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Neutrino Oscillation - Stony Brook NN Group
Neutrino Oscillation - Stony Brook NN Group

... The first detection of solar neutrinos by Ray Davis’s chlorine experiment, and the subsequent confirmation by Kamiokande using real-time directional information and the first detection of supernova neutrinos opened up a new exciting field of neutrino astronomy. For these great achievements Ray Davis ...
Cosmic calibration - TWiki
Cosmic calibration - TWiki

Neutrinos and SN1987A
Neutrinos and SN1987A

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Handout. Neutrino Relics from the Big Bang
Handout. Neutrino Relics from the Big Bang

... historical and aesthetic grounds, this is taken as evidence that there is a better model waiting to be discovered. o Why are there so many particles? We now know that all the elements of the periodic table (hydrogen, carbon, oxygen, etc.) are composed of the same fundamental particles—protons, neutr ...
Poster 4 layout 7F PDF
Poster 4 layout 7F PDF

Quantum Mechanics and Neutrino Oscillations
Quantum Mechanics and Neutrino Oscillations

Chapters 9, 11, 12 Summary
Chapters 9, 11, 12 Summary

Neutrinos
Neutrinos

neutrino weight watchers awarded physics nobel prize
neutrino weight watchers awarded physics nobel prize

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Tutorial material for weak interactions and more

The Black Hole Beta Decay:
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Neutrino mass and New Physics: Facts and Fancy

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Report: Revising the `Solar neutrino problem`

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Detecting particles in particle physics

... different types of particles and neutrino interactions using a program The human brain is one of the best pattern matching machines ever evolved. However, even we will get some of these wrong. Imagine how much harder it is to ask a computer to do this automatically. ...
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Folie 1 - E15

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Inquiring minds want to know

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... has some chance of being a left-handed particle and thus to be reabsorbed by another neutron - and the neutrinoless double beta decay can occur! The probability depends on the mass of the neutrino - the heavier it is, the more likely the process will arise. If an experiment discovers the decay, it w ...
Lorentz violating field theories and nonperturbative physics
Lorentz violating field theories and nonperturbative physics

... The coefficients need not be diagonal in flavor space either. Like neutrino masses, they may mix different species. In fact, three-parameter Lorentz-violating models can explain all observed neutrino oscillations (including LSND). However, many possible parameters have not been probed. The “full” n ...
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research project #1 - Soudan Underground Laboratory

... MN. The near detector and particle accelerator (beginning of beam) are in Fermilab, while the far detector is in Soudan. ...
ASEPS_Poster_Ishihara1_A0
ASEPS_Poster_Ishihara1_A0

... Abstract: Neutrinoless double beta decay (0) takes place only when neutrinos are Majorana neutrinos that have the nature of no distinction between particles and their own anti-particles. Majorana neutrino plays important role in the theory called Seesaw Mechanism, in which a left-handed Majorana ...
Open: Postdoc Position at the Massachusetts Institute of Technology
Open: Postdoc Position at the Massachusetts Institute of Technology

Physics Projects Brochure (Word Document)
Physics Projects Brochure (Word Document)

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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.
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