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The silicon-silicon single bond that forms the basis of the mythical silicon- based creature the Horta has a bond strength of 3.80 eV. What wavelength of photon would you need in a (mythical) phasor disintegration gun to destroy the Horta?

Short Answer

Expert verified
The required wavelength is 326.5 nm.

Step by step solution

01

Understanding the Problem

To solve this problem, we need to calculate the wavelength of a photon that has the same energy as the silicon-silicon bond strength, which is given as 3.80 eV. We will use the energy-wavelength relationship in physics that relates the energy of a photon to its wavelength.
02

Convert Energy from eV to Joules

The energy given is in electronvolts (eV). To use it with the wavelength formula, we first need to convert it to joules since 1 eV = 1.602 x 10^-19 J. Thus, the energy in joules is calculated as follows:\[ E = 3.80 \, \text{eV} \times 1.602 \times 10^{-19} \, \text{J/eV} = 6.088 \times 10^{-19} \, \text{J} \]
03

Use the Photon Energy Formula

The energy of a photon can be expressed using the formula: \[ E = \frac{hc}{\lambda} \] where \( h \) is Planck's constant (\( 6.626 \times 10^{-34} \, \text{Js} \)), \( c \) is the speed of light (\( 3.00 \times 10^8 \, \text{m/s} \)), and \( \lambda \) is the wavelength. We need to solve for \( \lambda \).
04

Rearrange the Formula to Solve for Wavelength

Rearrange the energy formula to find \( \lambda \): \[ \lambda = \frac{hc}{E} \] Substitute the values for \( h \), \( c \), and \( E \) into the formula to find \( \lambda \).
05

Substitute Values and Calculate Wavelength

Substitute the known values into the rearranged formula to find the wavelength:\[ \lambda = \frac{6.626 \times 10^{-34} \, \text{Js} \times 3.00 \times 10^8 \, \text{m/s}}{6.088 \times 10^{-19} \, \text{J}} \] \[ \lambda = \frac{1.9878 \times 10^{-25}}{6.088 \times 10^{-19}} \, \text{m} = 3.265 \times 10^{-7} \, \text{m} \]Convert the answer to nanometers (1 m = 10^9 nm):\[ \lambda = 326.5 \, \text{nm} \]
06

Conclusion: Interpret the Result

The wavelength of photon required to disintegrate a silicon-silicon single bond with an energy of 3.80 eV is approximately 326.5 nm. This wavelength falls in the ultraviolet range of the electromagnetic spectrum.

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Key Concepts

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

Wavelength Calculation
Calculating the wavelength of a photon involves understanding the relationship between energy and wavelength. This relationship can be described using the formula:
\[ E = \frac{hc}{\lambda} \]where:
  • \( E \) is the energy of the photon (in joules).
  • \( h \) is Planck's constant, approximately \( 6.626 \times 10^{-34} \text{Js} \).
  • \( c \) is the speed of light, which is approximately \( 3.00 \times 10^8 \text{m/s} \).
  • \( \lambda \) is the wavelength that we need to find (in meters).
To find the wavelength with the given photon energy, rearrange the equation to solve for \( \lambda \):
\[ \lambda = \frac{hc}{E} \]By placing the correct values into this formula, we can calculate the wavelength of a photon based on its energy.
Silicon-Silicon Bond
Silicon is known to form a wide array of compounds, prominently getting into bonds with other silicon atoms. The silicon-silicon bond is significant in various chemical reactions and structures.
In the given problem, the strength of a silicon-silicon single bond is given as 3.80 eV. An important aspect to note is that bond strength refers to the energy required to break a bond between atoms.
Silicon bonds are integral to the structure of many materials, most notably in semiconductors and synthetic materials. The energy value indicates how much energy, typically in the form of photons, is needed to disrupt this connection.
Understanding this helps comprehend the various technological applications of silicon, including integrated circuits and other electronic devices.
Ultraviolet Light
Ultraviolet (UV) light is part of the electromagnetic spectrum with wavelengths shorter than visible light.
Typically ranging from about 10 nm to 400 nm, UV light lies just beyond the violet end of visible light and is divided into several subcategories based on their wavelength.
  • UVA (320-400 nm): This range is closest to visible light and can penetrate deeper into materials.
  • UVB (290-320 nm): It is more energetic than UVA and is responsible for causing sunburn.
  • UVC (100-290 nm): This type is mostly absorbed by the Earth's atmosphere and is not commonly encountered in nature.
A photon with a wavelength of 326.5 nm, as calculated in the example, falls into the UVA range of ultraviolet light, indicating its capability to sever strong molecular bonds like those in silicon-silicon bonds. Understanding this can help harness UV light for material applications where specific reactions or bond disruptions are desirable.

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Most popular questions from this chapter

A 10.0-g marble is gently placed on a horizontal tabletop that is 1.75 m wide. (a) What is the maximum uncertainty in the horizontal position of the marble? (b) According to the Heisenberg uncertainty principle, what is the minimum uncertainty in the horizontal velocity of the marble? (c) In light of your answer to part (b), what is the longest time the marble could remain on the table? Compare this time to the age of the universe, which is approximately 14 billion years. (\(Hint\): Can you know that the horizontal velocity of the marble is \(exactly\) zero?)

The radii of atomic nuclei are of the order of 5.0 \(\times\) 10\(^{-15}\) m. (a) Estimate the minimum uncertainty in the momentum of an electron if it is confined within a nucleus. (b) Take this uncertainty in momentum to be an estimate of the magnitude of the momentum. Use the relativistic relationship between energy and momentum, Eq. (37.39), to obtain an estimate of the kinetic energy of an electron confined within a nucleus. (c) Compare the energy calculated in part (b) to the magnitude of the Coulomb potential energy of a proton and an electron separated by 5.0 \(\times\) 10\(^{-15}\) m. On the basis of your result, could there be electrons within the nucleus? (\(Note\): It is interesting to compare this result to that of Problem 39.72.)

(a) An atom initially in an energy level with \(E\) = -6.52 eV absorbs a photon that has wavelength 860 nm. What is the internal energy of the atom after it absorbs the photon? (b) An atom initially in an energy level with \(E\) = -2.68 eV emits a photon that has wavelength 420 nm. What is the internal energy of the atom after it emits the photon?

For crystal diffraction experiments (discussed in Section 39.1), wavelengths on the order of 0.20 nm are often appropriate. Find the energy in electron volts for a particle with this wavelength if the particle is (a) a photon; (b) an electron; (c) an alpha particle (\(m\) = 6.64 \(\times\) 10\(^{-27}\) kg).

Consider a particle with mass m moving in a potential \(U = {1\over2} kx^2\), as in a mass-spring system. The total energy of the particle is \(E = (p^2/2m) + 12 kx^2\). Assume that \(p\) and \(x\) are approximately related by the Heisenberg uncertainty principle, so \(px \approx h\). (a) Calculate the minimum possible value of the energy \(E\), and the value of \(x\) that gives this minimum E. This lowest possible energy, which is not zero, is called the \(zero-point \space energy\). (b) For the \(x\) calculated in part (a), what is the ratio of the kinetic to the potential energy of the particle?

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