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Fermi and the Theory of Weak Interactions
Fermi and the Theory of Weak Interactions

Fermi and the Theory of Weak Interactions
Fermi and the Theory of Weak Interactions

The Structure of Matter The Standard Model of Elementary Particles
The Structure of Matter The Standard Model of Elementary Particles

... Gauge bosons: particles that mediate (or transmit) the force between a pair of particles The 4 fundamental forces have different ranges and a different boson is responsible for each force. The mass of the boson establishes the range of the force. The bosons carry the force between particles. The Hig ...
Study of Neutrino Interactions at the T2K Near Detector Complex
Study of Neutrino Interactions at the T2K Near Detector Complex

... • Reduce cross-section uncertainties in the oscillation analyses ND280 will also contribute to increasing understanding of neutrino cross-sections in their own right -> High statistics -> Unique beam and detector features: • Quasimonochromatic beam at a lower energy than most previous measurements • ...
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... shows “neutral weak currents”. ...
DUAL NATURE OF DARK MATTER: COMPOSITE OF BOTH
DUAL NATURE OF DARK MATTER: COMPOSITE OF BOTH

The Standard Model of Particle Physics
The Standard Model of Particle Physics

Plasma_02 - StealthSkater
Plasma_02 - StealthSkater

arXiv:1501.03089v1 [nucl
arXiv:1501.03089v1 [nucl

... ¯ channels [1, 2]. This view has been recurrent [3], but only after the advent of unitary chiral perturbation theory (UChPT) it KN has taken a more assertive tone [4–9]. In this framework, a kernel (potential) derived from the chiral Lagrangians is the input into the Bethe-Salpeter equation in coupl ...
Observation of New-Particle Production by High
Observation of New-Particle Production by High

Jan 27, 2000 Lessons learnt from the heavy tau lepton Fig. 1 Fig. 2
Jan 27, 2000 Lessons learnt from the heavy tau lepton Fig. 1 Fig. 2

... identical interactions: the charm and strange quarks with the muon and the muon neutrino; and the top and bottom quarks with the tau lepton and its neutrino. We do not understand what causes this triplicity, nor do we know what generates the different masses. However, we expect the heavier family to ...
The Family Problem: Extension of Standard Model with a
The Family Problem: Extension of Standard Model with a

... It’s a special way to put in quantum mechanics (those matrices representing spins) and relativity simultaneously. In fact, the “space-time” notion may be defined also.  Apparently the way is so special. Why there is nothing else - a world of point-like Dirac particles, with interactions mediated by ...
shp_09 - Nevis Laboratories
shp_09 - Nevis Laboratories

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Slides - Indico

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Particle Physics and the LHC

... • If there are very large/small parameters in a quantum theory, there must be a good reason why they are so small…. • In general, there will be large quantum corrections to such parameters in higher orders of perturbation theory, in terms of other parameters which are not so small. • These quantum c ...
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Law of Conservation of Muons

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Standard Model

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Dernières Nouvelles de l`Univers

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Ten Lectures on the ElectroWeak Interactions

Fundamental interactions
Fundamental interactions

... 1.1.1.2 Experiments with antiprotons: antiprotonic atoms and collision studies. Present and future experiments with antiprotonic atoms focus on a high-resolution laser spectroscopy of antiprotonic helium and hydrogen atoms. The applications in terms of fundamental questions range from the test of c ...
Family Gauge Theory
Family Gauge Theory

Teaching the Standard Model in IB Physics by Debra Blake
Teaching the Standard Model in IB Physics by Debra Blake

... 10. Why can mass be measured in MeV/c2 ? 11. Using the Chart complete the following: _______________ have charges that are integers, and _______________ have charges that are fractions. 12. Baryons are particles that are made from quarks. The most common baryons are the neutron and the proton. Apply ...
Automatic scanning of emulsion films for the OPERA - INFN
Automatic scanning of emulsion films for the OPERA - INFN

... neutrinos on Earth. The Soudan2, MACRO and SuperKamiokande experiments studying atmospheric neutrinos, produced in the decay of secondary particles created in the interactions of primary cosmic rays with the nuclei of the Earth atmosphere, found strong indications for muon neutrino oscillations. A d ...
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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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