/*! 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 12 (a) What is the minimum potentia... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

(a) What is the minimum potential difference between the filament and the target of an x-ray tube if the tube is to produce x rays with a wavelength of \(0.150 \mathrm{nm} ?\) (b) What is the shortest wavelength produced in an x-ray tube operated at \(30.0 \mathrm{kV} ?\)

Short Answer

Expert verified
For part (a), the minimum potential difference between the filament and the target of an x-ray tube is approximately 8273 V or 8.27 kV. For part (b), the shortest wavelength produced in an x-ray tube operated at 30.0 kV is approximately 0.041 nm.

Step by step solution

01

Determine the minimum potential difference

The Planck-Einstein relation is given as \(E = hf\) where h is the Planck constant (approximately \(6.63 × 10^-34 m^{2} kg/s)\) and f is frequency. As frequency=Wavelength, you can rearrange the equation as \(E = \frac{hc}{λ}\). In the given problem, wavelength (\(λ\)) is 0.150 nm or 0.150 × \(10^-9\) m. Plug in the known values and solve for E, which is the energy of the photon.
02

Translate photon energy into voltage

In order to find the potential difference, you have to convert the energy of the photon into electron volts, as 1 eV is equivalent to 1.602 × \(10^-19\) J. Therefore, the minimum potential difference (V) can be given as \(E = eV\). Solving for V gives \(V = \frac{E}{e}\). Lastly, plug in the known values and solve for V.
03

Determine the shortest wavelength

Again start with the formula \(E = \frac{hc}{λ}\) but this time solve for the wavelength (\(λ\)). Given the potential difference (V) which is 30.0 kV or \(30.0 × 10^{3}\) V and using the relation \(E = eV\), you can calculate the energy (E). Finally, substituting the obtained value of E in the formula to solve for \(λ\) will give us the shortest wavelength.

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.

Planck-Einstein Relation
The Planck-Einstein relation is a fundamental concept in quantum physics, establishing the connection between the energy of a photon and its frequency. This relationship is encapsulated in the equation \( E = hf \), where \( E \) is the photon's energy, \( h \) is the Planck constant which is approximately \( 6.63 \times 10^{-34} \, \text{m}^2 \text{kg/s} \) and \( f \) is the frequency of the photon. Since the speed of light \( c \) is equal to the product of the frequency and the wavelength ( \( f = \frac{c}{\lambda} \) ), we can rearrange the equation to \( E = \frac{hc}{\lambda} \) by substituting for \( f \). This equation tells us that energy is inversely proportional to the wavelength, meaning that the shorter the wavelength, the higher the energy of the photon.

Photon Energy Conversion
Once the energy of a photon is determined using the Planck-Einstein relation, it's often useful to convert this energy into a more recognizable unit, such as electron volts (eV). The conversion is important because in the context of x-ray tubes and other electronic devices, energy levels are typically expressed in eV. One electron volt (1 eV) is defined as the amount of kinetic energy gained or lost by a single electron moving across an electric potential difference of one volt. It is numerically equivalent to \( 1.602 \times 10^{-19} \, \text{J} \). By using the relationship \( E = eV \) where \( E \) is the energy in joules and \( e \) is the elementary charge, you can calculate the potential difference that corresponds to a certain photon energy.

Minimum Potential Difference
In an x-ray tube, the minimum potential difference required to produce x-rays of a specific wavelength can be determined using the insights from the Planck-Einstein relation and the concept of photon energy conversion. By rearranging the equation \( E = \frac{hc}{\lambda} \) to solve for potential difference \( V \) and then multiplying by the elementary charge \( e \) to convert to electron volts, you get \( V = \frac{E}{e} \). This calculation reveals the minimum voltage that must be applied between the anode and cathode of the x-ray tube to yield x-rays of the desired wavelength. Real-world applications of this calculation are critical in medical imaging and material science where precise control of x-ray wavelengths is required.

Shortest Wavelength Calculation
The shortest wavelength that can be produced by an x-ray tube is determined by the maximum energy that can be imparted to the photons, which in turn is limited by the maximum voltage of the tube. Using the formula \( E = eV \) where \( V \) is the voltage applied to the x-ray tube, you can calculate the maximum energy of the emitted photons. Then, using the relation \( E = \frac{hc}{\lambda} \), you solve for the shortest possible wavelength \( \lambda \) by rearranging to \( \lambda = \frac{hc}{E} \). This gives us the theoretical limit for the shortest wavelength an x-ray tube can produce, which is essential for applications demanding high-resolution imaging or detailed spectral analysis.

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

In developing night-vision equipment, you need to measure the work function for a metal surface, so you perform a photoelectric-effect experiment. You measure the stopping potential \(V_{0}\) as a function of the wavelength \(\lambda\) of the light that is incident on the surface. You get the results in the table. $$ \begin{array}{l|llllll} \boldsymbol{\lambda}(\mathbf{n m}) & 100 & 120 & 140 & 160 & 180 & 200 \\ \hline \boldsymbol{V}_{0}(\mathbf{V}) & 7.53 & 5.59 & 3.98 & 2.92 & 2.06 & 1.43 \end{array} $$ In your analysis, you use \(c=2.998 \times 10^{8} \mathrm{~m} / \mathrm{s}\) and \(e=1.602 \times 10^{-19} \mathrm{C}\) which are values obtained in other experiments. (a) Select a way to plot your results so that the data points fall close to a straight line. Using that plot, find the slope and \(y\) -intercept of the best-fit straight line to the data. (b) Use the results of part (a) to calculate Planck's constant \(h\) (as a test of your data) and the work function (in eV) of the surface. (c) What is the longest wavelength of light that will produce photoelectrons from this surface? (d) What wavelength of light is required to produce photoelectrons with kinetic energy \(10.0 \mathrm{eV} ?\)

Consider Compton scattering of a photon by a moving electron. Before the collision the photon has wavelength \(\lambda\) and is moving in the \(+x\) -direction, and the electron is moving in the \(-x\) -direction with total energy \(E\) (including its rest energy \(m c^{2}\) ). The photon and electron collide head-on. After the collision, both are moving in the \(-x\) -direction (that is, the photon has been scattered by \(180^{\circ}\) ). (a) Derive an expression for the wavelength \(\lambda^{\prime}\) of the scattered photon. Show that if \(E \gg m c^{2}\), where \(m\) is the rest mass of the electron, your result reduces to $$ \lambda^{\prime}=\frac{h c}{E}\left(1+\frac{m^{2} c^{4} \lambda}{4 h c E}\right) $$ (b) A beam of infrared radiation from a \(\mathrm{CO}_{2}\) laser \((\lambda=10.6 \mu \mathrm{m})\) collides head-on with a beam of electrons, each of total energy \(E=10.0 \mathrm{GeV}\left(1 \mathrm{GeV}=10^{9} \mathrm{eV}\right) .\) Calculate the wavelength \(\lambda^{\prime}\) of the scattered photons, assuming a \(180^{\circ}\) scattering angle. (c) What kind of scattered photons are these (infrared, microwave, ultraviolet, etc.)? Can you think of an application of this effect?

A photon with wavelength \(\lambda=0.1385 \mathrm{nm}\) scatters from an electron that is initially at rest. What must be the angle between the direction of propagation of the incident and scattered photons if the speed of the electron immediately after the collision is \(8.90 \times 10^{6} \mathrm{~m} / \mathrm{s} ?\)

We can estimate the number of photons in a room using the following reasoning: The intensity of the sun's rays at the earth's surface is roughly \(1000 \mathrm{~W} / \mathrm{m}^{2}\). A typical room is illuminated by indirect light or by light bulbs so that its light intensity is some fraction of that value. (a) Estimate the intensity of the light that enters your room. (b) Model the light as entering uniformly at the ceiling and exiting uniformly at the floor. Estimate the area \(A\) of the floor and ceiling, and the height \(H\) of your room. (c) Estimate how long it takes light to travel from the ceiling to the floor of your room by dividing \(H\) by the speed of light. (d) Estimate the total power of the light that enters your room \(P\) by multiplying your estimated intensity \(I\) by the area of your ceiling \(A\). (e) Estimate the total light energy in your room \(E_{\text {room }}\) by multiplying the power \(P\) by the length of time it takes light to travel from ceiling to floor. (f) An average wavelength for light is in the middle of the visible spectrum, at roughly \(500 \mathrm{nm}\). What is the energy of a \(500 \mathrm{nm}\) photon? (g) The total number of photons in your room \(N\) is the ratio of the energy \(E_{\text {room }}\) to the energy per photon. What is your estimate for \(N ?\)

An ultrashort pulse has a duration of \(9.00 \mathrm{fs}\) and produces light at a wavelength of \(556 \mathrm{nm}\). What are the momentum and momentum uncertainty of a single photon in the pulse?

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.