Abstract:
This paper discusses some aspects of cosmological expansion as viewed by an observer. It identifies the rate of change of the angular distance $v_\Theta$ with respect to the observer's clock as a crucial quantity in properly understanding the expansion. Using this quantity and the angular distance, in addition to the traditional approach to visualization, provides a more vivid picture of the cosmological expansion and is key for adequately visualizing it.
PACS:98.62.Py, 98.80.-k, 98.80.Es
Received:September 2, 2013 Revised:October 15, 2013 Accepted: October 15, 2013