/*! 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} Problem 38 The light from an iron are inclu... [FREE SOLUTION] | 91Ó°ÊÓ

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The light from an iron are includes many different wavelengths. Two of these are at \(\lambda=587.9782 \mathrm{nm}\) and \(\lambda=\) 587.8002 \(\mathrm{nm}\) . You wish to resolve these spectral lines in first order using a grating 1.20 \(\mathrm{cm}\) in length. What minimum number of slits per centimeter must the grating have?

Short Answer

Expert verified
The grating must have at least 2753 slits per centimeter.

Step by step solution

01

Understand the Problem

We need to determine the minimum number of slits per centimeter that a grating must have in order to resolve two very close spectral lines at given wavelengths using first-order diffraction.
02

Write the Relevant Formula

The resolving power \( R \) of a grating is given by the formula \( R = \frac{\lambda}{\Delta \lambda} = mN \), where \( m \) is the order of the diffraction (which is 1 here), and \( N \) is the total number of slits illuminated. Here, \( \lambda \) is the average wavelength, and \( \Delta \lambda \) is the difference in the wavelengths.
03

Compute Average Wavelength and Wavelength Difference

Calculate the average wavelength \( \lambda \) and the difference \( \Delta \lambda \):\[ \lambda = \frac{587.9782 + 587.8002}{2} \, \text{nm} = 587.8892 \, \text{nm} \] \[ \Delta \lambda = 587.9782 \, \text{nm} - 587.8002 \, \text{nm} = 0.178 \, \text{nm} \]
04

Calculate the Resolving Power

Using the relation \( R = \frac{\lambda}{\Delta \lambda} \), calculate the resolving power: \[ R = \frac{587.8892}{0.178} = 3302.75 \]
05

Determine the Minimum Number of Slits

The total length of the grating is 1.20 cm (or 12 mm). For first-order diffraction \( m = 1 \), thus \( N = R \). Therefore, \( N = 3302.75 \) slits should fit in 1.20 cm for such resolution. Thus, the number of slits per centimeter \( d \) is given by \( d = \frac{N}{12 \, \text{mm}} \):\[ d = \frac{3302.75}{1.2} \approx 2752.3 \text{ slits/cm} \]
06

Round the Result Appropriately

Since the number of slits per centimeter must be a whole number, round up to the minimum necessary integer. Hence, the minimum number of slits per centimeter needed is 2753.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Resolving Power
In the context of diffraction gratings, resolving power is a critical concept. It describes the ability of a grating to separate or "resolve" two spectral lines with very similar wavelengths. For example, if two wavelengths are so close that they appear nearly indistinguishable, a device with high resolving power can discern them clearly.
  • The formula for resolving power is given by: \( R = \frac{\lambda}{\Delta \lambda} = mN \).
  • Here, \( \lambda \) is the average wavelength of the two lines, \( \Delta \lambda \) is the difference between the wavelengths, \( m \) is the diffraction order, and \( N \) is the number of slits illuminated.
  • The greater the resolving power, the better the grating is at distinguishing two close spectral lines.
Knowing how to calculate and interpret resolving power helps in choosing the right setup for spectral analysis.
Spectral Lines
Spectral lines are the distinct lines that represent wavelengths in a spectrum, usually emitted or absorbed by elements. These lines originate when electrons within an atom jump between energy levels, emitting or absorbing photons at specific wavelengths. In a spectrum, these lines appear as bright or dark lines and are unique to each element, acting like elemental fingerprints.• In the given problem, two spectral lines from an iron arc are being examined. • The wavelengths of interest are \( 587.9782 \, \text{nm} \) and \( 587.8002 \, \text{nm} \), which are very close.Understanding spectral lines is crucial for many scientific fields. It allows us to determine the composition of stars, identify elements in a sample, and measure environmental conditions.
Wavelength Difference
Wavelength difference, denoted as \( \Delta \lambda \), is a measure of how different two wavelengths are from one another. It is often very small for nearby spectral lines, making it challenging to resolve them.
  • In the provided problem, \( \Delta \lambda \) is calculated as the difference between \( 587.9782 \, \text{nm} \) and \( 587.8002 \, \text{nm} \).
  • This results in \( 0.178 \, \text{nm} \), a small difference that requires a precise instrument to detect.
Such small wavelength differences are common in spectroscopy and require instruments like diffraction gratings to discern effectively. Understanding and calculating \( \Delta \lambda \) is key in applications such as material analysis and astronomy where detailed spectral analysis is required.
Slits per Centimeter
Slits per centimeter is a measure of how many slits or openings are present on a diffraction grating per unit length. It is pivotal in determining the grating's resolving power.
  • More slits per centimeter generally equate to higher resolving power, allowing the device to resolve closer spectral lines.
  • In the exercise, determining the required slits per centimeter involves using the formula \( d = \frac{N}{1.2} \) where \( N \) is the total number of slits, which was calculated based on the resolving power to be about \( 3302.75 \).
  • This results in approximately \( 2752.3 \) slits per centimeter, which rounds up to \( 2753 \) slits per centimeter for practical manufacturing purposes.
The number of slits per centimeter is crucial in designing gratings efficiently for specific experimental needs, ensuring precise spectral resolution.

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Most popular questions from this chapter

The wavelength range of the visible spectrum is approximately \(400-700 \mathrm{nm} .\) White light falls at normal incidence on a diffraction grating that has 350 slits \(/ \mathrm{mm}\) . Find the angular width of the visible spectrum in (a) the first order and \((\mathrm{b})\) the third order. (Note: An advantage of working in higher orders is the greater angular spread and better resolution. A disadvantage is the overlapping of different orders, as shown in Example 36.4 .

Monochromatic light with wavelength 620 \(\mathrm{nm}\) passes through a circular aperture with diameter 7.4\(\mu \mathrm{m}\) . The resulting diffraction pattern is observed on a screen that is 4.5 \(\mathrm{m}\) from the aperture. What is the diameter of the Airy disk on the screen?

Due to blurring caused by atmospheric distortion, the best resolution that can be obtained by a normal, earth-based, visible-light telescope is about 0.3 arcsecond (there are 60 arcminutes in a degree and 60 arcseconds in an arcminute). (a) Using Rayleigh's criterion, calculate the diameter of an earth-based telescope that gives this resolution with 550 -nm light. (b) Increasing the telescope diameter beyond the value found in part (a) will increase the light-gathering power of the telescope, allowing more distant and dimmer astronomical objects to be studied, but it will not improve the resolution. In what ways are the Keck telescopes (each of 10- diameter) atop Mauna Kea in Hawaii superior to the Hale Telescope ( 5 -m diameter) on Palomar Mountain in California? In what ways are they not superior? Explain.

Plane monochromatic waves with wavelength 520 \(\mathrm{nm}\) are incident normally on a plane transmission grating having 350 slits \(\operatorname{mon}\) . Find the angles of deviation in the first, second, and third orders.

Intensity Pattern of \(N\) Slits. (a) Consider an arrangement of \(N\) slits with a distance \(d\) between adjacent slits. The slits emit coherently and in phase at wavelength \(\lambda\) . Show that at a time \(t,\) the electric field at a distant point \(P\) is $$ \begin{aligned} E_{P}(t)=& E_{0} \cos (k R-\omega t)+E_{0} \cos (k R-\omega t+\phi) \\ &+E_{0} \cos (k R-\omega t+2 \phi)+\cdots \\ &+E_{0} \cos (k R-\omega t+(N-1) \phi) \end{aligned} $$ where \(E_{0}\) is the amplitude at \(P\) of the electric field due to an individual slit, \(\phi=(2 \pi d \sin \theta) / \lambda, \theta\) is the angle of the rays reaching \(P(\text { as measured from the perpendicular bisector of the slit arrangement }\)), and \(R\) is the distance from \(P\) to the most distant slit. In this problem, assume that \(R\) is much larger than \(d .\) (b) To carry out the sum in part \((a),\) it is convenient to use the complex-number relationship $$ e^{i k}=\cos z+i \sin z $$ where \(i=\sqrt{-1}\) . In this expression, \(\cos z\) is the real part of the complex number \(e^{i k},\) and \(\sin z\) is its imaginary part. Show that the electric field \(E_{P}(t)\) is equal to the real part of the complex quantity $$ \sum_{n=0}^{N-1} E_{0} e^{i(k R-\omega+n \phi)} $$ (c) Using the properties of the exponential function that \(e^{A} e^{B}=e^{(A+B)}\) and \(\left(e^{A}\right)^{n}=e^{n A},\) show that the sum in part \((b)\) can be written as $$ E_{0}\left(\frac{e^{i N \phi}-1}{e^{i \phi}-1}\right) e^{i(k R-\omega t)}=E_{0}\left(\frac{e^{i N \phi / 2}-e^{-i N \phi / 2}}{e^{i \phi / 2}-e^{-i \phi / 2}}\right) e^{i(k R-\omega t+(N-1) \phi / 2]} $$ Then, using the relationship \(e^{i k}=\cos z+i \sin z,\) show that the (real) electric field at point \(P\) is $$ E_{p}(t)=\left[E_{0} \frac{\sin (N \phi / 2)}{\sin (\phi / 2)}\right] \cos [k R-\omega t+(N-1) \phi / 2] $$ The quantity in the first square brackets in this expression is the amphitude of the electric field at \(P .\) (d) Use the result for the electric-field amplitude in part (c) to show that the intensity at an angle \(\theta\) is $$ I=I_{0}\left[\frac{\sin (N \phi / 2)}{\sin (\phi / 2)}\right]^{2} $$ where \(I_{0}\) is the maximum intensity for an individual slit. (e) Check the result in part (d) for the case \(N=2\) . It will help to recall that \(\sin 2 A=2 \sin A \cos A\) . Explain why your result differs from Eq. \((35.10),\) the expression for the intensity in two-source interference, by a factor of \(4 .\) (Hint: Is \(I_{0}\) defined in the same way in both expressions?)

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