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Charge density, charged particles

The atomic scattering factor for electrons is somewhat more complicated. It is again a Fourier transfonn of a density of scattering matter, but, because the electron is a charged particle, it interacts with the nucleus as well as with the electron cloud. Thus p(r) in equation (B1.8.2h) is replaced by (p(r), the electrostatic potential of an electron situated at radius r from the nucleus. Under a range of conditions the electron scattering factor, y (0, can be represented in temis... [Pg.1363]

Electrostatic Interaction. Similarly charged particles repel one another. The charges on a particle surface may be due to hydrolysis of surface groups or adsorption of ions from solution. The surface charge density can be converted to an effective surface potential, /, when the potential is <30 mV, using the foUowing equation, where -Np represents the Faraday constant and Ai the gas law constant. [Pg.544]

If we were to forget that the flow of current is due to a random motion which was already present before the field was applied—if we were to disregard the random motion entirely and assume that each and every electron, in the uniform field X, moves with the same steady velocity, the distance traveled by each electron in unit time would be the distance v used in the construction of Fig. 16 this is the value which would lead to a current density j under these assumptions, since all electrons initially within a distance v of the plane AB on one side would cross AB in unit time, and no others would cross. Further, in a field of unit intensity, the uniform velocity ascribed to every electron would be the u of (34) this quantity is known as the mobility of the charged particle. (If the mobility is given in centimeters per second, the value will depend on whether electrostatic units or volts per centimeter are used for expressing the field strength.)... [Pg.44]

However, billiard balls are a pretty bad model for electrons. First of all, as discussed above, electrons are fermions and therefore have an antisymmetric wave function. Second, they are charged particles and interact through the Coulomb repulsion they try to stay away from each other as much as possible. Both of these properties heavily influence the pair density and we will now enter an in-depth discussion of these effects. Let us begin with an exposition of the consequences of the antisymmetry of the wave function. This is most easily done if we introduce the concept of the reduced density matrix for two electrons, which we call y2. This is a simple generalization of p2(x1 x2) given above according to... [Pg.38]

The dependence of T on energy for charged-particle decay can be found as follows. The decay rate is the probability density flux integrated over surface area at infinity, i.e. [Pg.36]

Fig. 4.10. Portion of the red spectrum of the H II galaxy Tololo 0633-415 with a redshift of 0.016, showing diagnostic features for helium (Ha and X 6678), electron density ([S n]) and ionization ([S hi]). The features marked cosmic ray are due to impacts of charged particles on the CCD detector. After Pagel et al. (1992). Fig. 4.10. Portion of the red spectrum of the H II galaxy Tololo 0633-415 with a redshift of 0.016, showing diagnostic features for helium (Ha and X 6678), electron density ([S n]) and ionization ([S hi]). The features marked cosmic ray are due to impacts of charged particles on the CCD detector. After Pagel et al. (1992).
Despite the fact that Bohr s stopping power theory is useful for heavy charged particles such as fission fragments, Rutherford s collision cross section on which it is based is not accurate unless both the incident particle velocity and that of the ejected electron are much greater than that of the atomic electrons. The quantum mechanical theory of Bethe, with energy and momentum transfers as kinematic variables, is based on the first Born approximation and certain other approximations [1,2]. This theory also requires high incident velocity. At relatively moderate velocities certain modifications, shell corrections, can be made to extend the validity of the approximation. Other corrections for relativistic effects and polarization screening (density effects) are easily made. Nevertheless, the Bethe-Born approximation... [Pg.76]

The central problem in the theory of geminate ion recombination is to describe the relative motion and reaction with each other of two oppositely charged particles initially separated by a distance ro- If we assume that the particles perform an ideal diffusive motion, the time evolution of the probability density, w(r,t), that the two species are separated by r at time t, may be described by the Smoluchowski equation [1,2]... [Pg.261]


See other pages where Charge density, charged particles is mentioned: [Pg.8]    [Pg.9]    [Pg.400]    [Pg.411]    [Pg.34]    [Pg.154]    [Pg.1613]    [Pg.1802]    [Pg.95]    [Pg.277]    [Pg.162]    [Pg.163]    [Pg.277]    [Pg.860]    [Pg.452]    [Pg.189]    [Pg.42]    [Pg.59]    [Pg.74]    [Pg.39]    [Pg.18]    [Pg.37]    [Pg.100]    [Pg.11]    [Pg.240]    [Pg.339]    [Pg.59]    [Pg.3]    [Pg.330]    [Pg.176]    [Pg.341]    [Pg.83]    [Pg.164]    [Pg.34]    [Pg.38]    [Pg.38]    [Pg.542]    [Pg.560]    [Pg.567]    [Pg.568]    [Pg.814]    [Pg.816]    [Pg.104]   
See also in sourсe #XX -- [ Pg.173 , Pg.174 , Pg.175 , Pg.176 ]




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Charged particles

Charged particles charge-current density

Charged-particle density

Charged-particle density

Current density, charged particles

Particle based density/charge distribution

Particle charge

Particle charge density

Particle charging

Particle density

Particle surface charge density

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