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Beyong the Higgs
Beyong the Higgs

Types of Radioactive Decay
Types of Radioactive Decay

One Force of Nature
One Force of Nature

Particle accelerators and detectors
Particle accelerators and detectors

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Particle accelerators

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... as particles traveling backwards in time, equivalent to antiparticles traveling forward in time  both lead to the prediction of antiparticles ! ...
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Beam Line - SLAC - Stanford University

CHAPTER 14: Elementary Particles
CHAPTER 14: Elementary Particles

... The number of leptons from each family is the same both before and after a reaction. We let Le = +1 for the electron and the electron neutrino; Le = −1 for their antiparticles; and Le = 0 for all other particles. We assign the quantum numbers Lμ for the muon and its neutrino and Lτ for the tau and i ...
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Nuclear Radiation

... Kinetic energy is an expression of the fact that a moving object can do work on anything it hits; it quantifies the amount of work the object could do as a result of its motion. The total mechanical energy of an object is the sum of its kinetic energy and potential energy. For an object of finite si ...
Dark Matter - Otterbein University
Dark Matter - Otterbein University

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Note 2e - Decay Processes

... It turns out that the linear momentum & angular momentum are also violated, and a third particle is needed in order for both momenta to be balanced before & after the  decay ...
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Answers

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Charged particles in a magnetic field

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A Possible Design of the NLC e Source

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Higgs - SMU Physics

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30 The Nucleus - mrphysicsportal.net

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Conservation Laws I - Department of Physics, HKU

Particle Accelerator
Particle Accelerator

... A small-scale example of this class is the cathode ray tube [CRT] in an ordinary old TV set. Other examples are the Cockcroft–Walton generator and the Van de Graaf generator. ...
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Antimatter

In particle physics, antimatter is material composed of antiparticles, which have the same mass as particles of ordinary matter but opposite charges, as well as other particle properties such as lepton and baryon numbers and quantum spin. Collisions between particles and antiparticles lead to the annihilation of both, giving rise to variable proportions of intense photons (gamma rays), neutrinos, and less massive particle–antiparticle pairs. The total consequence of annihilation is a release of energy available for work, proportional to the total matter and antimatter mass, in accord with the mass–energy equivalence equation, E = mc2.Antiparticles bind with each other to form antimatter, just as ordinary particles bind to form normal matter. For example, a positron (the antiparticle of the electron) and an antiproton (the antiparticle of the proton) can form an antihydrogen atom. Physical principles indicate that complex antimatter atomic nuclei are possible, as well as anti-atoms corresponding to the known chemical elements. Studies of cosmic rays have identified both positrons and antiprotons, presumably produced by collisions between particles of ordinary matter. Satellite-based searches of cosmic rays for antideuteron and antihelium particles have yielded nothing. There is considerable speculation as to why the observable universe is composed almost entirely of ordinary matter, as opposed to a more even mixture of matter and antimatter. This asymmetry of matter and antimatter in the visible universe is one of the great unsolved problems in physics. The process by which this inequality between particles and antiparticles developed is called baryogenesis.Antimatter in the form of anti-atoms is one of the most difficult materials to produce. Antimatter in the form of individual anti-particles, however, is commonly produced by particle accelerators and in some types of radioactive decay. The nuclei of antihelium (both helium-3 and helium-4) have been artificially produced with difficulty. These are the most complex anti-nuclei so far observed.
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