Physics
Scientific paper
Nov 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aps..psf.h2010b&link_type=abstract
American Physical Society, Inaugural Fall 2009 Meeting of the Prairie Section of the APS, November 12-14, 2009, abstract #H2.010
Physics
Scientific paper
In the early universe stellar cores were formed primarly in the galactic and pre-galactic arms. These cores were made up of a dense hydrogen mass prinarly which were slowly rotating. Orbiting these dense hydrogen cores were dense concentric rings of primarily hydrogen gas moving at a relatively fast rate. As the orbits of the rings decayed due to gravitational attraction, the rings of orbiting hydrogen matter tangentially collided and adhered to the pre-formed stellar core transfering the faster orbital angular momemtum of the rings to the stellar cores resulting in a faster rotating stellar bodies which over time began to rotate differentially due to internal forces from stellar burning.
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