George Smoot were able to measure minute variations, or 'anisotropies', in the background radiation that are the faint whispers left behind by developing clusters in the expanding universe. ❋ Unknown (2006)
New Scientist duly have an article to herald the launch, which claims that these so-called anisotropies are believed to be due to inflation ... ❋ Gordon McCabe (2009)
Smoot shared the 2006 Nobel Prize in Physics for measuring anisotropies in the CMB and is one of the authors of the ApJ paper. ❋ Unknown (2010)
These anisotropies with the SZ shadows and polarizations are, as the UT post here by Jean Tate indicates, weak correlations to these much earlier processes in the universe. ❋ Unknown (2010)
This is a an interesting result and it will be interesting to see how these anisotropies correlated with the CMB anisotropies. ❋ Unknown (2010)
The polarization of anisotropies and inverse Compton scattering signatures in the Sunyaev-Zel'dovich effect indicate stochastic fluctuations associated with inflation. ❋ Unknown (2010)
Planck satellite measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field. ❋ Unknown (2008)
These anisotropies are largely due to a quantum fluctuation, such as the scalar field of inflation inflaton, and we would not expect statistics which violated this, such as significant non-Gaussian distributions. ❋ Unknown (2010)
In the Seven-Year WMAP papers for example, WMAP's observations of CMB anisotropies were combined with observations of BAO to constrain dark energy. ❋ Unknown (2010)
The inflationary period smoothed anisotropies in a way which precluded their formation. ❋ Unknown (2009)
The B-modes are anisotropies due to polarization states. ❋ Unknown (2009)
In early 1991, anisotropies at many angular scales became evident in the data from the DMRs. ❋ Unknown (2007)
In fact, at least three such instances of apparent large-scale anisotropies have been claimed. ❋ Sean (2008)
In fact, this asymmetry between matter and antimatter can be made quantitative (for baryons such as protons and neutrons) through observations of the abundances of light elements in the universe (Big Bang Nucleosynthesis - BBN) and also from the pattern of anisotropies in the cosmic microwave background radiation (CMB). ❋ Mark (2008)
They were predicted to exist, these variations or anisotropies? ❋ Unknown (2006)
The in-depth analysis of the radiometer data has shown the presence of the long sought small temperature anisotropies, the seed of the structures in the Universe that we observe today. ❋ Unknown (2006)
We analyze the CMB temperature anisotropies generated by a single-mode adiabatic superhorizon perturbation. ❋ Sean (2008)
“Seeing” reversed: photons stream out of phototransmissors in all sorts of directions with anisotropies at different frequencies. ❋ Sean (2008)
Some people are fortunate enough to have programmatic, focused research agendas — when I was a postdoc at MIT in the early Nineties, Ed Bertschinger had collected around him an amazing set of postdocs and grad students, all focused on understanding temperature anisotropies in the cosmic microwave background and what they could tell us about the universe. ❋ Sean (2007)
