A number of solutions to this problem have been proposed, including several versions of an "inflationary model", in which space itself expanded faster than the speed of light early in the Big Bang, but ''after'' different areas exchanged radiation to even out the temperature. This model fits the data, as the CMB is only uniform at certain scales; over large enough areas anisotropies are visible in the field that match what one would expect from a rapidly expanding gas. However, there is no consensus on which explanation is correct, and each of the proposed solutions has its own problems.<ref name="Lisle" /> | A number of solutions to this problem have been proposed, including several versions of an "inflationary model", in which space itself expanded faster than the speed of light early in the Big Bang, but ''after'' different areas exchanged radiation to even out the temperature. This model fits the data, as the CMB is only uniform at certain scales; over large enough areas anisotropies are visible in the field that match what one would expect from a rapidly expanding gas. However, there is no consensus on which explanation is correct, and each of the proposed solutions has its own problems.<ref name="Lisle" /> |