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Of the 190 nm wavelength light incident on a 15.0-mm-thick piece of fused silica quartz glass, 35\% passes through the glass and the remainder is absorbed. What percentage of the light will pass through a 35.0 -mm-thick piece of the same glass?

Short Answer

Expert verified
The percentage of the 190 nm wavelength light that will pass through a 35.0 -mm-thick piece of the same fused silica quartz glass is \(7.24\%\).

Step by step solution

01

Identify the relevant information given in the problem

In this problem, we are given the wavelength of light (190 nm), the initial thickness of the glass (15.0 mm), the percentage of light passing through the initial glass thickness (35%), and the new thickness of the glass (35.0 mm).
02

Determine the absorption coefficient of the glass

The relationship between the light transmitted and the absorption coefficient can be described using the Beer-Lambert Law, which states that the transmitted intensity of light (I_t) is related to the initial intensity (I_0) through the equation: \(I_t = I_0 e^{-\alpha d}\) where - \(I_t\) is the transmitted intensity - \(I_0\) is the initial intensity - \(\alpha\) is the absorption coefficient - \(d\) is the thickness of the material We're given the percentage of light passing through the 15-mm thick glass: 35%. That means, \(I_t = 0.35 I_0\). We can use this information to determine the absorption coefficient \(\alpha\).
03

Calculate the absorption coefficient

To determine the absorption coefficient, plug in the given values into the Beer-Lambert Law equation: \(0.35 I_0 = I_0 e^{-\alpha \times 15}\) Dividing both sides by \(I_0\): 0.35 = \(e^{-\alpha \times 15}\) Take the natural logarithm of both sides: \(\ln(0.35) = -\alpha * 15\) Now solve for \(\alpha\): \(\alpha = -\frac{\ln(0.35)}{15}\) Calculate the value of \(\alpha\): \(\alpha \approx 0.0726 \, mm^{-1}\)
04

Calculate the percentage of light passing through the 35-mm thick glass

Now that we have determined the absorption coefficient, we can calculate the percentage of light passing through the 35-mm thick glass using the Beer-Lambert Law equation: \(I_t = I_0 e^{-\alpha d}\) Plug in the values: \(I_t = I_0 e^{-0.0726 \times 35}\) Divide both sides by \(I_0\): \(\frac{I_t}{I_0} = e^{-0.0726 \times 35}\) Calculate the value of \(\frac{I_t}{I_0}\): \(\frac{I_t}{I_0} \approx 0.0724\)
05

Convert the ratio to percentage

To express the result as a percentage, multiply the ratio by 100: Percentage of light passing through the 35-mm thick glass = \(0.0724 \times 100 = 7.24\%\) Thus, 7.24% of the light will pass through a 35.0 -mm-thick piece of the same glass.

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Key Concepts

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

Light Absorption
When light interacts with a material, some of the light's energy is absorbed. This is known as light absorption. In materials science and optics, understanding how a material absorbs light helps predict how much light will pass through it.
Absorption depends on various factors, including the thickness of the material and the wavelength of the light. A thicker material will generally absorb more light than a thinner one. Likewise, the particular characteristics of the material, such as its molecular structure, also play a significant role.
In the context of the Beer-Lambert Law, light absorption occurs exponentially with respect to the thickness of the material. As the thickness increases, the percentage of light passing through decreases significantly. This exponential relationship makes the Beer-Lambert Law a powerful tool in predicting transmitted light intensities in optical materials.
Transmitted Intensity
The transmitted intensity of light refers to how much of the initial light intensity remains after passing through a material. This is often a key measurement in optics and is crucial in applications ranging from sunglasses to scientific sensors.
In the Beer-Lambert Law, the formula for transmitted intensity is given by:
  • \(I_t = I_0 e^{-\alpha d}\)
    • Where:
      • \(I_t\) is the transmitted intensity
      • \(I_0\) is the initial intensity of the light
      • \(\alpha\) is the absorption coefficient
      • \(d\) is the thickness of the material

      This equation illustrates that as light passes through a material, its intensity is reduced exponentially by the factor \(e^{-\alpha d}\). Understanding transmitted intensity helps predict the effectiveness of materials in allowing light to pass through, which is essential in designing optical devices and materials.
Absorption Coefficient
The absorption coefficient \(\alpha\) is a fundamental parameter in optical physics. It quantifies how strongly a material absorbs light at a given wavelength.
The absorption coefficient depends on both the material properties and the frequency (or wavelength) of the incident light. A higher absorption coefficient means that the material is more effective at absorbing light, so less light will be transmitted through a given thickness.
In practical terms, the absorption coefficient is determined by plotting the intensity of light passing through materials of different thicknesses and analyzing the exponential decrease described by the Beer-Lambert Law. By determining this coefficient, scientists and engineers can predict the behavior of light in various applications, such as spectroscopy, optics, and even medical imaging.

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Most popular questions from this chapter

Following Example Problem \(19.5,\) show that the \(J=1 \rightarrow J=2\) rotational transition is allowed.

Selection rules in the dipole approximation are determined by the integral \(\mu_{x}^{m n}=\int \psi_{m}^{*}(\tau) \mu_{x}(\tau) \psi_{n}(\tau) d \tau .\) If this integral is nonzero, the transition will be observed in an absorption spectrum. If the integral is zero, the transition is "forbidden" in the dipole approximation. It actually occurs with low probability because the dipole approximation is not exact. Consider the particle in the one-dimensional box and set \(\mu_{x}=-e x\) a. Calculate \(\mu_{x}^{12}\) and \(\mu_{x}^{13}\) in the dipole approximation. Can you see a pattern and discern a selection rule? You may need to evaluate a few more integrals of the type \(\mu_{x}^{1 \mathrm{m}}\) The standard integral \\[ \begin{array}{c} \int x \sin \left(\frac{\pi x}{a}\right) \sin \left(\frac{n \pi x}{a}\right) d x \\ =\frac{1}{2}\left(\frac{a^{2} \cos \frac{(n-1) \pi x}{a}}{(n-1)^{2} \pi^{2}}+\frac{(n-1) \pi x}{a}\right) \\ -\frac{1}{2}\left(\frac{a^{2} \cos \frac{(n+1) \pi x}{a}}{(n+1)^{2} \pi^{2}}+\frac{a x \sin \frac{(n+1) \pi x}{a}}{(n+1) \pi}\right) \end{array} \\] is useful for solving this problem. b. Determine the ratio \(\mu_{x}^{12} / \mu_{x}^{14} .\) On the basis of your result, would you modify the selection rule that you determined in part (a)?

Show that the Morse potential approaches the harmonic potential for small values of the vibrational amplitude. (Hint: Expand the Morse potential in A Taylor-Maclaurin series.)

Overtone transitions in vibrational absorption spectra for which \(\Delta n=+2,+3, \ldots\) are forbidden for the harmonic potential \(V=(1 / 2) k x^{2}\) because \(\mu_{x}^{m n}=0\) for \(|m-n| \neq 1\) as shown in Section \(19.4 .\) However, overtone transitions are allowed for the more realistic anharmonic potential. In this problem, you will explore how the selection rule is modified by including anharmonic terms in the potential. We do so in an indirect manner by including additional terms in the expansion of the dipole moment \(\mu_{x}\left(x_{e}+x\right)=\mu_{0 x}+x\left(d \mu_{x} / d x\right)_{r_{e}}+\ldots\) but assuming that the harmonic oscillator total energy eigenfunctions are still valid. This approximation is valid if the anharmonic correction to the harmonic potential is small. You will show that including the next term in the expansion of the dipole moment, which is proportional to \(x^{2},\) makes the transitions \(\Delta n=\pm 2\) allowed. a. Show that Equation (19.8) becomes $$\begin{array}{l} \mu_{x}^{m 0}=A_{m} A_{0} \mu_{0 x} \int_{-\infty}^{\infty} H_{m}\left(\alpha^{1 / 2} x\right) H_{0}\left(\alpha^{1 / 2} x\right) e^{-\alpha x^{2}} d x \\ \quad+A_{m} A_{0}\left(\frac{d \mu_{x}}{d x}\right)_{x=0} \int_{-\infty}^{\infty} H_{m}\left(\alpha^{1 / 2} x\right) x H_{0}\left(\alpha^{1 / 2} x\right) e^{-\alpha x^{2}} d x \\ \quad+\frac{A_{m} A_{0}}{2 !}\left(\frac{d^{2} \mu_{x}}{d x^{2}}\right)_{x=0} \int_{-\infty}^{\infty} H_{m}\left(\alpha^{1 / 2} x\right) x^{2} H_{0}\left(\alpha^{1 / 2} x\right) e^{-\alpha x^{2}} d x \end{array}$$ b. Evaluate the effect of adding the additional term to \(\mu_{x}^{m n} .\) You will need the recursion relationship \\[ \alpha^{1 / 2} x H_{n}\left(\alpha^{1 / 2} x\right)=n H_{n-1}\left(\alpha^{1 / 2} x\right)+\frac{1}{2} H_{n+1}\left(\alpha^{1 / 2} x\right) \\] c. Show that both the transitions \(n=0 \rightarrow n=1\) and \(n=0 \rightarrow n=2\) are allowed in this case.

The rigid rotor model can be improved by recognizing that in a realistic anharmonic potential, the bond length increases with the vibrational quantum number \(n\). Therefore, the rotational constant depends on \(n,\) and it can be shown that \(B_{n}=B-(n+1 / 2) \alpha,\) where \(B\) is the rigid rotor value. The constant \(\alpha\) can be obtained from experimental spectra. For \\[ ^{1} \mathrm{H}^{81} \mathrm{Br}, B=8.46488 \mathrm{cm}^{-1} \text {and } \alpha=0.23328 \mathrm{cm}^{-1} . \text {Using this } \\] more accurate formula for \(B_{n},\) calculate the bond length for HBr in the ground state and for \(n=3\)

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