English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/140587
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:
DC FieldValueLanguage
dc.contributor.authorBartolo, Nicola-
dc.contributor.authorBarreiro, R. Belén-
dc.contributor.authorBonavera, Laura-
dc.contributor.authorCurto, Andrés-
dc.contributor.authorDiego, José María-
dc.contributor.authorGonzález-Nuevo, J.-
dc.contributor.authorHerranz, D.-
dc.contributor.authorLópez-Caniego, M.-
dc.contributor.authorMartínez-González, Enrique-
dc.contributor.authorToffolatti, L.-
dc.contributor.authorVielva, P.-
dc.contributor.authorRebolo López, Rafael-
dc.contributor.authorPlanck Collaboration-
dc.date.accessioned2016-11-23T08:06:03Z-
dc.date.available2016-11-23T08:06:03Z-
dc.date.issued2016-
dc.identifierdoi: 10.1051/0004-6361/201525836-
dc.identifiere-issn: 1432-0746-
dc.identifierissn: 0004-6361-
dc.identifier.citationAstronomy and Astrophysics 594: A17 (2016)-
dc.identifier.urihttp://hdl.handle.net/10261/140587-
dc.descriptionCosmology (including clusters of galaxies).-- et al.-
dc.description.abstractThe Planck full mission cosmic microwave background (CMB) temperature and E-mode polarization maps are analysed to obtain constraints on primordial non-Gaussianity (NG). Using three classes of optimal bispectrum estimators-separable template-fitting (KSW), binned, and modal-we obtain consistent values for the primordial local, equilateral, and orthogonal bispectrum amplitudes, quoting as our final result alone ƒlocalNL = 2.5 ± 5.7, ƒequilNL= -16 ± 70, , and ƒorthoNL = -34 ± 32 (68% CL, statistical). Combining temperature and polarization data we obtain ƒlocalNL = 0.8 ± 5.0, ƒequilNL= -4 ± 43, and ƒorthoNL = -26 ± 21 (68% CL, statistical). The results are based on comprehensive cross-validation of these estimators on Gaussian and non-Gaussian simulations, are stable across component separation techniques, pass an extensive suite of tests, and are consistent with estimators based on measuring the Minkowski functionals of the CMB. The effect of time-domain de-glitching systematics on the bispectrum is negligible. In spite of these test outcomes we conservatively label the results including polarization data as preliminary, owing to a known mismatch of the noise model in simulations and the data. Beyond estimates of individual shape amplitudes, we present model-independent, three-dimensional reconstructions of the Planck CMB bispectrum and derive constraints on early universe scenarios that generate primordial NG, including general single-field models of inflation, axion inflation, initial state modifications, models producing parity-violating tensor bispectra, and directionally dependent vector models. We present a wide survey of scale-dependent feature and resonance models, accounting for the >look elsewhere> effect in estimating the statistical significance of features. We also look for isocurvature NG, and find no signal, but we obtain constraints that improve significantly with the inclusion of polarization. The primordial trispectrum amplitude in the local model is constrained to be g = (-0.9 ± 7.7) X 10(68% CL statistical), and we perform an analysis of trispectrum shapes beyond the local case. The global picture that emerges is one of consistency with the premises of the ΛCDM cosmology, namely that the structure we observe today was sourced by adiabatic, passive, Gaussian, and primordial seed perturbations.-
dc.description.sponsorshipThe Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU).-
dc.publisherEDP Sciences-
dc.relation.isversionofPublisher's version-
dc.rightsopenAccess-
dc.subjectCosmic background radiation-
dc.subjectCosmology: observations-
dc.subjectCosmology: theory-
dc.subjectEarly universe-
dc.subjectInflation-
dc.subjectMethods: data analysis-
dc.titlePlanck 2015 results. XVII. Constraints on primordial non-Gaussianity-
dc.typeartículo-
dc.identifier.doi10.1051/0004-6361/201525836-
dc.relation.publisherversionhttp://dx.doi.org/10.1051/0004-6361/201525836-
dc.date.updated2016-11-23T08:06:03Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.contributor.funderScience Foundation Ireland-
dc.contributor.funderFundação para a Ciência e a Tecnologia (Portugal)-
dc.contributor.funderUK Space Agency-
dc.contributor.funderDepartment of Energy (US)-
dc.contributor.funderAgenzia Spaziale Italiana-
dc.contributor.funderCenter for Science (Finland)-
dc.contributor.funderAcademy of Finland-
dc.contributor.funderScience and Technology Facilities Council (UK)-
dc.contributor.funderNational Aeronautics and Space Administration (US)-
dc.contributor.funderIstituto Nazionale di Astrofisica-
dc.contributor.funderCentre National de la Recherche Scientifique (France)-
dc.contributor.funderDTU Space (Denmark)-
dc.contributor.funderSwiss Space Office-
dc.contributor.funderMax Planck Society-
dc.contributor.funderGerman Centre for Air and Space Travel-
dc.contributor.funderEuropean Space Agency-
dc.contributor.funderJunta de Andalucía-
dc.contributor.funderConsejo Superior de Investigaciones Científicas (España)-
dc.contributor.funderMinisterio de Economía y Competitividad (España)-
dc.contributor.funderEuropean Commission-
dc.contributor.funderEuropean Research Council-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100001602es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100001871es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003981es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000271es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/100000104es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100005184es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004794es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100004189es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100002946es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000844es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003339es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003329es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000780es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000781es_ES
Appears in Collections:(IFCA) Artículos
Files in This Item:
File Description SizeFormat 
XVIIConstraints.pdf15,63 MBAdobe PDFThumbnail
View/Open
Show simple item record
 

Related articles:


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.