Decaying dark matter and the value of the Hubble constant

Details Decaying dark matter and the value of the Hubble constant Decaying dark matter and the value of the Hubble constant

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...243..341s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 243, no. 2, March 1991, p. 341-343.

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Dark Matter, Degenerate Matter, Hubble Constant, Computational Astrophysics, Milky Way Galaxy, Spatial Distribution

Scientific paper

Sciama's decaying dark matter hypothesis (DDM) is used to determine the distance of four galaxies whose rotation curves are similar to those of the Galaxy and NGC 891, for which the DDM hypothesis agrees well with observation. A mean value for the Hubble constant is then derived from the observed redshifts of the five galaxies. The value obtained H = 54 + or - 7 km/sec M/pc agrees well with that derived independently from the DDM hypothesis H = 55 + or - 1 km/sec M/pc.

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