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Learning material
Learning material

... inside of an atom. Recall that even up to the beginning of the 20th century atoms were regarded as indivisible. Thompson was led to a different conclusion by his discovery of the electron as a constituent of atoms. Thomson’s model distributed the positive and negative charge uniformly through the at ...
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Atoms, X-rays and Synchrotron Radiation
Atoms, X-rays and Synchrotron Radiation

... the others because extremely energetic electrons emitting X-rays radiate away their energy more quickly than the lower-energy electrons emitting optical and infrared light. The Crab Nebula is one of the most studied objects in the sky, truly making it a cosmic icon. ...
Unit 2 Atomic structure
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... weak force eventually causes it to break up into a proton and an electron. • The force of gravity inside the atom is much weaker even than the weak force.  Every process we know in the universe can be explained in terms of these fundamental forces. ...
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Masterton and Hurley Chapter 3
Masterton and Hurley Chapter 3

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Worksheets for Chapter 7

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... In this paper, the author evaluates the cosmic background radiation due to the Cherenkov effect from FTL virtual photons created in a ZPF background. The calculated result shows that the spectrum and the mass density of energy due to the Cherenkov radiation almost coincides the cosmic background rad ...
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sofia3_mac - University of Glasgow

... During a flare, stored magnetic energy is distributed through corona and efficiently converted to KE of fast particles. Flare ‘standard model’ does a pretty good job at providing a framework for the whole flare phenomenon. However, theory of energy transport by electron beams runs into some trouble ...
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Bremsstrahlung



Bremsstrahlung (German pronunciation: [ˈbʁɛmsˌʃtʁaːlʊŋ], from bremsen ""to brake"" and Strahlung ""radiation"", i.e. ""braking radiation"" or ""deceleration radiation"") is electromagnetic radiation produced by the deceleration of a charged particle when deflected by another charged particle, typically an electron by an atomic nucleus. The moving particle loses kinetic energy, which is converted into a photon, thus satisfying the law of conservation of energy. The term is also used to refer to the process of producing the radiation. Bremsstrahlung has a continuous spectrum, which becomes more intense and whose peak intensity shifts toward higher frequencies as the change of the energy of the accelerated particles increases.Strictly speaking, braking radiation is any radiation due to the acceleration of a charged particle, which includes synchrotron radiation, cyclotron radiation, and the emission of electrons and positrons during beta decay. However, the term is frequently used in the more narrow sense of radiation from electrons (from whatever source) slowing in matter.Bremsstrahlung emitted from plasma is sometimes referred to as free/free radiation. This refers to the fact that the radiation in this case is created by charged particles that are free both before and after the deflection (acceleration) that caused the emission.
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