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Suppose we place a chamber \(10.0 \mathrm{cm}\) long with flat parallel windows in one arm of a Michelson Interferometer that is being illuminated by 600 -nm light. If the refractive index of air is 1.00029 and all the air is pumped out of the cell, how many fringe-pairs will shift by in the process?

Short Answer

Expert verified
10 fringe-pairs shift.

Step by step solution

01

Determine the Optical Path Length Difference

First, calculate the difference in optical path length when the chamber is filled with air versus when it is evacuated. The optical path length (OPL) with air is given by the equation: \[ \text{OPL}_{\text{air}} = n \times L \] where \( n = 1.00029 \) is the refractive index of air and \( L = 10.0 \text{ cm} = 0.1 \text{ m} \) is the chamber length. Thus, \[ \text{OPL}_{\text{air}} = 1.00029 \times 0.1 \text{ m} = 0.100029 \text{ m} \].When the chamber is evacuated, the refractive index of the vacuum is 1, so \[ \text{OPL}_{\text{vacuum}} = 1 \times L = 0.1 \text{ m} \].

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Key Concepts

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

Optical Path Length
The optical path length (OPL) is a crucial concept in understanding how light travels through different mediums. It measures the effective length that light travels in a medium, and not just the physical distance. The OPL depends on two factors:
  • The physical distance the light travels.
  • The refractive index of the medium through which it travels.
For example, if a light wave travels through a chamber of length \(L\), the optical path length changes based on the medium inside the chamber. It can be mathematically expressed as \( \text{OPL} = n \times L \), where \(n\) is the refractive index. When light travels through air, as mentioned in the problem, the refractive index \(n\) changes from that of a vacuum, which affects the time and phase of light waves traversing the path.
Understanding OPL helps in determining how changes in media affect light's phase and the behavior of instruments like the Michelson Interferometer.
Refractive Index
The refractive index, often denoted by \(n\), is a dimensionless number that describes how light propagates through a medium. It indicates how much slower light travels in a medium compared to in a vacuum.
Several important aspects of refractive index include:
  • It's greater than 1 for all materials except a vacuum.
  • The speed of light in a medium is given by \(c/n\), where \(c\) is the speed of light in a vacuum.
  • Higher refractive indices mean light travels slower in the medium.
In the problem, air has a refractive index of 1.00029. This slight increase from the refractive index of a vacuum (which is 1) makes an essential difference in the optical path length. By removing air and creating a vacuum, the optical path length changes, leading to observable interference patterns in the Michelson Interferometer. Understanding refractive index is key to predicting how light behaves as it moves through different environments.
Fringe Shift
Fringe shifts are observable changes in interference patterns that occur when the optical path length is altered, like in a Michelson Interferometer. They are a direct measurement of the changes in phase of light waves.
Fringe shifts are important because they quantify the difference in optical path length when a medium changes, such as when you evacuate air from the chamber in the Michelson Interferometer. Here's how it works:
  • Interference patterns form from the superposition of light waves traveling different paths.
  • A shift occurs when the path length changes, altering constructive and destructive interference conditions.
  • In the solution example, the difference in path lengths involves calculating how many wavelengths fit into that difference.
This specific example accounts for the difference when air is displaced, leading to a measurable fringe shift as the light's wavelength relates to its path length in the medium. Understanding fringe shifts allows us to precisely measure small changes in optical path length, essential in optical experiments and applications.

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