Study Material

How energy and matter interact is at the very foundation of physics. We will explore two of the most important aspects of such interactions, as well as developing skills in experimental physics. First, we will study optics, the properties of light and its interactions with matter. We will focus on the wave nature of light and effects such as refraction, diffraction and interference. In our second module we will study thermodynamics, a subject central to many branches of science, with applications from the smallest systems of atoms to the big bang. We will examine the concepts such as entropy, thermodynamic interactions, engines and heat. In the experimental physics module students will carry out in-depth experiments, each one spanning several weeks, building experimental skills. These skills will include the measurement of physical quantities; analysing data; assessing reliability and significance; and communicating scientific results. Experimental topics include the nature of light, the properties of matter, electrical circuits, astrophysics and others.

Learning Outcomes

Week 1:

  • The importance of Optics and Photonics

  • Understand the difference between Geometrical v. Physical v. Quantum optics

  • Geometrical Optics – review of basic topics

  • Reflection, Image formation from reflective surfaces

Week 2:

  • Understand refraction and image formation from refractive media

  • Learn the lens equation and its physical meaning/usage

  • Total Internal Reflection and Dispersion of light

  • Learn the foundations of Wave Optics and wave representation including plane waves and spherical waves

  • Discuss Ray Optics vs Wave Optics;

  • Learn about Rayleigh Scattering, Reflection, Refraction, lenses in the wave optics framework;

  • Huygens’ principle

Week 3:

Coherence of Light

  • understand and discuss the concept of spatial coherence, and use it to explain why fringes will not be seen from twin slits with unsuitable (incoherent) illumination

  • understand and discuss the concept of the temporal coherence length of light, and calculate the coherence length as a function of the centre wavelength and range of wavelengths detected

Interference - Double slit with slits of non-zero width

  • discuss and apply the Fraunhofer intensity pattern formed by a double slit where the slits have a non-zero width.

  • be able to sketch the intensity distribution illustrating the relative widths of the interference fringes and the central diffraction envelope

Interference in Thin Films

  • discuss the formation of interference fringes in light reflected from thin films

  • recognise the π phase change that occurs when reflection occurs at a boundary where the refractive index increases

  • explain and use the equation for net phase difference of the combining rays, as a function of the film thickness, the refractive indices of the film and surrounding media, and the wavelength of the light

  • use the phase difference between combining rays to find whether the rays undergo constructive, destructive or partial interference

  • discuss the formation of fringes of equal thickness (contour fringes) in non-uniform thin films

  • discuss single layer anti-reflection coatings and be able to relate the thickness of such a film to the refractive indices of the coating and coated material and to the wavelength of incident light

Week 4:

  • discuss the formation of fringes of equal thickness in uniform thin films

  • understand the relationship of the fringe spacing to the refractive indices of the film and surrounding media, the thickness of the film, and the wavelength of the light

The Michelson Interferometer and other types of interferometers

  • discuss the formation of interference fringes in an amplitude splitting interferometer

  • draw the layout of a Michelson interferometer with representative reflected and transmitted light rays, and explain the function and operation of the interferometer

  • describe some examples of amplitude splitting interferometers and their applications.

  • discuss the Mach–Zehnder, Sagnac and the Fabry–Perot interferometers

Diffraction by single slit

  • recognise and apply the Fraunhofer diffraction pattern for multiple slits and explain the effect on the pattern of increasing the number of slits [36.4]

  • describe transmission and reflection diffraction gratings and their use in spectrometers [36.5]

  • apply the equation for angle of diffraction as a function of diffraction order, wavelength, and slit separation

  • understand and use the terms angular dispersion

Week 5

Interference and Diffraction - Double slit with slits of non-zero width

  • discuss and apply the Fraunhofer intensity pattern formed by a double slit where the slits have a non-zero width, giving a single-slit diffraction envelope which modulates the peak intensity of two-source interference fringes within the envelope

  • be able to sketch the intensity distribution illustrating the relative widths of the interference fringes and the central diffraction envelope

  • explain the effects on the Fraunhofer diffraction pattern of changing the width of the slits, the separation of the slits, or the wavelength of the light

Diffraction by Multiple Slits

  • recognise and apply the Fraunhofer diffraction pattern for multiple slits and explain the effect on the pattern of increasing the number of slits

Week 6

Diffraction by Multiple Slits II

  • describe transmission and reflection diffraction gratings and their use in spectrometers

  • apply the equation for angle of diffraction as a function of diffraction order, wavelength, and slit separation

  • understand and use the terms angular dispersion and chromatic resolving power as applied to diffraction gratings

Diffraction from Circular Apertures

  • recognise the Fraunhofer diffraction pattern for a circular aperture and be able to draw the intensity distribution pattern illustrating the relative scales of the central and secondary maxima

  • apply the dependence of the angular scale of the Fraunhofer diffraction pattern (as given by the location of the first intensity minimum) for a circular aperture on the diameter of the aperture and on the wavelength of the light

  • define and apply Rayleigh’s criterion for resolution to circular apertures

Polarisation

  • define what is meant by unpolarised, plane polarised, circularly polarised, and partially polarised light

  • appreciate that the phenomena of polarisation show that light is a transverse wave

  • understand and discuss the use of polarising filters (such as Polaroid) to produce linearly polarised light

  • apply Malus’ law relating the intensity transmitted by a polarising filter to the angle between the plane of incident polarisation and the transmission axis

  • understand and discuss the production of polarised light by specular reflection at non-metallic surfaces, with complete linear polarisation at the Brewster angle

Birefringence

  • understand and discuss the phenomena of birefringence and its effect on polarized waves

  • understand and discuss the concept of ordinary and extraordinary waves in birefringent materials

  • explain how a quarter wave plate works

  • describe what is meant by the term circular polarisation

Week 7

Birefringence

  • understand and discuss the phenomena of birefringence and its effect on polarized waves

  • understand and discuss the concept of ordinary and extraordinary waves in birefringent materials

  • explain how a quarter wave plate works

  • describe what is meant by the term circular polarisation [33.5]

1st and 2nd Law of thermodynamics

  • ideal gas law

  • energy partition

  • 1st Law of thermodynamics

  • Heat engine

  • 2nd law of thermodynamics

Week 8

Probabilistic approach to entropy  

  • Concepts of microstates and macrostates

  • Definition/understanding of entropy in terms of probability & multiplicity

  • Einstein solid with 3 oscillators

  • 2 Einstein solids

  • Boltzmann hypothesis

Sackur-Tetrode Equation for entropy 

  • Entropy for a monoatomic ideal gas

  • Partition of space using Heisenberg Uncertainty Principle   

  • Sackur-Tetrode Equation

  • Isothermal and quasistatic expansion (or compression)

  • Free Expansion into a vacuum

  • Mixing of 2 gases

  • Reversible and Irreversible processes

Week 9

Equilibrium & 1st thermodynamic identity

  • Internal energy (U) and entropy (S) relationship to pressure (P), temperature (T) and volume (V)

  • Thermal Equilibrium

  • Entropy and energy flow

  • Mechanical Equilibrium

  • Thermodynamic Identity

  • First Law, Heat, & Entropy

  • Reversible and irreversible examples

Week 10

Chemical potential & applications of 1st thermodynamic identity  

  • Chemical potential

  • Diffusive equilibrium 

  • Thermodynamic Identity including chemical potential

  • Chemical potential for an ideal gas

  • Chemical potential for an Einstein solid

  • Chemical potential change at different heights

Enthalpy, Helmholotz & Gibbs free energies 

  • Enthalpy H

  • Enthalpy relationship to Heat and work

  • Helmholtz Free Energy F

  • Gibbs Free Energy G

  • Thermodynamic Potentials

  • Extraction of Heat and Work

Week 11

Thermodynamic potentials & 2nd law

  • Examples  using H,F, and G  

  • Electrolysis of water

  • Reversal of Electrolysis of Water

  • Hydrogen Fuel Cell

  • Derive generalised thermodynamic identities  

  • Redefine the Second Law in terms of Free Energy
    Phase diagrams & phase transitions

  • Phase changes

  • Phase diagrams

  • Stability and changes in phase with T and P

  • Gibbs Free Energy & Phase Diagrams

  • Variations in G with T and P

  • Clausius-Claperyon Relation: dP/dT,

  • Entropy changes, volume changes, and latent heats 

Week 12

Solutions and osmotic pressure 

  • Chemical Potential 

  • Gibbs Free Energy of a mixture

  • Gibbs Free Energy & Entropy of mixing

  • Chemical potential for dilute solutions/mixtures

  • Chemical potential & molality

  • Osmosis

  • Stopping Osmosis

  • Changing Boiling Points

Thermodynamics of black holes 

  • Schwarzschild radius

  • Entropy of Black Holes

  • Temperature of Black Holes

  • Evaporation of Black Holes