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dc.contributor.authorBurigana, C.-
dc.contributor.authorGruppuso, A.-
dc.contributor.authorLiguori, Michele-
dc.contributor.authorVielva, P.-
dc.date.accessioned2016-11-18T10:54:07Z-
dc.date.available2016-11-18T10:54:07Z-
dc.date.issued2016-
dc.identifierdoi: 10.1142/S0218271816300160-
dc.identifierissn: 0218-2718-
dc.identifiere-issn: 1793-6594-
dc.identifier.citationInternational Journal of Modern Physics D 25: 1630016 (2016)-
dc.identifier.urihttp://hdl.handle.net/10261/140416-
dc.descriptionBased on presentations at the Fourteenth Marcel Grossmann Meeting on General Relativity, Rome, July 2015.-- et al.-
dc.descriptionarXiv:1604.03819v1-
dc.description.abstractRecent cosmic microwave background (CMB) data in temperature and polarization have reached high precision in estimating all the parameters that describe the current so-called standard cosmological model. Recent results about the integrated Sachs-Wolfe (ISW) effect from CMB anisotropies, galaxy surveys, and their cross-correlations are presented. Looking at fine signatures in the CMB, such as the lack of power at low multipoles, the primordial power spectrum (PPS) and the bounds on non-Gaussianities, complemented by galaxy surveys, we discuss inflationary physics and the generation of primordial perturbations in the early universe. Three important topics in particle physics, the bounds on neutrinos masses and parameters, on thermal axion mass and on the neutron lifetime derived from cosmological data are reviewed, with attention to the comparison with laboratory experiment results. Recent results from cosmic polarization rotation (CPR) analyses aimed at testing the Einstein equivalence principle (EEP) are presented. Finally, we discuss the perspectives of next radio facilities for the improvement of the analysis of future CMB spectral distortion experiments.-
dc.description.sponsorshipCB, AG, ML and TT acknowledge partial support by ASI/INAF Agreement 2014-024-R.0 for the Planck LFI Activity of Phase E2.-
dc.publisherWorld Scientific Publishing-
dc.relation.isversionofPostprint-
dc.rightsopenAccessen_EN
dc.subjectElementary particle processes-
dc.subjectDark matter-
dc.subjectLarge scale structure of the universe-
dc.subjectObservational cosmology-
dc.subjectParticle-theory and field-theory models of the early universe-
dc.subjectOrigin and formation of the universe-
dc.subjectMicrowave-
dc.subjectRadio-
dc.subjectBackground radiations-
dc.subjectCosmology-
dc.subjectDark energy-
dc.titleRecent results and perspectives on cosmology and fundamental physics from microwave surveys-
dc.typeartículo-
dc.identifier.doi10.1142/S0218271816300160-
dc.relation.publisherversionhttp://dx.doi.org/10.1142/S0218271816300160-
dc.embargo.terms2017-05-01-
dc.date.updated2016-11-18T10:54:07Z-
dc.description.versionPeer Reviewed-
dc.language.rfc3066eng-
dc.contributor.funderAgenzia Spaziale Italiana-
dc.contributor.funderIstituto Nazionale di Astrofisica-
dc.relation.csic-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100003981es_ES
dc.identifier.funderhttp://dx.doi.org/10.13039/501100005184es_ES
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