MedPhys

Physik für FCRC

Physik für FCRC


K. N.
Diese Lernkarten bieten eine umfassende Übersicht über die medizinische Physik auf Universitätsniveau, mit einem Schwerpunkt auf Ultraschall, CT und nuklearmedizinischen Techniken. Sie behandeln Themen wie Artefakte, Dosimetrie, Bildqualität und technische Aspekte von Geräten. Medizinstudenten und Fachkräfte profitieren davon, um die physikalischen Grundlagen und praktische Anwendung in der medizinischen Bildgebung zu verstehen.
Cartes-fiches
172
Utilisateurs
1
Langue
Allemand
Catégorie
Médecine
Niveau
Université
Créé / Mis à jour
14.04.2015 / 14.04.2015

Cartes-fiches

Nucleus

protons and neutrons

Atomic mass (A)

protons + neutrons

Atomic number

number of protons

nuclides

same protons = same element

Isotope

same chemical properties, but different physical properties

electron orbit

K: 2

outer orbit shell

valence

determines the chemical, electrical and thermal properties of the element

ion

electrons <> protons

electron excitation

gains energy and moves to higher energy outer shell

Binding energy E and atomic number Z of

Iodine?

Barium?

Tungsten?

Lead?

energy to remove the electron from the an atom

high, as Z=atomic number is high

high for electron in the inner shell, closer to the nucleus

Binding energy  = E

energy to remove an electron from the shel

 

E increase  = atomic numbre Z increase

E increase = K shell, near to the nucleus

Electromagnetic radiation (EMR)

speed of light in vacuum

3 x 108 m/s

magnetic and electric components

wave and particle component

X-Ray

EMR from the electron

Gamma ray

from the nucleus

EMR

the wave model

f = 1 Hz = 1/s

 

in different media f constant----- speed changes

EMR

the particle model

photon

Wave equation

 

v = f x λ

velocity = frequency x wavelength

Planck-Einstein equation

E = h x f

Photon energy = Planck constant x frequency

E=h x c /λ = 1,24 /λ

photon fluence

number of photons in a slice of the beam

energy fluence

energy of all the photons in a fluence

beam intensity

energy fluence per time unit

Production of characteristic radiation

hit the inner electron

the outer electron falls  down

emission of a photon with energy = binding energy inner electron - bindung energy outer electron

 

determined by atomic number and unaffected by tube voltage

characteristic radiation of tungsten

Z = 74

Ek = 70 keV

EL = 12 keV

 

Kalpha= Ek- EL = 70 -12 = 58 keV

Bremsstrahlung

80% X-ray = Bremsstrahlung

K-shell, near the nucleus

continuous spectrum

beam intensity

area under the curve

increase with the kV = increase the photon energy

increasing mA (tube current) = no shape change

increase target number = increase the photon energy

Linear attentuation coefficient (µ)

µ = 0.693 /HVL (1/m)

fractional reduction of the energy per unit thickness

depends on the density of material

increase= density increase

             = atomic number increase

             = photon energy decreases

Mass attentuation coefficient (mac)

mac =  µ / density (cm2/g)

fractional reduction per unit mass

depends on energy and atomic number

beam hardening

become homogenous with high energy photons because low energy photon are more attenuated.

Photoelectric Absorption.

the photon completely disappears; its energy is transferred to one of the orbital electrons of the atom (K-shell).

Electron trops down from L to K-shell.

Photoelectric Absorption = Z3 / E3 (Z: atomic number; E =photon energy)

Increase with Z3

Decrease with the photon energy.

important, whenn Z is high, and the photon energy is low.

 

compton scatter

Photon hits the free electron in the outer shell.

new photon with lower energy and new direction, and electron with more energy.

80% in radiology are compton scatter, 20% are scattered.

important, whenn Z is low, and the photon energy is high.

 

scatter angle

angle between the incoming photon and the scatter photon.

0° = maximum energy for scatter photon, electrons travel 90° and has minimum energy

180° =  photon backward with minimum energy, electron travel 0° forward with the maximum energy

 

scatter angle up  =  the energy of the scatter photon down

Elastic scattering (Raleigh)

incoming photon is less energic to the binding electron.

photon deflected without energy loss.

high Z and low energy.

Pair production

photonw with high energy > 1.02 MeV (2*511 keV)

nucleus = production of positron and electron

E = mc2 (m: mass, c: speed of light)

Total infiltration

at least 2,5 mm Aluminium

Filter material

Al = 1,5 mm (Z= 13)

Copper = 0.1 - 0.3 mm (Z=29)

Filtration effects

-Beam hardening

-Increase the HVL

-Reduction of the number of photon

-shift to the the right

-no change in maximum photon energy

K-edge filter

Remove both high and low energy photon.

not in mammography

Luminescence

1. Fluorescence

2.Phosphorescence

Fluorescence

The photon excites an electron into one of the many higher energy vibrational states.
Some energy is transferred into vibrational energy and then the excited electron relaxes into the ground state, releasing a photon of lower energy then the photon initially absorbed.
 

phosphorescence

electron from the valence band to the conduction band

stuck in the conduction band until more energy by heat or light, then fall down the valence band with emmission of light.

 

1. heat = lithium fluoride

2. light = barium fluorohalide

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