(a) Show that a 30,000-line-per-centimeter grating will not produce a maximum for visible light. (b) What is the longest wavelength for which it does produce a first-order maximum? (c) What is the greatest number of lines per centimeter a diffraction grating can have and produce a complete second-order spectrum for visible light?

Short Answer

Expert verified

(a) The longest wavelength for which grating can produce the first-order maximum is 334 nm.

(b) The maximum wavelength of falling light on the grating is shorter than the visible spectrum's bottom bound, which starts from 380 nm

(c) The greatest number of lines per centimeter is6579, which can produce the second-order spectrum.

Step by step solution

01

Concept introduction

Visible light refers to the visible region of the electromagnetic spectrum that is, the range of wavelengths that trigger brightness and color perception in humans. It lies between 380 nm to 760 nm.

02

Given data

Grating lines on the diffraction grating are 30000 liner per cm, which means that the

distance between the two slits isd=1cm300001m100cm=3.34×107m

03

Determine the distance between the slit in the granting (a)

The equation for the constructive interference can be given as

dsinθ=…………………..(1)

Solving equation (1) for the minimum λ1when and θ=90.0°.

λ=dsinθm=3.34×107×sin90.0°1=3.34×107m1nm109m=334nm

Therefore, this grating cannot create a visible light maximum because the shortest wavelength of visible light is 380nm.

04

Determine the longest wavelength(b)

So, Compare the potential values of λ, the visible light wavelength range using the result of section (a).

The maximum wavelength that this grating can produce the first-order maximum is not within the range of visible light wavelengths.

Therefore, the maximum wavelength of light falling on the grating is shorter than the visible spectrum's lower bound

05

Produce a complete second-order spectrum for visible light (c)

Solving equation (1) for the maximumλ,andm=2,andθ=90.0°. Here the value of maximum wavelength for the visible light spectrum is 760 nm. Therefore,

d=maxsinθ=2×760nmsin90.0°×109m1nm=1.52×106m

Then the number of lines per cm will be

n=1cm1.52×106m1m100cm=6579

Therefore, The number of lines per centimeter 6579.

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Most popular questions from this chapter

The \(300 - m\)-diameter Arecibo radio telescope pictured in Figure \(27.28\) detects radio waves with a \(4.00{\rm{ }}cm\) average wavelength.

(a) What is the angle between two just-resolvable point sources for this telescope?

(b) How close together could these point sources be at the \({\rm{2}}\) million light year distance of the Andromeda galaxy?

Figure \(27.28\) A \(305 - m\)-diameter natural bowl at Arecibo in Puerto Rico is lined with reflective material, making it into a radio telescope. It is the largest curved focusing dish in the world. Although \(D\) for Arecibo is much larger than for the Hubble Telescope, it detects much longer wavelength radiation and its difdfraction limit is significantly poorer than Hubble's. Arecibo is still very useful, because important information is carried by radio waves that is not carried by visible light. (credit: Tatyana Temirbulatova, Flickr)

Consider a spectrometer based on a diffraction grating. Construct a problem in which you calculate the distance between two wavelengths of electromagnetic radiation in your spectrometer. Among the things to be considered are the wavelengths you wish to be able to distinguish, the number of lines per meter on the diffraction grating, and the distance from the grating to the screen or detector. Discuss the practicality of the device in terms of being able to discern between wavelengths of interest.

(a) What is the minimum angular spread of a \(633 - nm\) wavelength \({\rm{He - Ne}}\) laser beam that is originally \(1.00{\rm{ }}mm\) in diameter?

(b) If this laser is aimed at a mountain cliff \(15.0{\rm{ }}km\) away, how big will the illuminated spot be?

(c) How big a spot would be illuminated on the Moon, neglecting atmospheric effects? (This might be done to hit a corner reflector to measure the round-trip time and, hence, distance.) Explicitly show how you follow the steps in Problem-Solving Strategies for Wave Optics.

What is the ratio of thicknesses of crown glass and water that would contain the same number of wavelengths of light?

Using the result of the problem above, calculate the distance between fringes for 633nm light falling on double slits separated by 0.0800mm, located 3.00mfrom a screen as in Figure 27.56.

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