/*! 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 42 A semiconductor is struck by lig... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

A semiconductor is struck by light of slowly increasing frequency and begins to conduct when the wavelength of the light is \(580 \mathrm{nm}\); estimate the size of the energy gap \(E_{\mathrm{g}}\)

Short Answer

Expert verified
The energy gap \(E_g\) is approximately \(2.14 \, \text{eV}\).

Step by step solution

01

Understand the problem

You are asked to estimate the energy gap (\(E_g\)) of a semiconductor when it begins to conduct upon being struck by light with a wavelength of \(580 \, \text{nm}\). This is related to the energy of the photons corresponding to this wavelength.
02

Recall the formula for energy of a photon

The energy of a photon is calculated 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 \((3 \times 10^8 \, \text{m/s})\), and \(\lambda\) is the wavelength of the light.
03

Convert the wavelength to meters

The wavelength given is \(580 \, \text{nm}\), which needs to be converted to meters.\[ 580 \, \text{nm} = 580 \times 10^{-9} \, \text{m} \]
04

Calculate the energy of the photon

Substitute the values into the formula to find the energy of the photon.\[ E = \frac{6.626 \times 10^{-34} \, \text{J s} \times 3 \times 10^8 \, \text{m/s}}{580 \times 10^{-9} \, \text{m}} \approx 3.43 \times 10^{-19} \, \text{J} \]
05

Convert energy from joules to electronvolts

Since energy in semiconductors is commonly expressed in electronvolts (eV), convert the energy from joules to eV using the conversion factor \(1 \, \text{eV} = 1.602 \times 10^{-19} \, \text{J}\).\[ E \approx \frac{3.43 \times 10^{-19} \, \text{J}}{1.602 \times 10^{-19} \, \text{J/eV}} \approx 2.14 \, \text{eV} \]
06

Conclusion

The energy gap \(E_g\) of the semiconductor, where it starts to conduct, is approximately \(2.14 \, \text{eV}\).

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

Key Concepts

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

Photon Energy
Photon energy is a fundamental concept in understanding how light interacts with matter, especially in semiconductors. When light photons hit a semiconductor, their energy can be absorbed, causing electrons in the material to jump across the energy gap, known as the band gap. This movement of electrons allows the material to conduct electricity.
To calculate the energy of a photon, we use the formula:
  • \(E = \frac{hc}{\lambda}\)
where:
  • \(E\) stands for energy
  • \(h\) is Planck’s constant \((6.626 \times 10^{-34} \, \text{Js})\)
  • \(c\) is the speed of light \((3 \times 10^8 \, \text{m/s})\)
  • \(\lambda\) is the wavelength of light
In our specific problem, the wavelength was given as \(580 \, \text{nm}\), which must be converted into meters for the formula to work. Therefore, the calculation involves plugging in these values to determine the exact energy of the incoming photons. This energy is crucial as it correlates directly to the semiconductor's band gap.
Planck's Constant
Planck's constant is a key constant in quantum mechanics that relates the energy of a photon to its frequency. This constant is important because it helps describe the quantization of energy in electromagnetic waves.
Planck's constant, denoted as \(h\), has the value of \(6.626 \times 10^{-34} \, \text{Js}\). This small number illustrates just how tiny the energy packets (quanta) are at the atomic and subatomic levels.
In the context of semiconductors, Planck's constant allows us to calculate how much energy is associated with each photon of light that hits the material. It forms part of the equation \(E = hf\), where \(f\) is the frequency of the light. However, when dealing with wavelength instead, the equation becomes \(E = \frac{hc}{\lambda}\), simplifying the calculation for wavelengths when you know the speed of light \(c\) and wavelength \(\lambda\).
  • Planck's constant bridges the concepts of frequency and energy in photon calculations.
  • Its use in semiconductor physics is essential to understanding and predicting the behavior of light-matter interactions.
Conversion from Joules to Electronvolts
Energy in physics can often be expressed in different units. When working with semiconductors, energy levels are typically described in electronvolts (eV) instead of joules. This is because the electronvolt is a more convenient unit for the scale of energy commonly dealt with in semiconductor physics.
The conversion between these units involves the conversion factor:
  • \(1 \, \text{eV} = 1.602 \times 10^{-19} \, \text{J}\)
To convert energy from joules to electronvolts, you divide the energy in joules by this conversion factor. In the given problem, the energy calculated was \(3.43 \times 10^{-19} \, \text{J}\). Converting this energy into electronvolts gives us approximately \(2.14 \, \text{eV}\).
  • Electronvolts make it easier to communicate and understand energy changes at the atomic level.
  • This conversion is essential for comparing experimental results with theoretical predictions in material science.
  • Understanding this conversion allows for a more intuitive grasp of the energies involved in semiconductors and other small-scale systems.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

(II) (a) For copper at room temperature \((T=293 \mathrm{K})\) , calculate the Fermi factor, Eq. \(14,\) for an electron with energy 0.12 \(\mathrm{eV}\) above the Fermi energy. This represents the probability that this state is occupied. Is this reasonable? (b) What is the probability that a state 0.12 \(\mathrm{eV}\) below the Fermi energy is occupied? (c) What is the probability that the state in part \((b)\) is unoccupied? \(f(E)=\frac{1}{e^{\left(E-E_{\mathrm{F}}\right) / k T}+1}\)

(II) Show that the probability for the state at the Fermi energy being occupied is exactly \(\frac{1}{2}\) , independent of temperature.

(1I) For a one-dimensional potential well of width \(\ell,\) start with \(E=n^{2} \frac{h^{2}}{8 m \ell^{2}}, \quad n=1,2,3, \cdots\) and show that the number of states per unit energy interval for an electron gas is given by \(g_{\ell}(E)=\sqrt{\frac{8 m \ell^{2}}{h^{2} E}}\) Remember that there can be two electrons (spin up and spin down) for each value of \(n .[\) Hint. Write the quantum number \(n\) in terms of \(E .\) Then \(g_{t}(E)=2 d n / d E\) where \(d n\) is the number of energy levels between \(E\) and \(E+d E . ]\)

Use the uncertainty principle to estimate the binding energy of the \(\mathrm{H}_{2}\) molecule by calculating the difference in kinetic energy of the electrons between when they are in separate atoms and when they are in the molecule. Take \(\Delta x\) for the electrons in the separated atoms to be the radius of the first Bohr orbit, \(0.053 \mathrm{nm},\) and for the molecule take \(\Delta x\) to be the separation of the nuclei, 0.074 \(\mathrm{nm} .\) [Hint: Let \(\Delta p \approx \Delta p_{x} .\)

Show that the probability for the state at the Fermi energy being occupied is exactly \(\frac{1}{2}\), independent of temperature.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.