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Classification of the Elementary Particles
Classification of the Elementary Particles

... • (2) the leptons or light particles. These are the electrons, muons and neutrinos and their antiparticles, all with masses less than the pions and with spin 1/2. For reasons connected with statistical mechanics they are also called fermions. Leptons interact weakly with other particles. • (3) the m ...
Byond Particle Physics
Byond Particle Physics

History of Atomic Structure
History of Atomic Structure

... What: Their work developed into what is now modern chemistry. • Why: Trying to change ordinary materials into gold. ...
Where it all began
Where it all began

... Rutherford and Mardsen study α-particle scattering by light elements in hope to get deeper inside the nucleus (smaller Z): 1. They use a cloud chamber (Wilson) filled with Hydrogen: while α-particles have pretty much fixed range, Rutherford and Mardsen occasionally observe tracks up to 4 times longe ...
History of the Atom
History of the Atom

TIMELINE OF NUCLEAR PHYSICS
TIMELINE OF NUCLEAR PHYSICS

Week 1: Nuclear timeline (pdf, 233 KB)
Week 1: Nuclear timeline (pdf, 233 KB)

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the nature of atoms and electrons: the millikan, thomson, and
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PPT Lecture - Hss-1.us

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Unit 3 - Section 5.1 2014 States of Matter

Lecture 24: The fundamental building blocks of matter 1
Lecture 24: The fundamental building blocks of matter 1

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LC Atomic Structure [PDF Document]

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1 eV - Nikhef

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Models of the Atom:

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Fulltext PDF - Indian Academy of Sciences

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Developing an Atomic Model

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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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