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dc.contributor.authorMulryne, DJen_US
dc.date.accessioned2016-10-17T12:46:18Z
dc.date.available2016-09-01en_US
dc.date.issued2016-09-05en_US
dc.date.submitted2016-09-19T12:21:01.216Z
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/15890
dc.description21 pages, 5 figures
dc.description21 pages, 5 figures
dc.description21 pages, 5 figuresen_US
dc.description.abstractPyTransport constitutes a straightforward code written in C++ together with Python scripts which automatically edit, compile and run the C++ code as a Python module. It has been written for Unix-like systems (OS X and Linux). Primarily the module employs the transport approach to inflationary cosmology to calculate the tree-level power-spectrum and bispectrum of user specified models of multi-field inflation, accounting for all sub and super-horizon effects. The transport method we utilise means only coupled differential equations need to be solved, and the implementation presented here combines the speed of C++ with the functionality and convenience of Python. At present the code is restricted to canonical models. This document details the code and illustrates how to use it with a worked example.en_US
dc.relation.ispartofarXiven_US
dc.rightsarXiv record: https://arxiv.org/abs/1609.00381
dc.subjectastro-ph.COen_US
dc.subjectastro-ph.COen_US
dc.subjecthep-then_US
dc.titlePyTransport: A Python package for the calculation of inflationary correlation functionsen_US
dc.typeArticle
pubs.author-urlhttp://arxiv.org/abs/1609.00381v1en_US
pubs.notesNot knownen_US
pubs.publication-statusPublished onlineen_US
dcterms.dateAccepted2016-09-01en_US


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