AV_Paper1_TheAgeOfTheUniverse
... temperature differences in the Cosmic Microwave Background radiation in order to map the afterglow of the earliest moments of the universe. (NASA 1). This light lost energy as the universe expanded over 13.7 billion years, so WMAP recorded the light as microwaves. By making accurate measurements of ...
... temperature differences in the Cosmic Microwave Background radiation in order to map the afterglow of the earliest moments of the universe. (NASA 1). This light lost energy as the universe expanded over 13.7 billion years, so WMAP recorded the light as microwaves. By making accurate measurements of ...
No Slide Title
... Simple models of inflation predict: This is significant in that it is a clear departure from scale invariance. We expect ns to 1% by 2008 from the CMB. ...
... Simple models of inflation predict: This is significant in that it is a clear departure from scale invariance. We expect ns to 1% by 2008 from the CMB. ...