Weakly interacting massive particles, solar neutrinos, and solar oscillations

Details Weakly interacting massive particles, solar neutrinos, and solar oscillations Weakly interacting massive particles, solar neutrinos, and solar oscillations

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986natur.321..229d&link_type=abstract

Nature (ISSN 0028-0836), vol. 321, May 15, 1986, p. 229-231.

Computer Science

40

Particle Theory, Solar Neutrinos, Solar Oscillations, Weak Interactions (Field Theory), Helioseismology

Scientific paper

Weakly interacting, massive particles (WIMPs) have recently been proposed as a solution to the solar neutrino problem. Solar models which incorporate a relative number of 10-11WIMPs with appropriate scattering cross-section would reduce the predicted neutrino detections by 37Cl to the observed value, without significant changes in the solar structure outside the central region. The authors have subjected these models to an observational test of p-mode oscillation frequencies by computing frequency differences of low-degree, high-order oscillation frequencies. Although standard solar models also pass this test, WIMP models provide a better fit.

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