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Elementary Particles in Physics
Elementary Particles in Physics

Multi-Majoron Modes for Neutrinoless Double
Multi-Majoron Modes for Neutrinoless Double

... of several indications of an excess of electrons just below the endpoint in some of the experimental data for several types of decays [9]. Although the evidence for the excess has since diminished [10], the conclusion reached by the theoretical re-evaluation still stands: viable theories which can p ...
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Lecture 1

Flavor Physics Theory - DESY
Flavor Physics Theory - DESY

... Discussion 2.2 Considering the case k = 2 (two di↵erent amplitudes), can you show that |Āf¯/Af | = 1 if either 1 = 2 or 1 = 2 ? This type of CP violation can also occur in neutral meson decays. The contributions can be difficult to disentangle. As it involves strong phases that a hard to calculate, ...
The Oscillating Neutrino
The Oscillating Neutrino

Beyond the Standard Model - Southampton High Energy Physics
Beyond the Standard Model - Southampton High Energy Physics

... Minimal Flavour Violation (MFV) • All squark mixing due to CKM matrix • Universal scalar masses at high scale for ...
Electroweak precision data and right-handed gauge bosons
Electroweak precision data and right-handed gauge bosons

... The most stringent available limits on MWR then, arise from the KL − KS mass diference. As a matter of fact, under the following assumptions: (a) the left-right symmetry is manifest or pseudomanifest (b) the hadronic matrix elements are computed in the vacuum saturation approximation. Beall, Bander ...
Parity and Charge conjugation
Parity and Charge conjugation

... you to read through). They found there was no experimental confirmation in the case of weak interactions and proposed a test, which was carried out later that year by C.S. Wu (Phys. Rev. 105, 1413 (1957). This has 3 pages and again and easy to follow, although this experiment was somewhat a tricky o ...
( ) New Faculty Jan Egedal-Pedersen
( ) New Faculty Jan Egedal-Pedersen

... ­Combining precision experimental data with the latest theory indicates that the collision energy at CERN’s Large Hadron Collider (LHC), where CMS operates, will be sufficient to expose predicted but not yet observed particles—some incorporated within the framework of the Standard Model and others w ...
Chapter 11: The Sun Week 8 Chapter 11: The Sun SOHO http
Chapter 11: The Sun Week 8 Chapter 11: The Sun SOHO http

... the standard model, but electron neutrinos only constituted about 1/3 of all these neutrinos. Mikheyev-Smirnov-Wolfstein (MSW) effect proposed: neutrinos change form. The standard model from particle physics only predicted electron neutrinos - the standard model was wrong. ...
The Non-Thermal Universe - Astroparticle physics in the Netherlands
The Non-Thermal Universe - Astroparticle physics in the Netherlands

Physics 535 lecture notes: - 9 Oct 2nd, 2007 Homework: Griffiths: 4.8
Physics 535 lecture notes: - 9 Oct 2nd, 2007 Homework: Griffiths: 4.8

The Nucleus - American School of Milan
The Nucleus - American School of Milan

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see presentation slides

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The Weak Interaction - University of Warwick
The Weak Interaction - University of Warwick

... and Yang, after studying this, pointed out in 1956 that maybe these two particles could be the same particle. Of course this would be possible only if the parity is not preserved in these decays. They examined carefully the available evidence for parity conservation, and concluded that there was a l ...
Flavour symmetry -- 50 years after SU(3)
Flavour symmetry -- 50 years after SU(3)

... Isospin is mathematically described by the SU(2) group (analogously to spin). The strength of the strong interaction between any pair of nucleons is the same, independent of whether they are interacting as protons or as neutrons. ...
HEPAP Subpanel - LIGO
HEPAP Subpanel - LIGO

Conception of Generations
Conception of Generations

... In 1937 two American groups and one Japanese group succeeded to observe cosmic ray particles of the predicted mass. They were Neddermeyer and Anderson,4) Street and Stevenson,5) and Nishina, Takeuti and Ichinomiya.6) The cosmic ray meson, now called the muon, had the right mass, but it was not clear ...
pbarp - CERN Indico
pbarp - CERN Indico

non-relativistic Breit
non-relativistic Breit

MuNew Sesaps (1) WM
MuNew Sesaps (1) WM

... Our experimental muon lifetime τ will be compared with the accepted value of 2.197 μs, our calculated (from our τ) gW = 8(3π3ĥ/2τmµc2)1/4(MW/mμ) with accepted gw = 0.653, our calculated e=gwsinϑ√ħcε0 with the textbook value of 1.6x10-19 C, and our calculated v = 2MWc2/gw√ℏc= (2τmμc2/3π3ℏ)1/4 (mµc2/4 ...
The Standard Model and its Simple Extensions
The Standard Model and its Simple Extensions

Nuclear Stability and Radioactivity
Nuclear Stability and Radioactivity

The standard model of particle physics
The standard model of particle physics

< 1 2 3 4 5 6 7 ... 10 >

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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