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Revision: Dual Nature of Radiation and Matter >> Dual Nature of Radiation and Matter Physics (Theory) ISC (Science) ISC Class 12 CISCE

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Definitions [9]

Definition: Photoelectric Effect

The phenomenon of emission of electronsfrom metals under the effect of light is called 'photoelectric effect'.

Definition: Work Function

The minimum energy required for the emission of photoelectron from a metal is called the 'work function' of that metal.

Definition: Stopping Potential

The negative potential of P2 (relative to P1) at which the photoelectric current becomes zero is called 'stopping potential' or 'cut-off potential'.

Definition: Threshold Frequency or Cut-off Frequency

The lowest frequency of light which can emit photoelectrons from a material is called the 'threshold frequency' or 'cut-off frequency' of that material.

Definition: Intensity of Wave

The energy crossing per unit area per unit time perpendicular to the direction of propagation of wave is called the intensity of wave.

Definition: Matter Waves

According to de-Broglie, all material particles in motion have wave nature. The waves associated with moving particles of matter are called ‘de-Broglie waves' or 'matter waves'.

Definition: X-rays

X-rays are electromagnetic waves having wavelengths from 0.5 Å to 15 Å. X-rays of long wavelength are called soft X-rays and those of short wavelength are called hard X-rays.

Definition: Bremstrahlung or Braking Radiation

The continuous X-rays are produced by the slowing or braking down of the incident charged particles, the radiations are called bremstrahlung or braking radiation.

Definition: Compton Scattering

The scattering of a photon by an electron is called the Compton effect. This effect verifies quantum theory and particle nature of electromagnetic waves. The longer wavelength in the scattered beam are called Compton lines.

Formulae [7]

Formula: Photon Emission Rate

n = \[\frac {Pλ}{h c}\]

Formula: Kinetic Mass of Photon

m = \[\frac {E}{c^2}\] = \[\frac {hv}{c^2}\] = \[\frac {h}{cλ}\]

Formula: Momentum of Photon

p = \[\frac {E}{c}\] = \[\frac {h}{λ}\]

Formula: Radiation Power (Photon Form)

P = nh\[\frac {c}{λ}\]

Formula: de-Broglie Wavelength of Electron

λ = \[\frac {12.27}{\sqrt {V}}\]Å = \[\sqrt{\frac{150}{V}}\]Å

Formula: de Broglie Wavelength

λ = \[\frac {h}{p}\]

OR

λ = \[\frac {h}{mv}\]

Formula: Maximum Kinetic Energy of Electrons

vmax = \[\frac {1}{2}\]mv2 = hvmax

Theorems and Laws [2]

Law: Laws of Photoelectric Emission
  1. The rate of emission of photoelectrons from the surface of a metal varies directly as the intensity of the incident light falling on the surface.
  2. The maximum kinetic energy of the emitted photoelectrons is independent of the intensity of the incident light.
  3. The maximum kinetic energy of the photoelectrons increases linearly with an increase in the frequency of the incident light.
  4. If the frequency of the incident light is below a certain lowest value, then no photoelectron is emitted from the metal. This lowest frequency (threshold frequency) is different for different metals.
  5. As soon as the light is incident on the surface of the metal, the photoelectrons are emitted instantly; that is, there is no time-lag between the incidence of light and the emission of electrons.
Law: Moseley’s Law

Statement

The frequency of a spectral line in the X-ray spectrum varies as the square of the atomic number of the element emitting it.

\[\sqrt ν\] = k(Z − b)

or

ν = constant (Z − b)2

where
Z = atomic number,
b = screening factor,
k = constant.

Proof / Explanation:

Moseley studied characteristic X-rays emitted by different elements used as targets in an X-ray tube and determined their frequencies.

He plotted a graph with:

  • Atomic number Z on the x-axis

  • Square root of frequency \[\sqrt ν\] on the y-axis

For Kα and Kβ lines, the graph was a straight line.

Thus,

\[\sqrt ν\] ∝ (Z − b)

or

ν ∝ (Z − b)2

For Kα line:

ν = \[\frac {1}{4}\]Rc(Z−1)2

This is similar to Bohr’s formula and shows that Kα radiation is produced by the transition of an electron from the L-shell (n = 2) to the K-shell (n = 1). The term (Z−1) appears because one electron is removed from the K-shell.

Conclusion:

The frequency of characteristic X-rays depends on the atomic number of the element.

Importance of Moseley’s Law:

  1. It proved that atomic number, not atomic weight, determines the physical and chemical properties of elements.
  2. It helped refine the periodic table.
  3. It helped in the discovery of new elements such as hafnium, illinium, and rhenium.
  4. It helped to determine the atomic numbers of rare-earth elements and fix their correct positions in the periodic table.

Key Points

Key Points: Photoelectric Effect
  • Hertz (1887) observed that ultraviolet light makes electric discharge easier from a metal surface.
  • Hallwachs’ experiment showed that current flows only when ultraviolet light strikes the negative plate, not the positive plate.
  • J.J. Thomson (1898) proved that light falling on a metal surface causes the emission of electrons.
  • Lenard (1900) explained that electrons emitted from the negative plate are attracted to the positive plate, producing current.
  • Short-wavelength (high-frequency) light is more effective in producing photoelectric emission than long-wavelength light.
Key Points: Hertz and Lenard's Observations
  • Photoelectric current increases with incident light intensity when the frequency is kept constant.
  • For sufficiently high anode potential, the photoelectric current reaches a maximum (saturation current).
  • Stopping potential is independent of light intensity and depends on the maximum kinetic energy of photoelectrons.
  • A higher frequency of incident light produces photoelectrons with greater maximum kinetic energy.
  • No photoelectric emission occurs below a certain frequency, regardless of the intensity or duration of light.
Key Points: Determination of Planck's Constant

  • A graph of stopping potential V0 versus frequency ν is a straight line, showing a linear relation between them.
  • The slope of the V0 ν graph equals h/e, hence Planck’s constant h can be determined using the known value of electronic charge e.
Key Points: Properties of Photons
  • Radiation behaves like a stream of particles called photons during interaction with matter.
  • Photons travel in straight lines at the speed of light.
  • Each photon has energy E = hν = \[\frac {hc}{λ}\] and momentum p = \[\frac {E}{c}\].
  • On a change of medium, the speed and wavelength of a photon change, but its frequency remains constant.
  • Photon energy is independent of light intensity; higher intensity means more photons per second.
  • A photon has zero rest mass, but an equivalent mass given by
  • m = \[\frac {h}{cλ}\]
  • Photons are electrically neutral and are not deflected by electric or magnetic fields.
  • In photon–particle collisions, total energy and momentum are conserved.
  • A photon retains its identity until absorbed by an atom, after which its identity is lost.
Key Points: Failure of Wave Theory
  • Wave theory fails because it predicts that electron energy should increase with light intensity, but experiments show that it does not.
  • Wave theory cannot explain the existence of a threshold frequency, below which no photoelectrons are emitted.
  • Wave theory predicts a time lag in emission, but photoelectrons are emitted instantaneously.
Key Points: Planck's Photon Hypothesis
  • Wave theory failed to explain experimental observations of the photoelectric effect.
  • Black-body radiation contains all wavelengths, and classical theories could not explain its energy distribution.
  • Planck proposed that radiation is emitted discontinuously in small energy packets, now known as quanta (photons).
  • The energy of a photon is hνh\nuhν, and radiation energy is emitted only in integral multiples of hνh\nuhν.
  • Einstein (1905) explained the photoelectric effect using Planck’s photon hypothesis.
Key Points: Photoelectric Equation
  • Light consists of photons, each having energy hνh\nuhν; light intensity depends on the number of photons.
  • A photon transfers its entire energy to a single electron during photoelectric emission.
  • Part of the photon energy is used to overcome the work function, and the rest appears as kinetic energy of the electron.
  • Electrons emitted from the metal surface have maximum kinetic energy because they experience no energy loss in collisions.
  • Einstein’s photoelectric equation is
    Ek = hν − W = h(ν − ν0)
  • Increasing light intensity increases the number of photoelectrons, but not their maximum kinetic energy.
  • Photoelectric emission is instantaneous, and Einstein’s explanation fully accounts for all laws of the photoelectric effect.
Key Points: de-Broglie Wavelength
  • de Broglie proposed that moving material particles have an associated wave nature, analogous to that of photons.
  • The wavelength decreases with an increase in momentum or mass, and increases when the particle’s velocity decreases.
  • Matter waves exist only for moving particles and are independent of whether the particle is charged or uncharged, showing they are not electromagnetic in nature.
Key Points: Particle Nature of Radiation
  • Interference, diffraction, and polarisation are explained by the wave nature of radiation, whereas the photoelectric and Compton effects require the particle (photon) nature of radiation.
  • Radiation exhibits dual behaviour, behaving as a wave or a particle depending on the experimental context.
  • Planck (1900) proposed that radiation is emitted in discrete packets of energy, now known as photons.
  • Each photon has definite energy E = hν and momentum p = \[\frac {hν}{c}\], moving with the speed of light.
  • A photon has zero rest mass, but has kinetic (equivalent) mass \[\frac {hv}{c^2}\].
  • For a given frequency, all photons have the same energy and momentum, irrespective of intensity.
  • In photon–particle collisions, energy and momentum are conserved, and photons may be absorbed or newly created.
Key Points: Davisson–Germer Experiment (Electron Diffraction)
  • Davisson and Germer (1927) experimentally demonstrated electron diffraction, confirming the wave nature of electrons.
  • In the experiment, electrons accelerated by a potential difference are directed onto a nickel crystal, and the diffracted electrons are detected using a Faraday cylinder.
  • A prominent intensity peak (bump) is observed for electrons accelerated through 54 V, indicating diffraction.
  • The wavelength calculated using the de Broglie hypothesis matches closely with the wavelength obtained from Bragg’s diffraction condition.
  • The experiment directly verifies de Broglie’s hypothesis, demonstrating that moving particles exhibit wave-like behaviour.
Key Points: Production, Intensity and Quality of X-Rays
  • Coolidge X-ray tube (1913) uses thermionic emission—electrons are produced by heating a tungsten filament in a vacuum.
  • Electrons are accelerated by a high potential difference and strike a tungsten or molybdenum target, producing X-rays.
  • About 99.8% of the electron energy converts into heat, so copper mounting and water/oil cooling are used.
  • The intensity of X-rays depends on the filament current, which controls the number of electrons hitting the target.
  • The quality (penetrating power) of X-rays depends on the anode potential; a higher anode potential produces hard X-rays, a lower potential produces soft X-rays.
Key Points: Properties of X-Rays
  • X-rays are electromagnetic waves with wavelengths from 0.01 nm to 10 nm, overlapping UV and gamma rays.
  • They travel in straight lines with the speed of light.
  • X-rays are uncharged, so they are not deflected by electric or magnetic fields.
  • X-rays affect photographic plates.
  • They ionise gases through which they pass.
  • X-rays produce fluorescence in substances like barium platinocyanide and zinc sulphide.
  • X-rays show wave properties such as reflection, diffraction, interference, and polarisation.
  • X-rays are highly penetrating, can produce the photoelectric effect, and prolonged exposure is harmful to human tissues.
Key Points: X-Ray Spectra
  • A continuous spectrum consisting of radiations of all possible wavelengths with a lower wavelength limit.
  • A line spectrum or characteristic spectrum consisting of definite wavelengths superimposed on the continuous spectrum. The spectral lines are characteristic of the material used. 
key Points: Duane and Hunt Relation
  • Let λmin be the minimum wavelength of the X-ray corresponding to the maximum frequency vmax· This limiting value of X-rays is independent of the material of the target.
Key Points: Origin of Line Spectra
  • X-rays have very high energy and can remove inner-shell electrons, unlike optical light, which excites outer electrons.
  • Characteristic X-rays are produced when an inner electron is knocked out, and a higher-level electron fills the vacancy.
  • K-series lines (Kα, Kβ, Kγ) are formed when electrons fall to the K-shell from L, M, and N shells.
  • X-rays are produced either by bombarding a metal target with high-speed electrons or by using high-energy primary X-rays.
  • A minimum high voltage is required to eject inner-shell electrons; otherwise, no X-ray line spectrum is produced.
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