000763329 000__ 03813cam\a2200469Ki\4500 000763329 001__ 763329 000763329 005__ 20230306142305.0 000763329 006__ m\\\\\o\\d\\\\\\\\ 000763329 007__ cr\cn\nnnunnun 000763329 008__ 161010t20162016sz\\\\\\ob\\\\000\0\eng\d 000763329 019__ $$a960444542$$a960737474$$a962434454 000763329 020__ $$a9783319447698$$q(electronic book) 000763329 020__ $$a3319447696$$q(electronic book) 000763329 020__ $$z9783319447681 000763329 020__ $$z3319447688 000763329 035__ $$aSP(OCoLC)ocn960210457 000763329 035__ $$aSP(OCoLC)960210457$$z(OCoLC)960444542$$z(OCoLC)960737474$$z(OCoLC)962434454 000763329 040__ $$aN$T$$beng$$erda$$epn$$cN$T$$dN$T$$dIDEBK$$dYDX$$dN$T$$dAZU$$dGW5XE$$dOCLCF 000763329 049__ $$aISEA 000763329 050_4 $$aQB991.C64 000763329 08204 $$a523.1$$223 000763329 24504 $$aThe cosmic microwave background :$$bproceedings of the II José Plínio Baptista School of Cosmology /$$cJúlio C. Fabris [and four others] editors. 000763329 264_1 $$aSwitzerland :$$bSpringer,$$c[2016] 000763329 264_4 $$c©2016 000763329 300__ $$a1 online resource. 000763329 336__ $$atext$$btxt$$2rdacontent 000763329 337__ $$acomputer$$bc$$2rdamedia 000763329 338__ $$aonline resource$$bcr$$2rdacarrier 000763329 4901_ $$aAstrophysics and space science proceedings,$$x1570-6591 ;$$vvolume 45 000763329 504__ $$aIncludes bibliographical references. 000763329 5050_ $$aMini Courses -- Physics of the Cosmic Microwave Background Radiation (David Wands, Oliver F. Piattella, Luciano Casarini) -- The Observational Status of Cosmic Inflation after Planck (Jérôme Martin) -- Lecture notes on non-Gaussianity (Christian T. Byrnes) -- Problems of CMB data registration and analysis (O. V. Verkhodanov) -- Cosmic Microwave Background Observations (Rolando Dünner) -- Seminars -- Physics of Baryons (J.A. de Freitas Pacheco) -- Peculiar Velocity Effects on the CMB (Miguel Quartin) -- Warm in ation, cosmological fluctuations and constraints from Planck (Rudnei O. Ramos) -- A brief history of the Brazilian participation in CMB measurements (Thyrso Villela) -- Communications -- On dark degeneracy (Saulo Carneiro and Humberto A. Borges) -- The quantum-to-classical transition of primordial cosmological perturbations (Nelson Pinto-Neto) -- A Path-integral approach to CMB (Paulo H. Reimberg) -- Geometric scalar theory of gravity (Júnior Diniz Toniato). 000763329 506__ $$aAccess limited to authorized users. 000763329 520__ $$aThe series of texts composing this book is based on the lectures presented during the II José Plínio Baptista School of Cosmology, held in Pedra Azul (Espírito Santo, Brazil) between 9 and 14 March 2014. This II JBPCosmo has been entirely devoted to the problem of understanding theoretical and observational aspects of Cosmic Background Radiation (CMB). The CMB is one of the most important phenomena in Physics and a fundamental probe of our Universe when it was only 400,000 years old. It is an extraordinary laboratory where we can learn from particle physics to cosmology; its discovery in 1965 has been a landmark event in the history of physics. The observations of the anisotropy of the cosmic microwave background radiation through the satellites COBE, WMAP and Planck provided a huge amount of data which are being analyzed in order to discover important information regarding the composition of our universe and the process of structure formation. 000763329 588__ $$aDescription based on print version record. 000763329 650_0 $$aCosmic background radiation. 000763329 7001_ $$aFabris, Júlio. C.,$$eeditor. 000763329 77608 $$iPrint version:$$tCosmic Microwave Background.$$d[Place of publication not identified] : Springer Verlag 2016$$z9783319447681$$w(OCoLC)953709241 000763329 830_0 $$aAstrophysics and space science proceedings ;$$vv. 45. 000763329 852__ $$bebk 000763329 85640 $$3SpringerLink$$uhttps://univsouthin.idm.oclc.org/login?url=http://link.springer.com/10.1007/978-3-319-44769-8$$zOnline Access$$91397441.1 000763329 909CO $$ooai:library.usi.edu:763329$$pGLOBAL_SET 000763329 980__ $$aEBOOK 000763329 980__ $$aBIB 000763329 982__ $$aEbook 000763329 983__ $$aOnline 000763329 994__ $$a92$$bISE