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Accelerate This! - University of Houston
Accelerate This! - University of Houston

Teaching the Standard Model in IB Physics by Debra Blake
Teaching the Standard Model in IB Physics by Debra Blake

+ e - Indico
+ e - Indico

The Structure of Matter The Standard Model of Elementary Particles
The Structure of Matter The Standard Model of Elementary Particles

... If a particle has zero electric charge, the antiparticle can still be distinguished because of other quantum numbers Example: neutrino vs. antineutrino – have opposite lepton number Some particles are their own antiparticle and must be electrically neutral Example: photon vs. graviton Antimatter – m ...
Contact Charging in Granular Materials
Contact Charging in Granular Materials

N/Z = 2, 8, 20, 28, 50, 82, 126
N/Z = 2, 8, 20, 28, 50, 82, 126

The Large Hadron Collider, or LHC, is the most powerful particle
The Large Hadron Collider, or LHC, is the most powerful particle

... Some think that the LHC will destroy all life on Earth, others have a more optimistic outlook, thinking that it could reveal more about the Big Bang Theory, String Theory and the Standard Model. The Big Bang Theory basically states that the universe began as a singularity (a zone of infinite density ...
Dark matter density profiles in dwarf satellites
Dark matter density profiles in dwarf satellites

Elementary Particles Fundamental forces in Nature
Elementary Particles Fundamental forces in Nature

Radioactivity Mid-Unit Review Questions
Radioactivity Mid-Unit Review Questions

The Standard Model - University of Rochester
The Standard Model - University of Rochester

Experimental Tests of the Standard Model
Experimental Tests of the Standard Model

Exit Slip: Atomic Structure and Nuclear Chemistry-1
Exit Slip: Atomic Structure and Nuclear Chemistry-1

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HSB_Mclass_Notes_v1

Exercises Introduction 1.1 F.H What is the de Broglie
Exercises Introduction 1.1 F.H What is the de Broglie

Getting to Know Y . T ROBERT L
Getting to Know Y . T ROBERT L

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Contents

Notes – Atomic Structure
Notes – Atomic Structure

... controls if an atom is carbon or gold. Change the protons equals change the atom. The number of protons is the atomic number on the periodic table. The mass of one atom is decided by the protons and the neutrons as they both have mass where as electrons are essentially mass less. The mass of the ato ...
The nucleus
The nucleus

... As in electron emission, we have Q = K ν + K e+ and the kinetic energy of the positron is a continuous distribution with maximum value ( K e+ ) ...
1 - barnes report
1 - barnes report

gg higgs - University of Southampton
gg higgs - University of Southampton

New state of matter created at CERN
New state of matter created at CERN

... 5–10 compared to expectations without assuming QGP. A variety of indications thus point towards the formation of quarkgluon plasma in the lead–lead collisions. In summary, physicists at CERN have recreated matter in a state never seen before, at energy densities twenty times higher than that inside ...
PDF Document - Washington State University
PDF Document - Washington State University

4. Atomic Structure
4. Atomic Structure

Nuclear Forces and Mesons
Nuclear Forces and Mesons

< 1 ... 41 42 43 44 45 46 47 48 49 ... 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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