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Profile Documents Logout
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Document
Document

... • All matter is made of indivisible particles called atoms. • All atoms of a given element are identical in mass & properties. • Atoms are not created or destroyed - just rearranged in reactions. • Different atoms can combine in simple ratios to make compounds. Atoms, according to Dalton: ...
Energy: A Physicist`s View - University of Colorado Boulder
Energy: A Physicist`s View - University of Colorado Boulder

Nuclear Chemistry
Nuclear Chemistry

Particle detectors measuring fluxes of cosmic rays on Earth´s surface.
Particle detectors measuring fluxes of cosmic rays on Earth´s surface.

Elementary Particles: A Brief History
Elementary Particles: A Brief History

... initially in cosmic ray interactions and then with accelerators with their energies steadily increasing over the years. They were also complemented by new and more sensitive detection methods. These particles both confirmed existing theories of particle physics, and inspired new ideas about the work ...
Atoms: The Building Blocks of Matter
Atoms: The Building Blocks of Matter

Common problem against B and L genesis and its possible resolution
Common problem against B and L genesis and its possible resolution

Structure of Nuclear Matter
Structure of Nuclear Matter

Zealey Phys-in-Cont
Zealey Phys-in-Cont

... The atomic number (Z) of an atom or nucleus is the number of protons contained within the nucleus. Since atoms are electrically neutral and contain the same number of positive and negative charges, this is also the number of electrons in the atom. The chemical symbol given to the atom depends on it ...
1-Introduction
1-Introduction

... Firstly, alpha particles are a type of ionizing radiation ejected by the nuclei of certain unstable atoms. They have two protons and two neutrons giving them a charge of 2+ (identical to the nucleus of the helium atom). It is a relatively heavy, high-energy particle with a velocity in air that is ro ...
Monday, March 2, 2015
Monday, March 2, 2015

... If a photon can create an electron, it must also create a positive charge to balance charge conservation. In 1932, C. D. Anderson observed a positively charged electron (e+) in cosmic radiation. This particle, called the positron, had been predicted to exist several years earlier by P. A. M. Dirac. ...
document
document

Parts of an atoms - Mr-Durands
Parts of an atoms - Mr-Durands

Subthreshold antiproton production in nucleus
Subthreshold antiproton production in nucleus

Summary of Important Ideas in Quantum Physics
Summary of Important Ideas in Quantum Physics

Syllabus of Instrumentation and Methods in Astroparticle Physics
Syllabus of Instrumentation and Methods in Astroparticle Physics

Homework Book
Homework Book

... A nucleus of large mass number splits into two nuclei, releasing several electrons. ...
Detecting particles in particle physics
Detecting particles in particle physics

Dominoes - Learning on the Loop
Dominoes - Learning on the Loop

Nuclear physics
Nuclear physics

Ionizing Radiation
Ionizing Radiation

ZimanyiSchool2008novlong
ZimanyiSchool2008novlong

Lesson 1 Assignment - Rocky View Schools
Lesson 1 Assignment - Rocky View Schools

... b. Use the charge-to-mass ratio of the particle to determine whether it is an alpha particle, electron, or proton. Hint: Check your physics data sheet for the charges and masses. ...
Chemistry Chapter 3
Chemistry Chapter 3

atom
atom

... properties; atoms of different elements differ in properties. • Atoms cannot be subdivided, created, or destroyed • Atoms of different elements can combine in simple, whole number ratios to form compounds • In chemical rxn, atoms are combined, separated, or rearranged ...
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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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