The Sun and stars: Giving light to dark matter - INSPIRE

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The Sun and stars: Giving light to dark matter

Jordi Casanellas
(
- Potsdam, Max Planck Inst.
)
,
Ilídio Lopes
(
- Lisbon, CENTRA and
- Evora U.
)

Nov 19, 2014

12 pages

Published in:

Mod.Phys.Lett.A 29 (2014) 37, 1440001

Published: Nov 19, 2014

e-Print:

1411.6807 [astro-ph.CO]

DOI:

10.1142/S021773231440001X

View in:

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Abstract: (World Scientific)

During the last century, with the development of modern physics in such diverse fields as thermodynamics, statistical physics, and nuclear and particle physics, the basic principles of the evolution of stars have been successfully well understood. Nowadays, a precise diagnostic of the stellar interiors is possible with the new fields of helioseismology and astroseismology. Even the measurement of solar neutrino fluxes, once a problem in particle physics, is now a powerful probe of the core of the Sun. These tools have allowed the use of stars to test new physics, in particular the properties of the hypothetical particles that constitute the dark matter (DM) of the Universe. Here we present recent results obtained using this approach.

Note:

12 pages, 3 figures

95.35.+d
96.60.Ly
97.10.Sj
26.65.+t
Dark matter
Sun
solar neutrinos
helioseismology
asteroseismology
dark matter

References(102)

Figures(5)

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