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What (a) frequency, (b) photon energy, and (c) photon momentum magnitude (in \(\mathrm{keV} / \mathrm{c}\) ) are associated with \(\mathrm{x}\) rays having wavelength \(35.0 \mathrm{pm}\) ?

Short Answer

Expert verified
Frequency: \(8.57 \times 10^{18} \ \mathrm{Hz}\), Energy: \(35.4 \ \mathrm{keV}\), Momentum: \(35.4 \ \mathrm{keV}/c\).

Step by step solution

01

Convert Wavelength to Frequency

First, we need to convert the given wavelength of the x-ray into frequency. We use the equation \( u = \frac{c}{\lambda} \), where \( u \) is the frequency, \( c \) is the speed of light \((3.00 \times 10^8 \mathrm{\ m/s})\), and \( \lambda \) is the wavelength. Here the wavelength \( \lambda = 35.0 \mathrm{\ pm} = 35.0 \times 10^{-12} \mathrm{\ m} \). Calculate \( u = \frac{3.00 \times 10^8}{35.0 \times 10^{-12}} \approx 8.57 \times 10^{18} \mathrm{\ Hz}\).
02

Calculate Photon Energy

Now calculate the photon energy using \( E = h u \), where \( h \) is Planck’s constant \((6.626 \times 10^{-34} \mathrm{\ J \cdot s}) \) and \( u \) is the frequency found in Step 1. Substitute \( u = 8.57 \times 10^{18} \mathrm{\ Hz}\). Calculating gives \( E = 6.626 \times 10^{-34} \times 8.57 \times 10^{18} \approx 5.68 \times 10^{-15} \mathrm{\ J} \). Convert energy from joules to electron volts (eV; \(1 \ \mathrm{eV} = 1.602 \times 10^{-19} \mathrm{\ J})\): \( 5.68 \times 10^{-15} \mathrm{\ J} \times \frac{1 \mathrm{\ eV}}{1.602 \times 10^{-19} \mathrm{\ J}} \approx 35406 \mathrm{\ eV} = 35.4 \mathrm{\ keV} \).
03

Calculate Photon Momentum

Finally, find the momentum of the photon. We use the formula for momentum \( p = \frac{E}{c} \), where \( E \) is the energy in joules found in Step 2. Using \( E = 5.68 \times 10^{-15} \mathrm{\ J} \) and \( c = 3.00 \times 10^8 \mathrm{\ m/s} \). Calculate \( p = \frac{5.68 \times 10^{-15}}{3.00 \times 10^8} \approx 1.89 \times 10^{-23} \mathrm{\ kg \cdot m/s} \). Convert \( p \) to \( \mathrm{keV}/c \) using \( 1 \ \mathrm{eV}/c = 5.344 \times 10^{-28} \mathrm{\ kg \cdot m/s} \): \( \frac{1.89 \times 10^{-23}}{5.344 \times 10^{-28}} \approx 35406 \mathrm{\ eV}/c = 35.4 \mathrm{\ keV}/c \).

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Key Concepts

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

X-ray Wavelength
X-rays are a form of electromagnetic radiation, just like visible light, but with much shorter wavelengths. Understanding their wavelength is vital for various applications, from medical imaging to studying the structure of crystals.
  • The wavelength of x-rays typically ranges between 0.01 to 10 nanometers, often measured in picometers (pm) when they are very short, like in this exercise.
  • In scientific notations, x-ray wavelengths are generally expressed in meters, converting from picometers by multiplying by 10-12.
For the problem at hand, the given x-ray wavelength is 35 pm. This means it is highly energetic as shorter wavelengths correspond to higher energy levels. This fundamental property is why x-rays can penetrate substances and are useful in imaging technologies and detailed material investigations.
Frequency Calculation
The frequency of an electromagnetic wave is a measure of how many wave cycles pass a given point per second. This can be computed from the wavelength using the simple relationship:\[ u = \frac{c}{\lambda} \]Here, \( c \) is the speed of light, approximately \(3.00 \times 10^8 \mathrm{m/s}\), and \( \lambda \) is the wavelength. This equation highlights the inverse relationship between the wavelength and frequency, meaning the shorter the wavelength, the higher the frequency.In the exercise, the x-ray's wavelength of 35 pm was converted to meters, and then used to calculate the frequency: \[ u = \frac{3.00 \times 10^8}{35.0 \times 10^{-12}} \approx 8.57 \times 10^{18} \mathrm{Hz} \]This calculation results in x-rays having a very high frequency, which correlates to their ability to carry significant amounts of energy.
Photon Momentum
Photon momentum might initially seem paradoxical, as photons are massless. However, they do possess momentum as they travel at the speed of light. The momentum of a photon is computed using the relationship:\[ p = \frac{E}{c} \]Where \( E \) is the energy of the photon and \( c \) is the speed of light. Typically, photon energy is first calculated with Planck's formula, \( E = hu \), before calculating momentum. In the given problem, after finding the photon energy, momentum was calculated as: \[ p = \frac{5.68 \times 10^{-15}}{3.00 \times 10^8} \approx 1.89 \times 10^{-23} \mathrm{kg \cdot m/s} \]Moreover, it's common to express photon momentum in units of \( \mathrm{eV}/c \) or \( \mathrm{keV}/c \), underscoring its energy-like nature. In simpler terms, photon momentum helps explain phenomena such as radiation pressure, which is how light can exert force on objects.

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Most popular questions from this chapter

At what rate does the Sun emit photons? For simplicity, assume that the Sun's entire emission at the rate of \(3.9 \times 10^{26} \mathrm{~W}\) is at the single wavelength of \(550 \mathrm{~nm}\).

An ultraviolet lamp emits light of wavelength \(400 \mathrm{~nm}\) at the rate of \(400 \mathrm{~W}\). An infrared lamp emits light of wavelength \(700 \mathrm{~nm}\), also at the rate of \(400 \mathrm{~W}\). (a) Which lamp emits photons at the greater rate and (b) what is that greater rate?

Just after detonation, the fireball in a nuclear blast is approximately an ideal blackbody radiator with a surface temperature of about \(1.0 \times 10^{7} \mathrm{~K} .\) (a) Find the wavelength at which the thermal radiation is maximum and (b) identify the type of electromagnetic wave corresponding to that wavelength. (See Fig. 33-1.) This radiation is almost immediately absorbed by the surrounding air molecules, which produces another ideal blackbody radiator with a surface temperature of about \(1.0 \times 10^{5} \mathrm{~K}\). (c) Find the wavelength at which the thermal radiation is maximum and (d) identify the type of electromagnetic wave corresponding to that wavelength.

What are (a) the Compton shift \(\Delta \lambda\), (b) the fractional Compton shift \(\Delta \lambda / \lambda\), and \((\mathrm{c})\) the change \(\Delta E\) in photon energy for light of wavelength \(\lambda=590 \mathrm{~nm}\) scattering from a free, initially stationary electron if the scattering is at \(90^{\circ}\) to the direction of the incident beam? What are (d) \(\Delta \lambda,(\mathrm{e}) \Delta \lambda / \lambda\), and \((\mathrm{f}) \Delta E\) for \(90^{\circ}\) scattering for photon energy \(50.0 \mathrm{keV}\) (x-ray range)?

A photon undergoes Compton scattering off a stationary free electron. The photon scatters at \(90.0^{\circ}\) from its initial direction; its initial wavelength is \(3.00 \times 10^{-12} \mathrm{~m}\). What is the electron's kinetic energy?

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