
Mirror particles and mirror matter: 50 years of speculation and search
... symmetry in a more general sense, the existence of hypothetical right-handed protons, pR , was considered, though the term “mirror particles” was not used and pR and pL were assumed to interact “with the same electromagnetic field and perhaps the same pion field”. (Much later I learned that already ...
... symmetry in a more general sense, the existence of hypothetical right-handed protons, pR , was considered, though the term “mirror particles” was not used and pR and pL were assumed to interact “with the same electromagnetic field and perhaps the same pion field”. (Much later I learned that already ...
TK_LV_NExT
... Neutrino mode analysis: MiniBooNE saw the 3.0s excess at low energy region Antineutrino mode analysis: MiniBooNE saw the 1.4s excess at low and high energy region Since we find no evidence of Lorentz violation, we set limits on the combination SME coefficients. ...
... Neutrino mode analysis: MiniBooNE saw the 3.0s excess at low energy region Antineutrino mode analysis: MiniBooNE saw the 1.4s excess at low and high energy region Since we find no evidence of Lorentz violation, we set limits on the combination SME coefficients. ...
10/29/2007 Julia Velkovska PHY 340a
... Goal of the Lecture • (Re)introduce the fundamental particles of the Standard Model • Describe simple conservation laws • Make the connection between observables (decay rates) and coupling constants that we learn from the Standard model ...
... Goal of the Lecture • (Re)introduce the fundamental particles of the Standard Model • Describe simple conservation laws • Make the connection between observables (decay rates) and coupling constants that we learn from the Standard model ...
Study of Neutrino Interactions at the T2K Near Detector Complex
... CCQE: charged-current quasielastic • charged-current: W exchange, final-state muon • quasielastic: no mesons in the final state CC1π: charged-current, single pion • one pion in the final state ...
... CCQE: charged-current quasielastic • charged-current: W exchange, final-state muon • quasielastic: no mesons in the final state CC1π: charged-current, single pion • one pion in the final state ...
Method of wave equations exact solutions in studies of neutrinos
... evaluation of quantum theory of the spin light of neutrino (SLν) and spin light of electron (SLe) in matter, the two recently discussed new mechanisms of electromagnetic radiation produced by a neutrino and an electron moving in matter. A possibility to introduce an effective “matter induced Lorentz ...
... evaluation of quantum theory of the spin light of neutrino (SLν) and spin light of electron (SLe) in matter, the two recently discussed new mechanisms of electromagnetic radiation produced by a neutrino and an electron moving in matter. A possibility to introduce an effective “matter induced Lorentz ...
Neutrino

A neutrino (/nuːˈtriːnoʊ/ or /njuːˈtriːnoʊ/, in Italian [nɛuˈtrino]) is an electrically neutral elementary particle with half-integer spin. The neutrino (meaning ""little neutral one"" in Italian) is denoted by the Greek letter ν (nu). All evidence suggests that neutrinos have mass but that their masses are tiny, even compared to other subatomic particles. They are the only identified candidate for dark matter, specifically hot dark matter.Neutrinos are leptons, along with the charged electrons, muons, and taus, and come in three flavors: electron neutrinos (νe), muon neutrinos (νμ), and tau neutrinos (ντ). Each flavor is also associated with an antiparticle, called an ""antineutrino"", which also has no electric charge and half-integer spin. Neutrinos are produced in a way that conserves lepton number; i.e., for every electron neutrino produced, a positron (anti-electron) is produced, and for every electron antineutrino produced, an electron is produced as well.Neutrinos do not carry any electric charge, which means that they are not affected by the electromagnetic force that acts on charged particles, and are leptons, so they are not affected by the strong force that acts on particles inside atomic nuclei. Neutrinos are therefore affected only by the weak subatomic force and by gravity. The weak force is a very short-range interaction, and gravity is extremely weak on the subatomic scale. Thus, neutrinos typically pass through normal matter unimpeded and undetected.Neutrinos can be created in several ways, including in certain types of radioactive decay, in nuclear reactions such as those that take place in the Sun, in nuclear reactors, when cosmic rays hit atoms and in supernovas. The majority of neutrinos in the vicinity of the earth are from nuclear reactions in the Sun. In fact, about 65 billion (7010650000000000000♠6.5×1010) solar neutrinos per second pass through every square centimeter perpendicular to the direction of the Sun in the region of the Earth.Neutrinos are now understood to oscillate between different flavors in flight. That is, an electron neutrino produced in a beta decay reaction may arrive in a detector as a muon or tau neutrino. This oscillation requires that the different neutrino flavors have different masses, although these masses have been shown to be tiny. From cosmological measurements, we know that the sum of the three neutrino masses must be less than one millionth that of the electron.