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A Short History of the Missing Mass and Dark Energy Paradigms

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arxiv astro-ph/0005314 v1 pith:4ZYMGGFJ submitted 2000-05-15 astro-ph

classification astro-ph
keywords darkmasscolduniverseenergymatterstarsaccount
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In 1900 it was believed that almost 100% of the mass of the Universe resided in stars. Now, in the year 2000, such stars (and cold gas) are known to account for only ~1% its mass. The remaining mass of the Universe is thought to reside in hot baryons (~3%), cold dark matter (~30%) and dark energy (~66%). The present paper traces the evolution of our thinking about the density of the Universe during the Twentieth Century, with special emphasis on the of the discovery of cold dark matter.

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  1. MIGHTEE-HI / LADUMA: Investigating the link between baryons and dynamics with 130 resolved HI-selected galaxies

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    A 130-galaxy HI-selected sample yields a tight radial acceleration relation with an acceleration scale near 1.5e-10 m/s^2 and a MOND shape parameter around 4, and shows that the bTFR redshift-evolution signal is large...

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