atomic nucleus and radioactivity Flashcards

1
Q

what is radioactivity

A

• Spontaneous emission of small particles and/or radiation by unstable atomic nuclei to attain more stable nuclear state

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2
Q

who discovered radioactivity

A
  • Marie and Pierre Curie isolated two previously unknown radioactive materials, polonium and radium
  • Radioactivity was found to be unaffected by chemical and physical testing, showing that the radiation came from the atom itself – specifically from the disintegration or decay of an unstable nucleus
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3
Q

Ernest Rutherford 1893

A

began studying the nature of the rays that were emitted and they were classified into three distinct types according to their penetrating power

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4
Q

what are the three distinct types of rays emitted

A

alpha decay
beta decay
gamma decay

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5
Q

Alpha decay

A

positively charged, can barely penetrate a piece of paper. alpha rays are nuclei of helium atoms

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6
Q

Beta decay

A

negatively charged, pass through as much as 3mm of aluminium. Beta rays are electrons

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7
Q

Gamma decay

A

neutral, extremely penetrating. Gamma rays are high energy protons

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8
Q

what is alpha decay

A

the loss of 2 neutrons and 2 protons = changed atom. see pp for equation

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9
Q

alpha decay : smoke detector

A
  • Americium 241 has a half-life of 432.6 years
  • Emitted alpha particle ionises the air molecules which conduct current between two terminals
  • Smoke clings to ionised air molecules and slows them down
  • Current decreases and a transistor switch activate the alarm
  • Contains 0.3ug of the isotopes or 37Bq or 1 Ci of radioactivity
  • Radiation risk much smaller than background radiation
  • Sensitive to flaming stage of fire
  • Optical smoke detectors sensitive to smouldering stage of fire
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10
Q

what is beta decay

A
  • also called negatron decay
  • The electron emitted in beta decay is not an orbital electron; the electron is created in the nucleus itself
  • One of the neutrons changes to a proton and in the process throws off an electron
  • These particles are referred to as beta particles so as not to confuse them with orbital electrons
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11
Q

beta decay and the neutrino

A

• 1930 – Wolfgang Pauli proposed that there was a new particle that was very difficult to detect was emitted in beta decay, as well as the electron
• This new particle was names neutrino by Enrico Fermi 1934
• In 1956, complex experiments produced further evidenced for the neutrino, but by then physicists had already accepted existence
• The symbol for the neutrino is the Greek letter “nu”
see pp for equation

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12
Q

positron decay

A

• Occurs when there are too few neutrons compared to the number of protons. These isotopes lie below the stable isotype line
• In this type of beta decay, the particle that is emitted is called a positron, as it has the same mass as an electron of +1
• The positron is called the antiparticle to the electron
see pp for equation

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13
Q

positron-emission tomography

A
  • Nuclear medicine functional imaging technique that is used to observe metabolic processes in the body
  • The system detects pairs of gamma rays emitted indirectly by a positron-emitting radionuclide, which is introduced into the body on a biologically active molecule. 3D images of tracer concentration within the body are then constructed by computer analysis
  • Biological molecule e.g. fludeoxyglucose (FDG), an analogue of glucose, shows tissue metabolic activity corresponding to glucose uptake. Indicates cancer metastasis
  • 20 min scan
  • Red areas show more accumulates tracer substance and blue areas are regions where low
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14
Q

electron capture

A

• Electron capture occurs when a nucleus absorbs one of the orbiting electrons. Usually one of the innermost electrons
• Electron disappears and a proton becomes a neutron in the process
• A neutrino is emitted in electron capture decay
• This process has been detected by the emission of x-rays due to other orbital electrons jumping down to fill in the lower energy levels and releasing energy of that energy
see pp for equation

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15
Q

give 4 sources of instabilities

A
  • Too big
  • Too many neutrons for the protons
  • Not enough neutrons for the protons
  • Too much excess energy
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16
Q

nuclear stability

A

• Determined by the number of neutrons to protons
• Atomic number(Z) less than 20:
- Ration close to 1 fall in zone of stability
• Atomic number going from 21-83:
- Number of neutrons always greater than the number of protons
- Neutrons help to stabilise the nucleus and overcome repulsive electric forces of the protons
- Ration increases from 1 to 1.5 as Z increases from 21 to 83
• Atomic number greater than 83
- Ration greater than 1.5 (proportionally more neutrons needed to stabilise larger number of protons)
- All unstable and decay and are radioactive
- Outside zone of stability

17
Q

see pp for

A

neutron to proton ratio graph

18
Q

left of zone

A
  • Neutron rich
  • Changes neutrons to protons by β emission
  • n –> p + e
19
Q

right of zone

A
  • Proton rich
  • Tries to lose protons and gain neutrons
  • P + e –> n
  • Positron emission or electron capture
20
Q

just in zone but Z>83

A
  • Decay by emitting α particle to try to achieve a more stable nucleus
21
Q

odd-even rule

A

• When neutrons and protons both have even numbers, isotopes tend to be far more stable than when they are both odd
• Of all 264 stable isotopes, number of protons/neutrons
- 168 even/even
- 57 even/odd
- 50 odd/even
- 4 odd/odd

22
Q

radioactive decay series

A
  • Some nuclei cannot obtain stability in just one transformation
  • Uranium goes through 8 alpha decays and 6 beta decays before it reaches stability at lead
23
Q

gamma decay

A
  • Photons having very high energies. The decay of a nucleus by the emission of a gamma ray is much like the emission of photons by excited electrons
  • The gamma rays come from an excited nucleus that is trying to get back to its ground state
  • The nucleus could be in an excited state either from a collision with another particle or because it is a nucleus left over from a previous radioactive decay
  • A nucleus may remain in an excited state for some time before it emits a gamma ray. The nucleus is then said to be in a metastable state and is called an isomer
  • The nucleus can also return to its ground state by a process called internal conversion, where no gamma rays are emitted
  • The nucleus interacts with an electron and loses its energy in that way
  • The electron then loses energy as an x-ray
  • X-rays come from atom-electron interactions, while gamma rays come from nuclear processes
24
Q

conservation of nucleon number

A

• The following laws all hold true:
- Law of Conservation of Energy
- Law of Conservation of Linear Momentum
- Law of Conservation of Angular Momentum
- Conservation of Electric charge
- Law of Conservation of Nucleon Number
• The total number of nucleons stays the same in any decay, but the different types can change