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Antarctic detector offers first look at how Earth stops high-energy neutrinos in their tracks
Antarctic detector Earth stops high-energy neutrinos their tracks
2017/11/24
An interdisciplinary team of researchers using the IceCube Neutrino Observatory in Antarctica has measured how certain high-energy neutrinos are absorbed by the Earth, as opposed to passing through ma...
2017届国际中微子加速器研讨会（The 2017 International Workshop on Neutrinos from Accelerators）
2017届 国际中微子加速器 研讨会
2017/7/11
NUFACT2017 is the nineteenth in the series of yearly international workshops which started in 1999 and which until now was called International Workshop on Neutrino Factories. The change of name to In...
Neutrinos and Their Charged Cousins: Are They Secret Sharers?
Neutrinos Charged Cousins Secret Sharers
2011/9/14
“Neutrinos they are very small. They have no charge and have no mass and do not interact at all.” So wrote the renowned author John Updike, erring twice in one couplet. Indeed, neutrinos are the most ...
Gravitational interactions between fast neutrinos and the formation of bound rotational states
Gravitational neutrinos Circular states
2011/8/31
The gravitational forces exerted between fast neutrinos at short distances are examined using Newton’s gravitational law, special relativity, and the equivalence principle. It is found that the magnit...
Model Independent Constraints on Solar Neutrinos
Model Independent Constraints Solar Neutrinos
2011/4/7
Model Independent Constraints on Solar Neutrinos 。
Oil tankers fitted with neutrino detectors, hundreds of thousands of tonnes in mass, could be floated offshore to check for undeclared nuclear fission reactors. That's the idea of physicists in France...
RENO: An Experiment for Neutrino Oscillation Parameter theta_13 Using Reactor Neutrinos at Yonggwang
Neutrino Oscillation Reactor Neutrinos
2010/3/16
The RENO experiment is a short baseline neutrino experiment in Korea aiming to measure the neutrino mixing angle theta_13 or set limit to sin^2(2 theta_13) less than 0.02. This document describes phys...
Geo-neutrinos, electron anti-neutrinos produced in beta decays of naturally occurring radioactive isotopes in the Earth, are a unique direct probe of our planet's interior. We report the first observa...
The research activities in collaboration with Enzo Flaminio are summarized and discussed.
Communicating with nuclear-powered submarines – which can remain underwater essentially indefinitely – is a major challenge because seawater is opaque to most of the electromagnetic spectrum. Neutrino...
Massive and massless neutrinos on unbalanced seesaws
neutrino mass type-I seesaw majorana neutrinos
2009/7/31
The observation of neutrino oscillations requires new physics beyond the standard model (SM). A SM-like gauge theory with p lepton families can be extended by introducing q heavy right-handed Majoran...
Equation of State of Protoneutron Star with Trapped Neutrinos
protoneutron star neutrino equation of state
2007/8/15
2006Vol.45No.5pp.901-905DOI:
Equation of State of Protoneutron Star with Trapped Neutrinos
ZHANG Hua and JIA Huan-Yu
Institute of Modern Physics, Southwest Jiaotong Univ...
Muon Anomalous Magnetic Moment in the Supersymmetric
Models with and Without Right-Handed Neutrinos
muon anomalous magnetic moment SUSY
right-handed neutrino
2007/8/15
2002Vol.37No.2pp.179-188DOI:
Muon Anomalous Magnetic Moment in the Supersymmetric
Models with and Without Right-Handed Neutrinos
FENG Tai-Fu,1 HUANG Tao,2 LI Xue-Qian,1 LIU Xia...
Interference Phase of Mass Neutrinos in Kerr Space-Time
interference phase Kerr space-time gravitational redshift
2007/8/15
2003Vol.40No.6pp.742-744DOI:
Interference Phase of Mass Neutrinos in Kerr Space-Time
HUANG Xiu-Ju and WANG Yong-Jiu
Institute of Physics, Hunan Normal University, Chan...
11-Apr-2007，New Haven, Conn. The initial data from the 10-year long "MiniBooNE" experiment at the Department of Energy’s Fermilab significantly clarifies the overall picture of how the neutrino fundam...