paramagnetism(redirected from Asperomagnetism)
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force of attraction or repulsion between various substances, especially those made of iron and certain other metals; ultimately it is due to the motion of electric charges.
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A property exhibited by substances which, when placed in a magnetic field, are magnetized parallel to the field to an extent proportional to the field (except at very low temperatures or in extremely large magnetic fields). Paramagnetic materials always have permeabilities greater than 1, but the values are in general not nearly so great as those of ferromagnetic materials. Paramagnetism is of two types, electronic and nuclear.
The following types of substances are paramagnetic:
1. All atoms and molecules which have an odd number of electrons. According to quantum mechanics, such a system cannot have a total spin equal to zero; therefore, each atom or molecule has a net magnetic moment which arises from the electron spin angular momentum. Examples are organic free radicals and gaseous nitric oxide.
2. All free atoms and ions with unfilled inner electron shells and many of these ions when in solids or in solution. Examples are transition, rare-earth, and actinide elements and many of their salts. This includes ferromagnetic and antiferromagnetic materials above their transition temperatures. For a discussion of these materials See Antiferromagnetism, Ferrimagnetism, Ferromagnetism
3. Several miscellaneous compounds including molecular oxygen and organic biradicals.
4. Metals. In this case, the paramagnetism arises from the magnetic moments associated with the spins of the conduction electrons and is called Pauli paramagnetism.
Relatively few substances are paramagnetic. Aside from the Pauli paramagnetism found in metals, the most important paramagnetic effects are found in the compounds of the transition and rare-earth elements which have partially filled 3d and 4f electron shells respectively.
Electronic paramagnetism arises in a substance if its atoms or molecules possess a net electronic magnetic moment. The magnetization arises because of the tendency of a magnetic field to orient the electronic magnetic moments parallel to itself.
Nuclear paramagnetism arises when there is a net magnetic moment due to the magnetic moments of the nuclei in a substance. Nuclear magnetic moments are about 103 times smaller than electron magnetic moments. As a result, nuclear paramagnetism produces effects 106 times smaller than electron paramagnetic or diamagnetic effects. See Diamagnetism, Magnetic resonance, Nuclear moments
the property of substances, placed in an external magnetic field, to be magnetized—that is, acquire a magnetic moment—in the direction of the field. Thus, the action of the magnetization J that arises within the paramagnetic substance is added to that of the external field. In this regard, paramagnetism is the opposite of diamagnetism, where the magnetic moment that arises in a substance under the action of a field is oriented against the direction of the external magnetic field strength H. Paramagnetic substances are therefore attracted to the poles of magnets (hence the term “paramagnetism”) and diamagnetic substances are repelled. Ferromagnetic and antifer-romagnetic substances also have paramagnets’ property of being magnetized along a field. When, however, there is no external field, the magnetization of paramagnetic substances is equal to zero and the substances lack a magnetic structure—mutual ordered orientation of the magnetic moments of their atoms. Ferromagnetic and antiferromagnetic substances, on the other hand, retain their magnetic structure when H = 0. The term “paramagnetism” was introduced in 1845 by M. Faraday, who divided all substances except ferromagnets into diamagnetic and paramagnetic substances.
Paramagnetism is characteristic of substances whose particles —atoms, molecules, ions, or atomic nuclei—have intrinsic magnetic moments that, in the absence of an external field, are oriented randomly, with the result that J = 0. When an external field is applied, the magnetic moments of paramagnets’ atoms are oriented mainly with the field. In weak fields, the magnetization of paramagnetic substances increases with field strength according to the law J = χH, where χ is the magnetic susceptibility of a mole of the substance; for paramagnets, χ is always positive and usually is of the order of magnitude 10–5–10–3. If the field is very strong, the magnetic moments of the paramagnetic particles are all oriented strictly with the field; that is, magnetic saturation is reached. For a constant field strength, an increase in the temperature T means an increase in the disorienting effect of the particles’ thermal motion and a decrease in magnetic susceptibility. In the simplest case, the susceptibility obeys Curie’s law χ = C/T, where C is the Curie constant, which depends on the nature of the substance. Deviations from Curie’s law are connected primarily with the interaction of particles (the effect of a crystal field) and are provided for by the Curie-Weiss law.
Paramagnetism is characteristic of many pure elements in the metallic state: alkali metals; alkaline-earth metals; some metals of the transition groups with an unfilled d or f shell—the groups of iron, palladium, platinum, the rare-earth elements, and the actinides. Alloys of these metals are also paramagnetic. In addition, paramagnetism is exhibited by salts of the iron group, salts of the group of rare-earth elements from Ce to Yb, salts of the actinides, and aqueous solutions thereof. Other substances characterized by paramagnetism include alkali-metal vapors; molecules of gases, such as O2 and NO; some organic molecules (biradicals); and a number of complex compounds. Ferromagnetic and antiferromagnetic substances become paramagnets at temperatures exceeding the Curie point or the Néel point, respectively, that is, the temperatures of the phase transition to the paramagnetic state.
The existence in atoms or ions of magnetic moments responsible for the paramagnetism of substances can be due to several factors: the orbital motion of the electrons about the nuclei (orbital paramagnetism), the spin angular momentum of the electrons (spin paramagnetism), and the magnetic moments of the atomic nuclei (nuclear paramagnetism). The magnetic moments of atoms, ions, and molecules are primarily a result of the spin and orbital moments of the electron shells. They are approximately 1,000 times greater than the magnetic moments of the nuclei. The paramagnetism of a metal consists primarily of the paramagnetism associated with the conduction electrons (Pauli paramagnetism) and the paramagnetism of the electron shells of the atoms (ions) of the metal’s crystal lattice. Since changes in temperature have practically no effect on the motion of conduction electrons in metals, the paramagnetism connected with conduction electrons is independent of temperature. It follows that the magnetic susceptibility of, for example, the alkali and alkaline earth metals is independent of temperature, since the electron shells of these metals’ ions lack a magnetic moment, and the metals’ paramagnetism is due exclusively to conduction electrons. For substances lacking the conduction electrons in which only the nucleus has a magnetic moment, such as the helium isotope He3, the paramagnetism is extremely small (x ~ 10–9–10–12) and can be observed only at extremely low temperatures (T < 0.1 °K).
According to the classical theory of P. Langevin (1906), the paramagnetic susceptibility of dielectrics is given by the formula χ = Nμa2/3kT, where N is the number of magnetic atoms in a mole of the substance, μa the magnetic moment of the atom, and k the Boltzmann constant. This formula was derived by the methods of statistical physics for a system of essentially nonin-teracting atoms located in a weak magnetic field or at high temperature—that is, when μaH << kT. The formula provides a theoretical explanation of the Curie law. In strong magnetic fields or at low temperatures, that is, when μaH << kT, the magnetization of paramagnetic dielectrics tends toward Nμa2, or toward saturation. The quantum theory of paramagnetism, which takes into account the space quantization of the moment μa (L. Brillouin, 1926), gives a similar expression for the susceptibility χ of dielectrics when μaH << kT: x = NJ (J + 1)μa2gj2/3kT, where j is the quantum number that determines the total angular momentum of the atom and gj is the Landé splitting factor. The paramagnetic susceptibility of semiconductors Xes owing to conduction electrons has, in the simplest case, an exponential dependence on the temperature T: Xes + AT½ exp(—ΔE/2kT), where A is a constant of the substance and ΔE is the width of the forbidden band of the semiconductor. The peculiarities of the individual structure of semiconductors strongly distort this dependence. In the simplest case, for metals —if we ignore Landau diamagnetism and the interaction of electrons—we have XeM = 3Nμe2/2E0, where E0 is the Fermi energy and μe is the magnetic moment of an electron; here ΞeM is independent of the temperature. In the absence of a strong interaction between nuclear spins and the electron shells of atoms, nuclear paramagnetism is characterized by the quantity Ξn = Nμn2/3KT; the electronic paramagnetic susceptibility is approximately 106 times larger than this quantity, since μe ~ 103μn.
Research on the paramagnetism of different substances and on electron paramagnetic resonance (the resonance absorption by paramagnets of the energy of an electromagnetic field) has made it possible to determine the magnetic moments of individual atoms, ions, molecules, and nuclei, to study the structure of complex molecules and molecular complexes, and to perform fine structural analysis of materials used in technology. Paramagnetic substances are made use of in physics to obtain temperatures below 1°K.
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Dorfman, la. G. Magnitnye svoistva istroenie veshchestva. Moscow, 1955.
Abragam, A. Iadernyi magnetizm. Moscow, 1963. (Translated from English.)
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Fizika magnitnykh dielektrikov. Leningrad, 1974.
IA. G. DORFMAN