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Find the momentum of \((a)\) a \(10.0-\mathrm{MeV}\) gamma ray; (b) a \(25-\mathrm{keV} \times\) ray ;(c) a \(1.0-\mu \mathrm{m}\) infrared photon; \((d)\) a 150-MHz radio-wave photon. Express the momentum in \(\mathrm{kg} \cdot \mathrm{m} / \mathrm{s}\) and \(\mathrm{eV} / \mathrm{c}\)

Short Answer

Expert verified
Gamma-ray: 5.34e-21 kg·m/s, 2.997e15 eV/c. X-ray: 1.335e-23 kg·m/s, 7.49e12 eV/c. Infrared: 6.63e-28 kg·m/s, 3.718e8 eV/c. Radio-wave: 3.313e-34 kg·m/s, 1.859e2 eV/c.

Step by step solution

01

Understand the underlying physics

The momentum of a photon can be calculated using the relation: \[ p = \frac{E}{c} \] where \( p \) is the momentum, \( E \) is the energy of the photon, and \( c \) is the speed of light (approximately \(3.00 \times 10^8 \;\mathrm{m/s} \)).
02

Convert energy to Joules

To find the momentum in \( \text{kg} \cdot m/s \), convert the given photon energy into Joules. 1 eV = \( 1.602 \times 10^{-19} \;\text{J} \).(a) For the 10.0 MeV gamma ray: \[ E = 10.0 \times 10^6 \;\text{eV} \times 1.602 \times 10^{-19} \;\text{J/eV} = 1.602 \times 10^{-12} \;\text{J} \](b) For the 25 keV x-ray: \[ E = 25 \times 10^3 \;\text{eV} \times 1.602 \times 10^{-19} \;\text{J/eV} = 4.005 \times 10^{-15} \;\text{J} \](c) For the 1.0 µm infrared photon, use the energy-wavelength relationship: \[ E = \frac{hc}{\lambda} \]Here, \(h\) is Planck's constant (\(6.626 \times 10^{-34} \;\text{J.s}\)), and \( \lambda \) is wavelength (\( 1.0 \mu m = 1.0 \times 10^{-6} \;m\)).\[ E = \frac{(6.626 \times 10^{-34} \;\text{J.s})(3.00 \times 10^8 \;\text{m/s})}{1.0 \times 10^{-6}\;m} = 1.988 \times 10^{-19} \;\text{J} \](d) For the 150 MHz radio-wave photon, convert frequency to energy \[ E = hf \]\( f = 150 \times 10^6 \;\text{Hz} \)\[ E = (6.626 \times 10^{-34} \;\text{J.s})(1.50 \times 10^8 \;\text{Hz}) = 9.939 \times 10^{-26} \;\text{J} \]
03

Calculate the momentum in kg·m/s

Use the photon momentum formula \[ p = \frac{E}{c} \].(a) For the 10.0 MeV gamma ray: \[ p = \frac{1.602 \times 10^{-12} \;\text{J}}{3.00 \times 10^8 \;\text{m/s}} = 5.34 \times 10^{-21} \;\text{kg·m/s}\](b) For the 25 keV x-ray: \[ p = \frac{4.005 \times 10^{-15} \;\text{J}}{3.00 \times 10^8 \;\text{m/s}} = 1.335 \times 10^{-23} \;\text{kg·m/s}\](c) For the 1.0 µm infrared photon: \[ p = \frac{1.988 \times 10^{-19} \;\text{J}}{3.00 \times 10^8 \;\text{m/s}} = 6.63 \times 10^{-28} \;\text{kg·m/s}\](d) For the 150 MHz radio-wave photon: \[ p = \frac{9.939 \times 10^{-26} \;\text{J}}{3.00 \times 10^8 \;\text{m/s}} = 3.313 \times 10^{-34} \;\text{kg·m/s}\]
04

Calculate the momentum in eV/c

Since 1 eV/c = 1.7827 x 10^-36 kg·m/s, convert the previously found momentums to eV/c.(a) For the 10.0 MeV gamma ray: \[ p = 5.34 \times 10^{-21} \;\text{kg·m/s} / 1.7827 \times 10^{-36} \;\text{kg·m/s per eV/c} = 2.997 \times 10^{15} \;\text{eV/c} \](b) For the 25 keV x-ray: \[ p = 1.335 \times 10^{-23} \;\text{kg·m/s} / 1.7827 \times 10^{-36} \;\text{kg·m/s per eV/c} = 7.49 \times 10^{12} \;\text{eV/c} \](c) For the 1.0 µm infrared photon: \[ p = 6.63 \times 10^{-28} \;\text{kg·m/s} / 1.7827 \times 10^{-36} \;\text{kg·m/s per eV/c} = 3.718 \times 10^{8} \;\text{eV/c} \](d) For the 150 MHz radio-wave photon: \[ p = 3.313 \times 10^{-34}\; \text{kg·m/s} / 1.7827 \times 10^{-36}\; \text{kg·m/s per eV/c} = 1.859 \times 10^2 \; \text{eV/c} \]

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Key Concepts

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

photon energy
Photon energy is a critical concept in understanding light and other forms of electromagnetic radiation. It relates to the energy carried by a single photon and is directly proportional to the photon's frequency. The energy of a photon can be calculated using the equation: \[ E = hf \] where:
  • E is the photon energy in joules (J),
  • h is Planck's constant (6.626 × 10^-34 Jâ‹…s),
  • f is the frequency of the photon in hertz (Hz).
To find the energy of a photon, you simply multiply the frequency of the light by Planck's constant. This simple relationship reveals how different forms of light, from gamma rays to radio waves, have different amounts of energy tied to their frequencies.
momentum formula
The momentum of a photon is another critical property that we'll explore. Photon momentum is given by the formula: \[ p = \frac{E}{c} \] where:
  • p is the photon momentum,
  • E is the energy of the photon,
  • c is the speed of light (3.00 × 10^8 m/s).
Photon momentum might sound tricky because photons don't have mass. However, they do have energy and travel at the speed of light. This relationship shows that even though they are massless, photons still carry momentum, which is directly proportional to their energy.
energy conversion
When calculating photon momentum, sometimes the energy might be given in electron volts (eV) instead of joules (J). To use the momentum formula, we may need to convert energy from eV to J. The conversion is straightforward:
  • 1 eV = 1.602 × 10^-19 J,
For example, if you have an energy of 10.0 MeV, you convert it to joules like this: \[ E = (10.0 \times 10^6 \; \text{eV}) \times (1.602 \times 10^{-19} \; \text{J/eV}) = 1.602 \times 10^{-12} \; \text{J} \] This conversion ensures that you're using consistent units when applying formulas. Consistency in units is key to correctly interpreting and solving physical problems.
Planck's constant
Planck's constant (6.626 × 10^-34 J·s) plays a vital role in quantum mechanics and the study of photons. It appears in the formulas for both photon energy and the energy-wavelength relationship:
  • Photon Energy: \[ E = hf \]
  • Energy-Wavelength Relationship: \[ E = \frac{hc}{\lambda} \]
This constant helps bridge the gap between wave-like and particle-like behaviors of light. It is fundamental in understanding how light interacts with matter. High-frequency photons, such as gamma rays, have much higher energies due to Planck's constant in their energy calculations.
wavelength-energy relationship
The wavelength-energy relationship for photons is given by the equation: \[ E = \frac{hc}{\lambda} \] where:
  • E is the photon energy,
  • h is Planck's constant (6.626 × 10^-34 J·s),
  • c is the speed of light (3.00 × 10^8 m/s),
  • λ is the wavelength of the photon.
This relationship shows that as wavelength decreases, the energy carried by the photon increases. For example, a gamma-ray photon with a very short wavelength will carry a significantly larger amount of energy compared to a radio-wave photon with a much longer wavelength. It also illustrates the different characteristics of various types of electromagnetic waves in terms of their energy and potential applications.

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Most popular questions from this chapter

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