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The role of elementary particle accelerators
The role of elementary particle accelerators

The Scattering of α and β Particles by Matter and the
The Scattering of α and β Particles by Matter and the

... It is well known that the α and β particles suffer deflexions from their rectilinear paths by encounters with atoms of matter. This scattering is far more marked for the β than for the α particle on account of the much smaller momentum and energy of the former particle. There seems to be no doubt th ...
Dark Matter Candidates - SLAC
Dark Matter Candidates - SLAC

... none of the Standard Model neutrinos are suitable, but their right-handed counterparts might be acceptable. Active neutrinos in a 4th generation would be acceptable except for the fact that they would have been detected in sensitive underground experiments by now. ...
SUPERSYMETRY FOR ASTROPHYSICISTS
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... – SM particles have Rp = 1, SUSY particles have Rp = −1 – Requires 2 superpartners in each interaction • Consequence: the lightest SUSY particle (LSP) is stable and cosmologically significant. What is the LSP? 30 Jul – 1 Aug 07 ...
"A Cryogenic, High-field Trap for Large Positron Plasmas and Cold Beams" Non-Neutral Plasma Physics V , M. Schauer, T. Mitchell, R. Nebel Eds., AIP Conf. Proc. No. 692 (AIP, New York, 2003), pp. 149-161. J.R. Danielson, P. Schmidt, J.P. Sullivan, et al (PDF)
"A Cryogenic, High-field Trap for Large Positron Plasmas and Cold Beams" Non-Neutral Plasma Physics V , M. Schauer, T. Mitchell, R. Nebel Eds., AIP Conf. Proc. No. 692 (AIP, New York, 2003), pp. 149-161. J.R. Danielson, P. Schmidt, J.P. Sullivan, et al (PDF)

Fall/Winter 1994, Vol. 24, No. 3 - SLAC
Fall/Winter 1994, Vol. 24, No. 3 - SLAC

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PowerPoint file - CUE Web Summary for halldweb.jlab.org

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The theory of dipoles vortex Author: Prof. Vasile Tudor, The

... -normal condition, in which the particle is in our universe, and the corresponding antiparticle symmetry manifests itself in the complementary Universe; -the State reversed, in which Poles vortex have changed compared with the normal case. Unlike the normal condition, which is more or less stable, t ...
Precise Matter and Antimatter Tests of the Standard Model with e +,p
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The Schwarzschild Proton - Hawaii Institute for Unified Physics
The Schwarzschild Proton - Hawaii Institute for Unified Physics

arXiv:1412.5987v1 [hep-ex] 18 Dec 2014
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... We present the results of a comprehensive study of the luminosity function, energetics, prompt gamma-ray correlations, and classification methodology of short–hard and long–soft GRBs (SGRBs & LGRBs), based on observational data in the largest catalog of GRBs available to this date: BATSE catalog of ...
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"Positron scattering from atoms and molecules using a magnetized beam" Phys. Rev. A 66 (2002), 042708. J.P. Sullivan, S.J. Gilbert, J.P. Marler, R.G. Greaves, S.J. Buckman and C.M. Surko (PDF)

Beamline Instrumentation for Future Parity-Violation Experiments Robert Michaels
Beamline Instrumentation for Future Parity-Violation Experiments Robert Michaels

... experiments and dark matter experiments. Due to its high energy resolution and efficiency, HPGe detectors are also used to analyze the radioactive of material. IHEP had built a HPGe detector three years ago, used for the lowradioactive materials selected for Daya Bay experiment. But for the future J ...
Barish Communications 07-06
Barish Communications 07-06

Lecture 13 - PPD - STFC Particle Physics Department
Lecture 13 - PPD - STFC Particle Physics Department

Radiometric Dating - mercerislandschools.org
Radiometric Dating - mercerislandschools.org

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... • pions decay to polarised muons and are injected in storage ring • decay electrons emerge preferentially in direction of muon spin • detect those electrons with high enough energy to be in the direction of the muon motion detecting a signal of the muon spin in forward direction signal oscillates wi ...
Introduction to the Weak Interaction, Volume 1
Introduction to the Weak Interaction, Volume 1

Little Higgs dark matter and its collider signals
Little Higgs dark matter and its collider signals

... ~ Output ~ Distribution of MT2 ...
< 1 ... 5 6 7 8 9 10 11 12 13 ... 69 >

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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