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The mean kinetic energy of thermal neutrons is given by \(3 k T / 2\), where \(k\) is Boltzmann's constant and \(T\) is their absolute temperature. Calculate the mean De Broglie wavelength of neutrons at room temperature \(\left(27^{\circ} \mathrm{C}\right)\).

Short Answer

Expert verified
The mean De Broglie wavelength of neutrons at room temperature is approximately 1.81 × 10^-10 m.

Step by step solution

01

Convert Temperature to Kelvin

The given temperature is 27°C. To convert to Kelvin, use the formula: \[ T(K) = T(°C) + 273.15 \] Thus, the temperature in Kelvin is: \[ T = 27 + 273.15 = 300.15 \, K \]
02

Calculate Kinetic Energy

The mean kinetic energy of the neutrons is given by the formula: \[ KE = \frac{3}{2} k T \] Where \( k = 1.38 \times 10^{-23} \, J/K \) is Boltzmann's constant. Substituting the values, we get the kinetic energy:\[ KE = \frac{3}{2} \times 1.38 \times 10^{-23} \times 300.15 \approx 6.2073 \times 10^{-21} \, J \]
03

Relate Kinetic Energy to Velocity

Kinetic energy is also given by: \[ KE = \frac{1}{2} m v^2 \] Equating and solving for velocity:\[ \frac{3}{2} k T = \frac{1}{2} m v^2 \rightarrow v^2 = \frac{3kT}{m} \rightarrow v = \sqrt{\frac{3kT}{m}} \]
04

Calculate the Mass of a Neutron

The mass of a neutron \( m \) is approximately \( 1.675 \times 10^{-27} \, kg \). We will use this value in our calculations.
05

Calculate Neutron Velocity

Substitute the values into the velocity equation:\[ v = \sqrt{\frac{3 \times 1.38 \times 10^{-23} \times 300.15}{1.675 \times 10^{-27}}} \approx 2190 \, m/s \]
06

Calculate the De Broglie Wavelength

De Broglie wavelength \( \lambda \) is given by:\[ \lambda = \frac{h}{mv} \] Where \( h = 6.626 \times 10^{-34} \, Js \) is Planck's constant. Substitute the values:\[ \lambda = \frac{6.626 \times 10^{-34}}{1.675 \times 10^{-27} \times 2190} \approx 1.81 \times 10^{-10} \, m \]

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Key Concepts

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

Thermal Neutrons
Thermal neutrons are fascinating particles that move at velocities typical of gases at room temperature. These neutrons are neither too fast nor too slow, but just perfect for carrying out numerous nuclear reactions. They have energies still comparable to the thermal motion of atoms in a substance at room temperature, usually around 0.025 electron volts (eV).

Their importance cannot be overstated as they play a crucial role in nuclear reactors and neutron scattering experiments. Due to their particular energy levels, thermal neutrons are exceptionally adept at inducing fission in certain isotopes, which is critical for sustaining nuclear reactions.
  • Energy Level: comparable to thermal motion of atoms in a substance
  • Velocities: similar to average gas molecules at the same temperature
  • Applications: vital in nuclear reactors and scientific research
Kinetic Energy
Kinetic energy is a fundamental concept that describes the energy of motion. For thermal neutrons, their average kinetic energy is determined by the temperature of the surrounding environment, particularly through the formula \( KE = \frac{3}{2} k T \), where \( k \) is the Boltzmann constant and \( T \) is the temperature in Kelvin.

This formula helps us see that as the temperature increases, so does the kinetic energy of the neutrons. The kinetic energy is vital since it correlates directly with how fast these neutrons move, which can be calculated further by relating it to the velocity equation \( KE = \frac{1}{2} m v^2 \). Understanding kinetic energy in neutrons allows us to grasp how these particles behave under various thermal conditions.
  • Relates motion to temperature
  • Determines how fast particles move
  • Critical in calculating other related properties like velocity
Planck's Constant
Planck's constant \( h \) is a fundamental value in physics that connects the energy of a photon to its frequency. Defined as \( h = 6.626 \times 10^{-34} \, \text{Js} \), it is crucial in the calculation of the De Broglie wavelength, linking the properties of particles to wave behavior.

In the realm of quantum mechanics, Planck's constant plays an integral role in the formula \( \lambda = \frac{h}{mv} \), where it helps determine the wavelength associated with particles like neutrons. Its small value helps to bridge the understanding of how microscopic particles, like thermal neutrons, can also exhibit wave-like behavior, a key aspect of wave-particle duality.
  • Relates energy to frequency of photons
  • Central to wave-particle duality
  • Essential for calculating wavelengths of particles
Room Temperature
Room temperature is a common reference point in scientific experiments and calculations, typically considered to be around 25°C or 298 K. For thermal neutrons and various calculations in physics, it's important to convert this temperature to Kelvin, providing consistency for physics equations.

At room temperature, several properties of materials and particles, including neutrons, can be predicted. By converting the room temperature to Kelvin using \( T(K) = T(°C) + 273.15 \), physicists and students alike ensure they are working within a universal framework, helping to standardize scientific discourse and findings.
  • Baseline for many scientific experiments
  • Standardized measure in Kelvin for consistency
  • Influences particle energy and behavior
Neutron Velocity
Neutron velocity refers to the speed at which a neutron moves, greatly influenced by its kinetic energy and mass. By using the equation \( v = \sqrt{\frac{3kT}{m}} \), we can determine the velocity of thermal neutrons. Here, \( m \) is the neutron's mass, while \( kT \) represents the kinetic energy at a given temperature.

Understanding the velocity helps in predicting how neutrons will interact with matter. Their speed plays a critical role in nuclear reactions and other applications where their path and time of flight are essential to results.
  • Dependent on kinetic energy and mass
  • Key factor in nuclear reactions and material interactions
  • Use equation to derive exact velocity values

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Most popular questions from this chapter

A beam of \(0.1 \mathrm{~nm}\) X-rays is reflected from a crystal at a glancing angle of \(10.3^{\circ}\). Calculate the spacing between the reflecting crystal planes.

Calculate the fractional change in the photon energy as a result of Compton scattering through an angle of \(90^{\circ}\) for photons of: a. X-rays with a wavelength of \(0.025 \mathrm{~nm}\); b. \(\quad y\) rays with an energy of \(1 \mathrm{MeV}\).

A \(100 \mathrm{~mW}\) argon laser emits a beam of light of wavelength \(488 \mathrm{~nm}\) in vacuo. a. How many photons does the laser emit each second b. What current will flow through a photoelectric cell whose cathode (emitting. plate) is illuminated by the laser's light beam if \(10 \%\) of the photons release an electron from it. c. What potential will be required between the cell's electrodes in order to stop the current, if the threshold frequency of the cathode is \(5.2 \cdot 10^{14} \mathrm{~Hz}\).

The spacing between adjacent parallel planes in a crystal is \(0.3 \mathrm{~nm}\). Calculate the smallest glancing angle at which Bragg diffraction will be observed with radiation of wavelength \(0.3 \AA\).

The frequency, \(f\), of a harmonic oscillator of mass \(m\) and elasticity constant \(k\) is given by the equation \(f=\frac{1}{2 \pi} \sqrt{k / m}\). The energy of the oscillator is given by \(E=p^{2} / 2 m+k x^{2} / 2\), where \(p\) is the system's linear momentum and \(x\) is the displacement from its equilibrium position. Use the uncertainty principle, \(\Delta x \cdot \Delta p \approx \hbar / 2\), to express the oscillator's energy \(E\) in terms of \(x\) and show, by taking the derivative of this function and setting \(d E / d x=0\), that the minimum energy of the oscillator (its ground state energy) is \(E_{\min }=h f / 2\).

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