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Average squared magnetization

E. Average Squared Magnetization of an Open Chain of Ising Spins... [Pg.267]

The average squared magnetization (ASM) of an open, one-dimensional (ID) chain of N spins (each interacting exclusively with its nearest neighbors) is given by the formula [18]... [Pg.292]

III. C of two different properties of the ID Ising model, namely, its average squared magnetization and its partition function. [Pg.307]

The unpaired electron has the complication that it is not localized on a single point but, in general, is delocalized on the entire molecule. So, in every point of space where the molecular orbital (MO) containing the unpaired electron has a non-zero value, the average electron magnetic moment sensed by the nucleus is different from zero and is proportional to (Sz) times the fraction of unpaired electron present at that point. Such a fraction is called spin density p, which for a single electron is given by the square of its wavefunction at that point. [Pg.30]

To understand an electron—atom collision means to be able to calculate correctly the T-matrix elements for excitations from a completely-specified entrance channel to a completely-specified exit channel. Quantities that can be observed experimentally depend on bilinear combinations of T-matrix elements. For example the differential cross section (6.55) is given by the absolute squares of T-matrix elements summed and averaged over magnetic quantum numbers that are not observed in the final and initial states respectively. This chapter is concerned with differential and total cross sections and with quantities related to selected magnetic substates of the atom. [Pg.199]

J is the two site transfer integral (J 1 eV), and g(E ) is the density of states at the mobility edge (assumed to be constant over an energy interval kT). The factor 17 is, in units of a", the average square of the projected three site areas on a plane perpendicular to the magnetic field... [Pg.259]

Figure 1. The magnetic interlayer coupling in Fe/Cu/Fe bcc (001) trilayers. The squares denote the coupling energies for the pure trilayer and the circles the coupling energies for the dilute trilayers with 50% of intermixing in a single monolayer at each Fe/Cu interface. One example of an averaged interlayer coupling is indicated by the diamonds. Figure 1. The magnetic interlayer coupling in Fe/Cu/Fe bcc (001) trilayers. The squares denote the coupling energies for the pure trilayer and the circles the coupling energies for the dilute trilayers with 50% of intermixing in a single monolayer at each Fe/Cu interface. One example of an averaged interlayer coupling is indicated by the diamonds.
Figure 2 Orbital magnetic moments in bcc-Fe Coi-a . The triangles pointing up-and downwards represent the theoretical moments of Fe and Co, respectively, while the concentration weighted sum is given by circles. Full and open symbols stand for results obtained with and without the OP-term included (SOPR- and SPR-KKR-CPA, resp.). Experimental data [15] for the average magnetic moment (bottom) stemming from magneto mechanical and spectroscopic g-factors are given by full squares and diamonds. Figure 2 Orbital magnetic moments in bcc-Fe Coi-a . The triangles pointing up-and downwards represent the theoretical moments of Fe and Co, respectively, while the concentration weighted sum is given by circles. Full and open symbols stand for results obtained with and without the OP-term included (SOPR- and SPR-KKR-CPA, resp.). Experimental data [15] for the average magnetic moment (bottom) stemming from magneto mechanical and spectroscopic g-factors are given by full squares and diamonds.
The rate of radiocarbon formation in the upper atmosphere depends on a number of factors, which include the intensity of the incoming cosmic radiation, the activity of the sun, and the magnetic field of the earth (the latter affects the way cosmic rays travel). It can be safely stated, however, that radiocarbon is formed at a steady rate that averages just about 2.4 atoms of radiocarbon per second for every square centimeter of the earth s atmosphere outer surface. [Pg.300]


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See also in sourсe #XX -- [ Pg.292 , Pg.293 , Pg.294 ]




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