Emergence of Cosmic Structure: The First Two Centuries of the First Two Eons

Details Emergence of Cosmic Structure: The First Two Centuries of the First Two Eons Emergence of Cosmic Structure: The First Two Centuries of the First Two Eons

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..apr.h8002t&link_type=abstract

American Physical Society, April Meeting, 2003, April 5-8, 2003 Philadelphia, Pennsylvania, MEETING ID: APR03, abstract #H8.002

Astronomy and Astrophysics

Astronomy

Scientific paper

The process by which we have come to appreciate the large scale structure of universe of superclusters and voids resembles a game of snakes and ladders or "lose on the swings what you gain on the roundabouts." In practice, for a number of decades, some people were working on what we now think of as astronomy of the second half of the 20th century while others were simultaneously working on distinctly 19th century astronomy. It is possible to argue about whether this is just a description or some sort of explanation. Incidentally, the K term (which we now call Hubble's constant, H) arose within stellar astronomy to describe a seemingly analogous phenomenon among hot stars.

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