... compared with those calculated for large scale structures such as galaxy clusters based on CMB data in the early Universe, don’t match up. And as yet, there is no way to reconcile them or make them fit. “This model is quite interesting...
... kind at this scale and sensitivity and will open a new window (low frequency radio) into the early universe, analogous to the detection of gravitational waves by LIGO and the details of the CMB by Planck,” says Polidan in his...
... field strength and structure in galaxies Since the starburst phenomenon was most likely more common in the early universe when close encounters among galaxies occurred frequently, detailed study of Messier 82 – as the nearest starburst galaxy - can...
... leftover radiation of the Big Bang and studies of this phenomena offer a unique window into the very early Universe and Planck scale physics, I.e. Physics on the tiniest of scales (a Planck length is 1.61×10−35 metres!). How the CMB got...
... first place. Luckily, data from the Planck satellite has already given scientists a snapshot of how the early Universe looked by studying the leftover radiation from the big bang; the cosmic microwave background (C. But since...
... in our understanding of how the inflow of material is regulated around the most intense starburst galaxies in the early Universe. It shows what can be achieved when scientists from a variety of disciplines come together to exploit the capabilities...