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The Pearcey function and the cusp catastrophe

dc.contributor.advisorSprung, Donald
dc.contributor.authorMacBeath, Darryl
dc.contributor.departmentPhysics and Astronomyen_US
dc.date.accessioned2016-09-23T18:38:52Z
dc.date.available2016-09-23T18:38:52Z
dc.date.issued2016-11
dc.description.abstractThe subject of this work is a theoretical analysis of the Pearcey function. In optics, thin lens theory supposes that all rays focus at a unique point where the field converges. For a real lens, the focal point is replaced by a cusp, which is the end point of a caustic curve dividing the bright field region from the dark. My particular interest is the pattern of nodal points within the cusp. By investigating the stationary points for the cusp catastrophe, asymptotic approximations are found for the Pearcey function. This in turn leads to the development of finding the positions of nodal points inside, and outside a caustic. Also values for $|P|$ on a small circle surrounding a node are examined and show reasonable accuracy of order $10^{-8}$.en_US
dc.description.degreeMaster of Science (MSc)en_US
dc.description.degreetypeThesisen_US
dc.description.layabstractIdentifying the nodes of the Pearcey function.en_US
dc.identifier.urihttp://hdl.handle.net/11375/20436
dc.language.isoenen_US
dc.subjectPearcey functionen_US
dc.subjectcusp catastropheen_US
dc.subjectTheoretical physicsen_US
dc.subjectopticsen_US
dc.titleThe Pearcey function and the cusp catastropheen_US
dc.typeThesisen_US

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