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Particle accelerators
Particle accelerators

... To reach higher and higher energies linear accelerators had to be built longer and longer. Then in 1900 Lawrence had the idea of bending the stream of electrons in a magnetic field – sort of wrapping up the accelerating electron beam. Synchrotron The enormous machine (LHC) at CERN near Geneva, due t ...
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Cosmic Rays - High Energy Physics at Wayne State

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... Building Blocks of Matter Atom- A basic unit of matter consisting of a dense central nucleus surrounded by a cloud of negatively charged electrons. • Element- A pure chemical substance composed of one type of atom. • Periodic Table of the Elements- An arrangement of elements in columns based on a s ...
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Particle accelerators
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... • Charged particles can be accelerated by an electric field. • Colliders produce head-on collisions which are much more energetic than hitting a fixed target. The center of mass energy is 2E in a collider but only m2E for a fixed target (E = energy, m = mass of the particles, E»m, c=1). • The LHC ...
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... Matter behavior at the atomic nucleus scale is a fascinating subject of study. Quarks and gluons interactions are the source of their confinement in hadrons, but also of the existence of extreme states, such as those within astrophysical objects. These states can be created through ion beams produce ...
Schrödinger`s Wave Mechanical Model
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... This work showed that any form of matter possesses a wavelength which is a wave property, so he proved that matter could behave like waves. However, the wave properties of matter only become significant as the form of matter becomes smaller. This work resulted in what is known as the Wave-Particle ...
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... As in the 1st quantization case, ĵ 0  x  is not non-negative so that it cannot represent the probability density of finding a particle at x. Now, we define an anti-particle as a “particle” whose attribute quantum numbers are all equal but of opposite signs to those of its particle partner. Some e ...
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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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