000308161 001__ 308161
000308161 005__ 20211110134939.0
000308161 037__ $$aPUBDB-2016-03512
000308161 041__ $$aEnglish
000308161 0881_ $$ahep-ph/0309238; DESY-03-152; PIC-2003-THBT01
000308161 088__ $$2arXiv$$ahep-ph/0309238
000308161 088__ $$2DESY$$aDESY-03-152
000308161 088__ $$2Other$$aPIC-2003-THBT01
000308161 1001_ $$0P:(DE-H253)PIP1005321$$aCovi, Laura$$b0$$eCorresponding author$$udesy
000308161 1112_ $$a23rd International Conference on Physics in Collision$$cZeuthen$$d2003-06-26 - 2003-06-28$$gPIC 2003$$wGermany
000308161 245__ $$aStatus of observational cosmology and inflation
000308161 260__ $$c2003
000308161 300__ $$a67-80
000308161 3367_ $$2ORCID$$aCONFERENCE_PAPER
000308161 3367_ $$033$$2EndNote$$aConference Paper
000308161 3367_ $$2BibTeX$$aINPROCEEDINGS
000308161 3367_ $$2DRIVER$$aconferenceObject
000308161 3367_ $$0PUB:(DE-HGF)29$$2PUB:(DE-HGF)$$aReport$$mreport
000308161 3367_ $$2DataCite$$aOutput Types/Conference Paper
000308161 3367_ $$0PUB:(DE-HGF)8$$2PUB:(DE-HGF)$$aContribution to a conference proceedings$$bcontrib$$mcontrib$$s1473400107_30638
000308161 520__ $$aWe review the latest developments in the determination of the cosmological parameters from the measurement of the Cosmic Microwave Background Radiation (CMBR) anisotropies and of the Large Scale Structure (LSS) of the Universe. We comment finally on the implications for the primordial spectrum and the consequences for inflationary models.
000308161 536__ $$0G:(DE-HGF)POF3-899$$a899 - ohne Topic (POF3-899)$$cPOF3-899$$fPOF III$$x0
000308161 588__ $$aDataset connected to INSPIRE
000308161 650_7 $$2INSPIRE$$atalk: Zeuthen 2003/06/26
000308161 650_7 $$2INSPIRE$$acosmological model
000308161 650_7 $$2INSPIRE$$acosmic background radiation
000308161 650_7 $$2INSPIRE$$aanisotropy
000308161 650_7 $$2INSPIRE$$apolarization
000308161 650_7 $$2INSPIRE$$ainflation
000308161 650_7 $$2INSPIRE$$aenergy: density
000308161 650_7 $$2INSPIRE$$amatter: density
000308161 650_7 $$2INSPIRE$$abaryon: density
000308161 650_7 $$2INSPIRE$$adark matter
000308161 650_7 $$2INSPIRE$$atemperature
000308161 650_7 $$2INSPIRE$$aneutrino
000308161 650_7 $$2INSPIRE$$ainterpretation of experiments
000308161 693__ $$0EXP:(DE-H253)HERA(machine)-20150101$$1EXP:(DE-588)4159571-3$$5EXP:(DE-H253)HERA(machine)-20150101$$aHERA$$eFacility (machine) HERA$$x0
000308161 7870_ $$0PUBDB-2016-03507$$aRiemann, S. et.al.$$d2003$$iIsPartOf$$r$$tPhysics in collisions. Proceedings, 23rd International Conference, PIC 2003, Zeuthen, Germany, June 26-28, 2003
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.pdf$$yOpenAccess
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.gif?subformat=icon$$xicon$$yOpenAccess
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000308161 8564_ $$uhttps://bib-pubdb1.desy.de/record/308161/files/0309238.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000308161 909CO $$ooai:bib-pubdb1.desy.de:308161$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000308161 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1005321$$aDeutsches Elektronen-Synchrotron$$b0$$kDESY
000308161 9131_ $$0G:(DE-HGF)POF3-899$$1G:(DE-HGF)POF3-890$$2G:(DE-HGF)POF3-800$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$aDE-HGF$$bProgrammungebundene Forschung$$lohne Programm$$vohne Topic$$x0
000308161 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000308161 9201_ $$0I:(DE-H253)L-20120731$$kL$$lBibliothek und Dokumentation$$x0
000308161 980__ $$acontrib
000308161 980__ $$aVDB
000308161 980__ $$aUNRESTRICTED
000308161 980__ $$areport
000308161 980__ $$aI:(DE-H253)L-20120731
000308161 9801_ $$aFullTexts