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Study of Gamma-ray Spectrum by
  using Scintillation detector and
      Single channel Analyzer
Radioactive decays
Radioactive decay is the spontaneous breakdown of an
atomic nucleus resulting in the release of energy and
matter from the nucleus. We know that a radioisotope has
unstable nuclei that does not have enough binding energy
to hold the nucleus together. radioisotope would like to be
stable isotopes so they are try to be stabilize. In the
process, they will release energy and matter from their
nucleus and often transform into a new element. This
process, called transmutation, is the change of one
element into another as a result of changes within the
nucleus. The radioactive decay and transmutation process
will continue until a new element is formed that has a
stable nucleus and is not radioactive.
Types of Decay
 Alpha Decay


 Beta Decay
-                                  +1

+                                  -1

 Electron Capture.
 Gamma Decay
 Gamma decay occurs because the nucleus is at too high
 energy state. The nucleus falls down to a lower energy
 state and, in the process, emits a high energy photon
 known as a gamma particle. Flash Flash 1
What is gamma ray?


Gamma radiation is one of the three types of natural
radioactivity. Gamma rays are electromagnetic radiation.
Gamma rays are the most energetic form of electromagnetic
radiation, with a very short wavelength between 0.003 nm -
0.03 nm.
 They are produced by sub-atomic particle interactions such
as electron-positron annihilation, radioactive decay.
Radioactive source (Na-22)
Sodium-22 is the radioactive source which has 11 protons
And 11 neutrons and by beta plus it is decay to Neon-22.

In general of stable nuclei
Decay scheme in general
Na-22 Decay scheme


                     Sodium      11

                   /10%

          3.7 ps                        90%




          Neon
                          22Na        22Ne   + γ + β+ + υe
Interaction of gamma radiation with matter
 Photoelectric effect
When a gamma-ray collides with an orbital electron of an atom
 of the material through which it is passing it can transfer all its
 energy to the electron and cease to exist. On the basis of the
 Principle of Conservation of Energy we can deduce that the
 electron will leave the atom with a kinetic energy equal to the
 energy of the gamma-ray, This electron is called a
 photoelectron.
 Compton effect
gamma-ray transfers only part of its energy to a valance electron
which is essentially free. Notice that the electron leaves the atom and
the gamma-ray deflects off in a different direction to that with which
it approached the atom. This deflected or scattered gamma-ray can
undergo further Compton Effects within the material. this effect is
sometimes called Compton Scattering.
 Pair production
The incident Gamma Ray photon will interact with mater
 through pair production if its energy is greater than 1.02
 Mev , in this process positron and electron will produced
 then the positron annihilate the two photons of 0.511
 Mev produced of opposite direction.
Scintillation detector
  Is a detector which consist of a material which produce a
  flashes of light when absorb a radiation. These materials are
  variously called fluorescent materials, Scintillator .(we use
  Thallium activated sodium iodide)Nai(TL).
Properties of Scintillators
 High scintillation efficiency.
 The conversion of radiation into light should be linear over a
  wide range of energies.
 The medium should be transparent to the scintillation light.
 The decay time of the produced scintillation light should be
  short.
 The index of refraction of the scintillator should be suitable.
Parts of scintillation detector
                                        Anode
                              PMT
              Scintillator                      Multi-channel
                                                analyzer

               Nai(Tl)




Radioactive
                                            Amplifier
source
                              Dynodes
               Photocathode
Nai(Tl) spectrum for Na-22

                   Electron positron annihilation
                   peak at 0.511 Mev


        X-ray

                 Compton
                 edge


                                     Photopeak 1275 Kev
Thanks for Attention


Prepared by




        Fourth stage –physics Department -2010-2011

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Gamma ray spectrum by using na i(tl)detector ..

  • 1. Study of Gamma-ray Spectrum by using Scintillation detector and Single channel Analyzer
  • 2. Radioactive decays Radioactive decay is the spontaneous breakdown of an atomic nucleus resulting in the release of energy and matter from the nucleus. We know that a radioisotope has unstable nuclei that does not have enough binding energy to hold the nucleus together. radioisotope would like to be stable isotopes so they are try to be stabilize. In the process, they will release energy and matter from their nucleus and often transform into a new element. This process, called transmutation, is the change of one element into another as a result of changes within the nucleus. The radioactive decay and transmutation process will continue until a new element is formed that has a stable nucleus and is not radioactive.
  • 3. Types of Decay  Alpha Decay  Beta Decay - +1 + -1  Electron Capture.  Gamma Decay Gamma decay occurs because the nucleus is at too high energy state. The nucleus falls down to a lower energy state and, in the process, emits a high energy photon known as a gamma particle. Flash Flash 1
  • 4. What is gamma ray? Gamma radiation is one of the three types of natural radioactivity. Gamma rays are electromagnetic radiation. Gamma rays are the most energetic form of electromagnetic radiation, with a very short wavelength between 0.003 nm - 0.03 nm. They are produced by sub-atomic particle interactions such as electron-positron annihilation, radioactive decay.
  • 5. Radioactive source (Na-22) Sodium-22 is the radioactive source which has 11 protons And 11 neutrons and by beta plus it is decay to Neon-22. In general of stable nuclei
  • 6. Decay scheme in general
  • 7. Na-22 Decay scheme Sodium 11 /10% 3.7 ps 90% Neon 22Na 22Ne + γ + β+ + υe
  • 8. Interaction of gamma radiation with matter  Photoelectric effect When a gamma-ray collides with an orbital electron of an atom of the material through which it is passing it can transfer all its energy to the electron and cease to exist. On the basis of the Principle of Conservation of Energy we can deduce that the electron will leave the atom with a kinetic energy equal to the energy of the gamma-ray, This electron is called a photoelectron.
  • 9.  Compton effect gamma-ray transfers only part of its energy to a valance electron which is essentially free. Notice that the electron leaves the atom and the gamma-ray deflects off in a different direction to that with which it approached the atom. This deflected or scattered gamma-ray can undergo further Compton Effects within the material. this effect is sometimes called Compton Scattering.
  • 10.  Pair production The incident Gamma Ray photon will interact with mater through pair production if its energy is greater than 1.02 Mev , in this process positron and electron will produced then the positron annihilate the two photons of 0.511 Mev produced of opposite direction.
  • 11. Scintillation detector Is a detector which consist of a material which produce a flashes of light when absorb a radiation. These materials are variously called fluorescent materials, Scintillator .(we use Thallium activated sodium iodide)Nai(TL). Properties of Scintillators  High scintillation efficiency.  The conversion of radiation into light should be linear over a wide range of energies.  The medium should be transparent to the scintillation light.  The decay time of the produced scintillation light should be short.  The index of refraction of the scintillator should be suitable.
  • 12. Parts of scintillation detector Anode PMT Scintillator Multi-channel analyzer Nai(Tl) Radioactive Amplifier source Dynodes Photocathode
  • 13. Nai(Tl) spectrum for Na-22 Electron positron annihilation peak at 0.511 Mev X-ray Compton edge Photopeak 1275 Kev
  • 14. Thanks for Attention Prepared by Fourth stage –physics Department -2010-2011