• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
institut de física corpuscular - Instituto de Física Corpuscular
institut de física corpuscular - Instituto de Física Corpuscular

Rare $ B $ Decays as Tests of the Standard Model
Rare $ B $ Decays as Tests of the Standard Model

Mirror particles and mirror matter: 50 years of speculation and search
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 ...
or ppt
or ppt

Analysis of the 4-year IceCube high
Analysis of the 4-year IceCube high

TK_LV_NExT
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. ...
Simulation study of optical degradation monitoring in the SNO+
Simulation study of optical degradation monitoring in the SNO+

the capture of magnetic inelastic dark matter in the sun.
the capture of magnetic inelastic dark matter in the sun.

JPD@Muon potential
JPD@Muon potential

7 Neutrino emission from choked gamma-ray bursts
7 Neutrino emission from choked gamma-ray bursts

Measurement of lifetime for muons captured inside nuclei
Measurement of lifetime for muons captured inside nuclei

... Charge Quarks, particles Gluons ...
10/29/2007 Julia Velkovska PHY 340a
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 ...
hep-ph - Royal Holloway, University of London
hep-ph - Royal Holloway, University of London

Study of Neutrino Interactions at the T2K Near Detector Complex
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 ...
Interactions/Weak Force/Leptons
Interactions/Weak Force/Leptons

Science AMANDA and IceCube
Science AMANDA and IceCube

Working Group Talks Gobinda Majumdar Issues In The Construction
Working Group Talks Gobinda Majumdar Issues In The Construction

The Oscillating Neutrino
The Oscillating Neutrino

Lecture 1
Lecture 1

The Standard Model and its Simple Extensions
The Standard Model and its Simple Extensions

Ten Lectures on the ElectroWeak Interactions
Ten Lectures on the ElectroWeak Interactions

Lowering the IceCube Detection Threshold by Wavelength
Lowering the IceCube Detection Threshold by Wavelength

Method of wave equations exact solutions in studies of neutrinos
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 ...
Operational Status and Power Upgrade Prospects of the
Operational Status and Power Upgrade Prospects of the

HEPAP Subpanel
HEPAP Subpanel

1 2 3 4 5 ... 8 >

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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report