Classical Mechanics
Classical Mechanics
5th Edition
ISBN: 9781891389221
Author: John R. Taylor
Publisher: University Science Books
Question
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Chapter 16, Problem 16.16P

(a)

To determine

Prove that 2f=1r2r2(rf).

(a)

Expert Solution
Check Mark

Answer to Problem 16.16P

Proved that 2f=1r2r2(rf).

Explanation of Solution

As f(r) is spherically symmetric, so r should satisfy r=x2+y2+z2, where x,y,z are the three Cartesian coordinates.

Write the expression for 2f.

    2f=2fx2+2fy2+2fz2        (I)

Take double derivative of f(r).

    2x2[f(r)]=x(xf(r))=x[f(r)rx]        (II)

Use x2+y2+z2 for r in the equation (II).

    2x2[f(r)]=x[f(r)xx2+y2+z2]=x[f(r)(12)x2+y2+z2(2x)]=[f(r)1x2+y2+z2xx]+[f(r)x(x2+y2+z2)12x]+[xf(r)(x2+y2+z2)12x]=[f(r)1x2+y2+z2]+[f(r)(12)x(x2+y2+z2)322xx]+[xf(r)(x2+y2+z2)12x]        (III)

Solve equation (III).

    2x2[f(r)]=f(r)rf(r)x2(x2+y2+z2)32+[f(r)(12)(x2+y2+z2)122x(x2+y2+z2)12x]=f(r)rf(r)x2r3+f(r)x2r2        (IV)

Similarly, second derivative of function with respect to y can be written as,

    2y2[f(r)]=f(r)rf(r)y2r3+f(r)y2r2        (V)

Similarly, second derivative of function with respect to z can be written as,

    2z2[f(r)]=f(r)rf(r)z2r3+f(r)z2r2        (VI)

Use equation (IV), (V), and (VI) in (I).

    2f=f(r)rf(r)x2r3+f(r)x2r2+f(r)rf(r)y2r3+f(r)y2r2+f(r)rf(r)z2r3+f(r)z2r2=3f(r)rf(r)[x2+y2+z2]r3+f(r)[x2+y2+z2]r2=3f(r)rf(r)r2r3+f(r)r2r2=2f(r)r+f(r)         (VII)

Solve 1r2r2(rf)

    1r2r2(rf)=1rr[x(rf)]=1rr[rf(r)+1f(r)]=1r[rf(r)+1f(r)+f(r)]=1r[rf(r)+2f(r)]=2f(r)r+f(r)        (VIII)

Equate equation (VII) and (VIII).

    2f=1r2r2(rf)        (IX)

Conclusion:

Therefore, 2f=1r2r2(rf).

(b)

To determine

Prove that 2f=1r2r2(rf) using the formula inside the back cover for 2 in spherical polar co-ordinates.

(b)

Expert Solution
Check Mark

Answer to Problem 16.16P

Proved that 2f=1r2r2(rf) using the formula inside the back cover for 2 in spherical polar co-ordinates..

Explanation of Solution

Write the expression for 2f in spherical polar co-ordinates.

    2f=1r2r2(rf)+1r2sinθθ(sinθfθ)+1r2sin2θ2fϕ2        (X)

f is a function of r only, so the second term and third term will vanishes. Hence the equation (XI) becomes,

    2f=1r2r2(rf)+1r2sinθθ(sinθ×0)+1r2sin2θ×0=1r2r2(rf)        (XI)

Conclusion:

Therefore, it is proved that 2f=1r2r2(rf) using the formula inside the back cover for 2 in spherical polar co-ordinates.

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