Quantum Physics: Chapter 2

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Questions and Answers

What is the fundamental assumption in applying the Rayleigh-Jeans law to blackbody radiation?

  • Electromagnetic radiation is emitted in continuous waves. (correct)
  • The intensity of radiation decreases exponentially with wavelength.
  • The blackbody is in thermal equilibrium with its surroundings at all times.
  • Energy is quantized, existing only in discrete packets.

Under what conditions does Planck's Law approximate the classical Rayleigh-Jeans Law for blackbody radiation?

  • At extremely short wavelengths and low temperatures.
  • At extremely long wavelengths and high temperatures. (correct)
  • At extremely long wavelengths and low temperatures.
  • At extremely short wavelengths and high temperatures.

What is the significance of the constant 'h' as introduced by Planck in the context of blackbody radiation?

  • It represents the energy per unit volume of the blackbody.
  • It links the energy of a photon to its frequency. (correct)
  • It determines the speed of light in a vacuum.
  • It is the proportionality constant in Stefan's Law.

In the photoelectric effect, what determines the kinetic energy of the emitted electrons?

<p>Both the frequency of the incident light and the work function of the metal. (B)</p> Signup and view all the answers

What experimental observation regarding the photoelectric effect could not be explained by classical physics but is accounted for by quantum theory?

<p>The existence of a threshold frequency below which no electrons are emitted, regardless of the light's intensity. (D)</p> Signup and view all the answers

How does the quantum mechanical interpretation of light explain the instantaneous emission of electrons in the photoelectric effect, even at low intensities?

<p>Each photon carries discrete energy; electrons are ejected when a single photon transfers sufficient energy to overcome the work function. (C)</p> Signup and view all the answers

Which aspect of the Compton Effect provides evidence for the particle-like nature of electromagnetic radiation?

<p>The conservation of both energy and momentum in the scattering process, as if the photon were a particle. (C)</p> Signup and view all the answers

In the Compton scattering, if the scattering angle increases, what happens to the energy of the scattered photon?

<p>The energy of the scattered photon decreases. (D)</p> Signup and view all the answers

The de Broglie hypothesis posits that matter has a wave-like nature. What happens to the de Broglie wavelength of a particle as its momentum increases?

<p>The de Broglie wavelength decreases linearly with momentum. (A)</p> Signup and view all the answers

In the Davisson-Germer experiment, what phenomenon observed in the scattering of electrons provided evidence for the wave nature of electrons?

<p>The observation of specific scattering angles at which the intensity of scattered electrons was maximum. (B)</p> Signup and view all the answers

How is the concept of a 'wave packet' used to reconcile the wave-particle duality in quantum mechanics?

<p>It represents a particle as a superposition of waves, localized in space, with properties of both waves and particles. (C)</p> Signup and view all the answers

If the group velocity of a wave packet representing a particle is known, what physical quantity does this velocity correspond to?

<p>The classical velocity of the particle. (C)</p> Signup and view all the answers

What is the key implication of the Heisenberg Uncertainty Principle regarding simultaneous measurements of a particle's position and momentum?

<p>It is fundamentally impossible to know both the exact position and the exact momentum of a particle at the same time. (B)</p> Signup and view all the answers

According to the Heisenberg Uncertainty Principle, if the uncertainty in the energy of a quantum state decreases, what happens to the uncertainty in the time at which the system occupies that state?

<p>The uncertainty in time increases. (C)</p> Signup and view all the answers

How does the phenomenon of electron diffraction differ fundamentally from the diffraction of classical waves, such as light?

<p>Electron diffraction demonstrates wave-particle duality for matter, which has no direct analogue in classical wave phenomena. (D)</p> Signup and view all the answers

What is the physical significance of the 'work function' in the context of the photoelectric effect, and how does it influence electron emission?

<p>It represents the minimum energy required to remove an electron from the metal surface and determines the threshold frequency for photoemission. (A)</p> Signup and view all the answers

In the context of quantum mechanics, which scenario best exemplifies the principle of quantization?

<p>An electron transitioning between discrete energy levels in an atom. (A)</p> Signup and view all the answers

Consider a scenario where the wavelength of incident photons in Compton scattering is significantly larger than the Compton wavelength. How would this affect the energy transfer?

<p>The energy transfer would be minimal, and the wavelength shift of the scattered photon would be negligible. (A)</p> Signup and view all the answers

What is the underlying reason why classical physics fails to accurately describe blackbody radiation at short wavelengths?

<p>Classical physics assumes that energy can be divided into arbitrarily small amounts, leading to the ultraviolet catastrophe. (D)</p> Signup and view all the answers

How does the concept of wave-particle duality influence the design and interpretation of modern quantum experiments?

<p>It necessitates the design of experiments that consider both wave-like and particle-like behaviors, understanding that quantum entities exhibit both aspects. (B)</p> Signup and view all the answers

Flashcards

Black-body radiation

Electromagnetic radiation emitted by a black body.

Stefan's Law

The energy emitted by hotter objects is more than colder ones.

Wien's Displacement Law

The peak wavelength shifts shorter as black body temperature increases.

Ultraviolet catastrophe

An incorrect theory that predicts infinite energy output at short wavelengths.

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Energy of oscillator

Energy of an oscillator in cavity walls.

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Photoelectric Effect

Ejection of electrons from a metal surface by electromagnetic radiation.

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Photons

Light consists of discrete energy packets.

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E = hf

The relationship between a photon's energy and frequency.

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Compton Effect

Change in wavelength when X-rays scatter off free electrons.

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Compton Shift Formula

The formula for the change in photon wavelength after Compton scattering.

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Wave-particle duality

Light exhibits wave and particle properties.

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de Broglie wavelength

Wavelength of a particle

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Davisson-Germer experiment

Evidence verifying de Broglie's hypothesis.

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Wave packet

A localized wave resulting from constructive interference

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Phase speed

Speed with which individual wave crests move.

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Group speed

Speed of the overall wave packet.

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Double-Slit Experiment

Wave nature reappears by interference effects in the form of particle distribution

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Heisenberg uncertainty principle

It is impossible to know both position and momentum simultaneously with infinite accuracy

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Heisenberg uncertainty principle

One more relation expressing uncertainty principle is related to energy and time which is given by

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Study Notes

  • Chapter 2 explores Quantum Physics

Objectives

  • To learn experimental results explained by the particle theory of electromagnetic waves
  • To learn the particle properties of waves and the wave properties of particles
  • To understand the uncertainty principle

Blackbody Radiation and Planck's Hypothesis

  • Electromagnetic radiation emitted by a black body is called black-body radiation

Basic Laws of Radiation

  • All objects emit radiant energy
  • Hotter objects emit more energy per unit area than colder ones.
  • Stefan's Law: P = σAeT⁴, where P is power, σ is the Stefan-Boltzmann constant, A is the surface area, e is the emissivity, and T is temperature
  • The peak of the wavelength distribution shifts to shorter wavelengths as black body temperature increases
  • Wien's Displacement Law: λmT = constant
  • Rayleigh-Jeans Law states the intensity or power per unit area I(λ,T)dλ emitted in the wavelength interval λ to λ+dλ from a blackbody: I(λ,T) = (2πckBT) / λ⁴
  • Rayleigh-Jeans Law agrees with experimental measurements only for long wavelengths
  • Rayleigh-Jeans Law predicts an energy output that diverges towards infinity as wavelengths become smaller, known as the ultraviolet catastrophe.
  • Planck's Law states the intensity or power per unit area I(λ,T)dλ emitted in the wavelength interval λ to λ+dλ from a blackbody: I(λ,T) = (2πhc²/λ⁵) * (1 / (e^(hc/λkT) - 1) )
  • Assumptions of Planck's Law include energy of an oscillator in cavity walls being given by En = nhf
  • Emission/absorption of energy will be integral multiples of hf, where h is Planck's constant and f is frequency
  • Planck's Law resolves the ultraviolet catastrophe because the denominator tends to infinity faster than the numerator (λ⁻⁵), thus aligning with experimental observations: I(λ, T) → 0 as λ → 0
  • For very large λ, I(λ, T) → 0 as λ → ∞, which can be approximated by the equation exp(hc/λkT) - 1 ≈ hc/λkT, leading to I(λ, T) → 2πcλ⁻⁴kT
  • Planck's constant was derived from a fit between Planck's law and experimental data: h = 6.626 × 10⁻³⁴ J·s

Photoelectric Effect

  • Photoelectric Effect is the ejection of electrons from the surface of certain metals when irradiated by electromagnetic radiation of suitable frequency
  • Classical predictions for the photoelectric effect: electron ejection should be frequency independent, KE of electrons should increase with light intensity, measurable time interval between incidence of light and ejection of photoelectrons, and KMAX should not depend on the incident light frequency.
  • Experimental observations of the photoelectric effect: no photoemission below threshold frequency, KMAX is independent of light intensity, effect is instantaneous, KE of the most energetic photoelectrons is KMAX = eΔVs and increases with increasing frequency.

Einstein's Interpretation

  • Classical predictions contradict actual experimental results
  • Electromagnetic waves carry discrete energy packets called photons
  • The energy E per packet depends on frequency f: E = hf
  • More intense light corresponds to more photons, not higher energy photons
  • Each photon moves in vacuum at the speed of light (c = 3 × 10⁸ m/s) and carries a momentum p = E/c
  • Einstein's photoelectric equation: Kmax = hf − ϕ, where ϕ is the work function.

Compton Effect

  • When X-rays are scattered by free/nearly free electrons, they suffer a change in their wavelength which depends on the scattering angle
  • Classical predictions regarding the effect of oscillating electromagnetic waves on electrons include: oscillations in electrons in all directions, radiation pressure causing electrons to accelerate in the direction of propagation, different electrons moving at different speeds after the interaction, and the scattered wave frequency showing Doppler-shifted values.
  • Photon is treated as a particle having energy E = hf = hc/λ₀ and zero rest energy
  • In the scattering process, the total energy and total linear momentum of system is conserved
  • λ₀ = wavelength of the incident photon
  • p₀ = h/λ₀ = momentum of the incident photon
  • E₀ = hc/λ₀ = energy of the incident photon
  • λ' = wavelength of the scattered photon
  • p' = h/λ' = momentum of the scattered photon
  • E' = hc/λ' = energy of the scattered photon

Compton Shift

  • Conservation of energy in Compton scattering: E₀ = E' + K
  • Conservation of momentum: p₀ = p'cosθ + pcosΦ (x-component) and 0 = p'sinθ − psinΦ (y-component)
  • Relativistic equations: v = speed of electron, m = mass of electron, p = γmv = momentum of the electron
  • γ = 1 / √(1 - v²/c²), E = √(p²c² + m²c⁴) = total relativistic energy of the electron
  • K = E − mc² = kinetic energy of the electron
  • The Compton shift formula: λ' − λ₀ = h/mc (1 − cosθ)

Photons and Electromagnetic Waves

  • Light exhibits diffraction and interference phenomena explicable in terms of wave properties
  • The Photoelectric effect and Compton Effect can only be explained taking light as photons/particles
  • Light's true nature is best described by considering both wave and particle nature together, which complement each other.

de Broglie Hypothesis

  • Wavelength associated with a particle of mass m moving with velocity v: λ = h/p = h/mv
  • The momentum (p) of an electron accelerated through a potential difference of ΔV: p = mv = √(2meΔV)
  • Frequency of the matter wave associated with the particle: f = E/h, where E is the total relativistic energy of the particle.

Davisson and Germer Experiment

  • Davisson and Germer Experiment verified the de Broglie hypothesis
  • Central assumption: electron as a wave
  • Idea: determine the wavelength of the electron using Bragg's diffraction law and compare it with the de Broglie's wavelength
  • A beam of electrons is produced by a heated filament and accelerated by a potential V (around 54V)
  • The electron beam is then scattered by a nickel crystal
  • Intensities of the scattered electrons are measured as a function of the angle $
  • The angle $ is between the incident beam and the scattered beam
  • Bragg's diffraction law: d sin φ = nλ
  • d is the inter-atomic spacing in nickel which is roughly 0.215 nm
  • For the first diffraction maximum, n equals 1
  • Substituting experimental numbers, the electron wavelength is approximately λ = 0.165 nm
  • Conservation of energy is used to calculate the electron wavelength according to de Broglie's hypothesis: ½mv² = eV
  • The momentum of the electron is defined p = mv = √(2meV)
  • Wavelength is defined as λ= h/p, which expands to h/(mv) further expands to h/√(2meV)
  • Substituting, for V=54 V, the result is λ = 0.167 nm
  • The derived wavelength agrees with that from the Bragg's diffraction law

Quantum Particle

  • Adding a large number of waves with constructive interference in a small localized region of space forms a wavepacket, representing a quantum particle
  • Mathematical representation of a wave packet formed by two waves:
  • y₁ = A cos(k₁x − ω₁t) and y₂ = A cos(k₂x − ω₂t), where k = 2π/λ and ω = 2πf
  • The resultant wave is given by y = y₁ + y₂
  • y = 2A[cos((Δk/2)x − (Δω/2)t) cos(((k₁+k₂)/2)x − ((ω₁+ω₂)/2)t)], where Δk = k₁ − k₂ and Δω = ω₁ − ω₂
  • Phase speed: the speed with which wave crest of individual wave moves, (vp = fλ) or (vp = ω/k)
  • Group speed: the speed of the wave packet, (vg= Δω/Δk)
  • Relation between group speed (vg) and phase speed (vp)is vp = ω/k = fλ, where ω = kvp
  • vg = dw/dk = d(kvp)/dk = k (dvp/dk) + vp
  • By substituting for k, vg = vp − λ( dvp/dλ)
  • The relation between group speed (vg) and particle speed (u): ω = 2πf = (2π/h)E, and k = (2π/λ) = p/(h/π) = 2πp/h
  • vg = dw/dk = (2π/h) dE/dp
  • For a classical particle moving with speed u, the kinetic energy E is given by E = (½)mu² = p²/2m and dE = (2p dp)/2m, or dE/dp = p/m = u
  • Group velocity is defined as vg = dw/dk= dE/dp= u

Double-Slit Experiment Revisited

  • d sin θ = mλ, where m is the order number and λ is the electron wavelength
  • Electrons are detected at localized spots on the detector screen
  • The probability of arrival at the spot is determined by finding the intensity of two interfering waves

Uncertainty Principle

  • Heisenberg uncertainty states it is fundamentally impossible to make simultaneous measurements of a particle's position and momentum with infinite accuracy, (Δx)(Δpx) ≥ h/4π
  • A relation stating the uncertainty principle related to energy and time is (ΔE)(Δt) ≥ h/4π.

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