Next-to-leading resummations in cosmological perturbation theory release_wwo2turlrvde3p7azqolwmdbxq

by Stefano Anselmi, Sabino Matarrese, Massimo Pietroni

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abstracts[] {'sha1': 'fd1a85fb002a340494b89f41d0321f04164a2953', 'content': 'One of the nicest results in cosmological perturbation theory is the\nanalytical resummaton of the leading corrections at large momentum, which was\nobtained by Crocce and Scoccimarro for the propagator. Using an exact evolution\nequation, we generalize this result, by showing that a class of next-to-leading\ncorrections can also be resummed at all orders in perturbation theory. The new\ncorrections modify the propagator by a few percent in the Baryonic Acoustic\nOscillation range of scales, and therefore cannot be neglected in resummation\nschemes aiming at an accuracy compatible with future generation galaxy surveys.\nSimilar tools can be employed to derive improved approximations for the Power\nSpectrum.', 'mimetype': 'text/plain', 'lang': 'en'}
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{'index': 1, 'creator_id': None, 'creator': None, 'raw_name': 'Sabino Matarrese', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
{'index': 2, 'creator_id': None, 'creator': None, 'raw_name': 'Massimo Pietroni', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
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language en
license_slug ARXIV-1.0
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release_date 2010-11-19
release_stage submitted
release_type article
release_year 2010
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title Next-to-leading resummations in cosmological perturbation theory
version v1
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work_id u42xhb6fdvbc5govtvx7774364
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arxiv.base_id 1011.4477
arxiv.categories ['astro-ph.CO', 'hep-ph', 'hep-th']
arxiv.comments 29 pages, 18 figures. Accepted for publication in JCAP
superceded True