Photons interact with matter in fascinating ways, shaping how radiation behaves around us. From the photoelectric effect to pair production , these processes determine how energy is transferred and absorbed in materials.
Understanding photon interactions is key to grasping radiation's impact on our world. We'll explore how different materials and energies affect these interactions, and how we can use this knowledge for protection and practical applications.
Photon Interactions
Photoelectric Effect and Compton Scattering
Top images from around the web for Photoelectric Effect and Compton Scattering Compton scattering - Wikipedia View original
Is this image relevant?
Wave-corpuscular duality of photons and massive particles | Introduction to the physics of atoms ... View original
Is this image relevant?
Effet photoélectrique — Wikipédia View original
Is this image relevant?
Compton scattering - Wikipedia View original
Is this image relevant?
Wave-corpuscular duality of photons and massive particles | Introduction to the physics of atoms ... View original
Is this image relevant?
1 of 3
Top images from around the web for Photoelectric Effect and Compton Scattering Compton scattering - Wikipedia View original
Is this image relevant?
Wave-corpuscular duality of photons and massive particles | Introduction to the physics of atoms ... View original
Is this image relevant?
Effet photoélectrique — Wikipédia View original
Is this image relevant?
Compton scattering - Wikipedia View original
Is this image relevant?
Wave-corpuscular duality of photons and massive particles | Introduction to the physics of atoms ... View original
Is this image relevant?
1 of 3
Photoelectric effect occurs when a photon transfers all its energy to an atomic electron
Electron is ejected from the atom with kinetic energy equal to photon energy minus binding energy
Predominant at low photon energies (below 100 keV for most materials)
Cross-section varies approximately as Z 4 / E 3 Z^4/E^3 Z 4 / E 3 , where Z is atomic number and E is photon energy
Compton scattering involves partial energy transfer from photon to electron
Scattered photon continues with reduced energy and changed direction
Dominant process for intermediate photon energies (0.1 to 10 MeV for most materials)
Energy of scattered photon given by E ′ = E 1 + E m e c 2 ( 1 − cos θ ) E' = \frac{E}{1 + \frac{E}{m_ec^2}(1-\cos\theta)} E ′ = 1 + m e c 2 E ( 1 − c o s θ ) E , where θ is scattering angle
Both processes contribute to ionization and energy deposition in matter
Pair Production and Cross-section
Pair production creates an electron-positron pair from a high-energy photon
Requires photon energy of at least 1.022 MeV (twice the electron rest mass)
Occurs in the electric field of an atomic nucleus
Dominant process for high photon energies (above 10 MeV for most materials)
Cross-section increases with atomic number and photon energy
Cross-section represents probability of photon interaction per atom
Total cross-section is sum of individual process cross-sections
Measured in units of area (barns, 1 barn = 1 0 − 24 cm 2 1 \text{ barn} = 10^{-24} \text{ cm}^2 1 barn = 1 0 − 24 cm 2 )
Varies with photon energy and atomic number of absorber
Used to calculate attenuation coefficients and interaction probabilities
Attenuation Properties
Attenuation Coefficient and Mean Free Path
Attenuation coefficient quantifies photon beam intensity reduction in matter
Linear attenuation coefficient (μ) measured in cm^-1
Mass attenuation coefficient (μ/ρ) in cm^2/g, independent of material density
Beam intensity follows exponential decay : I = I 0 e − μ x I = I_0 e^{-\mu x} I = I 0 e − μx
Mean free path represents average distance traveled by photon before interaction
Calculated as inverse of linear attenuation coefficient: λ = 1 / μ \lambda = 1/\mu λ = 1/ μ
Varies with photon energy and material composition
Longer mean free path indicates greater penetration depth
Half-value Layer and Energy Absorption
Half-value layer (HVL) thickness of material that reduces beam intensity by half
Related to attenuation coefficient: H V L = ln ( 2 ) / μ HVL = \ln(2)/\mu H V L = ln ( 2 ) / μ
Used in radiation shielding calculations and quality assurance
Multiple HVLs can be used to achieve desired attenuation (tenth-value layer)
Energy absorption describes transfer of photon energy to matter
Energy absorption coefficient (μen) accounts for energy carried away by scattered photons
Fraction of photon energy absorbed depends on interaction process and material
Important for dosimetry and radiation protection calculations
Energy absorption build-up factor corrects for multiple scattering events