maths excursions - 2011/12 - semester 2

A series of entertaining pieces of maths, light-hearted and accessible to students at all levels and the general maths audience.
An initiative of the postgrad students in the School of Maths.
All are welcome!

autotune
Monday, 30th of April 2012, 2pm, Roger Steven LT 04, Dr Kevin Houston (Leeds)
The Mathematics of Auto-Tune

Singers use Auto-Tune to ensure that they are pitch perfect. This piece of software has had a huge impact on the music industry and led to uproar when used on the X Factor. The talk explains how it and popular console games such as Sing Star use mathematics to produce their effects. Along the way we will try to solve the puzzle of the Beatles' Magical Mystery Chord and discover if you can hear the shape of a drum.

large deviation theory
Wednesday, 14th of March 2012, 2pm, Leonard Rogers Room (8.22d), level 8, School of Maths, Lee Zhuo Zhao (Cambridge)
An Introduction to large deviation theory

An introduction to large deviation theory The central limit theorem is one of the first important results students encounter in a statistics course, although I would argue it is a deep result of probability. One consequence of this theorem is that the sum of a sequence i.i.d. random variables has an exponentially decaying tail, just like the normal distribution. Large deviation theory aims to explore the exact asymptotics of this decay and therefore place a quantitative value on the probability of freak events. In this talk I will try and motivate and introduce the theory using only rudimentary results of probability and analysis and finally show an application related to my research into branching processes.




codes
Wednesday, 22nd of February 2012, 2pm, Roger Stevens LT 16, David Bradley-Williams (Leeds)
Number theory, secrecy and code breaking

Number theory, group theory, computability and complexity theory are all strands of mathematics which are depended upon for ensuring secrecy via encryption, and for extracting other people's secrets through cryptoanalysis. I will combine these strands to mention how mathematics was used by the Allies to shorten World War II and by each of us every day to protect our secret information. But why should we trust our secrets are safe?



Pick's Theorem
Wednesday, 1st of February 2012, 2pm, Roger Stevens LT 16, Richard Elwes (Leeds)
Pick's Theorem and Ehrhart Polynomials

Pick's Theorem is one of the jewels of elementary geometry: a single, simple formula which determines the areas of a huge range of shapes. We will also meet the more mysterious Ehrhart Polynomials, which generalise Pick's theorem to shapes in higher dimensions. These objects have many applications to problems in computer science and optimisation.





2011/12 - semester 1

VanderWaerden
Wednesday, 12th October 2011, 2pm, Roger Stevens LT 04,  Imre Leader (Cambridge)
Van der Waerden's Theorem
Lecture slides
Suppose we are presented with a long string of beads. The beads come in two colours, red and blue, but there is not necessarily any pattern to the way they are threaded on the string. Can we guarantee to find three equally-spaced beads of the same colour? For example, if the 5th, 7th and 9th beads were all blue then this would count. This question leads to some beautiful mathematics.



Groups as graphs
Wednesday, 26th 2011, October 2pm, Roger Stevens LT 16, Cong Chen (Leeds)
Groups as Graphs
Lecture slides
Given a group, we can specify a list of generators and colours. Once we’ve done this we can draw a map, like one of the Underground, of the group - because you can get anywhere by following those generators. What do these pictures look like, and what can they tell us about the group?



magnet
Wednesday, 9th November 2011, 2pm, Roger Stevens LT 18, Tina Davies (Leeds)
The solar magnetic field - what it looks like, what it does, and how it might have got there

Lecture slides
Just like the Earth, the Sun has a magnetic field, and it is this field that is responsible for the vast majority of both the features we see on the Sun and the 'space weather' we experience on Earth. I will show observations of solar features and explain how these match up with magnetic activity on the sun, and then give an overview of the physics behind what is happening and the current problems this poses for theorists.



Acoustic problems
Wednesday, 16th November 2011, 2pm, Roger Stevens LT 16, Anastasia Kisil (Cambridge)
Acoustic problems, Wiener-Hopf method and rational approximation
Lecture slides
Many real life problems result in partial differential equations (PDEs) so our ability to solve them is important. There are no standard methods that can solve all PDEs like there are for ordinary differential equations (ODEs). In this talk I will talk about one beautiful method of solving certain PDEs called Wiener-Hopf method. I will also demonstrate how it can be useful in solving some wave propagation problems.



Codes
Wednesday, 7 December 2011 2pm, Roger Stevens LT 06 - CANCELLED DUE TO ILLNESS , David Bradley-Williams (Leeds)
Number theory, secrecy and code breaking

Number theory, group theory, computability and complexity theory are all strands of mathematics which are depended upon for ensuring secrecy via encryption, and for extracting other people's secrets through cryptoanalysis. I will combine these strands to mention how mathematics was used by the Allies to shorten World War II and by each of us every day to protect our secret information. But why should we trust our secrets are safe?


2010/11

angeldevil Wednesday, 2nd February 2011, 2 - 3pm, Roger Stevens LT12
Stijn Vermeeren (Leeds): Angel vs. Devil: a mathematical chase
Lecture slides
The Angel flies between squares on an infinite chess board; every second he can fly a fixed distance k. But every second The Devil eats one square, which the Angel is not allowed to use anymore. Can the Angel (if k is big enough) survive forever, or can the Devil always trap the Angel by devouring all squares around him? This simple-sounding question was an open problem for many years, and was only resolved in 2006. Still, it is possible to sketch a solution without using any advanced mathematics, which I will present to you. The talk will contain many pictures and has a happy ending.



infinitesimals
Wednesday, 16th February 2011, 2 - 3pm, Roger Stevens LT12
Alexandra Omar Aziz (Leeds): Infinitesimals
Lecture slides
I shall discuss the concept of infinitesimals, infinitely small numbers, and explain how their use can be given a rigorous mathematical foundation. After a short historical introduction, I shall explain the model-theoretic background underlying their construction and give some examples from nonstandard calculus.



brownian_motion
Wednesday, 2nd March 2011, 2 - 3pm, Roger Stevens LT12
Dr Mike Tehranchi (Cambridge): What is Brownian motion?
Lecture slides
In 1827, Robert Brown observed the random motion of microscopic particles suspended in water. Motivated by his observations, mathematicians define Brownian motion to be a continuous stochastic process with independent and stationary increments. Brownian motion is central to probability theory since it is the key example of a Markov process, a Gaussian process, and a martingale. This talk will explore Brownian motion from these different perspectives, and indicate applications to partial differential equations and complex analysis.



weather

Wednesday, 16th March 2011, 2 - 3pm, Roger Stevens LT12
Dr James Cranch (Leicester): Maps between spheres

Some mathematicians think that the set of maps between spheres of high dimensions is an object more fundamental than the integers. While I won't have nearly enough time to make that sound even remotely sensible, I will be able to demonstrate why it's a topic that has fascinated mathematicians ever since the 1930s, even though the state of our understanding of the subject in 2011 is still laughably bad.



waether_forecasting
Wednesday, 23rd March 2011, 3 - 4 pm, Roger Stevens LT16 !!! Different time and room!!!
Julian Mak (Leeds): Mathematical Aspects of Weather Forecasting, (With thanks to Dr. Keith Ngan, Met Office)
Lecture slides
Although essentially a problem in classical physics, the problem of describing the dynamics of the atmosphere and ocean (both regarded as fluids) are still far from being completely understood. In this talk, I shall focus on the problem of modelling the dynamics of fluids via the Navier-Stokes equations, an essential component in weather prediction. The talk is split into two parts: first, how one would, ideally, solve the equations and therefore obtain the dynamics; second, what people actually do. This talk will also include a historical background on weather forecasting, a brief history of the Met Office, and certain details about the current weather / climate model employed by the Met Office, known as the “Unified Model”.