Jackson 1 2 Homework Solution

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    Jackson 1.2 Homework Problem Solution

    Dr. Christopher S. BairdUniversity of Massachusetts Lowell

    PROBLEM:

    The Dirac delta function in three dimensions can be taken as the improper limit as ! of the"aussian function

    D; x , y , z=#$/#$e%p[ # x#y#z#]

    Consider a 'eneral ortho'onal coordinate system specified by the surfaces u( constant) v( constant)w( constant) with len'th elements du/U) dv/V) dw/Win the three perpendicular directions. Show that

    xx *=uu * vv * ww*UVW

    by considerin' the limit of the "aussian above. +ote that as ! only the infinitesimal len'th

    element need be used for the distance between the points in the e%ponent.

    SOL!"O#:

    Start with the 'eneral property of a Dirac delta,

    x y zdx dy dz=&

    Substitute in our representation,

    lim!

    D ; x , y , zdx dy dz=&

    +ow transform the volume element into the new coordinate system

    lim!

    D ; x , y , zdu

    U

    dv

    V

    dw

    W=&

    -e do not know e%actly how the one system of coordinates transforms into the other) so we cannottransformDin a direct manner. Let us instead define an intermediate variable function Faccordin' to,

    Fu , v ,w =lim!

    D; x , y , zu ,v ,w &

    U V W

    -ith this definition our inte'ral becomes

    Fu ,v ,w du dv dw=&

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    Because we are inte'ratin' over all space) we are free to make a chan'e of variables which ust shifts

    the ori'in.

    Fuu *, vv *,ww *dudv dw=&

    Comparin' this to the very first e/uation we see that it is identical e%cept with different inte'rationlabels and therefore,

    Fuu *, vv *, ww*=uu *vv * ww *

    so that) after plu''in' back in) we have

    uu * vv * ww *=lim!

    D; x , y , zu ,v , w&

    U V W

    Solve forD,

    lim !

    D ; x , y , z u ,v ,w =uu * vv *ww *U V W

    The entity on the left) no matter what coordinate system it is represented in) is ust what we mean by

    the 'eneral three0dimensional Dirac delta,

    xx *=uu * vv * ww *UVW

    +ow note that we never used the e%plicit form ofD) so we have solved the problem in a way that the

    book did not intend. Let us try solvin' the problem usin' a method that uses the e%plicit form ofD.

    D; x , y , z=#$/#$e%p[&

    ##x#y#z#]

    Make a chan'e of variablesxx1x*) etc. 23therwise we will not end up with the most 'eneral case.4

    D; xx *, yy *, zz*=#$/ #$ e%p[ # xx *#yy *#zz*#]

    5s !)Dwill become 6ero unlessx1x* approaches 6ero as well. 7n calculus) we remember that

    x1x* approachin' 6ero becomes dx. Therefore we have,

    D; xx *, yy *, zz*=#$/ #$ e%p[ # dx

    #dy#dz

    #]-e reco'ni6e the last part in parentheses as the incremental arc len'th element dss/uared,

    D; xx *, yy *, zz*=#$/ #$ e%p[ #ds#]

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    8%pand the arc len'th in the new coordinate system,

    D=#$ / #

    $

    e%p[ # du#

    U#

    dv#

    V#

    dw#

    W# ]

    +ote that dxdu /Uand we are not makin' that claim here. 9ather) the entire three0dimensionalincremental arc len'th dsis the same in all ortho'onal coordinate systems. +ow e%pand the increments

    back into differences,

    D=#$ / #$e%p[ # uu *#

    U#

    vv *#

    V#

    ww *#

    W# ]

    D= e

    uu *#/#

    #U

    #

    #

    evv *

    #/#

    #V

    #

    #

    eww *

    #/#

    #W

    #

    #

    +ow make the substitution &:Uin the first bracket) #:Vin the second bracket) and $:W in the last bracket. -e can do this as lon' as we let &) #) and $'o to 6ero ust like we were

    lettin' 'o to 6ero.

    D=[ euu *

    #/#&

    #

    #& ][evv *

    #/##

    #

    ## ][eww *

    #/#$

    #

    #$ ]U V W-e now let the alpha*s approach 6ero. 8ach term in brackets on the ri'ht side becomes a one0

    dimensional linear Dirac delta. The left side becomes the 'eneral e%pression for the three0dimensionalDirac delta,

    xx *=uu * vv * ww *UVW

    +ow this is a very useful result. Suppose we have a point char'e. 7n spherical coordinates) we can find

    the representation of its Dirac delta usin' the above e%pression. ;or spherical coordinates

    u=r , v=, w= and the len'th elements are dr ,r d, rsin d so thatU=&) V= &r, W=&

    rsin and

    xx *=rr* * *&

    r#sin

    2Spherical Coordinates4

    +ote that it is fairly strai'ht0forward to prove usin' Dirac delta properties that

    */ sin=coscos * so that the three0dimensional Dirac delta in spherical coordinates isoften written

    xx *=rr* cos cos * *&

    r#

    as it is on p. ! inJackson.

    Similarly in cylindrical coordinates)u=r , v=, w=zand the len'th elements aredr ,r d, dzso that

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    U=&) V=&

    r, W=& and

    xx *=rr* *zz*&

    r2Cylindrical Coordinates4

    5ssume that instead of a point char'e) we have a line char'e shaped into a rin') centered on theza%is)located at some radius r* and polar an'le *. The char'e is distributed alon' the rin' accordin' to theline char'e density . The total char'e density in this case would be,

    =uu * vv *U V w 2Spherical Coordinates4

    = rr* *

    r2Spherical Coordinates4