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The threshold wavelength for the photoelectric effect in a specific alloy is \(400 . \mathrm{nm}\). What is the work function in \(\mathrm{eV} ?\)

Short Answer

Expert verified
Answer: The work function of the alloy is 3.1 eV.

Step by step solution

01

Identify given information and constants

The information provided by the exercise is: - Threshold wavelength (\(λ_{threshold}\)) = 400 nm - Planck's constant (\(h\)) = 6.626 x 10^-34 Js - Speed of light (\(c\)) = 3 x 10^8 m/s - Electron charge (\(e\)) = 1.602 x 10^-19 C
02

Convert the threshold wavelength to meters

To work with the threshold wavelength in the equations, we need to have it in meters. So, we will convert the wavelength from nm to meters: \(λ_{threshold} = 400\,\text{nm} \times \frac{1\,\text{m}}{10^9\,\text{nm}} = 4 \times 10^{-7}\,\text{m}\)
03

Calculate the energy when electrons are ejected

Now, we can use Planck's equation to find the energy (\(E\)) needed to eject electrons as: \(E = \frac{h \times c}{λ_{threshold}}\) Substitute the known values into the equation: \(E = \frac{(6.626 \times 10^{-34}\,\text{Js}) \times (3 \times 10^8\,\text{m/s})}{(4 \times 10^{-7}\,\text{m})} = 4.9695 \times 10^{-19}\,\text{J}\)
04

Convert the energy into electron volts

To find the energy in electron volts (eV), we will divide the energy in joules by the electron charge: \(E_{eV} = \frac{E}{e} = \frac{4.9695 \times 10^{-19}\,\text{J}}{1.602 \times 10^{-19}\,\text{C}} = 3.1\,\text{eV}\)
05

Find the work function

The work function is the minimum energy required to eject electrons, and in this case, it is equal to the calculated energy in electron volts: Work function = \(E_{eV} = 3.1\,\text{eV}\) Hence, the work function of the specific alloy is \(3.1\,\text{eV}\).

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Key Concepts

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

Threshold Wavelength
The photoelectric effect involves understanding the concept of a **threshold wavelength**. This is the specific wavelength of light at which electrons begin to be ejected from a material's surface due to the absorption of photons. If the wavelength of the incident light is longer than the threshold wavelength, no electrons will be emitted. Conversely, if the wavelength is shorter, electrons are emitted.

The relationship between the wavelength of the light and its energy is fundamental: shorter wavelengths correspond to higher energy photons. This can be calculated using the formula:
  • \( E = \frac{h \times c}{\lambda_{threshold}} \)
where \( E \) is energy in joules, \( h \) is Planck's constant, \( c \) is the speed of light, and \( \lambda_{threshold} \) is the threshold wavelength.
In our example, the threshold wavelength was given as 400 nm, which when converted to meters becomes \( 4 \times 10^{-7} \) m. This is a typical calculation to determine the start of electron emission in the photoelectric effect.
Work Function
The **work function** emerges as a key term when discussing the photoelectric effect. It represents the minimum energy needed to remove an electron from a solid's surface. This energy is unique to each material and depends on its electronic structure.

When we say the work function, we often express it in electron volts (eV). One electron volt is the energy gained by an electron when it is accelerated through one volt of electric potential. The work function can be calculated using the energy determined by threshold wavelength:
  • First, find the energy (in joules) using Planck's equation: \( E = \frac{h \times c}{\lambda} \).
  • Then convert the result from joules to electron volts by dividing by the electron charge: \( E_{eV} = \frac{E}{e} \).
In the given problem, this energy was found to be \( 3.1 \, \text{eV} \), indicating the minimum energy required to eject an electron from the alloy's surface with the given threshold wavelength of light.
Planck's Constant
Understanding **Planck's constant** is crucial when analyzing the photoelectric effect. This fundamental constant plays a central role in quantum mechanics, as it relates the energy of photons to their frequency. Planck's equation, \( E = h \times f \), shows how Planck's constant \( h \) bridges the gap between wave and particle nature of light.

Planck's constant has a value of \( 6.626 \times 10^{-34} \, \text{Js} \), where \( J \) stands for joules and \( s \) for seconds. It appears in equations related to both the threshold wavelength and the energy calculations in electron ejection scenarios:
  • Through the formula \( E = \frac{h \times c}{\lambda_{threshold}} \), it helps calculate the energy of the photon at the threshold wavelength.
Its small magnitude points to the incredibly minuscule scale of quantum effects, where even tiny energies correspond to sizable effects at the atomic or subatomic levels. This reinforces how Planck's constant is a pivot in understanding and predicting the behavior of electrons in materials subjected to electromagnetic radiation.

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Most popular questions from this chapter

Scintillation detectors for gamma rays transfer the energy of a gamma-ray photon to an electron within a crystal, via the photoelectric effect or Compton scattering. The electron transfers its energy to atoms in the crystal, which re-emit it as a light flash detected by a photomultiplier tube. The charge pulse produced by the photomultiplier tube is proportional to the energy originally deposited in the crystal; this can be measured so an energy spectrum can be displayed. Gamma rays absorbed by the photoelectric effect are recorded as a photopeak in the spectrum, at the full energy of the gammas. The Compton-scattered electrons are also recorded, at a range of lower energies known as the Compton plateau. The highest-energy of these form the Compton edge of the plateau. Gamma-ray photons scattered \(180 .^{\circ}\) by the Compton effect appear as a backscatter peak in the spectrum. For gamma-ray photons of energy \(511 \mathrm{KeV}\) calculate the energies of the Compton edge and the backscatter peak in the spectrum.

X-rays of wavelength \(\lambda=0.120 \mathrm{nm}\) are scattered from carbon. What is the Compton wavelength shift for photons detected at \(90.0^{\circ}\) angle relative to the incident beam?

Ultra-high-energy gamma rays are found to come from the Equator of our galaxy, with energies up to \(3.5 \cdot 10^{12} \mathrm{eV}\). What is the wavelength of this light? How does the energy of this light compare to the rest mass of a proton?

The existence of a cutoff frequency in the photoelectric effect a) cannot be explained using classical physics. b) shows that the model provided by classical physics is not correct in this case. c) shows that a photon model of light should be used in this case. d) shows that the energy of the photon is proportional to its frequency. e) All of the above.

After you told him about de Broglie's hypothesis that particles of momentum \(p\) have wave characteristics with wavelength \(\lambda=h / p\), your 60.0 -kg roommate starts thinking of his fate as a wave and asks you if he could be diffracted when passing through the 90.0 -cm-wide doorway of your dorm room. a) What is the maximum speed at which your roommate can pass through the doorway in order to be significantly diffracted? b) If it takes one step to pass through the doorstep, how long should it take your roommate to make that step (assume the length of his step is \(0.75 \mathrm{~m}\) ) in order for him to be diffracted? c) What is the answer to your roommate's question? Hint: Assume that significant diffraction occurs when the width of the diffraction aperture is less that 10.0 times the wavelength of the wave being diffracted.

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