Physics – Nuclear Physics
Scientific paper
Sep 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...102....8r&link_type=abstract
Astronomy and Astrophysics, vol. 102, no. 1, Sept. 1981, p. 8-11.
Physics
Nuclear Physics
3
Energy Transfer, Gravitational Effects, Nuclear Physics, Solar Neutrinos, Perturbation Theory, Steady State, Stellar Models, Transient Response
Scientific paper
It is proposed that a part of the energy emitted by the sun and other stars is due to a gravitational energy release (L/GN/), induced by nuclear energy generation processes. The L(GN) involves a reduction in pressure resulting from the decrease in the number of free particles per gram of stellar material in the energy generation region. The basic reference steady-state results are obtained using accurate self-consistent equation of state and solar structure calculations that reproduce temperature, density, and chemical abundance profiles of a standard evolution model of the present sun. For the standard model used, a transient rate of temperature decrease and coupled rate of density increase between one and two orders of magnitude greater than the steady-state magnitudes will yield an estimated L(GN) of about 0.0010 solar L.
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