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Автор Raffelt, Georg G.
Дата выпуска 1999
dc.description ▪ Abstract  Low-mass particles, such as neutrinos, axions, other Nambu-Goldstone bosons, and gravitons, are produced in the hot and dense interior of stars. Therefore, astrophysical arguments constrain the properties of these particles in ways that are often complementary to cosmological arguments and to laboratory experiments. This review provides an update on the most important stellar-evolution limits and discusses them in the context of other information from cosmology and laboratory experiments.
Формат application.pdf
Издатель Annual Reviews
Копирайт Annual Reviews
Название PARTICLE PHYSICS FROM STARS
DOI 10.1146/annurev.nucl.49.1.163
Print ISSN 0163-8998
Журнал Annual Review of Nuclear and Particle Science
Том 49
Первая страница 163
Последняя страница 216
Аффилиация Raffelt, Georg G.; Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, München, 80805 Germany; e-mail: raffelt@mppmu.mpg.de
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