Abstract
view Abstract Citations (12) References (20) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Oscillations in Solar Models with Weakly Interacting Massive Particles Gilliland, Ronald L. ; Dappen, Werner Abstract Solar models containing concentrations as low as 10-11 by number of weakly interacting massive particles (WIMPs), accreted from a galactic background population, are consistent with the observed flux of high-energy solar neutrinos. The structural changes produced in the solar core have also been shown to produce changes in the oscillation frequencies of g-modes and p-modes of low angular degree and high radial order. In this paper the authors examine the predictions for solar oscillations over a large range of possible WIMP properties. Publication: The Astrophysical Journal Pub Date: January 1988 DOI: 10.1086/165970 Bibcode: 1988ApJ...324.1153G Keywords: Particle Interactions; Solar Neutrinos; Solar Oscillations; Stellar Models; Weak Interactions (Field Theory); Particle Flux Density; Stellar Cores; Stellar Interiors; Vibration Mode; Solar Physics; ELEMENTARY PARTICLES; NEUTRINOS; SUN: INTERIOR; SUN: OSCILLATIONS full text sources ADS |
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