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Electron Neutrino Sources from the Core of the Earth
Electron Neutrino Sources from the Core of the Earth

APS study - braidwood
APS study - braidwood

Slides
Slides

Detecting sterile neutrinos with KATRIN
Detecting sterile neutrinos with KATRIN

Physics 127 Descriptive Astronomy Homework #15
Physics 127 Descriptive Astronomy Homework #15

The Big Bang
The Big Bang

Student Seminar Subatomic Physics, blok 1+2 2002/03
Student Seminar Subatomic Physics, blok 1+2 2002/03

... Chapter 1: New results in neutrino physics Recently, new results from the Sudbury neutrino observatory and the Super Kamiokande collaboration proved that neutrino’s must have mass, in contrast to the standard concept of weak interactions. The reason that we know they have mass is due to the fact tha ...
ppt - Infn
ppt - Infn

... Summary and/or Conclusions Study of 0nbb decay entered a new era. No longer is the aim just to push the sensitivity higher and the background lower, but to explore specific regions of the values. In agreement with the `phased’ program the plan is to explore the `degenerate’ region (0.1-1 eV) ...
The list of publications
The list of publications

... Reviewer: N.A. Lyutorovich ...
``Semi-leptonic weak interaction processes in nuclei and their role to
``Semi-leptonic weak interaction processes in nuclei and their role to

... Similar results hold for the COBRA detector The resulting fluxes are of the same order with those expected at the SNS at Oak Ridge (ORLaND experiment) ...
n,n - Osaka University
n,n - Osaka University

... 207Bi + n (Q=-9.77 MeV) 206Bi + 2n (Q=-17.86 MeV) With lead perchlorate (a clear liquid that dissolves easily in water) one can detect the e-, providing a direct measurement the energy of the ne’s from E(e-) and the number of neutrons emitted. In most cases (except the no-neutron NC case), detect ne ...
File - AMS02 BOLOGNA
File - AMS02 BOLOGNA

The Birth, Life, and Death of Stars
The Birth, Life, and Death of Stars

... They are very light. A neutrino weighs at least a million times less than an electron, but the precise mass is still unknown. In nature, they are produced in great quantities in the sun and in smaller quantities in the Earth. In the laboratory, scientists can make neutrino beams with particle accele ...
Understanding the Universe from Deep Underground
Understanding the Universe from Deep Underground

Neutrinos and Weak Interactions, Lecture 2
Neutrinos and Weak Interactions, Lecture 2

The Standard Model of Particle Physics Piet Mulders
The Standard Model of Particle Physics Piet Mulders

... just as photons (T = 2.7 K background) for all three kinds of neutrinos (ne, nm en nt) about 400 per cm3 ...
Nuclear Nomenclature
Nuclear Nomenclature

OscSNS: Precision Neutrino Measurements at
OscSNS: Precision Neutrino Measurements at

Icarus – wire production - Faculty of Physics University of Warsaw
Icarus – wire production - Faculty of Physics University of Warsaw

efectos de la presión hidrostática sobre la energía de enlace para
efectos de la presión hidrostática sobre la energía de enlace para

Rehearsal questions
Rehearsal questions

Common problem against B and L genesis and its possible resolution
Common problem against B and L genesis and its possible resolution

Inverse b Processes and Nonconservation
Inverse b Processes and Nonconservation

... antiparticle is not strictly forbidden, although the particle at issue is an entity distinct from the corresponding antiparticle. It was noted that neutrino may be such a particle mixture and consequently that there is a possibility of real transitions neutrino  antineutrino in vacuum, provided tha ...
Física Teórica de Partículas
Física Teórica de Partículas

On Morphing Neutrinos and Why They Must Have Mass
On Morphing Neutrinos and Why They Must Have Mass

< 1 2 3 4 5 6 7 >

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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