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 |
Выпуск |
1 |