dc.contributor.author | Mulryne, DJ | en_US |
dc.date.accessioned | 2016-10-17T12:46:18Z | |
dc.date.available | 2016-09-01 | en_US |
dc.date.issued | 2016-09-05 | en_US |
dc.date.submitted | 2016-09-19T12:21:01.216Z | |
dc.identifier.uri | http://qmro.qmul.ac.uk/xmlui/handle/123456789/15890 | |
dc.description | 21 pages, 5 figures | |
dc.description | 21 pages, 5 figures | |
dc.description | 21 pages, 5 figures | en_US |
dc.description.abstract | PyTransport 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.ispartof | arXiv | en_US |
dc.rights | arXiv record: https://arxiv.org/abs/1609.00381 | |
dc.subject | astro-ph.CO | en_US |
dc.subject | astro-ph.CO | en_US |
dc.subject | hep-th | en_US |
dc.title | PyTransport: A Python package for the calculation of inflationary correlation functions | en_US |
dc.type | Article | |
pubs.author-url | http://arxiv.org/abs/1609.00381v1 | en_US |
pubs.notes | Not known | en_US |
pubs.publication-status | Published online | en_US |
dcterms.dateAccepted | 2016-09-01 | en_US |