Slide 1Backreaction as an explanation for Dark Energy ? with some remarks on cosmological perturbation theory James M. Bardeen University of Washington The Very Early Universe…

Slide 1 When Black Holes Collide Frans Pretorius Princeton University STScI Colloquium February 18, 2009 STScI Colloquium February 18, 2009 Slide 2 Outline I Motivation:…

Slide 1 Large-angle anomalies in the microwave background: Are they real? What do they mean? Ted Bunn University of Richmond TexPoint fonts used in EMF. Read the TexPoint…

Slide 1 Direct Dark Matter Searches Aldo Ianni, INFN-LNGS 12 Mar., 2014 Cagliari 1 Slide 2 Evidence of Dark Matter Spiral galaxies rotation curves:  halo ~ 10  stars…

Slide 1 WMAP Slide 2 The Wilkinson Microwave Anisotropy Probe was designed to measure the CMB. –Launched in 2001 –Ended 2010 Microwave antenna includes five frequency…

CMB and Secondaries: the Cold Spot Isabella Masina (Ferrara U., Italy & CP3-SDU, Denmark) Based on: I.M, A.Notari, JCAP 0902:019,2009. arXiv:0808.1811  JCAP 0907:035,2009.…

Large-scale Structure: Theory & Observations Josh Frieman Structure Formation & Evolution, Santiago, October 2002 The Structure Formation Cookbook 1. Initial Conditions:…

Astrobites: The astro-ph âReaderâs Digestâ for Undergraduates The astro-ph âReaderâs Digestâ Christopher M. Faesi (Harvard Univ.) on behalf of the Astrobites collaboration…

Forthcoming CMB experiments and expectations for dark energy Carlo Baccigalupi Outline “Classic” dark energy effects on CMB “Modern” CMB relevance for dark energy:…

Can Backreaction Mimic Dark Energy? with comments on using large scale inhomogeneity to modify the DL-z relation James M. Bardeen University of Washington CIfAR/Linde Fest…