Titlebook: Neutrinos in Particle Physics, Astronomy and Cosmology; Zhi-Zhong Xing,Shun Zhou Book 2011 Springer-Verlag Berlin Heidelberg 2011 ATSTC.Co

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書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology影響因子(影響力)




書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology影響因子(影響力)學(xué)科排名




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書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology被引頻次




書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology被引頻次學(xué)科排名




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書目名稱Neutrinos in Particle Physics, Astronomy and Cosmology讀者反饋學(xué)科排名

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Seesaw Mechanisms of Neutrino Masses,een their theoretical naturalness and experimental testability. Possible collider signatures of TeV seesaw mechanisms and their consequences on non-unitary neutrino mixing and CP violation will also be discussed.

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Book 2011 and neutrino cosmology. The intrinsic properties and fundamental interactions of neutrinos are described, as is the phenomenology of lepton flavor mixing, seesaw mechanisms and neutrino oscillations. The cosmic neutrino background, stellar neutrinos, supernova neutrinos and ultrahigh-energy cosmic

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Neutrinos from Stars, we shall concentrate on the neutrinos generated from thermal nuclear reactions in the solar core. The production processes, experimental detection and flavor conversions of solar neutrinos will be discussed in detail.

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Book 2011 book is intended for researchers and graduate students in the fields of particle physics, particle astrophysics and cosmology. .Dr. Zhizhong Xing is a professor at the Institute of High Energy Physics, Chinese Academy of Sciences, China; Dr. Shun Zhou is currently a postdoctoral fellow at the Max Planck Institute for Physics, Germany..

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Neutrinos from Supernovae,ntal detection of the neutrino burst from the SN 1987A, we shall explore its implications on neutrino masses and neutrino lifetimes. The flavor conversions of supernova neutrinos, including the effects of collective neutrino oscillations, will be discussed in detail.

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Neutrinos and Cosmological Structures, chapter we shall first describe how the CMB and large-scale structures (LSS) formed, and then discuss how to constrain neutrino masses from the measurements of the CMB and LSS. We shall also comment on sterile neutrinos as a possible candidate of warm dark matter in the Universe.