Weekly seminars
Our local anisotropic Universe and large-scale isotropy
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Europe/Paris
Auditorium Vivargent (Annecy-le-Vieux)
Auditorium Vivargent
Annecy-le-Vieux
Description
Our local Universe is anisotropic. However, on large scales the cosmic
microwave background radiation data demonstrates clearly that the Universe
is highly isotropic. I use the convergence to CMB dipole and also of the
bulk flow of galaxies as indicators of the anisotropy. By measuring these
quantities in SNe Ia (Union II data) and the galaxy redshift data (2MRS),
we can determine whether and on what scales the transition to isotropy
occurs and whether it is consistent with the expectation of LCDM model.