Multipole moments. Dipole moment. The second moment µ is more commonly called the dipole moment, of the charge. distribution and is a vector

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Dipole moment Multipole moments The second moment µ is more commonly called the dipole moment, of the charge distribution and is a vector µ = µ x ˆx + µ y ŷ + µ z ẑ where the α component is given by µ α = qr i i α i= where α can be x, y, or z and r i is the coordinate of the i th particle relative to some origin. The dimensions of the dipole moment are charge-length and the most common unit for the dipole moment in Chemistry is the Debye, (D), and D =0-8 esu-cm. This is a cgs unit and is still used even though the official system of units in now the SI system. An easy way to convert between the systems is to note that in the cgs system the dipole moment of a proton and an electron separated by Angstrom is 4.809 0-8 esu cm or 4.809D. In the SI system the same dipole moment is (.6077 0-9 C)(0-0 M) or.608 0-9 CM so D is equal to (.608/4.809) 0-9 CM or.586 0-0 CM/D. In theoretical work the dipole moment is often reported in atomic units and by the same reasoning 4.809D is equal to (electron charge)(/0.5977 )a0 or.88976 au so D is equivalent to 0.946 au. Conversely atomic unit of dipole moment is equal to.5459d. Calculate the dipole moment in D and au for the charge distributions given below. The distances are given in Angstroms and e is the proton charge. charge x y z e 0 e 0 - -e 0 0 0

charge x y z e 0 e 0 - -e 0 0 0 How is the dipole moment affected if we shift the origin of the coordinate system to the point? The particles have not moved but are now at the terminus of the vector r i so relative to the new origin µ becomes α or µ α ( ) = q i (r iα α ) = q i r iα α i= i= i= q i µ α ( ) = µ α (0) α Q Where Q is the total charge of the distribution and if the charge distribution is neutral, Q is zero and the dipole moment is invariant to a change of origin. ote that when we move to the new origin we simply translate the coordinate system. We keep the x, y, z axis in the two systems parallel. Suppose we don t move the origin but rotate the coordinate axis keeping them orthogonal. Lets call the original coordinate axis xyzand,, the rotated system x, y, z. The vector µ is the two systems is µ = µ x ˆx + µ y ŷ + µ z ẑ = µ x ˆx + µ y ŷ + µ z ẑ Taking the dot product of both sides with primed system are all orthogonal we obtain µ x = µ x ˆx i ˆx + µ y ŷ i ˆx + µ z ẑ i ˆx ˆx, recognizing that the unit vectors in the The dot products are equal to the cosines of the angle between the various axis which we call a, a & a and so xx yx zx µ = µ a + µ a + µ a x y z x xx yx zx

With a similar expression for µ & µ. These relationships are often written in matrix form as µ x axx ayx a zx µ x µ = a a a µ y xy yy zy y µ z axz ayz a zz µ z y z Using the Einstein summation convention we can write the relationship between the components of the dipole moment in the rotated and un-rotated systems as µ = µ a α β βα and although the individual components of the dipole moment change when the coordinate axis are rotated, its magnitude doesnt so we must have or µ µ = µ µ α α α α µ µ = µ a µ a = µ µ a a = µ µ which requires a α α α αα β βα α β αα βα α α a = δ αα βα αβ where δαβ is the Kronecker delta which is if α = β and zero otherwise. Consider the charge distribution charge x y z e 0 e 0 - -e 0 0 0 rotate the coordinate axis about x by 0 degrees. Compare the components and magnitude of the dipole moment in the two coordinate frames.

a. Calculate the interaction energy (in J and ev) between a proton at the origin and the charge distribution given below (distances are in Angstroms and e is the proton charge). charge x y z e 5 -e 6 b. Calculate the interaction energy with the proton due to the dipole moment of the distribution. Express your answer in J and ev. c. Comment on the difference between the results of parts a and b. Quadrupole and Higher Moments There are two common definitions for the quadrupole moment of a charge distribution. The first and least common in Chemistry equates the quadrupole moment tensor with the second moment tensor A αβ defined above. The second definition and the one we will use almost exclusively defines it as ote that but δ Θ = = αβ αβ qi( ξi αξiβ δαβξi ) Aαβ ξi i= i= Θ F = A F + δ F ξ 6 αβ αβ αβ αβ αβ αβ i= δαβ Fαβ Fαα α Fα α βφ φ i = = = = = 0 by Laplaces equation. So the energy of the second moment in a field gradient can be written in terms of the quadrupole moment tensor as A F = Θ F αβ αβ αβ αβ Θαβ is often called the Buckingham definition of the quadrupole moment. There are 9 elements for the quadrupole moment tensor but not all are unique. Permuting the indices doesn t change its value so Θ =Θ αβ βα

Additionally the tensor is traceless, so Θ =Θ +Θ +Θ = 0 αα xx yy zz So knowing any two of the diagonal elements will determine the third. In the most general case where none of the element are related by the symmetry of the charge distribution, we will have unique non-diagonal elements, Θxy, Θxz & Θ yz and any two diagonal elements for a total of 5. Symmetry often reduces this number significantly. If we have a linear charge distribution along the z axis, all non-diagonal elements are zero, and Θ xx =Θ yy = Θ and only one element is unique. zz Express the quadrupole moment tensor of the following charge distributions in terms of the charges Q and bond lengths. C array along the z axis V Atom charge x y z q 0 0 - -q 0 0 0 q 0 0 Planar D in the xy plane h Atom charge x y z q cos0 sin0 0 q - cos0 sin0 0 q 0-0 4 -q 0 0 0

Tetrahedral array atom charge x y z q q q 4 q 5-4q 0 0 0 Calculate numerical values for the quadrupole tensors of the above charge distributions assuming that q= 0.eand = Angstrom. eport your results in the SI and atomic unit systems. In a similar fashion we can replace the third moment W αβγ with an octupole moment tensor defined as Ω = + + αβχ qi(5 ξi αξiβξiγ ξi ( ξi αδβγ ξiβδαγ ξi γδαβ )) i= because one can show, with the use of Laplaces equation, W F = Ω F! 5 αβγ αβγ αβγ αβγ There are 7 elements ( ) of this tensor but again not all are unique. As with the quadrupole moment, permuting any two indices doesnt change the value of the element. For example, Ω xxy =Ω xyx =Ω yxx additionally the tensor is traceless, for example Ω αα y =Ω xxy +Ω yyy +Ω zzy = 0

So knowing any two of the elements Ωααβ determines the third. In the most general case where none of the elements are related by the symmetry of the charge distribution, one could have a maximum of 7 unique elements. The working expression for the potential energy of a charge distribution in an electrostatic potential is then V ext = Qφ( ) µ α F α Θ αβ F αβ i5 Ω αβγ F αβγ i5i 7 Φ αβγδ F αβγδ where for completeness we include the hexadecapole moment tensor, The general formula for a multipole moment of order L is where L M αβ γ = ( )L Q L! ξ = ξ + ξ + ξ i ix iy iz i= ξ i L+ L ξ iα ξ iβ ξ iγ ξ i Φ αβγδ & 0 M = Q, M α =, µ α M αβ =Θ, αβ M αβγ =Ω, etc. αβγ