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KNUST1 - Indico
KNUST1 - Indico

... • Raises many unanswered questions: mass? flavour? unification? ...
Document
Document

JPD@Muon potential
JPD@Muon potential

... Not by beamshtrahlung as with e+/e- but by muon decay (e, n) Reduced background at high energy due to increased muon lifetime ...
Measurement of lifetime for muons captured inside nuclei
Measurement of lifetime for muons captured inside nuclei

Document
Document

Introduction to Supersymmetry
Introduction to Supersymmetry

Document
Document

... provide a successful basis for explaining the microphysics of the present universe, but additional symmetries are needed to address important questions about earlier times Origin of matter, unification, size of the Fermi constant, neutrino mass, gravity,… • High precision, low-energy studies provide ...
TK_LV_NExT
TK_LV_NExT

... 3. Test of Lorentz violation Lorentz violation is realized as a coupling of particle fields and background fields, so the basic strategy to find Lorentz violation is: (1) choose the coordinate system (2) write down the Lagrangian, including Lorentz-violating terms under the formalism (3) write down ...
10/29/2007 Julia Velkovska PHY 340a
10/29/2007 Julia Velkovska PHY 340a

Studies of effective theories beyond the Standard Model
Studies of effective theories beyond the Standard Model

SOME REMARKS ON THE BOSON MASS SPECTRUM IN A 3-3
SOME REMARKS ON THE BOSON MASS SPECTRUM IN A 3-3

... We obtained a mass spectrum depending on a single free parameter a to be tuned. One can observe that, although the fermion representations and even the order in the parameter matrix η2 are not the same with those chosen in Ref. [3], the resulting mass spectrum exhibits the same structure. That means ...
Flipped SU(5) - cosmology - Arizona State University
Flipped SU(5) - cosmology - Arizona State University

New Approach to Supernova Simulations - GSI
New Approach to Supernova Simulations - GSI

... Neutrino test particles represent “2nd fluid”, do NOT escape freely (neutrino trapping), and need to be followed in time. Neutrinos created in center and are “light” fluid on which “heavy” baryon fluid descends ...
Quark matter formation in dense stellar objects
Quark matter formation in dense stellar objects

...  which are essentially the equations similar to the rate equations above with the neutrino (antineutrino) energy included in the momentum integrations. In the rate equations above, e implies the difference of electron and positron densities. It is straight forward to verify that baryon number and ...
European Strategy for Particle Physics
European Strategy for Particle Physics

Experimental Observation Of Lepton Pairs Of Invariant Mass Around
Experimental Observation Of Lepton Pairs Of Invariant Mass Around

PARTICLE PHYSICS - STFC home | Science & Technology
PARTICLE PHYSICS - STFC home | Science & Technology

Here - Winter Nuclear and Particle Physics Conference
Here - Winter Nuclear and Particle Physics Conference

hep-ph - Royal Holloway, University of London
hep-ph - Royal Holloway, University of London

The Family Problem: Extension of Standard Model with a
The Family Problem: Extension of Standard Model with a

Stability - HAL
Stability - HAL

Zerwas_PASCOSMerida
Zerwas_PASCOSMerida

... • production of SUSY particles in pairs • (Cascade-) decays to the lightest SUSY particle • LSP stable, neutral and weakly interacting: neutralino (χ1) • experimental signature: missing ET ...
Working Group Talks Gobinda Majumdar Issues In The Construction
Working Group Talks Gobinda Majumdar Issues In The Construction

dirac and majorana fermions
dirac and majorana fermions

... however, is a second order equation and φ and ∂φ/∂t can be fixed arbitrarily at a given time. This leads to the existence of negative densities. These problems are related and have to do with the existence of particles and antiparticles, for which we need the interpretation of φ itself as an operato ...
arXiv:1501.03541v1 [hep
arXiv:1501.03541v1 [hep

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Neutrino oscillation

Neutrino oscillation is a quantum mechanical phenomenon whereby a neutrino created with a specific lepton flavor (electron, muon or tau) can later be measured to have a different flavor. The probability of measuring a particular flavor for a neutrino varies periodically as it propagates through space.First predicted by Bruno Pontecorvo in 1957, neutrino oscillation has since been observed by a multitude of experiments in several different contexts. Also, it turned out to be the resolution to the long-standing solar neutrino problem.Neutrino oscillation is of great theoretical and experimental interest, since observation of the phenomenon implies that the neutrino has a non-zero mass, which was not included as part of the original Standard Model of particle physics.
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