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A positive charge q is fired head-on at a distant positive charge Q (which is held stationary), with an initial velocityv0 . It comes in, decelerates to v=0, and returns out to infinity. What fraction of its initial energy(12mv02) is radiated away? Assume v0c, and that you can safely ignore the effect of radiative losses on the motion of the particle. [ Answer (1645)(qQ)(v0c)3. ]

Short Answer

Expert verified

The fraction of the radiated initial energy of the charge is 1645qQv0c3.

Step by step solution

01

Expression for the relation of conservation of energy for the point charge:

Write the expression for the relation of conservation of energy for the point charge.

12mv02=12mv2+qQ40x 鈥︹ (1)

Here, v is the final velocity, x is the distance of closest approach towards charge Q, m is the mass of a charge,v0 is the initial velocity of the charge q,0 is the permittivity of free space, q is the fired charge, and Q is the stationary charge.

02

Determine the final velocity of a particle:

Rearrange the equation (1),

12mv2=12mv02-qQ40xv2=v02-2qQ4m0x......(2)

Here,x0=2qQ4m0v02

Let,

k=qQ4m0

Hence, the above equation becomes,

Andx0=2kv02

Substitute k=qQ4m0in equation (2).

v=v02-2kx

03

Determine the total radiated power radiated by the charge q:

Using Larmor鈥檚 formula, write the expression for the total power radiated.

dW=0q2a26cdt 鈥︹ (3)

Here, a is the acceleration of the charge due to Coulomb鈥檚 repulsive force, which is given as:

a=kx2

Substitute a=kx2in equation (2).

dW=0q2kx226xdtW=0q26ck2x4dtW=0q2k26c1x4dxvW=0q2k26c1x4dxv02-2kx

On further solving, the above equation becomes,

W=0q2k26c1x4dx2kx0-2kxW=0q2k26cx01x4dx2kx0-2kxW=20q2k26c2kx0dxx41x0-1xW=20q2k26c2k1615x05/2

Again on further solving,

W=0q22k3/26c1615x05/2W=22k22k0q22k3/26c1615x05/2W=0q224ck16152kx05/2W=0q224ck1615v05

Substitute the value of k in the above expression.

W=0q224cqQ4m01615v05W=800q45cQv05W=8qmv0545c3Q

04

Determine the fraction of initial energy of charge q:

Calculate the fractional of the initial energy of charge q.

f=WWif=8qmv0545c3Q12mv02f=8qmv0545c3Q2mv02f=1645qQv0c3

Therefore, the fraction of the radiated initial energy is 1645qQv0c3.

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Most popular questions from this chapter

(a) Does a particle in hyperbolic motion (Eq. 10.52) radiate? (Use the exact formula (Eq. 11.75) to calculate the power radiated.)

(b) Does a particle in hyperbolic motion experience a radiation reaction? (Use the exact formula (Prob. 11.33) to determine the reaction force.)

[Comment: These famous questions carry important implications for the principle of equivalence.]

Find the angle max at which the maximum radiation is emitted, in Ex. 11.3 (Fig. 11.13). Show that for ultra relativistic speeds ( close toc), max(1)/2. What is the intensity of the radiation in this maximal direction (in the ultra relativistic case), in proportion to the same quantity for a particle instantaneously at rest? Give your answer in terms of.

An ideal electric dipole is situated at the origin; its dipole moment points in the z direction and is quadratic in time:

p(t)=12p0t2z^鈥夆赌夆赌夆赌(<t<)

wherep0is a constant.

  1. Use the method of Section 11.1.2 to determine the (exact) electric and magnetic fields for all r > 0 (there's also a delta-function term at the origin, but we're not concerned with that).
  2. Calculate the power, P(r,t), passing through a sphere of radius r.
  3. Find the total power radiated (Eq. 11.2), and check that your answer is consistent with Eq. 11.60.21

Equation 11.14 can be expressed in 鈥渃oordinate-free鈥 form by writing p0cos=p0r^. Do so, and likewise for Eqs. 11.17, 11.18. 11.19, and 11.21.

As you know, the magnetic north pole of the earth does not coincide with the geographic north pole鈥攊n fact, it鈥檚 off by about 11. Relative to the fixed axis of rotation, therefore, the magnetic dipole moment of the earth is changing with time, and the earth must be giving off magnetic dipole radiation.

(a) Find the formula for the total power radiated, in terms of the following parameters: (the angle between the geographic and magnetic north poles), M (the magnitude of the earth鈥檚 magnetic dipole moment), and (the angular velocity of rotation of the earth). [Hint: refer to Prob. 11.4 or Prob. 11.11.]

(b) Using the fact that the earth鈥檚 magnetic field is about half a gauss at the equator, estimate the magnetic dipole moment Mof the earth.

(c) Find the power radiated. [Answer: 410-5W]

(d) Pulsars are thought to be rotating neutron stars, with a typical radius of 10 km, a rotational period of 10-3s, and a surface magnetic field of 108T. What sort of radiated power would you expect from such a star? [Answer: 21036W].

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