Nonlinear Patterns - Mathematical Tripos - Exam Paper, Exams of Mathematics

This is the Exam Paper of Mathematical Tripos which includes Solitons and Instantons, Nonlinear Schr¨Odinger Equation, Stationary Soliton Solutions, Differential Equation, Effective Lagrangian, Harmonic Potential, Derrick Scaling Argument, Abelian Higgs Model etc. Key important points are: Nonlinear Patterns, Simple Bifurcation, Earth’s Magnetic Field, Axisymmetric Dipole Magnetic Field, Induced Velocity, Equatorial Dipole Magnetic Field, General Set of Equations, Amplitudes and Phases

Typology: Exams

2012/2013

Uploaded on 02/26/2013

devbrata
devbrata 🇮🇳

4.5

(15)

62 documents

1 / 3

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
MATHEMATICAL TRIPOS Part III
Monday, 8 June, 2009 1:30 pm to 3:30 pm
PAPER 70
NONLINEAR PATTERNS
Attempt no more than TWO questions.
There are THREE questions in total.
The questions carry equal weight.
STATIONERY REQUIREMENTS SPECIAL REQUIREMENTS
Cover sheet None
Treasury Tag
Script paper
You may not start to read the questions
printed on the subsequent pages until
instructed to do so by the Invigilator.
pf3

Partial preview of the text

Download Nonlinear Patterns - Mathematical Tripos - Exam Paper and more Exams Mathematics in PDF only on Docsity!

MATHEMATICAL TRIPOS Part III

Monday, 8 June, 2009 1:30 pm to 3:30 pm

PAPER 70

NONLINEAR PATTERNS

Attempt no more than TWO questions. There are THREE questions in total. The questions carry equal weight.

STATIONERY REQUIREMENTS SPECIAL REQUIREMENTS

Cover sheet None Treasury Tag Script paper

You may not start to read the questions printed on the subsequent pages until instructed to do so by the Invigilator.

2

1 A model of the earth’s magnetic field is represented by the interaction of three modes, arising in a simple bifurcation, with the following symmetries:

(a) an axisymmetric dipole magnetic field; (b) an equatorial dipole magnetic field which changes sign under a rotation about the axis of π; (c) an induced velocity field with the same symmetry as the equatorial dipole.

It is assumed that the earth is symmetric with respect to longitude, and that the system is invariant under a change of sign of all magnetic fields, leaving the velocity field unchanged. Finally, it is known that the equations describing the magnetic field evolution are linear in the magnetic field.

Justify the statement that the axisymmetric field can be represented by a real variable B, while the other fields can be represented by complex variables A, V.

Write down the most general set of equations that respect the above conditions, and show that when these are truncated at cubic order they take the form, where the ci, di are complex in general, and the μi, ωi and e are real:

B˙ = μ 1 B + (c 1 A∗V + c.c.) − e|V |^2 B, A^ ˙ = (μ 2 + iω 2 )A + c 2 V B − d 2 |V |^2 A − d 3 V 2 A∗, V^ ˙ = (μ 3 + iω 3 )V + c 3 AB − d 4 V |V |^2 − d 5 V |A|^2 − d 6 V ∗A^2 − d 7 V B^2 ,

and show that c 1 and |c 3 | can be taken as unity without loss of generality.

Now take d 2 = d 3 = d 5 = d 6 = d 7 = 0, and d 4 , c 2 real. Derive equations (which need not be solved) governing the amplitudes and phases of the variables for solutions of the equations where the moduli of A, V, B are constant. Find explicitly a relation between the parameters for which such a solution with A, B 6 = 0 bifurcates from one with A, B = 0, V 6 = 0.

Part III, Paper 70