'Cmb data' diaporamas de présentation

L. Fauvet, J.F. Macías-Pérez, F.-X. Désert

Modeling of the galactic polarized foreground emissions to minimize the contamination of the BB modes. L. Fauvet, J.F. Macías-Pérez, F.-X. Désert. Summary. ¤ Polarized foregrounds ¤ 3D modeling of the galaxy ¤ Contamination of the CMB data

763 views • 60 slides

Cosmic Microwave Background

Cosmic Microwave Background. Carlo Baccigalupi, SISSA CMB lectures at TRR33, see the complete program at darkuniverse.uni-hd.de/view/Main/WinterSchoolLecture5 These lectures are available in pdf format at people.sissa.it/~bacci/work/lectures. CMB and foregrounds. Outline .

456 views • 23 slides

Chaplygin gas in decelerating DGP gravity

Chaplygin gas in decelerating DGP gravity Matts Roos University of Helsinki Department of Physics and Department of Astronomy 43rd Rencontres de Moriond, Cosmology La Thuile (Val d'Aosta, Italy) March 15 - 22, 2008 Contents Introduction The DGP model The Chaplygin gas model

546 views • 21 slides

Mildly Mixed Coupled cosmological models

Mildly Mixed Coupled cosmological models. *La Vacca, B., Colombo, arXiv:0810.0127 & NewA. (Higher neutrino mass allowed if CDM & DE are coupled) *La Vacca, Kristiansen, Mainini,B., Colombo, arXiv:0902.2711 & JCAP (Do WMAP data favor neutrino mass and a coupling between CDM and DE?)

342 views • 21 slides

Early & Late Inflation Theory cf. CMB+LSS @ CITA

Early & Late Inflation Theory cf. CMB+LSS @ CITA. Concordance (pre-WMAP2++) & discordant notes. The “basic parameters”: LCDM with power law index and no/little GW is concordant. Some discord .. always. Extension to larger parameter lists.

255 views • 11 slides

p03-butterworth

112 views • 1 slides