Quantum Mechanics: Electric and Magnetic Fields

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Questions and Answers

Which of the following best describes the relationship between electric and magnetic fields?

  • They are strongly interconnected, especially when time-dependent. (correct)
  • Magnetic fields can be isolated while electric fields cannot.
  • Electric fields create magnetic monopoles.
  • They are independent and do not influence each other.

What is the physical significance of the electric potential at a point?

  • The force exerted on a positive charge at that point.
  • The work done in bringing a unit positive charge from infinity to that point. (correct)
  • The charge density at that point.
  • The kinetic energy of an electron at that point.

According to Maxwell's equations, what phenomenon does the term $\mu_0\epsilon_0 \frac{\partial \vec{E}}{\partial t}$ in the Ampere-Maxwell law represent?

  • The electric field generated by a stationary charge.
  • The magnetic force on a moving charge.
  • The displacement current due to a time-varying electric field. (correct)
  • The flow of current through a conductor.

Which of the following statements is a consequence of Gauss's law for magnetic fields?

<p>Magnetic field lines always form closed loops. (C)</p> Signup and view all the answers

What does the Poynting vector describe in the context of electromagnetic waves?

<p>The energy flux (energy per unit area per unit time) and direction of energy flow. (B)</p> Signup and view all the answers

Which of the following best describes blackbody radiation?

<p>Radiation emitted by an object that absorbs all incident electromagnetic radiation. (C)</p> Signup and view all the answers

What was the key assumption made by Max Planck that resolved the ultraviolet catastrophe in blackbody radiation theory?

<p>Energy is emitted and absorbed in discrete packets called quanta. (D)</p> Signup and view all the answers

In the context of atomic spectra, what do Fraunhofer lines represent?

<p>Absorption lines in the solar spectrum caused by elements in the sun's atmosphere. (D)</p> Signup and view all the answers

How did Einstein explain the photoelectric effect?

<p>By postulating that light consists of particles called photons, each with energy E=hv. (C)</p> Signup and view all the answers

What is the Compton effect?

<p>The change in wavelength of X-rays when they are scattered by matter. (C)</p> Signup and view all the answers

In Compton scattering, what factors determine the Compton shift (change in wavelength)?

<p>The angle of scattering. (D)</p> Signup and view all the answers

According to de Broglie's hypothesis, what property is associated with matter in motion?

<p>Wave-like behavior (C)</p> Signup and view all the answers

What phenomenon did Davisson and Germer's experiment demonstrate?

<p>The wave nature of electrons. (A)</p> Signup and view all the answers

In the double-slit experiment with electrons, what is observed when electrons are sent through the slits one at a time?

<p>An interference pattern builds up over time, even though each electron passes through individually. (C)</p> Signup and view all the answers

What is a wave packet in quantum mechanics?

<p>A superposition of waves with slightly different frequencies and wavelengths, resulting in a localized wave. (C)</p> Signup and view all the answers

What is the physical significance of the group velocity of a wave packet?

<p>It represents the speed at which the overall shape of the wave packet propagates, corresponding to the particle's velocity. (C)</p> Signup and view all the answers

According to the Heisenberg uncertainty principle, what is the fundamental limit on the precision with which certain pairs of physical properties of a particle, such as position and momentum, can be known?

<p>The product of the uncertainties in these properties must be greater than or equal to a certain value ($\hbar/2$). (A)</p> Signup and view all the answers

What is the primary implication of the Heisenberg uncertainty principle for the possibility of an electron existing inside the nucleus?

<p>It suggests that if an electron were confined within the nucleus, its momentum and hence kinetic energy would be so high that it's unlikely to be bound there. (D)</p> Signup and view all the answers

What are the key requirements for a wave function to be considered well-behaved?

<p>It must be finite, single-valued, continuous, and normalizable. (D)</p> Signup and view all the answers

In the context of quantum mechanics, what does it mean for a wave function to be normalizable?

<p>The integral of the absolute square of the wave function over all space is equal to 1, representing the total probability of finding the particle. (C)</p> Signup and view all the answers

What is the significance of operators in quantum mechanics?

<p>They are used to extract physical observables from the wave function. (D)</p> Signup and view all the answers

In quantum mechanics, what is the expectation value of an observable?

<p>The average value of the observable that would be obtained from a large number of identical measurements. (B)</p> Signup and view all the answers

What is the time-independent Schrödinger equation used to find?

<p>The energy eigenvalues and stationary states of a quantum system. (A)</p> Signup and view all the answers

For a free particle (experiencing no external forces), what can be said about its energy according to the Schrödinger equation?

<p>The energy can take any continuous value. (B)</p> Signup and view all the answers

Flashcards

Electric Fields

Electric fields result from electric charges; charges can be isolated and are either positive or negative.

Magnetic Fields

Magnetic fields usually arise from dipoles (north and south poles) that cannot be isolated from each other.

Maxwell's Equations

Maxwell's equations (1860) summarize electric and magnetic fields and paved the way for electromagnetic wave descriptions.

Gauss's Law (Electric)

Describes how divergence of the electric field relates to charge density.

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Gauss's Law (Magnetic)

The divergence of the magnetic field is uniformly zero, implying the absence of magnetic monopoles.

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Faraday's Law

The curl of the electric field is equal to the rate of change of the magnetic field.

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Ampere-Maxwell Law

The magnetic field's curl is determined by current density and displacement current.

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Electromagnetic Waves

Light can be treated as electromagnetic waves where electric and magnetic vectors are mutually perpendicular.

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Energy of EM Waves

Energy of EM waves is proportional to the amplitude squared, independent of frequency.

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Black Body

Gustav Robert Kirchhoff studied absorption properties; black bodies absorb all incident rays.

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Cavity Radiation

A heated cavity emits radiation of every possible frequency, limited by absorption rate.

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Planck's Energy Quantization

Energy of harmonic oscillator is restricted to multiples of fundamental frequency times a constant (h)

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Atomic Spectra

Atoms of different elements have distinct spectra, allowing elemental identification and spectrum analysis.

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Photoelectric effect

Emission of electrons happen when radiation of appropriate wavelenths interacts with matter

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Photons Explanation

Einstein explained the effect considering light to behave as particles called photons.

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Compton Effect

Arthur H Compton found that scattered X-rays have different wavelengths compared to incident wavelength.

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Compton's particle treatment

Compton treated these problems as particle-particle collisions.

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De Broglie Wavelength

Objects in motion exhibit wave properties with wavelength inversely proportional to momentum.

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Wave Packets

Use superposition of waves to estimate position and momentum of a moving particle.

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Phase Velocity

The phase velocity is the velocity of an arbitrary point marked on the wave

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Group velocity

Velocity that describes the wave group is the average in the amplitude of pulses

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Heisenberg Uncertainty Principle

Cannot simultaneously know position and momentum exactly.

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Heisenberg's Gamma ray microscope

Illustrated with thought experiment about using light to 'see' electrons.

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Good wave function characteristics

Must be finite, continuous, and single valued

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Superposition of wave functions

Linear combinations solve SWE.

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Study Notes

  • Unit I: Review of Concepts Leading to Quantum Mechanics

Review of Electric and Magnetic Fields

  • Electric fields arise from electric charges, which can be isolated as positive or negative types.
  • The electron's charge is the fundamental unit of electric charge, approximately 1.602x10^-19 C.
  • Atoms are neutral, however gaining enough energy, an electron can be removed by thermal energies from the nucleus.
  • The atom becomes a positive ion, and the electron is a negative ion.
  • Electric charges can be isolated, creating electric fields, with the electric potential quantifying the charge's strength, representing the work needed to bring a unit positive charge from infinity.
  • Electric potential at a distance x from a charge: Vx = Q / (4πε₀x).
  • Electric potential is inversely proportional to the distance from the test charge.
  • External work is required to move a positive charge in a positive field.
  • Electric field due to a point charge: Ex = Q / (4πε₀x²).
  • Electric field is inversely proportional to the square of the distance from the test charge.
  • Electric field in terms of electric potential: Ex = -dVx / dx.
  • Electric fields can be visualized using flux lines indicating the force direction on a positive charge, lines directed outwards for positive charges and inwards for negative charges.
  • The flux of electric field lines indicates the electric field strength and the amount of charge present.
  • Magnetic fields are typically dipolar (north and south poles) and currently cannot be isolated, though magnetic monopoles are theoretically possible.
  • Magnetic field strength is inversely proportional to the square of the distance from the magnetic dipole, mirroring electric fields.
  • The magnetic potential is inversely proportional to the distance from a reference point.
  • Magnetic field lines form continuous loops both inside and outside magnetic materials, with flux indicating field strength.
  • Magnetic fields are created by current carrying solenoids and the current's direction determines polarity.
  • Electric and magnetic fields show a robust interplay, especially with time-dependent quantities.
  • Ampere's and Faraday's laws confirm strong electrical and magnetic forces; current via a straight conductor creates a magnetic field and electromagnetic induction produces current in a coil within a varying magnetic field.

Maxwell's Equations in a Medium

  • Maxwell summarized the existing ideas of electric and magnetic fields and their related phenomena into four equations in 1860.
  • Describing radiation with these equations paved the way as an electromagnetic wave.
  • Ñ operator (nabla operator): Ñ = i(∂/∂x) + j(∂/∂y) + k(∂/∂z), where i, j, and k are unit vectors.
  • V operating on a scalar produces a vector, giving rise to the gradient of the field.
  • For example, the electric potential at a point is the result of the V operator operating on an electric potential. - Vv = i(∂V/∂x) + j(∂V/∂y) + k(∂V/∂z) = iEx + jEy + kEz = Ē.
  • Dot product of the V operator with a vector field yields a scalar, the divergence, representing the field's rate of change in three orthogonal directions.
  • Applying the cross product of the V operator gives the curl of the field, a vector perpendicular to both V and the original vector.
  • An additional identity of the V operator shows that the curl of the curl of a vector is the same as the gradient of the divergence of a field minus the Laplacian acting on the vector.
  • This is VxVxĒ = V(V.Ē) – V²Ē.
  • V² = V.V= (∂²/∂x²) + (∂²/∂y²) + (∂²/∂z²) and is the scalar Laplacian operator.

Gauss's Law

  • For electric fields, the divergence of the electric field is equal to the charge density divided by ε₀ (Gauss' law for electric fields), due to a system of charges enclosed by surface,.
  • For magnetic fields, the divergence of the magnetic field is zero.
  • V. B = 0 (Gauss' law for magnetic fields) implies the absence of magnetic monopoles.

Faraday's Law of Electromagnetic Induction

  • The curl of the electric field is equal to the rate of change of the magnetic field, VxẺ = -∂B/∂t

Ampere-Maxwell Circuital Law

  • The curl of the magnetic field is given by the current density and the displacement current, VxB = μ₀J + με₀(∂E/∂t).
  • This law extends Ampere's law, where the second term is the displacement current with time-varying electric fields from Maxwell.

Maxwell's Equations in Free Space

  • Maxwell's equations are rewritten in free space where there are no sources of charges and currents.
  • Free Space Equations
  • V.E = 0
  • V.B = 0
  • VxẺ = -∂B/∂t
  • VxB = με₀ (∂E/∂t)
  • Taking the curl of the curl of the electric field can be written as ∇ × (V x Ē) = ∇ × (-∂B/∂t. This process reduces to V(V.E) – V²E = (-∂/∂t)(∇ × B).
  • A simplified equation with curl of B is given by ∇² = (μ₀ε₀)(∂²E/∂t²), through substitution.
  • The general wave equation form comes after observing that με₀ = 1/c², with c as the speed of light.
  • Light can be treated as electromagnetic waves, with perpendicular electric and magnetic vectors to the direction of radiation propagation.
  • A 1D electric wave can be written as Ex = Exo sin(wt + kz), associated with radiation propagating in the Z direction.
  • This states the electric field vector has only an x component where all other components equal zero..
  • Maxwell's third equation is needed for the associated magnetic component of the EM wave to be evaluated. Evaluating the curl of the electric field VxE = ijk [∂/∂x ∂/∂y ∂/∂z] [Ex 0 0] = i x 0 + j * (∂Ex/∂z) + k*0 = ĵ * (∂/∂z) [Exo cos(wt + kz)].
  • Integration yields the EM wave's magnetic component. This is expressed as B = ĵ * k * Exo cos(wt + kz) * (-1/w) = ĵ * Exo cos(wt + kz) * (-1/w).
  • EM waves have coupled electric and magnetic field components mutually perpendicular and also perpendicular to radiation direction

Energy of EM Waves

  • Classically, wave energy corresponds to intensity, which is equivalent to the square of wave amplitudes.
  • The associated energy of an electric field per unit volume of free space is En = (1/2)ε₀E².
  • Electric component's energy content = (1/2) ε₀Exo² cos² (wt + kz)
  • Magnetic component's energy content = (1/2μo)Byo² = (1/2)(1/c²μ₀)Exo² = ε₀/(2)Exo²
  • Total energy content of the wave is the sum of two components = ε₀Exo².
  • EM waves transmit energy in a perpendicular direction to E and B field variations, calculated via the Poynting vector, s = (1/μo)E × B = c.ε₀E² .
  • Average energy of the wave transmitted over time and area can be expressed.

Polarisation of EM Waves

  • Light is a transverse EM wave; but natural light is typically unpolarized where propagation planes are equally probable.
  • Linearly polarized light is a plane wave with alignment, when the light is a combination of a wave that has horizontal polarization and a wave with vertical polarization, with similar amplitude.
  • A superposition of two plane waves with a 90° phase difference is circularly polarized, when an electromagnetic wave is the result of the superposition of two plane waves that differ in relation to amplitude or is other than 90°, the light is said to be elliptically polarized.
  • The classical EM wave model gives frequency independence regarding for energy for some phenomena of light with matter.

Blackbody Radiation

  • The interaction of radiation and matter includes the ways a material absorbs radiation, and wavelengths giving it color.
  • Gustav Robert Kirchhoff observed materials absorbing all rays and emitting all radiations absorbed if heated, called a black body. Blackbody radiation is modeled as cavity radiation emission of every frequency rate at particular temperatures of the body and energy limited by the absorption rate.
  • The thermodynamic equilibrium limited the energy emitted at a particular frequency based on absorption and emission processes.
  • The radiation density in an equilibrium depends on the cavity temperature, regardless of structure, shifting to lower wavelengths.
  • Modeling blackbody emission involves emissions from harmonic oscillators on cavity walls. The harmonic oscillators emit at particular wavelengths.
  • Emission is restricted to radiations forming standing waves within, and at wavelengths equal to a = λn / 2.
  • Frequencies that can be sustained in the cavity are v = nc/2a.

Max Plancks Equation

  • Max Planck solved blackbody emission by quantizing energy states depending on harmonic oscillation.
  • This meant the energy per volume of radiations is p(v)dv = (8πv²/c³)kBT .
  • The solution stated that the energy of a harmonic oscillator is restricted to frequencies v and a constant h approximately(h = 6.6x10−34Js) E = nhv, due to radiation emerging from collections of harmonic oscillators and energies. where the energy of the radiations from the oscillators has to be packets of hν.
  • In these terms, energy can be described as (E) = (hv*e^(-hv/kT))/(1-e^(-hv/kT)). and the energy density of radiations can be evaluated as p(v)dv = (8πhv^3)/(c^3) *1/((e^(hv/kT))-1) dv.
  • Max Planck unknowingly established energy quantization in systems.

Atomic Spectra

  • Atomic spectroscopy identifies and quantifies elemental sample composition using distinct element spectra.
  • Robert Bunsen and Gustav Kirchhoff discovered absorption lines in the solar spectra, also known as Fraunhofer lines.
  • Classical atomic models could not explain discrete line emissions, but models were proposed in response stating accelerated charges radiate energy through electron orbiting and emission.
  • Modern atomic models describe line spectra by referring to state transitions.

Dual Nature of Radiation

  • Radiation is part of the electromagnetic spectrum, also EM waves, where conventional wave theory explains reflection, refraction, interference, diffraction and polarization of light.
  • Einstein explained the photoelectric effect as a particle interaction, paving the way for wave particle duality.
  • The Photo electric displayed a particle nature when the interaction is at atomic / sub atomic particles.

Compton Effect

  • Arthur H Compton studied X-ray scattering.
  • Arthur H Compton observed that if a an electron emitted, the beam has a different wavelength as compared to the incident radiation.
  • Classical X-ray treatment failed to explain X-rays of the type that had a higher wavelength.
  • Treating this problem as a particle collision with momentum of photons. This is written as P = h/ λ, with wavelength of incident x-ray is scattered alongside the transfer of energy.
  • Due to considering energy and momentum after the collision, this gives an increase in the wavelength of a photon after the collision and gives .
    • λf – λᵢ = Δλ = h/mₑc (1 - cos θ)
  • This value is known as the compton shift, and depends on:
  • Incident of X-rays
  • Scattering Material
  • Angle of Xrays scattering

Dual Nature Of Matter

  • Louis de Broglie proposed moving matter displays wave characteristics, a = h/mv (mv is the momentum of the particle).
  • Larger particles have smaller wavelength by observation, where they are difficult to measures.
  • Experiments by Davisson and Germer demonstrate wave nature using crystals, confirming matter’s dual characteristics.
  • This concept has been confirmed when measuring heavier particles.
  • Hitachi in the 1980s showed the electrons scattering patterns are very close to a diffraction pattern produced by a double slit experiment when showing the diffraction of electrons.

Young's Double Slit experiment

  • A double slit experiment reveals electrons as particles arriving at distinct locations but forming interference patterns when many electrons pass through individually.

Wave Packets

  • Matter waves require mathematical representation for moving particles, where both position and momentum can be estimated with reasonable accuracy.
  • The superposition of two waves gives a resultant, as described: y = y₁ + y2 = 2Asin(ωt + kx)⋅cos ((Δωt+Δk⋅x)/2).
  • Due to group of superimposed waves, the particle's momentum comes from estimating waves of a wavelet, and inferred by maximum amplitude of the amplitude.

Describing momentum and position of particles

  • This process makes accurate estimations of a particle's momentum and position. Given momentum is taken from the wavelength and the position represents maximum amplitude
  • Phase velocity of waves refers to the high frequency components of the wave and is given by vp= ω/к
  • Group wave velocity refers to the speed of travel, expressed as Vg= dw/dк
  • A relation between both velocities describes group velocity as dw/dk, where w is the angular frequency of the wave, yielding group velocity Vg in which dE = hdw.
  • In a dispersive medium the group velocity is Vg = Vph + k *dvph / dλ

Schrodingers Cat

  • Quantum systems are not subjected to observations, since the observations interfere with the quantum behavior of the particles being studied

Uncertainty Principle

  • Position and propagation constant are intrinsically related through the uncertainty principle.
  • In summary he product of the standard deviations in the estimates of the position and the propagation constant was shown to be greater than or at the most equal to. . ie., Δx. Δk ≥ 1/2
  • This then translates to the standard form of the uncertainty principle when the propagation constant is transformed to the momentum through the relation p = hk

Heisenberg's Gamma ray microscope:

  • Heisenberg proposed the gamma ray microscope (as a thought experiment to illustrate the uncertainty principle) where it is evident that one should use y rays to observe electrons, which in turn scatter the radiation onto the objective lens of the microscope. In that order it resolves Ax is related to momentum p with the relation : ∆x. ∆px ≈ 2h > h/4π

Electrons Inside the Nucleus

  • High energy beta particles emission from nuclei challenges electron existence inside the nucleus, uncertainty principle used.
    • With related uncertainties of DeltaX≈ 10^ (-14)m the minimum momentum is given by:
      The minimum uncertainty in the momentum of the electron then can be estimated as Δp =h / 2. Δχ= 5.28 × 10^−21 kgms^-1

Wave Functions

  • Moving particles are represented by packets, wave packet can be described by x, y, z in a function referred to as state functions, functions must be :
  • y must be finite, continuous and single valued in the regions of interest.
  • The derivatives of the wave function must be finite, continuous and single valued in the regions of interest.
  • The wave function y must be normalizable

Observables:

  • The physical parameters associated with the particle such as energy, momentum are observable as measured by experiment and by the wave function
  • Operations can be carried out on a function f to yield results, which is why the wave function can yield results: αψ = α ψ() αψ α αψ

Linear superposition of waves from SWE

  • In a quantum system when multiple states, with each being a wave equations then a separate linear combination can also be expressed as such , with 4,(x) + m.

Time dependant and independant Schrodingers Equation.

  • All systems can me summarised in the following format , with some operators in the following forms : Ê= Total Energy KE Kinetic energy PE - Potential energy - Schrodinger’s form. Êψ(x,t) = ΚΕψ(x,t) + Vψ(x, t) A time indépendant system can also be defined as functions where $(t) ≠ 0: h² d²ψ(x) + Εψ(x) – Vψ(x) = 0. 2m dx2

Template for quantum equations

  • (1) Define / set up the physical system (define particle nature, boundaries of potential, total energy of the particle etc)
  • (2) Write the Schrodinger's wave equation and apply the known conditions
  • (3) Obtain the general form of the wave function
  • (4) Check/verify the wave function for it's characteristics: finiteness, discreteness and continuity of and its derivatives.
  • Normalization of the wave functions
  • (5) Interpret the solution, get implications on the quantum system.

Free Patrical Soluton

  • Particle without external forces, implying force = 0, constant is zero, constant is 0.
  • When writing 1D (one dimensional) for a free particle wave for the system : h² d²ψ(x) + Εψ(x) = 0 or 2² +E = 0

==Start of section for page 22== Some typical solved Numericals

  1. A simple problem shows to Estimate the Compton's shift.

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