Published 1990 | Version v1
Book

Solar oscillation frequency and solar neutrino predictions

Creators

  • 1. Osservatorio Astronomico, Bologna (Italy)

Description

The global quantities of mass, radius, surface effective temperature, luminosity, and the internal composition structure are used to calculate a mass zone model employed in pulsation analyses. The construction of this model is done by integrating the equations of pressure balance and luminosity conservation from the surface to the center in one pass. Pulsation mechanisms are discussed, frequencies are compared with observations, and the frequencies of weakly interacting massive particles are analyzed. It is concluded that solar-oscillation frequencies are predicted to be very close to those observed, but solar neutrino-flux predictions continue to be much larger than observed. 33 refs

Additional details

Publishing Information

Publisher
Astronomical Society of the Pacific.
Imprint Place
San Francisco, CA (USA)
Imprint Title
Confrontation between stellar pulsation and evolution; Proceedings of the Conference (ASP Series, Vol. 11), Bologna, Italy, May 28-31, 1990
Imprint Pagination
616 p.
Journal Page Range
p. 388-400.

Conference

Title
Confrontation between stellar pulsation and evolution.
Dates
28-31 May 1990.
Place
Bologna (Italy).

Optional Information

Notes
Imprint:Sponsered by Ministero dell'Universita e della Ricerca Scientifica e Tecnologica, Universita di Bologna, CNR, and others.
Secondary number(s)
CONF-9005249--.