A parallel-plate capacitor C, with plate separation d, is given an initial charge (±)Q0. It is the0n connected to a resistor R, and discharges, Q(t)=Q0e-t/RC.

(a) What fraction of its initial energy(Q02/2C) does it radiate away?

(b) If C=1pF,R=1000Ω,and role="math" localid="1653972749344" d=0.1mm, what is the actual number? In electronics we don’t ordinarily worry about radiative losses; does that seem reasonable, in this case?

Short Answer

Expert verified

(a) The fraction of energy radiated is EradE0=μ06πcd2R3C2.

(b) The actual number for the fractional energy loss is2.2×10-9 which is safe to neglect.

Step by step solution

01

Given Information:

Given data:

The decay of charge after a certain time interval is Qt=Q0e-t/RC.

The capacitance of a capacitor is C=1pF.

The resistance of a resistor is R=1000Ω

The position of the charge is d=0.1mm.

02

Determine the fraction of the radiated initial energy:

(a)

Write the expression for a fraction of energy radiated.

EradE0=0Pdt(Q022C) …… (1)

Here, P is the total radiated power from the parallel plate capacitor, and C is the capacitance of a capacitor.

Write the expression for the total radiated power from the parallel plate capacitor.

P=μ06πcp¨2 …… (2)

Here, μ0 is the magnetic permeability, c is the speed of light, and p is the dipole moment.

Write the expression for the dipole moment.

p=Qtd

Substitute Qt=Q0e-t/RCin the above expression.

p=Q0e-tRCd

Take the double differentiation of the above equation.

p˙=-Q0RCe-tRCdp¨=Q0RC2etRCd

Substitute p¨=Q0RC2e-tRCdin equation (2).

P=μ06πcQ0RC2e-tRCd2

Now, substitute P=μ06πcQ0RC2e-tRCd2to calculate the fraction of the radiated initial energy.

EradE0=0μ06πcQ0RC2e-tRCd2Q022cEradE0=μ06πcQ02d2RC40e-tRC2dt×2CQ02EradE0=μ03πcQ02d2RC4RC2e-2tRC0×CQ02EradE0=μ06πcd2R3C2........(3)

Therefore, the fraction of energy radiated is EradE0=μ06πcd2R3C2.

03

Determine the actual number:

(b)

Substituteμ0=4π×10-7H/m,d=0.1mm,c=3×108m/s,R=1000Ω andC=1pF in equation (3).

EradE04π×10-7H/m6π3×108m/s0.1mm×10-3m1mm21000Ω31pF×10-12F1pF2EradE0=2.2×10-9

As the fraction is very small, so this will be safe to neglect.

Therefore, the fractional energy loss is2.2×10-9 which is safe to neglect.

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Most popular questions from this chapter

A particle of mass m and charge q is attached to a spring with force constant k, hanging from the ceiling (Fig. 11.18). Its equilibrium position is a distance h above the floor. It is pulled down a distance d below equilibrium and released, at timet=0.

(a) Under the usual assumptions (dλh), calculate the intensity of the radiation hitting the floor, as a function of the distance R from the point directly below q. [Note: The intensity here is the average power per unit area of floor.]

FIGURE 11.18

At whatR is the radiation most intense? Neglect the radiative damping of the oscillator.

(b) As a check on your formula, assume the floor is of infinite extent, and calculate the average energy per unit time striking the entire floor. Is it what you’d expect?

(c) Because it is losing energy in the form of radiation, the amplitude of the oscillation will gradually decrease. After what timebhas the amplitude been reduced to d/e? (Assume the fraction of the total energy lost in one cycle is very small.)

Use the “duality” transformation of Prob. 7.64, together with the fields of an oscillating electric dipole (Eqs. 11.18 and 11.19), to determine the fields that would be produced by an oscillating “Gilbert” magnetic dipole (composed of equal and opposite magnetic charges, instead of an electric current loop). Compare Eqs. 11.36 and 11.37, and comment on the result.

Use the result of Prob. 10.34 to determine the power radiated by an ideal electric dipole, , at the origin. Check that your answer is consistent with Eq. 11.22, in the case of sinusoidal time dependence, and with Prob. 11.26, in the case of quadratic time dependence.

As you know, the magnetic north pole of the earth does not coincide with the geographic north pole—in fact, it’s 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:ψ (the angle between the geographic and magnetic north poles), M (the magnitude of the earth’s magnetic dipole moment), andω (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’s magnetic field is about half a gauss at the equator, estimate the magnetic dipole moment Mof the earth.

(c) Find the power radiated. [Answer: 4×10-5W]

(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: 2×1036W].

we calculated the energy per unit time radiated by a (non-relativistic) point charge- the Larmor formula. In the same spirit:

(a) Calculate the momentum per unit time radiated.

(b) Calculate the angular momentum per unit time radiated.

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