Tensors for Physics

(Marcin) #1

130 8 Integration of Fields


HereJis theJacobi determinant, also calledfunctional determinant, which can be
computed according to


J=εμνλ

∂rμ
∂p 1

∂rν
∂p 2

∂rλ
∂p 3

. (8.47)

Notice thatJdp 1 dp 2 dp 3 can also be written as


Jdp 1 dp 2 dp 3 =dsμ

∂rμ
∂p 1

dp 1 , (8.48)

where dsμis the surface element of a surface parameterized byp 2 ,p 3 , withp 1 =
const., cf. Sect.8.2.3.
Two examples for general coordinates are discussed next.


(i) Cylinder Coordinates


Consider a circular cylinder whose axis coincides with thez-axis. The presentation
r={ρcosφ, ρsinφ,z}is used, whereρ,φ,zare the parameters, see also (8.16).
Now the volume integral is


V =


V

f(r(ρ, φ,z)) ρdρdφdz. (8.49)

When the region in space to be integrated over is a cylinder with radiusRand length
L, and furthermore the integrand is independent of the angleφ, the relation (8.49)
reduces to


V = 2 π

∫R

0

ρdρ

∫L

0

dzf(r(ρ,z)). (8.50)

The factor 2πstems from the integration overφ.Forf=1, one obtains the volume
V=πR^2 Lof the circular cylinder.


(ii) Spherical Coordinates


The standard parametrization with the spherical coordinatesr,θ,φcorresponds to
r={rcosφsinθ,rsinφsinθ,rcosθ}. The volume integral is given by


V =


V

f(r(r,θ,φ))r^2 drsinθdθdφ=


V

f(r(r,θ,φ))r^2 drd^2 ̂r. (8.51)

Here, as in (8.31), the symbol d^2 ̂r=sinθdθdφstands for the scalar surface element
of the unit sphere. Sometimes it is advantageous to useζ =cosθas integration
variable instead ofθ. Then one has


d^2 ̂r=−dζdφ. (8.52)
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