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2 The interaction of energetic particles with material
2 The interaction of energetic particles with material

... The static particle in the material must be ‘bounded’ in order to transfer moment. Bremstrahlung can NOT occur in vacuum, although conservation of energy would allow this. [In the following: 1- note that the momentum ǁPǁ of a photon with energy E equals E/c. The speed of light c often occurs as term ...
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... Independent of the issue of whether nuclei can exist with Zα > ∼ 1, atoms with such nuclei could not be regarded as stable, in that they could interact with their accompanying positron(s) and change their state (at least temporarily). However, since there are no longlived nuclei with Z > ∼ 100, this ...
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Chapter31-32 - LSU Physics

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Atomic Structure Notes

... The mass of an atom is mostly from the __protons___ and ____neutrons________. Find O on the periodic table. It’s mass is _16.00___ amu. It has _8_ protons. It must have _8_ neutrons. Electrically neutral atoms (as opposed to ions) have one electron for every proton. Fill in this chart for these neut ...
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Homework_Problems_129

... Reading: Chapter 7 of Griffiths (plus you may need to review earlier material) 28. Find rotational invariants corresponding to the following processes: a. Natural optical activity: rotation of the direction of the polarization of linearly polarized light propagating in an isotropic medium. b. Farada ...
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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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