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Volumn 77, Issue 9, 2009, Pages 807-817

Quadrupolar contact fields: Theory and applications

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EID: 69149101944     PISSN: 00029505     EISSN: None     Source Type: Journal    
DOI: 10.1119/1.3138700     Document Type: Article
Times cited : (8)

References (77)
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    • Cartesian tensor forms for the multipole expansion for the electric field are given without derivation in Ref. 2, p. 146, up to the quadrupole term and are derived in Refs. 3 and 4, p. 51, to all orders. Spherical tensor forms are derived to all orders in Ref. 2, p. 145, and in Ref. 4, p. 53. Cartesian tensor forms for the multipole expansion for the magnetic field are derived in Ref. 2, p. 184, up to the dipole term and in Ref. 5 to all orders. The spherical tensor form is derived to all orders in Ref. 6
    • Cartesian tensor forms for the multipole expansion for the electric field are given without derivation in Ref. 2, p. 146, up to the quadrupole term and are derived in Refs. 3 and 4, p. 51, to all orders. Spherical tensor forms are derived to all orders in Ref. 2, p. 145, and in Ref. 4, p. 53. Cartesian tensor forms for the multipole expansion for the magnetic field are derived in Ref. 2, p. 184, up to the dipole term and in Ref. 5 to all orders. The spherical tensor form is derived to all orders in Ref. 6.
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    • For the definition of the magnetic scalar potential see Ref. 6. Various definitions of the Cartesian magnetic quadrupole moment are discussed in C. G. Gray, Definition of the magnetic quadrupole moment, Am. J. Phys. 48, 984-985 (1980).
    • For the definition of the magnetic scalar potential see Ref. 6. Various definitions of the Cartesian magnetic quadrupole moment are discussed in C. G. Gray, "Definition of the magnetic quadrupole moment," Am. J. Phys. 48, 984-985 (1980).
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    • G. Gray "Simplified derivation of the magnetostatic multipole expansion using the scalar potential," Am. J. Phys. 46, 582-583 (1978) (In the first of these papers the multipole expansion is derived using the vector potential A defined by B= ∇ × A. Recall that ∇ · B=O. In the second paper the multipole expansion is obtained using the magnetic scalar potential Φ defined by B=-V ∇ Φ. Recall that ∇ × B=(4π/c)J=0 outside the source region, where J is the source current density.)
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    • In the notation in Sec. IV C the octopole-dipole interaction gives rise to terms of types Vl1l2l3, with 11l2l, 314 the regular long-range r-5 term, 312, 112, and 110, the last three being contact terms with 312 the largest of the three for the cases studied. The 314 term affects all but s- and p-states, 312 and 112 affect only p-states, and 110 affects only s- and p-states
    • -5 term), 312, 112, and 110, the last three being contact terms with 312 the largest of the three for the cases studied. The 314 term affects all but s- and p-states, 312 and 112 affect only p-states, and 110 affects only s- and p-states.
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    • Reference 2, p. 149.
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    • Reference 2, p. 162.
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    • G. Karl and V. A. Novikov, Quadrupolar contact terms and hyperfine structure, Phys. Rev. C 74, 024001-1-7 (2006);
    • G. Karl and V. A. Novikov, "Quadrupolar contact terms and hyperfine structure," Phys. Rev. C 74, 024001-1-7 (2006);
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    • See also G. Karl and V. Novikov, Hyperfine structure in Ω-nucleus system, Fiz. B 14, 75-78 (2005) and M. I. Krivoruchenko and A. Faessler, Decays, contact p-wave interactions and hyperfine structure in omega exotic atoms, Nucl. Phys. A 803, 173-209 (2008).
    • See also G. Karl and V. Novikov, "Hyperfine structure in Ω-nucleus system," Fiz. B 14, 75-78 (2005) and M. I. Krivoruchenko and A. Faessler, "Decays, contact p-wave interactions and hyperfine structure in omega exotic atoms," Nucl. Phys. A 803, 173-209 (2008).
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    • Reference 2, p. 148. In a private communication Dr. Jackson notes that his method gives an alternative simple derivation of our results, Eqs, 30) and 31
    • Reference 2, p. 148. In a private communication Dr. Jackson notes that his method gives an alternative simple derivation of our results, Eqs. (30) and (31).
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    • For two third-rank tensors T and U the full contraction is T, U, T αβγUγβα. If a partial contraction occurs, for example, for T: U, the αβ component is (T:U)αβ=TαμνU νμβ, and for A·T with vector A and second-rank tensor T the a component is (A·T)α=A μTμα. The general rule is contract nearest neighbors first, then next nearest neighbors, etc, When the tensors are symmetric, as in this paper, we can be cavalier about the order of the indices, Further discussion of this Milne Chapman notation for Cartesian tensors is given in Appendix B in Ref. 4. Note also that with flat-space Cartesian components, there is no need to distinguish covariant (indices down) and contravariant (indices up) components
    • μα. The general rule is contract nearest neighbors first, then next nearest neighbors, etc. (When the tensors are symmetric, as in this paper, we can be cavalier about the order of the indices.) Further discussion of this Milne Chapman notation for Cartesian tensors is given in Appendix B in Ref. 4. Note also that with flat-space Cartesian components, there is no need to distinguish covariant (indices down) and contravariant (indices up) components.
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    • More rigorous arguments can be given. See, for example
    • More rigorous arguments can be given. See, for example, C. P. Frahm, "Some novel delta-function identities," Am. J. Phys. 51, 826-829 (1983).
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    • Nonsymmetric second-rank tensors contain also an antisymmetric l = 1 (vector) part. For a discussion, with examples, see Ref. 4, pp. 490 and 544.
    • Nonsymmetric second-rank tensors contain also an antisymmetric l = 1 (vector) part. For a discussion, with examples, see Ref. 4, pp. 490 and 544.
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    • Reference 4, p. 489
    • Reference 4, p. 489.
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    • (2) is used (see, for example, Ref. 2, pp. 146 and 151).
    • (2) is used (see, for example, Ref. 2, pp. 146 and 151).
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    • Reference 4, p. 452
    • Reference 4, p. 452.
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    • For Ar and other atoms, we calculate 〈Ψ0́|(1/3) Σiqiri2|Ψ 0〉, where qi=-e is the charge of electron i with radial coordinate ri and Ψ0 is the ground electronic state wave function. For N2 and other molecules the electronic contribution is calculated with the same formula as for atoms and the nuclear contribution from the molecular geometry using (1/3)Σiq iri2, where qi is the charge of nucleus i with radial coordinate ri
    • i.
  • 50
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    • The mean diamagnetic susceptibility of an atom or molecule is Χd, e2/6mec2 〈Ψ0|Σiri2|Ψ 0〉, Ref. 35, where Ψ0 is the ground electronic state wave function and Σi is a sum over the electrons. Thus the electronic contribution to ⊖ can be obtained from χd, and the nuclear contribution can be calculated from the equilibrium bond lengths and angles
    • d, and the nuclear contribution can be calculated from the equilibrium bond lengths and angles.
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    • Similar theorems are proved for the magnetic field B in Ref. 2, p. 187. Alternative proofs for the electric and magnetic cases are given in Ref. 9.
    • Similar theorems are proved for the magnetic field B in Ref. 2, p. 187. Alternative proofs for the electric and magnetic cases are given in Ref. 9.
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    • Earnshaw's theorem states that stable equilibrium points in source-free regions of electrostatic fields do not exist, that is, a minimum of φ(r) is not possible if it satisfies ∇2φ=0. This nonexistence of a minimum is clear from Eq, 31) because if we choose r0 at an assumed minimum, we get a contradiction. The same argument shows that maxima also cannot exist. Thus, if an equilibrium point r exists satisfying E(r, ∇φ(r, 0, it must be a saddle point of φ(r) or belong to a region of constant φ
    • 0 at an assumed minimum, we get a contradiction. The same argument shows that maxima also cannot exist. Thus, if an equilibrium point r exists satisfying E(r)=-∇φ(r)= 0, it must be a saddle point of φ(r) or belong to a region of constant φ.
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    • 41Maxwell's relation for the Laplacian is (Ref. 42) φav- φ0 ≃(R2 /10, ∇2 φ) 0, where R is the radius of a small sphere surrounding point r 0, φav is the spherical average of φ, φ0 is the value of φ at r0, and (∇2φ)0 is the Laplacian of φ at r 0. The Laplacian of φ is thus a measure of how much φ deviates from its local average value. The result follows from Eqs, 34) and (35, this time without assuming that the sphere contains zero charge, by choosing R small so that we can neglect O(R3) and higher order terms in the expansion Eq, 34) and using 〈r2〉, 3/5)R 2 and 1:1=3. In terms of the surface average over a small sphere surrounding point r0 we have (Ref. 53) φsurf av- φ0 ≃ R2/6,
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    • Note that our quadrupole moment Q is half that defined in Ref. 21, and our Coulomb law is q/r [see Eq. (1)] and that in Ref. 21 is q/πr.
    • Note that our quadrupole moment Q is half that defined in Ref. 21, and our Coulomb law is q/r [see Eq. (1)] and that in Ref. 21 is q/πr.
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    • E. Durand, Électrostatique (Masson, Paris, 1964), Tome I, p. 93. For the field line equation of a general axial multipole, see p. 97.
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