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Radiation Dosimetry (An Introduction to Radiation Physics) Naslinda Noor Rizan, MSc Medical Physicist Gleneagles Penang [email protected]

Radiation Dosimetry (an Introduction to Radiation Physics)

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Radiation Dosimetry Introduction

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Page 1: Radiation Dosimetry (an Introduction to Radiation Physics)

Radiation Dosimetry

(An Introduction to Radiation Physics)

Naslinda Noor Rizan, MScMedical Physicist

Gleneagles [email protected]

Page 2: Radiation Dosimetry (an Introduction to Radiation Physics)

Structure of the Atom (Bohr Model)

Nucleus contains protons (+ve) and neutrons(no charge)

Nucleus contains protons (+ve) and neutrons (no charge)

P +N = A (mass no)

No of protons =Z (atomic no)

Orbiting electron e (- ve)

Nomenclature: A Z X

Only allowed certain discrete energy.

define shells or energy levels

K, L, M, N…..etc Max e- shell formula : 2n2

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Page 3: Radiation Dosimetry (an Introduction to Radiation Physics)

Physics of the Very Small (is

Very Strange) Standard Model of Matter Particles

(building blocks of atoms)

Leptons(build electrons) Quarks

(build protons, neutron...etc)

Boson(carrier of the fundamental forces in the universe)

1. e- & e- neutrino2. muon & muon neutrino3. tau & tau neutrino

1. Up & down2. Charm & strange3. Top & bottom

1. Gluon (strong force)2. Photon (electromagnetic force)3. Z & W (weak force)4. Graviton (cause gravity)

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Page 4: Radiation Dosimetry (an Introduction to Radiation Physics)

Nuclide & EnergyGeneral term for atoms with specific number protons and neutrons. (atom = nuclide + e-)

Isotope = nuclide with same Z (e.g 1H1, 1H2, 1H3 )Isotone = nuclide with same neutrons (N)Isomer - nuclide with same AIsobar - nuclide with same A& Z but different energy state.

Potential energy increases (from inner to outer valence)

Binding energy increases (from outer to inner shell)Amount of energy needed to remove electron from it’s orbit

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Page 5: Radiation Dosimetry (an Introduction to Radiation Physics)

Units & FormulaAtomic mass unit (amu) = 1/12 mass of C-12 = 1.67X10-27 kg

Amu E = mc2

Where m = 1.66 x 10-27 kg.

C = 3x108 m/sec , therefore

E = 1.49 x 10-10 J (1Mev = 1.6 x 10-13 J)

E = 931.25 Mev

e- = 0.000548 amup+ =1.00727 amuneutron = 1.00866 amu

E = hv = hc λ

Planck’s Constant, h = 6.626 070 040 x 10-34 J sSpeed of light, C = 3x108 m/secAvogadro’s No NA= 6.0221 ×1023 mol-1 (atoms ,molecules etc)Joules = kg.m2/s2

Mass per atom = Aw

NA

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Page 6: Radiation Dosimetry (an Introduction to Radiation Physics)

Units & FormulaKinetic energy

Total energy

Energy at rest

e- energy at rest = 0.511MeV

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Page 7: Radiation Dosimetry (an Introduction to Radiation Physics)

Radiation

IonizingHas enough energy to ionize matter directly or indirectly

Non-ionizingCannot ionize matter, energy lower than ionizing potential

Directly ionising (charged particles - e-, p+, α particles, heavy ionsDeposit energy directly in matter

Indirectly ionising (neutral particles (photons, neutronsDeposit energy through 2 step process

1. Release charge particle2. Charge particle deposit energy in matter

Source

RadioisotopeGenerated source

X-ray tube Linear Accelerator (LINAC)

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Page 8: Radiation Dosimetry (an Introduction to Radiation Physics)

Production of Ionizing photon

Characteristic x-ray : e- transition between atomic shell

Bremstrahlung: e- nucleus Coulomb interaction

Gamma ray: nuclear transition

Annihilation quanta: positron -e- annihilation

X ray tube output spectrum

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Page 9: Radiation Dosimetry (an Introduction to Radiation Physics)

Manufactured source1.X-ray tube

2.Linear Accelerator

(basic principle: e- accelerating onto a metal target to produce photons)

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Page 10: Radiation Dosimetry (an Introduction to Radiation Physics)

X-ray Tube

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Page 11: Radiation Dosimetry (an Introduction to Radiation Physics)

Linear accelerator (the very basic)

Electron gun

WaveguideBending magnets

Target

Primary collimator

collimators

Flattening filter

RF Source

http://www.irsn.fr/fr/professionnels_sante/documentation/documents/[email protected]

Page 12: Radiation Dosimetry (an Introduction to Radiation Physics)

Radiation interaction

Photon

e-

Rayleigh Scattering (low energy photon - why the sky is blue)PhotoelectricCompton ScatteringPair Production

Characteristic x-raysBremstrahlung

http://ozradonc.wikidot.com/photon-interactions

conversion of photon into a moving electron (e- then goes on to ionize the medium) scattering of a photon by a

(free) electron that leads to a moving electron and a lower energy photon (most important in radiotherapy) conversion of a photon into a

matter/antimatter pair of electrons.The two moving electrons share the remainder of the initial photon energy. Eventually the positron annihilates at the end of its range giving two 511 keV photons (important in SPECT and PET imaging)

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Page 13: Radiation Dosimetry (an Introduction to Radiation Physics)

Dominance of process

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http://ocw.mit.edu/courses/nuclear-engineering/22-01-introduction-to-ionizing-radiation-fall-2006/lecture-notes/energy_dep_photo.pdf

photon energy and atomic number, Z of the absorbing material

For both the photoelectric effect and pair production the photon is totally absorbed while for Compton scattering a photon of degraded energy remains.

Page 14: Radiation Dosimetry (an Introduction to Radiation Physics)

Mv or MeV??To produce a 6MV photon in linac you need a 6MeV electron but the output would be in a spectrum with max energy of 6MeV (photon).

Therefore for convenience we refer to photon from x-ray tube using its electric potential (MV or kV)

Electron output and radioisotope has mono-energetic energy and is correctly termedas keV or MeV

(*e- output in LINAC is produce but removing target and flattening filter)[email protected]

Page 15: Radiation Dosimetry (an Introduction to Radiation Physics)

Radioactivity

Unstable parent unstable atomic nuclei – don’t have enough binding energy to hold the nucleus together due to an excess of either protons or neutron

Alpha

Beta

Gamma

Segre Chart

Decay mode

http://algebralab.com/practice/practice.aspx?file=Reading_TheBandOfStability.xml

Neutron rich

Proton rich

Stable

Nucleus too big

Too many protons or too many neutrons

Page 16: Radiation Dosimetry (an Introduction to Radiation Physics)

α - Alpha DecayDuring alpha decay, an atom's nucleus sheds two protons and two neutrons in a packet that scientists call an alpha particle.

alpha particle is a fast moving helium nucleus. Alpha particles carry a charge of +2 and strongly interact with matter. They travel only a few inches through air and can easily be stopped with a sheet of paper.

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Page 17: Radiation Dosimetry (an Introduction to Radiation Physics)

β-Beta DecayToo many neutrons or too many protons. One of the protons or neutrons is transformed into the other.

Beta+ (positron)Electron Capture a neutron decays into a

proton, an electron, and an antineutrinoa proton decays into a

neutron, a positron, and a neutrino

decay by capturing one of the electrons that surround the nucleus.

Beta-

𝛾- Gamma Decay

A nucleus changes from a higher energy state to a lower energy state through the emission of electromagnetic radiation

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Page 18: Radiation Dosimetry (an Introduction to Radiation Physics)

Formulas Half life, T1/2 = ln2/ƛ

Decay constant, = ln2/Tƛ 1/2

Activity, A = A0e- tƛ

Units Bq (Baquerel) = 1 disintigration per second1mCi = 37MBq1MBq = 27µCi

time taken for half or nuclei present to decay

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