SkyrmionSkyrmion Scattering and Nuclear Physics
To understand a complex system such as the world we live in, it is useful to understand its parts. An atom, for example, consists of electrons and the atomic nuclei, which in turn consist of protons and neutrons. As particle accelerators have revealed, protons and neutrons are also made up of smaller particles, each one contains three quarks. And so, now that we know the protagonists, we need to understand how they interact. Apart from gravity, there are three interactions: the electromagnetic interaction which acts only on charged particles (such as electrons and protons); the weak interaction which only affects certain particles and is very weak indeed; and the strong interaction which holds atomic nuclei together. The strong interaction is much stronger (and much more complicated) than the other two, but it falls off very rapidly with distance. In the theory of the strong interaction known as quantum chromodynamics (QCD), quarks interact via yet another type of particle called gluons. At the very high energies found in particle accelerators such as LHC in Geneva, QCD explains experimental findings to an amazing accuracy. However, at lower energy levels, quarks like to stick together, either in threes to form protons and neutrons or in twos to form particles known as pions. As a consequence, a single quark can never be observed on its own. This means that QCD becomes very complicated at low energies and it is extremely difficult to calculate the properties of a proton from QCD.An alternative approach to this problem was devised in 1961 by the British physicist Tony Skyrme (19221987), before QCD was discovered. Skyrme proposed a theory which involves only the particles that are directly observable, the protons, neutrons and pions. The theory is very elegant, since protons and neutrons are described as topological solitons, which can be thought of as knots in a field of pions. In Skyrme's honour, these solitons are known as Skyrmions. In 1979, the American theoretical physicist Edward Witten showed that the Skyrme model captures the essential features of QCD for low energies. This means that we can use the Skyrme model to describe the phenomena in nuclear physics.In standard nuclear physics, atomic nuclei are bound states of protons and neutrons under rules which have to be determined for each case. This approach gives accurate results but does not provide a unified picture coming from first principles such as QCD. The Skyrme model lies between standard nuclear physics and QCD, and thus provides a different perspective on nuclear physics experiments.Although the Skyrme model is much simpler than QCD, many difficulties remain. Since protons and neutrons obey the laws of quantum mechanics, the Skyrme model with its Skyrmions also needs to be quantized. There are some technical issues (namely the calculation of what are called FinkelsteinRubinstein constraints) which I have recently resolved. Using these techniques masses and excitation energies of atomic nuclei have been calculated and achieved remarkable qualitative agreement with nuclear physics. Despite its motivation from physics, this project is firmly rooted in mathematical physics using sophisticated mathematical tools devised by pure and applied mathematicians.A vast amount of nuclear physics experiments is concerned with the scattering of atomic nuclei  for example hitting a helium atom with a proton and measuring how the atomic nuclei break up. Such experiments can be compared to SkyrmionSkyrmion scattering, an area of research which is currently in need of development. The aim of my project is to use both analytical approximations and numerical calculations to understand SkyrmionSkyrmion scattering. There are early indications that the Skyrme model can help us to make experimental predictions in situations that are difficult to address with the standard techniques of nuclear physics.
Id  159 
URI  http://gow.epsrc.ac.uk/NGBOViewGrant.aspx?GrantRef=EP/I034491/1 
Grant Value  100427 
Funders 
[224] UK Engineering and Physical Sciences Research Council

Publications 
Krusch, Steffen and Foster, David J
(2013)
Negative Baryon density and the Folding structure of the B=3 Skyrmion.
Journal of Physics A: Mathematical and Theoretical,
46
(26).
pp. 265401265419.
ISSN 17518113.
(doi:https://doi.org/10.1088/17518113/46/26/265401)
(Full text available)
Haberichter, Mareike and Battye, Richard A.
(2013)
Isospinning baby Skyrmion solutions.
Physical Review D: Particles, Fields, Gravitation, and Cosmology,
88
(12).
p. 125016.
ISSN 05562821.
(doi:https://doi.org/10.1103/PhysRevD.88.125016)
(Full text available)
Battye, Richard A. and Haberichter, Mareike and Krusch, Steffen
(2014)
Classically Isospinning Skyrmion Solutions.
Physical Review D: Particles, Fields, Gravitation, and Cosmology,
90
(12).
pp. 125035125069.
ISSN 05562821.
EISSN 15502368.
(doi:https://doi.org/10.1103/PhysRevD.90.125035)
(Full text available)
Krusch, Steffen and Muhamed, Abera A
(2015)
Moduli Spaces of Lumps on Real Projective Space.
Journal of Mathematical Physics,
56
(8).
082901.
ISSN 00222488.
(doi:https://doi.org/10.1063/1.4928925)
(Full text available)
Krusch, Steffen and Foster, David J
(2014)
Scattering of Skyrmions.
Nuclear Physics B,
897
.
pp. 697716.
ISSN 05503213.
EISSN 18731562.
(doi:https://doi.org/10.1016/j.nuclphysb.2015.06.011)
(Full text available)
Haberichter, Mareike
(2014)
Isospinning Skyrmions.
In:
Quarks2014 Proceedings.
(Full text available)
Ashcroft, Jennifer and Krusch, Steffen and Haberichter, Mareike
(2015)
Baby Skyrme models without a potential term.
Physical Review D: Particles, Fields, Gravitation, and Cosmology,
91
(10).
p. 105032.
ISSN 05562821.
EISSN 15502368.
(doi:https://doi.org/10.1103/PhysRevD.91.105032)
(Full text available)

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