The Cosmic Flows project : voyage to the Great Attractor - LUTH

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CLUES 2 nd generation A simulation of the Local Universe using cosmicflows-1 peculiar velocities as initial conditions (+WMAP7) with direct comparison to the observed galaxy distribution (white dots) : only CDM. Preliminary results (yesterday) Sorce, Courtois and CLUES collab
CLUES Structure Formation with cold and warm Dark Matter http://www.clues-project.org/ Evolution of the gas density in the Local Group for CDM (left) and WDM (right), 4096^3 resimulation, from z=41 to z=0. same color table and density scale was used. Cosmological Parameters Species WDM, 1 keV L box 64 Mpc/h Ω Λ 0.76 Ω m 0.24 Ω bar 0.0418 h 0.73 σ 8 0.75 N 0.95 Iseed 186592 Spectrum EisHu approximation with an exponential cut-off according to a 1keV WDM particle
Page 1 and 2: The Cosmic Flows project : voyage t
Page 3 and 4: The large scale cosmic flows constr
Page 5 and 6: 2004 : Advent of the new giant radi
Page 7: 2008 : Cosmicflows-‐1 2012 : Co
Page 10 and 11: Results from cosmicflows-‐1 in
Page 16 and 17: Constraint simulations using peculi
Page 18 and 19: CLUES 2 A simulation of the Local U
Page 20: Preliminary results (yesterday) Com
Page 25 and 26: Status of Current observaGonal surv
Page 27 and 28: Preliminary results from cosmicflow
Page 29 and 30: Future surveys and simulaGons 2015
Page 31: Thank you hope you will take home s

The Cosmic Flows project : voyage to the Great Attractor - LUTH

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