Chin and Stothers 1976
Chin, C.-W., and R. Stothers, 1976: Limit on the secular change of the gravitational constant based on studies of solar evolution. Phys. Rev. Lett., 36, 833-835, doi:10.1103/PhysRevLett.36.833.
The past and present observable properties of the Sun have been theoretically calculated on the assumption that the gravitational constant G increases or decreases with time. Consideration of Davis's experimental upper limit on the present solar neutrino flux and of terrestial paleontological data sets a limit on the absolute rate of change of G, namely, |G'0/G0|<1×10-10/yr, if other standard constants do not also change with time.
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Chin, C.-W., and Stothers, R.: Limit on the secular change of the gravitational constant based on studies of solar evolution, Phys. Rev. Lett., 36, 833-835, doi:10.1103/PhysRevLett.36.833, 1976.
Chin, C.-W., and R. Stothers (1976), Limit on the secular change of the gravitational constant based on studies of solar evolution, Phys. Rev. Lett., 36, 833-835, doi:10.1103/PhysRevLett.36.833.
Chin, C.-W., and R. Stothers, 1976: Limit on the secular change of the gravitational constant based on studies of solar evolution. Phys. Rev. Lett., 36, 833-835, doi:10.1103/PhysRevLett.36.833.
Chin, C.-W., & Stothers, R. 1976, Phys. Rev. Lett., 36, 833, doi:10.1103/PhysRevLett.36.833.
Chin C-W, Stothers R. Limit on the secular change of the gravitational constant based on studies of solar evolution, Phys Rev Lett 1976;36:833-835. doi:10.1103/PhysRevLett.36.833.
C.-W. Chin, R. Stothers, Phys. Rev. Lett. 36, 833-835, doi:10.1103/PhysRevLett.36.833 (1976).
