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dc.contributor.authorCyr-Racine, Francis-Yan
dc.contributor.authorSigurdson, Kris
dc.contributor.authorZavala, Jesús
dc.contributor.authorBringmann, Torsten
dc.contributor.authorVogelsberger, Mark
dc.contributor.authorPfrommer, Christoph
dc.date.accessioned2017-03-24T19:49:53Z
dc.date.available2017-03-24T19:49:53Z
dc.date.issued2016-06
dc.date.submitted2016-02
dc.identifier.issn2470-0010
dc.identifier.issn2470-0029
dc.identifier.urihttp://hdl.handle.net/1721.1/107699
dc.description.abstractWe formulate an effective theory of structure formation (ETHOS) that enables cosmological structure formation to be computed in almost any microphysical model of dark matter physics. This framework maps the detailed microphysical theories of particle dark matter interactions into the physical effective parameters that shape the linear matter power spectrum and the self-interaction transfer cross section of nonrelativistic dark matter. These are the input to structure formation simulations, which follow the evolution of the cosmological and galactic dark matter distributions. Models with similar effective parameters in ETHOS but with different dark particle physics would nevertheless result in similar dark matter distributions. We present a general method to map an ultraviolet complete or effective field theory of low-energy dark matter physics into parameters that affect the linear matter power spectrum and carry out this mapping for several representative particle models. We further propose a simple but useful choice for characterizing the dark matter self-interaction transfer cross section that parametrizes self-scattering in structure formation simulations. Taken together, these effective parameters in ETHOS allow the classification of dark matter theories according to their structure formation properties rather than their intrinsic particle properties, paving the way for future simulations to span the space of viable dark matter physics relevant for structure formation.en_US
dc.description.sponsorshipMIT Research Support Committee (Reed Fund)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevD.93.123527en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleETHOS—an effective theory of structure formation: From dark particle physics to the matter distribution of the Universeen_US
dc.typeArticleen_US
dc.identifier.citationCyr-Racine, Francis-Yan et al. “ETHOS—an Effective Theory of Structure Formation: From Dark Particle Physics to the Matter Distribution of the Universe.” Physical Review D 93.12 (2016): n. pag. CrossRef. Web. 24 Mar. 2017. © 2016 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorVogelsberger, Mark
dc.relation.journalPhysical Review Den_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2016-06-28T22:00:14Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsCyr-Racine, Francis-Yan; Sigurdson, Kris; Zavala, Jesús; Bringmann, Torsten; Vogelsberger, Mark; Pfrommer, Christophen_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-8593-7692
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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