Find the interaction energy (0E1.E2dτ0E1-E2dτinEq.2.47)

for two point

charges q1and q2a distance aapart.

Short Answer

Expert verified

The interaction energy isW=q1q24πε0a.

Step by step solution

01

Determine the expression for electric fields.

Write the expression for the interaction energy.

W=ε0E1-E2dτ

Here, E1is the electric field due to chargeq1.E2is the electric field due to chargelocalid="1654680864961" q2.dτ

is the volume element, and ε0is the permittivity of free space.

Write the expression for the electric field due to charge.

E1=Kq1r2(r^)

Here, Kis the Coulomb’s constant, ris the distance from the charge, and

r^is the unit vector that represents the direction of an electric field due to charge.

Write the expression for the electric field due to chargelocalid="1654685113455" q2.

localid="1654685109004" E2=Kq2R2(R^)

Here,Ris the distance from the charge, andlocalid="1654685092952" R^is the unit vector that represents the direction of an electric field due to chargelocalid="1654685088381" q2.

Consider the diagram for the configuration is shown in figure below.

Here,θis the angle made by the electricE1field with the zaxis andβis the angle between the two electric field vectors at point P.

02

Determine value of R

The value of R in the figure above, according to the law of cosines, is,

R=r2+a2-2arcosθ

Squaring on the side

2RdR=2rdr-2adrcosθRdR=rdr-adrcosθRdR=(r-acosθ)dr

03

Determine the value of the interaction energy.

Now to redraw the above figure,

Draw a perpendicular from the charge q2as shown in above figure.

From above figure, the angle between the two electric field vectors' cosine is represented as follows:

cosβ=r-acosθR

Rewrite the interaction energy term in the following way:

W=ε0E1E2cosθβdτ

Substitute kq1r2for E1,kq2R2for E2and r2drsinθdθdfor dτand r-acosθRfor cosβin the equation.

localid="1654684150710" W=ε0kq1r2kq2r2r-cosθRr2drsinθdθdϕ=ε0K2q1q2r-cosθRdrsinθdθdϕ

Now substitute RdR for (r-acosθ)drin the equation.

localid="1654684297608" W=ε0K2q1q2r-cosθRr2drsinθdθdϕ=ε0K2q1q2dRR2(sinθdθdϕ)

Integrate the above equation,

W=ε0K2q1q2aRR20sinθdθ0dϕ=ε0K2q1q21--1a(-cosπ-(-cos0))(2π-0)=ε0K2q1q2a(2)(2π)

Substitute 14πε0 for Kin above equation.

W=ε014πε02q1q2a(2)(2π)=q1q24πε0a

Hence, the interaction energy isW=q1q24πε0a.

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Most popular questions from this chapter

We know that the charge on a conductor goes to the surface, but just

how it distributes itself there is not easy to determine. One famous example in which the surface charge density can be calculated explicitly is the ellipsoid:

x2a2+y2b2+z2c2=1

In this case15

σ=Q4πabc(x2a4+y2b4+z2c4)-1/2

(2.57) where Q is the total charge. By choosing appropriate values for a , b and c. obtain (from Eq. 2.57):

(a) the net (both sides) surface charge density a(r) on a circular disk of radius R; (b) the net surface charge density a(x) on an infinite conducting "ribbon" in the xy plane, which straddles they axis from x = - a to x = a (let A be the total charge per unit length of ribbon);

(c) the net charge per unit length λ(x)on a conducting "needle," running from x = - a to x = a. In each case, sketch the graph of your result.

(a) A point chargeqis inside a cavity in an uncharged conductor (Fig. 2.45). Is the force onq necessarily zero?

(b) Is the force between a point charge and a nearby uncharged conductor always

attractive?

Use Eq. 2.29 to calculate the potential inside a uniformly charged

solid sphere of radiusRand total charge q.Compare your answer to Pro b. 2.21.

Use Gauss's law to find the electric field inside and outside a spherical shell of radius Rthat carries a uniform surface charge densityσCompare your answer to Prob. 2.7.

All of electrostatics follows from 1/r2the character of Coulomb's law, together with the principle of superposition. An analogous theory can therefore be constructed for Newton's law of universal gravitation. What is the gravitational energy of a sphere, of mass M and radius R,assuming the density is uniform? Use your result to estimate the gravitational energy of the sun (look up the relevant numbers). Note that the energy is negative-masses attract,whereas (like) electric charges repel.As the matter "falls in," to create the sun, its energy is converted into other forms (typically thermal), and it is subsequently released in the form of radiation. The sun radiates at a rate of 3.86×1026W; if all this came from gravitational energy, how long would the sun last? [The sun is in fact much older than that, so evidently this is notthe source of its power.]

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