Actions for Horizontal branch stars as a probe of non baryonic dark matter [electronic resource].

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Horizontal branch stars as a probe of non baryonic dark matter [electronic resource].

Published
Berkeley, Calif. : Lawrence Berkeley National Laboratory, 1989.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description
Pages: 8 : digital, PDF file
Additional Creators
Lawrence Berkeley National Laboratory and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
The solar neutrino problem can be interpreted as a signature for the existence and properties of certain dark matter candidate particles (''cosmions''). We investigate the breaking of convection by neutrino-like cosmions in horizontal branch (HB) stars. These particles may affect globular clusters in the inner galaxy or in dwarf spheroidals where the dark matter density is larger than in the solar neighborhood, leading to an observable reduction of the HB lifetime. 10 refs., 1 fig.
Report Numbers
E 1.99:lbl-26589
E 1.99: conf-881212-2
conf-881212-2
lbl-26589
Subject(s)
Other Subject(s)
Note
Published through SciTech Connect.
01/01/1989.
"lbl-26589"
" conf-881212-2"
"DE89015448"
Particle astrophysics workshop, Berkeley, CA, USA, 8-10 Dec 1988.
Silk, J.; Raffelt, G.; Salati, P.; Bouquet, A.
Funding Information
AC03-76SF00098
View MARC record | catkey: 13826637