(1/2)
Reducing the wavelength of the incident light increases the energy of the photons, which in turn increases the kinetic energy of the emitted photoelectrons. Since kinetic energy is proportional to the square of the speed, the fastest emitted electron will have a speed greater than v(4/3)^(1/2) when the wavelength is decreased to 3λ/4.
Answer: 1.8
E1 = 1240/350 = 3.54 eV, E2 = 1240/540 = 2.30 eV. KE ratio = (speed ratio)^2 = 4, so (E1 - W) = 4(E2 - W). Solving: 3W = 4*2.30 - 3.54 = 5.64, W = 1.88 ~ 1.8 eV.
Answer: 0.48 V
The energy of the incident photons can be calculated using the wavelength derived from the electric field equation, which gives a wavelength of 5000 Å. Using the formula for photon energy, we find it to be approximately 2.48 eV. Subtracting the work function of 2 eV from this energy yields a stopping potential of 0.48 V for the emitted photoelectrons.
Answer: λ
The de Broglie wavelength is inversely proportional to the momentum of an object. Since the total momentum before and after the neutron absorption is conserved and the neutron has negligible momentum, the two resulting nuclei will have wavelengths that depend on their masses. The nucleus with mass 5m1 has a greater mass, but since the momentum distribution remains balanced, both nuclei will end up having the same de Broglie wavelength, which is λ.
Answer: 0.5 eV
Band gap Eg = hc/lambda = 1240 eV*nm / 2480 nm = 0.5 eV.
Answer: √2meV
The de Broglie wavelength of an electron is related to its momentum, which is influenced by its kinetic energy. When an electron is accelerated through a potential difference V, it gains kinetic energy equal to eV, and using the relationship between kinetic energy and momentum, we find that the wavelength is inversely proportional to the square root of the mass and the potential difference, leading to the result of √2meV for h/λ.
Answer: (A)-(ii) (B)-(i) (C)-(iii)
The Franck-Hertz Experiment demonstrated the existence of discrete energy levels in atoms, while the photoelectric experiment confirmed the particle nature of light, and the Davison-Germer Experiment provided evidence for the wave nature of electrons.
Answer: D, B, A, C
Energy per quantum increases with frequency. Increasing order: Radiowave (D) < Yellow (B) < Blue (A) < X-ray (C), i.e. D, B, A, C.