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Neutrinos in Astrophysics and Cosmology - INFN Sezione di Ferrara

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Mass Limits on Hot Dark Matter Axions <strong>and</strong> <strong>Neutr<strong>in</strong>os</strong><br />

Hannestad,<br />

Hannestad,<br />

Mirizzi & Raffelt<br />

hep-ph/0504059<br />

hep ph/0504059<br />

m a<br />

Axions<br />

95% 95 CL<br />

< 1.05 eV (95% (95 CL)<br />

Hannestad, Hannestad,<br />

astro-ph/0409108<br />

astro ph/0409108<br />

(Seesaw proceed<strong>in</strong>gs, Paris, 2004)<br />

95% 95 CL<br />

Georg Raffelt, Max-Planck-Institut für Physik, München, Germany IDAPP 2d Meet<strong>in</strong>g, 12-13 May 2006, <strong>Ferrara</strong>, Italy<br />

Σm ν<br />

Σ<br />

<strong>Neutr<strong>in</strong>os</strong><br />

< 0.65 eV (95% (95 CL)

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