Titlebook: Current Aspects of Neutrino Physics; David O. Caldwell Book 2001 Springer-Verlag Berlin Heidelberg 2001 Beta decay.Lepton.Neutrino.Particl

結(jié)束

https://doi.org/10.1007/978-3-030-11428-2table consequences. A combination of particle physics, nuclear physics and astrophysics is needed for a full determination of the fundamental properties of neutrinos. This chapter reviews what has been achieved thus far and the future prospects for understanding the nature of neutrino masses and mixing.

kidney

Neutrino Mixing Schemes,table consequences. A combination of particle physics, nuclear physics and astrophysics is needed for a full determination of the fundamental properties of neutrinos. This chapter reviews what has been achieved thus far and the future prospects for understanding the nature of neutrino masses and mixing.

FECK

The Nature of Massive Neutrinos,f the neutrino with other elementary-particles required to explain the nuclear beta decay observations, and neutrinos became an inseparable part of elementary particle physics. The discussion of their discovery and the rest of the history of neutrinos is the subject of the previous chapter.

hidebound

Direct Measurements of Neutrino Mass,nonzero masses? And if so, what are their mass values? The answers to these questions are important both for our theoretical understanding of fundamental interactions of nuclei and particles and because the answers have significant astrophysical and cosmological implications.

Institution

Studies of Neutrino Oscillations at Reactors,eutrino oscillations involving reactor .. More recently, the Chooz [6.5] and Palo Verde [6.6, 6.7] experiments have confirmed these findings with greater sensitivity. The purpose of this chapter is to highlight the developments involving reactor neutrinos and to outline the current status and future studies.

熱情贊揚(yáng)

Pde5-Inhibitors

ESPY

Neutrino Flavor Transformation in Supernovae and the Early Universe,ncurrently, we are undergoing a fantastic increase in the capabilities of observational astronomy, and this promises to provide new insights into the evolution of the Universe. Tantalizingly, these two great trends in science are synergistically linked, at least when it comes to neutrinos!

憂(yōu)傷

High Energy Neutrino Astronomy: Towards Kilometer-Scale Detectors,elds, neutrinos meet the basic requirements for astronomy. Their unique advantage arises from a fundamental property: they are affected only by the weakest of nature’s forces (but for gravity) and are therefore essentially unabsorbed as they travel cosmological distances between their origin and us.

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