'Cosmic microwave background anisotropies' presentation slideshows

The Scalar,Vector and Tensor Contributions of a Stochastic Background of Primordial Magnetic Fields to CMB Anisotropies. Daniela Paoletti University and INFN of Ferrara INAF/IASF-Bologna. Work in collaboration with Fabio Finelli and Francesco Paci For more details:

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Significant effects of second KK particles on LKP dark matter physics

Significant effects of second KK particles on LKP dark matter physics. Mitsuru Kakizaki (ICRR, Univ. of Tokyo & Bonn Univ.). August 29, 2005 @ Bonn Univ. Collaborated with Shigeki Matsumoto (KEK) Yoshio Sato (Saitama U. & Munich, Tech. U.) Masato Senami (ICRR). Refs:

283 views • 19 slides

Cosmic Neutrino Background

Cosmic Neutrino Background. Zong-Kuan Guo NCU, Taiwan, March 30, 2013. particles:. h istory of the relic neutrinos. ~0.3MeV. ~0.1MeV. ~1eV. ~1MeV. n eutrino decoupling. e ? e ? annihilation. photon decoupling. structure formation. BBN. the weak reaction rate:.

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McWilliams Center for Cosmology Colloquium Chris Hirata California Institute of Technology Wednesday, February 29, 20

127 views • 1 slides