Possible mass limits for quantum double galaxies

Details Possible mass limits for quantum double galaxies Possible mass limits for quantum double galaxies

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.126..409d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 126, no. 2, Oct. 1986, p. 409-412.

Astronomy and Astrophysics

Astrophysics

Galactic Structure, Mass Distribution, Quantum Mechanics, Range (Extremes), Cosmology, Gravitational Constant, Relativistic Theory, Schroedinger Equation, Time Dependence

Scientific paper

When cosmic quantum mechanics is applied to a double galaxy, the result is mass limits in order for the two galaxies to form a quantum binary system. For a non-relativistic theory (based on the Schrödinger wave equation), the mass limits are: (mg)max ≈ 1012M_sun; and (mg)min ≈ 1010M_sun;. One possible consequence appears to be a Newtonian gravitational constant that varies with cosmic time, with its value larger in the cosmic past.

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