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Consider the motion of a particle with mass m and electric charge qein the field of a (hypothetical) stationary magnetic monopole qmat the origin:

B=μ04qmr2r^

(a) Find the acceleration of qe, expressing your answer in terms of localid="1657533955352" q, qm, m, r (the position of the particle), and v(its velocity).

(b) Show that the speed v=|v|is a constant of the motion.

(c) Show that the vector quantity

Q=m(r×v)-μ0qeqm4πr^

is a constant of the motion. [Hint: differentiate it with respect to time, and prove-using the equation of motion from (a)-that the derivative is zero.]

(d) Choosing spherical coordinates localid="1657534066650" (r,θ,ϕ), with the polar (z) axis along Q,

(i) calculate , localid="1657533121591" Qϕ^and show that θis a constant of the motion (so qemoves on the surface of a cone-something Poincare first discovered in 1896)24;

(ii) calculate Qr^, and show that the magnitude of Qis

Q=μ04π|qeqmcosθ|;

(iii) calculate Qθ^, show that

dt=kr2,

and determine the constant k .

(e) By expressing v2in spherical coordinates, obtain the equation for the trajectory, in the form

drdϕ=f(r)

(that is: determine the function )f(r)).

(t) Solve this equation for .r(ϕ)

Short Answer

Expert verified

(a) The acceleration of qeis μ0qm4mπr2qv×r^.

(b) The speed v=vis a constant of the motion.

(c) The vector quantity is a constant of the motion.

(d)

(i) Qϕ^is and θis a constant of the motion.

(ii) The value of Qr^is Qcosθand the magnitude of Qis proved.

(iii) The value of Qθ^is -Qsinθand dϕdt=kr2is proved.

The constant k is Qm.

(e) The function f (r) is rrvk2-sin2θ.

(f) r(ϕ)is AcosarcosAr0+sinθ(ϕ-ϕ0.

Step by step solution

01

Identification of the given data

The given data is listed below as:

  • The mass of the particle is, m
  • The electric charge of the particle is, qe
  • The stationary magnetic monopole is qm,
02

Significance of the magnetostatics

Magnetostatics is described as the study of the magnetic fields in the systems where the currents remain steady. However, magnetostatics is described as the electrostatics’ magnetic analogue where there are stationary charges.

03

(a) Determination of the acceleration

The equation of the force of the particle is expressed as:

F= ma

…(i)

Here, m is the mass of the particle and a is the acceleration of the particle.

The equation of the force of the particle can also be written as:

F=μ0qm4πr2qv×r^

…(ii)

Here, qmis the stationary magnetic monopole, v is the velocity of the particle, r is the position of the particle, q is the particle’s charge, role="math" localid="1657535676962" μ0is the permeability constant r^and is the position vector.

Equalling the equation (i) and (ii).

role="math" localid="1657536121138" ma=μ0qm4πr2qv×r^a=μ0qm4mπr2qv×r^

Thus, the acceleration of qeis μ0qm4mπr2qv×r^.

04

(b) Determination of the speed

The magnitude of the velocity of the particle is conserved. Hence, the equation of the speed of the particle is expressed as:

av=0

Here, is the acceleration of the particle andv is the velocity of the particle.

The above equation can also be written as:

a.v=dvdtv=12ddt(v2)=0

Hence, the equation is proved.

Thus, the speed v=vis a constant of the motion.

05

(c) Determination of the prove that the vector quantity is a constant of the motion

The equation of the vector quantity is expressed as:

Q=m(r×v)-μ0qeqm4πr^

…(iii)

Here, qmis the stationary magnetic monopole, v is the velocity of the particle, r is the position of the particle, qeis the particle’s electric charge, μ0is the permeability constant, m is the mass of the particle and is r^the position vector.

Differentiating the above equation with respect to time.

dQdt=m(v×v+r×a)-μ0qeqm4πvr-rrr2=mr×μ0qeqm4mπr2v×r^-μ0qeqm4πr2(vr-rr)=μ0qeqm4πr2(r×(v×r^))-μ0qeqm4πr2(vr-rr) …(iv)

For the triple product, the BAC-CAB rule is used.

r×(v×r)=v(rr^)-r^(rv)=vr-r^rr˙=vr-rr^

Substitute the above value in the equation (iv).

dQdt=μ0qeqm4πr2(vr-r˙r)-μ0qeqm4πr2(vr-r˙r)

= 0

As the derivate is zero, hence it can be stated that the vector quantity is a constant of the motion.

Thus, the vector quantity is a constant of the motion.

06

(d) (i) Determination of Q.ϕ¯

The equation of the cross product of the particle’s position and the velocity is expressed as:

r×v=r×(r˙r^+rθ˙θ^+rsinθϕ˙ϕ^)=r2θ˙ϕ^-r2sinθθ^ϕ˙

Substitute the values from the above equation in the equation (iii).

Q=mr2θ˙ϕ^-mr2sinθθ^ϕ˙-μ0qeqm4πr^

…(v)

The dot product of the above equation with is expressed as:

Qϕ^=mr2θ˙ϕ˙ϕ^-μ0qeqm4πr^ϕ^=mr2θ˙=0

As both the variables are mutually orthogonal. Hence, localid="1657620419227" θ˙=0and it is constant of motion.

Thus, localid="1657620427016" Q.ϕ^is 0 and θis a constant of the motion.

07

(d) (ii) Determination of Q.r^

The dot product of the equation (v) with r^is expressed as:

Qr^=mr2θ˙ϕ^r^-mr2sinθθ^ϕ˙r^-μ0qeqm4πr^r^=Qcosθ

The above equation can also be expressed as:

Qcosθ=μ0qeqm4πQ=μ0qeqm4πcosθ

Thus, the value of Qr^is Qcosθand the magnitude of Qis proved.

08

(d) (iii) Determination of Q.θ^

The dot product of the equation (v) with is expressed as:

Q.θ^=mr2θ˙ϕ^θ^-mr2sinθθ^-μ0qeqm4πr^θ^=-Qsinθ

The above equation can also be expressed as:

-Qsinθ=-mr2sinθϕ˙φ˙=Qmr2

…(vi)

As the dot product Qθ^is , -Qsinθthen the constant is kexpressed as:

k=Qm

Substitute the value of the above equation in equation (vi).

φ˙kr2dϕdt=kr2

Thus, Qθ^the value of-Qsinθ is and dϕdt=kr2is proved.

The constant kis Qm.

09

(e) Determination of the function f (r)

The equation of expressing the square of the velocity in the spherical coordinates is expressed as:

v2=r˙+r2sin2θϕ˙2+r2θ˙2

Substitute 0 for θ˙and Qmr2for in the above equation.

role="math" localid="1657618825571" v2=r˙2+r2sin2θQ2m2r4=r˙2+C2r2C2=sin2θQ2m2

The chain rule has been applied in the differential equation of the curve.

r˙=drdt=drdϕdϕdt=drdϕϕ˙r˙ϕ˙=drdϕ

…(vii)

The equation of the position of the particle is expressed as:

r˙=v2-C2r2

Substitute v2-C2r2for r˙andQmr2for ϕ˙in the equation (vii).

drdϕ=rmQr2v2-C2=rrvk2-sin2θ=f(r) …(viii)

Thus, f(r)the function is rrvk2-sin2θ.

10

(f) Solving the equation

The equation (viii) can be recalled as:

drdϕ=rrvk2-sin2θdϕ=drrrvk2-sin2θ

Integrating the above equation with the limits.

ϕoϕdϕ=rordrrrvk2-sin2θ

ϕ-ϕ0kvrordrrr2-A2

Substitute sin2θk2v2for in the above equation.

ϕ-ϕo=kvAarccosArrro=1sinθarccosAr-arccosAr0arccosAr=arccosAro+sinθ(ϕ-ϕo)cosarccosAr=cosarccosAro+sinθ(ϕ-ϕo

Hence, further as:

Ar=cosarccosAr0+sinθ(ϕ-ϕ0r=AcosarccosAr0+sinθ(ϕ-ϕ0)

The term Ar0is the integration constant and it rotates around the orbit.

Thus, r(ϕ)is AcosarccosAro+sinθ(ϕ-ϕo).

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Most popular questions from this chapter

(a) Prove that the average magnetic field, over a sphere of radius R, due to steady currents inside the sphere, is

Bave=μ042m˙4

where mbis the total dipole moment of the sphere. Contrast the electrostatic result, Eq. 3.105. [This is tough, so I'll give you a start:

Bave=14π3R3fBd

Write BUas ×A, and apply Prob. 1.61(b). Now put in Eq. 5.65, and do the surface integral first, showing that

1rd43,

(b) Show that the average magnetic field due to steady currents outside the sphere is the same as the field they produce at the center.

A circularly symmetrical magnetic field ( B depends only on the distance from the axis), pointing perpendicular to the page, occupies the shaded region in Fig. 5.58. If the total flux (B.da) is zero, show that a charged particle that starts out at the center will emerge from the field region on a radial path (provided it escapes at all). On the reverse trajectory, a particle fired at the center from outside will hit its target (if it has sufficient energy), though it may follow a weird route getting there. [Hint: Calculate the total angular momentum acquired by the particle, using the Lorentz force law.]

Find and sketch the trajectory of the particle in Ex. 5.2, if it starts at

the origin with velocity

(a)v(0)=EBy(b)v(0)=E2By(c)v(0)=EB(y+z).

A magnetic dipole m=m0z^ is situated at the origin, in an otherwiseuniform magnetic field B=B0z^ . Show that there exists a spherical surface, centered at the origin, through which no magnetic field lines pass. Find the radius of this sphere, and sketch the field lines, inside and out.

Magnetostatics treats the "source current" (the one that sets up the field) and the "recipient current" (the one that experiences the force) so asymmetrically that it is by no means obvious that the magnetic force between two current loops is consistent with Newton's third law. Show, starting with the Biot-Savart law (Eq. 5.34) and the Lorentz force law (Eq. 5.16), that the force on loop 2 due to loop 1 (Fig. 5.61) can be written as

F2=μ04πl1l2r^r2dl1dl2

Figure 5.60

Figure 5.61

In this form, it is clear that F2=-F1, since role="math" localid="1657622030111" r^changes direction when the roles of 1 and 2 are interchanged. (If you seem to be getting an "extra" term, it will help to note thatdl2r^=dr.)

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