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An electron is released from rest and falls under the influence of gravity. In the first centimeter, what fraction of the potential energy lost is radiated away?

Short Answer

Expert verified

The fraction of the potential energy lost is 2.7610-22.

Step by step solution

01

Expression for a fraction of the potential energy lost:

Write the fraction of the potential energy lost is radiated.

f=UradUpotential 鈥︹ (1)

Here,Urad is the radiated energy andUpotential is the potential energy.

02

Determine the dipole moment:

Write the expression for the radiated energy.

Urad=Pt 鈥︹ (2)

Here, P is the power, and t is the time.

Let the distance travelled by the electron be y, and its initial velocity be uu=0.

If an electron travels a distance y in a time t, express the required equation.

y=12gt2t=2yg

Here, g is the gravitational acceleration.

Write the expression for the total radiated power.

P=06cpt2 鈥︹ (3)

Here, p is the dipole moment which is given as:

p=-eyy^y=-pey^12gt2=-pey^p=-12get2y^.......(4)

03

Determine the radiated energy:

Take the double differentiation of equation (4).

p=-12ge2ty^p=-gey^pt=ge

Substitutept=ge in equation (3).

P=06cge2

Substitute P=06cge2and t=2ygin equation (2).

Urad=06cge22ygUrad=0ge26c2yg

04

Determine the fraction of the potential energy lost:

Write the expression for the loss in potential energy of an electron falling a distance.

Upotential=mgy

SubstituteUrad=0ge26c2yg andUpotential=mgy in equation (1).

f=0ge26c2ygmgyf=0g2e26cmg2ygf=0e26cm2gy

Here, m is the mass of an electron m=9.1110-31kg.

Substitute 0=410-7H/m,e=1.610-19C,c=3108m/s,m=9.1110-31kg,g=9.81m/s2andy=1cm in the above expression.

f=410-7H/m1.610-19C263108m/s9.1110-31kg29.81m/s21cm10-2m1cmf=2.7610-22

Therefore, the fraction of the potential energy lost is2.7610-22 .

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Most popular questions from this chapter

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.

Deduce Eq. 11.100 from Eq. 11.99. Here are three methods:

(a) Use the Abraham-Lorentz formula to determine the radiation reaction on each end of the dumbbell; add this to the interaction term (Eq. 11.99).

(b) Method (a) has the defect that it uses the Abraham-Lorentz formula鈥攖he very thing that we were trying to derive. To avoid this,F(q) let be the total d-independent part of the self-force on a charge q. Then

F(q)=Fint(q)+2F(q2)

WhereFint is the interaction part (Eq. 11.99), andF(q2) is the self-force on each end. Now,F(q) must be proportional to q2, since the field is proportional to q and the force is qE. SoF(q2)=(14)F(q) Take it from there.

(c) Smear out the charge along a strip of length L oriented perpendicular to the motion (the charge density, then, is =qL); find the cumulative interaction force for all pairs of segments, using Eq. 11.99 (with the correspondence q2dy, at one end and at the other). Make sure you don鈥檛 count the same pair twice.

Question: In Ex. 11.3 we assumed the velocity and acceleration were (instantaneously,

at least) collinear. Carry out the same analysis for the case where they are

perpendicular. Choose your axes so that v lies along the z axis and a along the x axis

(Fig. 11.14), so thatv=vz^,a=ax^,andr^=蝉颈苍胃肠辞蝉x^+sinv=vz^,a=ax^,andr^=蝉颈苍胃肠辞蝉x^+sinsiny^+肠辞蝉胃z^Check that P is consistent with the Lienard formula.

dP诲惟=0q2a2162c1-尾肠辞蝉胃2-1-2sin2胃肠辞蝉21-尾肠辞蝉胃5,P=0q2a246蟺肠[Answer: .For relativistic velocities ( 1) the radiation is again sharply peaked in the forward

direction (Fig. 11.15). The most important application of these formulas is to circular motion-in this case the radiation is called synchrotron radiation. For a relativistic electron, the radiation sweeps around like a locomotive's headlight as the particle moves.]

Calculate the electric and magnetic fields of an oscillating magnetic dipole without using approximation . [Do they look familiar? Compare Prob. 9.35.] Find the Poynting vector, and show that the intensity of the radiation is exactly the same as we got using approximation .

a)Find the radiation reaction force on a particle moving with arbitrary velocity in a straight line, by reconstructing the argument in Sect. 11.2.3 without assuming (tr)=0. [Answer: (0q24/6蟺肠)(a+32a2/c2)]

(b) Show that this result is consistent (in the sense of Eq. 11.78) with the power radiated by such a particle (Eq. 11.75).

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