Physics Facts Flashcards
Force =
M * A (F = force; M = mass; A=acceleration)
1 Joule =
1 kg m2/s2 = 1 Newton-meter
Kinetic Energy
(m * v2)/2 (m = mass in Kg; v = velocity (m/s))
Potential Energy
m * g * h (m = mass in kg; g = gravitational acceleration; h = height above floor)
Atomic Number (Z)
of protons in nucleus of atom
Atomic mass number (A)
of protons + neutrons in nucleus of atom
Compare the following particles in terms of Mass, Rest Energy (MeV), and Charge
Particle Mass (kg) Rest Energy (MeV) Charge (e) *
Electron 9.11 x 10^-31 0.511 -1
Positron 9.11 x 10^-31 0.511 +1
Proton 1.67 x 10^-27 938.2 +1
Neutron 1.68 x 10^-26 939.5 0
Alpha 6.65 x 10^-27 3729 +2
* unit of charge is 1.6 x 10-19 coulomb
Electron volt (eV):
kinectic energy gained by electron after being accelerated through a potential difference of one volt
1eV = 1.6021 * 10-12 ergs = 1.6021 * 10-19 joules = 3.83 * 10-20 cal
(remember that joules = (Kg * m2)/ s2))
Alpha Particle:
helium nuclei (2 protons + 2 neutrons)
Beta minus particle
electron emitted by nucleus
Beta plus particle
positron emitted by nucleus (same mass as electron but with a +charge)
Neutron
part of nucleus of atom (has no charge)
Gamma ray
X-ray emitted from nucleus
Speed of light (in vacuum):
3 x 108 m/s
What is the relationship between wavelength, frequency (v) in Hz, speed of light (c):
Speed of light (c) = wavelength * frequency (v)
or Wavelength = speed of light/frequency
or Frequency (v) = speed of light (c)/ wavelength
Example: What is the frequency of a photon with a wavelength 15 * 10-11m
Frequency (v) = (3 * 108 m/s) / (15 x 10-11m) = 2 * 1018 Hz
Example: What is the wavelength of the typical EM waves used to accelerate electrons in a linear accelerator (typically frequency of 3000 MHz)?
Wavelength = (3 * 108 m/s)/(3 * 109 Hz) = 0.1m or 10cm
Hz is cycles per second.
Energy of Photon:
E= hv (E = energy of photon; v= frequency of photon, h = Planck’s constant = 6.626 x 10^-34 joules-second)
or **v = E/h **
or E= hc/wavelength (since Frequency (v) = speed of light (c)/ wavelength)
Example: What is the energy of a photon with wavelength 15 * 10-11m?
E = (1.24 * 10-12 MeV*m) / (15 x 10-11 m) = 0.0083 MeV
(remember that hc = 1.24 * 10-12 MeV*m because h = 6.626 *10-34 joules * second or 4.136 * 10-15 eV * second and c = 3 * 108 m/s; remember to multiply eV * 10-6 to get to MeV!!!)
Wavelength formula
Wavelength = speed of light (c)/frequency (v)
or Wavelength = speed of light (c)/(E/h)
so Wavelength = hc/E (hc = 1.24 * 10-12 MeV*m)
Example: What is wavelength of 100 keV photon? Wavelength = (1.24 \* 10<sup>-12 </sup>MeVm)/0.1 MeV) = **1.24 \* 10<sup>-11</sup>**
Characteristic x-ray
photon given off when outer orbit electron moves to fill a inner electron shell vacancy caused by an incoming electron causes ionization of an atom
Bremsstrahlung (braking radiation):
produced when incoming electron interacts with positive charge of the atomic nucleus
source of most x-ray production
energy lost by incoming electron is given off as a photon
Bremsstrahlung production efficiency = (electron energy in eV) * (atomic # of target) * 10-9
At diagnostic energies (<120keV) bremsstrahlung efficiency is ~1%, At therapeutic MV energies it is 15-50%!
Thoraeus filter
Tin (closest to x-ray tube) →copper → aluminum
used to harden orthovoltage beams (characteristic x-ray of aluminum is only 1.5keV and is absorbed by air before hitting patient)
Calculate electron energy conversion to photon energy
F = 3.5 * 10-4 ZE (Z = atomic #; E = maximum energy of electrons in MeV)
Calculate Beam Intensity Transmission
T = I/I0
Beam Attenuation (single energy source)
I = Ioe-µx (x = thickness of filter; µ = linear attenuation coefficient (a function of filter material and energy of photon beam))
Example: Initial intensity = 2000 photons, µ= 0.2mm-1, thickness = 3mm
I = 1098 photons
Linear attenuation coefficient
= µ
- probability that a given photon will be attenuated in a unit thickness of a particular attenuator
- varies with photon energy and filter composition (atomic number, Z)
-a larger number (closer to 1.0) indicates a higher probability of photon attenuation
The CT number (in Hounsfield units) = 1000 x [(umaterial - uwater)/uwater where u = the linear attenuation coefficient
Describe beam hardening
only occurs with a polyenergetic or heterogeneous beam (mono-energetic beams cannot be “hardened”!!)
Homogeneity coefficient (HC):
-ratio of first HVL to second HVL (a larger value (closer to 1.0) means the beam is more uniform)
Half value layer
HVL = 0.693/µ (ln 2 = 0.693; µ = linear attenuation coefficient)
- typically mm Al for superficial x-rays; mm Cu for orthovoltage; mm Pb for megavoltage
- beam shielding blocks are typically 5 HVL of shielding (<5% transmission)
As attenuation coefficient decreases, HVL increases. For photon energies from 100keV to 20 MeV, HVL initially increases (due to Compton interactions) and then decreases (as pair production becomes more prevalent at higher energies)
Mass attenuation coefficient
(µ/ρ); linear attenuation coefficient divided by mass density of the material (measured in cm2/g)
Coherent Scatter
incoming photon is completely absorbed by electrons of an atom which causes the electrons to vibrate and radiate a photon with identical energy in a different direction
-only occurs at very low photon energies
-can cause blurring of diagnostic X-ray images
-of no importance in high energy XRT
Photoelectric Effect
incoming high-energy photon ejects an inner shell electron with subsequent filling of vacant electron shell causing emission of characteristic x-rays. Incoming photon is completely absorbed (it disappears!).
-the ejected electron has the kinetic energy of the incoming photon minus the binding energy of the electron
(Incoming photon - binding energy of electron = kinetic energy of ejected electron)
- characteristic x-ray energy equals the energy difference between electron shells (outer shell electron fills the empty spot in the inner shell)
- the probability of photoelectric interaction: Z3/E3 (Z=atomic #; E = energy of photon)
- more likely to happen in high Z material (like bone)
- less likely to happen with increasing photon energy
The photoelectric effect is predominant for photon energies in the range of 10 keV (For soft tissue, the PE and Compton effects are equal at 25 keV.For bone, the PE and Compon effects are equal at 40 keV)
In imaging (such as kV CB CT), High Z-material will cause alot of artifact due to dominance of the photoelectric effect at kV energies!!
Compton Effect
high energy photon knocks a loosely held outer shell electron from an atom (leaving a positively charged ion), with the remaining energy forming a lower energy photon traveling in a different direction
- depends only on electron density (electrons per unit mass) and is independent of the atomic number of the absorbing material! (electron density is directly proportional to the physical density)
- Energy change is related to the angle of scatter (Θ); calculate using the change in the photon’s wavelength (λ); remember units of λ are in meters
The scattered photon is always less energetic than the incoming photon; the most energetic 90° photon is .511 MeV
The Compton photon can be scattered at any angle, but the Compton electron is emitted at an angle limited to 0-90° with respect to the direction of the incident photon.
Maximum energy is transferred to the electron when the photon is backscattered (so less energy is transferred to the scattered photon; 180° (from original direction) backscatter photon has the least energy, 255.5keV or less), the Compton electron then goes off in the direction exactly opposite to the backscattered photon (0° relative to the direction of the initial photon)
Example: Calculate Energy change of incoming 1 MeV photon that produces a scattered photon at 90° from incoming direction:
Remember: E = hc/λ so λ= hc/E (hc = 1.24 * 10-12 MeVm)
∆λ = 2.4 * 10-12 (1-cos Θ)m (Θ is angle between the paths of initial and scattered photon) → ∆λ = 2.4 * 10-12 (1-cos 90°)m = 2.4 * 10-12m
λf= λi + ∆λ
λi = hc/E = 1.24 * 10-12 (m * MeV)/ 1 MeV = 1.24 * 10-12 m
λf =λi + ∆λ = 1.24 * 10-12m + 2.4 * 10-12 m = 3.64 * 10-12 m
So the Scattered photon energy (E) = hc/λ = 1.24 * 10-12 MeVm)/3.64 * 10-12 m = 0.3407 MeV (340.7 keV)
For imaging, such as MV CB CT, the artifact from high-Z materials will be relatively less than with a kV CB CT since most interactions with MV energies is Compton and is not affected by Z nearly as much as the photoelectric effect (such as in kV imaging)
Pair Production
Incoming photon interacts with electric field of nucleus (electric field strength depends on Z), creating an electron and a positron (positive electron).
-Incoming photon is completely absorbed.
-most important above 10MeV
- requires at least 1.02 MeV incoming photon (since each particle in the pair has a rest mass of 0.511 MeV); excess energy above 1.02 MeV is divided as kinetic energy
- Likelihood of interaction is directly proportional to the log of Z
- positron then undergoes Pair Annihilation with a different free electron (producing two annihilation photons, each of 0.511 MeV.
Pair Annihilation
Positron (created by pair production) interacts with a nearby (different) free electron, causing the annihilation of both and creating two photons with energy of 0.511MeV each, which travel in opposite directions
Photonuclear Interaction (gamma-n interaction):
-only occurs with photon energy above 15MeV
-high energy photon is absorbed by nucleus → forms unstable nucleus → to regain stability, a neutron is emitted from the nucleus; neutron then interacts with another nucleus making it radioactive
-Can result in transiently (~10 min) radioactivity of parts of the linear accelerator (beam flattening filters, wedges; especially if made of copper)
Mass energy absorption coefficient
**μen/ρ ** (μen= linear energy coefficient; ρ = density of material in the attenuator
Temperature/Pressure Correction
C = (760/P) * (273.2 + t/295.2) where P and t are the given pressure and temperature
Higher temperature thins the air (rarefies it), and the TC offsets this
Higher Pressure compresses the air, and the PC offsets this
Ion Chamber collection efficiency (f)
charge collected / charge liberated by initial ionization
TLD dose to patient
calibration dose * (patient reading/calibration reading)
Calculating a Half Life or Remaining Activity
**A(T) = A0 (1/2)T ** (when time is measured in half lives)
Example: T1/2 = 3 hours, T = 10 hours, A0 = 100Bq → A(T) = 100 (0.5)3.333 = 100 (0.099) = 9.9 Bq
or
A(t) = A0e-λt (when time is measured in a unit of time, e = 2.71828 and λ=0.6931/T1/2 and t= time (days/hours etc in same unit as T1/2)
Example: A(t) = 100e-2.31=100 (0.099) = 9.9Bq when T1/2 = 3 hours, t = 10 hours)
Gas Ionization Detectors
Geiger-Mueller (G-M) counters (can detect very amounts of radiation such as from a lost I125 seed), proportional counters (can discriminate type of radiation and measure exposure rates; example is a portable ionization chamber called a cutie pie), ionization chambers (used to calibrate linacs and measure treatment beam characteristics)
In general, ionization chambers are filled with a gas and have two electrodes; ionizing radiation causes ionized ion pairs to travel to the positive and negative electrodes)
Electrodes must be polarized, which requires voltage (supplied by battery or other voltage source)
Geiger-Mueller counters
Used to detect low intensity radiation
Usually measures exposure in counts per minute (cpm) or exposure per hour (mR/hr or R/hr); 5mR/hr is about 250cpm
G-M counters are very sensitive since one ionization event creates a pulse of current in which all of the chamber volume ionizes at once (the chamber must then reset before it can register another ionization event); thus they have a dead time; so in a high-intensity radiation field the G-M counter can read zero (above 4R/hr)
G-M counters can under-respond at energies <30keV because of beam attenution in the walls (high Z material, usually metal), and over-respond at moderate energies (30-100keV) because of the photoelectric effect of high Z material walls
Neutron Dosimeters
Linacs with energy >10MV produce neutrons; low Z moderating detectors are required to detect (hydrogen or boron detectors)