Light incident on a grating for spectroscopy

In summary, we discussed an equation involving the angle of incidence on a grating and the spacing of its slits. By manipulating the equation, we arrived at the solution m(lambda)=d[sin(theta-phi)+sin(phi)], which was confusing at first. However, through collaboration, we were able to understand the derivation.
  • #1
KaiserBrandon
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0

Homework Statement


if light incident on a grating makes an angle phi with the normal of the grating, show that the equation m(lambda)=d(sin(theta)) becomes m(lambda)=d[sin(theta-phi)+sin(phi)]

Homework Equations



m(lambda)=d(sin(theta)) d=spacing of slits, theta=angle displaced from normal of the grating
m(lambda)=d[sin(theta-phi)+sin(phi)]

The Attempt at a Solution


I've been working on trying to get a solution to this equation for quite some time now, and the only thing that makes sense is the equation m(lambda)=d*sin(theta-phi). don't know where +sin(phi) comes from.
 
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  • #2
I don't get either of those answers!
Maybe we can put our heads together and sort out our differences!
grating.jpg
 
  • #3


I would first verify the given equation m(lambda)=d(sin(theta)) by checking its derivation and ensuring that all the necessary assumptions and approximations have been made. Then, I would proceed to solve the given problem by considering the geometry of the situation.

When light is incident on a grating, it is diffracted into different orders (m) depending on the angle of incidence (theta) and the spacing of the grating (d). This can be described by the equation m(lambda)=d(sin(theta)). However, if the angle of incidence is not directly perpendicular to the grating, but at an angle phi, the light will be diffracted at an angle of theta-phi. Therefore, the equation becomes m(lambda)=d(sin(theta-phi)). This explains the first part of the given solution.

Now, we need to consider the effect of the angle phi on the diffracted light. At an angle of phi, the light will also be diffracted, but at an angle of theta. This is because the angle of incidence is now perpendicular to the grating, and therefore the light will not be diffracted further. This explains the second part of the given solution, d[sin(phi)].

In summary, the equation m(lambda)=d[sin(theta-phi)+sin(phi)] takes into account the overall diffraction of the light at an angle phi from the normal of the grating. It is important to note that this equation is an approximation and may not hold true for all cases. Further analysis and experimentation may be needed to fully understand the effects of incident angle on grating spectroscopy.
 

FAQ: Light incident on a grating for spectroscopy

What is a grating and how is it used in spectroscopy?

A grating is a device with a series of closely spaced parallel lines or grooves on its surface. When light is incident on a grating, it is diffracted into its component wavelengths, allowing for the analysis of the light's spectrum. In spectroscopy, a grating is used as a dispersive element to separate and measure the wavelengths of light emitted or absorbed by a sample.

What is the difference between a transmission grating and a reflection grating?

A transmission grating is a type of grating where the light passes through the grooves and is diffracted, while a reflection grating reflects the light off of the grooves and is also diffracted. Transmission gratings are typically used in spectroscopy, while reflection gratings are used in other applications such as laser systems.

How does the spacing of the grating affect the spectral resolution?

The spacing of the grating, also known as the groove density, directly affects the spectral resolution of the spectroscopy system. A higher groove density results in a higher spectral resolution, meaning the ability to distinguish between closely spaced wavelengths. This is because a higher groove density results in a larger angular dispersion of the diffracted light.

What is the relationship between the incident angle and the diffraction angle for a grating?

The incident angle, or the angle at which the light hits the grating, is equal to the diffraction angle, or the angle at which the diffracted light is observed, for a grating. This is known as the grating equation: nλ = d(sinθi + sinθd), where n is the diffraction order, λ is the wavelength of light, d is the groove spacing, θi is the incident angle, and θd is the diffraction angle.

How can the grating equation be used to determine the wavelength of light?

The grating equation can be rearranged to solve for the wavelength of light: λ = d(sinθi + sinθd)/n. By measuring the diffraction angles and knowing the groove spacing and diffraction order, the wavelength of light can be calculated. This is the principle behind using a grating in spectroscopy to determine the wavelengths present in a sample.

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