/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Q9.18 Question: The index of refracti... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Question:The index of refraction of diamond is 2.42. Construct the graph analogous to Fig. 9.16 for the air/diamond interface. (Assume .) In particular, calculate (a) the amplitudes at normal incidence, (b) Brewster's angle, and (c) the "crossover" angle, at which the reflected and transmitted amplitudes are equal.

Short Answer

Expert verified

Answer

(a) The value of amplitude at the normal incidence is E0T=0.585E0I.

(b) The value of Brewster’s angle is 67.550.

(c) The value of crossover angle is 78.240.

Step by step solution

01

Write the given data from the question

(Assumeμ1=μ2=μ0 .)

The "crossover" angle, at which the reflected and transmitted amplitudes are equal.

02

Determine the formula of amplitude at the normal incidence, Brewster’s angle and crossover angle

Write the formula of amplitude at the normal incidence.

E0TE0I=2α+β …… (1)

Here,α is purely imaginary, βis real.

Write the formula ofBrewster’s angle.

θB=tan-n2n1 …… (2)

Here, role="math" localid="1658736610477" n1 is the refractive index of the first object and n2 is the refractive index of the second object.

Write the formula of crossover angle.

α21-sin2θ=1-n1n22sin2θ ….. (3)

Here, α is purely imaginary, n1 is the refractive index of the first object and is the refractive index of the second object.

03

(a) Determine the value of amplitude at the normal incidence

From Fresnel’s equation

β=μ1ν1μ2ν2=μ1μ2n2n1

Here, n1 is the refractive index of the first object, n2 is the refractive index of the second object, ν1 is the velocity of the first object, and ν2is the velocity of the second object.

Substitute 2.42 for n2 and 1 for n1 in the above equation β.

β=2.421=2.42

Sinceμ1=μ2=μ0 and the refractive index of the air is 1.

Determine the reflected amplitude wave is

E→0R=α-βα+βE→0I

Determine the transmitted wave is

E→0T=2α+βE→0T

Here amplitudes of reflected and transmitted waves depend on angle of incidence.

Thus, the amplitude of the reflected and transmitted waves is

α=1-sin2θTcosθ1=1-n1n22sin2θ1cosθ1 …… (4)

The graph that represents the air diamond interaction is displayed in the following illustration.

Electric field ratio is represented on the y axis, while incidence angle is represented on the -x axis.

At the normal incidence θ1=0°.

Substitute 2.42 for n2, 00 forθ1, and 1 for n1 into above equation (4).

α=1-12.422sin0cos0=1

Then, the ratio of the reflected and incident amplitudes is

E0RE0I=α-βα+β or β into equation (1).

Substitute 1 for α and 2.42 for β into above equation.

E0RE0I=1-2.421+2.42=-0.415

Determine the ratio of transmitted and incident amplitude is

Substitute 1 for and 2.42

E0TE0I=21+2.42=0.585E0T=0.585E0I

Therefore, the value of amplitude at the normal incidence is E0T=0.585E0I.

04

(b) Determine the value of Brewster’s angle

At Brewster’s angle

tanθB≅n2n1

Determine the Brewster’s angle.

Substitute 1 for α and 2.42 for βinto equation (2).

θB=tan-12.42=67.55°

Therefore, the Brewster’s angle is 67.550.

05

(c) Determine the value of crossover angle

As given reflected and transmitted amplitudes are equal.

E→0R=E→0T

Then,

α-β=2α=β+2

Substitute 2.42 for β into above equation.

Then we know that

α=1-n1n22sin2θ1cosθ1α=1-n1n22sin2θcos2θα2cos2θ=1-n1n22sin2θα21-sin2θ=1-n1n22sin2θ

Determine the crossover angle.

Substitute 1 for n1 and 2.42 for n2 into equation (3).

α21-sin2θ=1-12.422sin2θ4.4221-sin2θ=1-12.422sin2θsinθ=0.979

From the above equation, the angle is

θ=sin-10.979=78.24°

Therefore, the value of crossover angle is 78.240 .

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

Question:According to Snell's law, when light passes from an optically dense medium into a less dense one the propagation vector bends away from the normal (Fig. 9.28). In particular, if the light is incident at the critical angle

θc=sin-(n2n1)

Then , and the transmitted ray just grazes the surface. If exceeds , there is no refracted ray at all, only a reflected one (this is the phenomenon of total internal reflection, on which light pipes and fiber optics are based). But the fields are not zero in medium ; what we get is a so-called evanescent wave, which is rapidly attenuated and transports no energy into medium 2.26

Figure 9.28

A quick way to construct the evanescent wave is simply to quote the results of Sect. 9.3.3, with and

kT=kTsinθTx^+cosθTz^

the only change is that

sinθT=n1n2sinθI

is now greater than, and

cosθT=1-sin2θT

is imaginary. (Obviously, can no longer be interpreted as an angle!)

(a) Show that

E→T(r,t)=E→0Te-kzeI(kx-Ӭt)

Where

k≡Ӭc(n1²õ¾±²Ôθ1)2-n22

This is a wave propagating in the direction (parallel to the interface!), and attenuated in the direction.

(b) Noting that (Eq. 9.108) is now imaginary, use Eq. 9.109 to calculate theirreflection coefficient for polarization parallel to the plane of incidence. [Notice that you get reflection, which is better than at a conducting surface (see, for example, Prob. 9.22).]

(c) Do the same for polarization perpendicular to the plane of incidence (use the results of Prob. 9.17).

(d) In the case of polarization perpendicular to the plane of incidence, show that the (real) evanescent fields are

Er,t=E0e-kzcoskx-Ó¬ty^Br,t=E0Ó¬e-kzksinkx-Ó¬tx^+kcoskx-Ó¬tz^

(e) Check that the fields in (d) satisfy all of Maxwell's equations (Eq. 9.67).

(f) For the fields in (d), construct the Poynting vector, and show that, on average, no energy is transmitted in the z direction.

[The naive explanation for the pressure of light offered in Section 9.2.3 has its flaws, as you discovered if you worked Problem 9.11. Here’s another account, due originally to Planck.] A plane wave traveling through vacuum in the z direction encounters a perfect conductor occupying the region z≥0, and reflects back:

E(z,t)=E0[cos(kz-Ó¬t)-cos(kz+Ó¬t)]x^,(z>0),

(a) Find the accompanying magnetic field (in the region role="math" localid="1657454664985" (z>0).

(b) Assuming inside the conductor, find the current K on the surface z=0, by invoking the appropriate boundary condition.

(c) Find the magnetic force per unit area on the surface, and compare its time average with the expected radiation pressure (Eq. 9.64).

[The naive explanation for the pressure of light offered in section 9.2.3 has its flaws, as you discovered if you worked Problem 9.11. Here's another account, due originally to Planck.] A plane wave travelling through vaccum in the z direction encounters a perfect conductor occupying the region z≥0, and reflects back:

E(z,t)=E0[coskz-Ó¬t-coskz+Ó¬t]x^,(z>0)

  1. Find the accompanying magnetic field (in the region (z>0))
  2. Assuming B=0inside the conductor find the current K on the surface z=0, by invoking the appropriate boundary condition.
  3. Find the magnetic force per unit area on the surface, and compare its time average with the expected radiation pressure (Eq.9.64).

Question: Use Eq. 9.19 to determineA3andδ3in terms ofrole="math" localid="1653473428327" A1,A2,δ1, andδ2.

a) Derive Eqs. 9.179, and from these obtain Eqs. 9.180.

(b) Put Eq. 9.180 into Maxwell's equations (i) and (ii) to obtain Eq. 9.181. Check that you get the same results using (i) and (iv) of Eq. 9.179.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.