Difference between revisions of "Electron capture" - New World Encyclopedia

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{{Nuclear physics}}
'''Electron capture''' (sometimes called '''Inverse Beta Decay''') is a [[decay mode]] for [[isotope]]s that will occur when there are too many [[proton]]s in the [[atomic nucleus|nucleus]] of an [[atom]] and insufficient energy to emit a [[positron]]; however, it continues to be an inviable decay mode for [[radioactive]] isotopes that can decay by [[positron emission]]. If the energy difference between the parent atom and the daughter atom is less than 1.022 [[MeV]], positron emission is forbidden and electron capture is the sole decay mode. For example, [[Rubidium]]-83 will decay to [[Krypton]]-83 solely by electron capture (the energy difference is about 0.9 MeV).
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'''Electron capture''' (sometimes called '''Inverse Beta Decay''') is a [[decay mode]] for [[isotope]]s that will occur when there are too many [[proton]]s in the [[atomic nucleus|nucleus]] of an [[atom]] and insufficient energy to emit a [[positron]]; however, it continues to be an inviable decay mode for [[radioactive]] isotopes that can decay by [[positron emission]]. If the energy difference between the parent atom and the daughter atom is less than 1.022 [[MeV]], positron emission is forbidden and electron capture is the sole decay mode.
  
In this case, one of the orbital [[electron]]s, usually from the K or L [[electron shell]] ('''K-electron capture''', also '''K-capture''', or '''L-electron capture''', '''L-capture'''), is captured by a proton in the nucleus, forming a [[neutron]] and a [[neutrino]]. Since the proton is changed to a neutron, the number of neutrons increases by 1, the number of protons decreases by 1, and the [[atomic mass]] number remains unchanged. By changing the number of protons, electron capture transforms the [[nuclide]] into a new [[chemical element|element]]. The atom moves into an [[excited state]] with the inner shell missing an electron. When transiting to the ground state, the atom will emit an [[X-rays|X-ray photon]] (a type of [[electromagnetic radiation]]) and/or [[Auger electrons]].
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== Examples and explanation ==
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Consider, for example, [[rubidium]]-83, which will decay to [[krypton]]-83 solely by electron capture (the energy difference is about 0.9 MeV).
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In this case, one of the orbital [[electron]]s, usually from the K or L [[electron shell]] ('''K-electron capture''', also '''K-capture''', or '''L-electron capture''', '''L-capture'''), is captured by a proton in the nucleus, forming a [[neutron]] and a [[neutrino]]. Since the proton is changed to a neutron, the number of neutrons increases by 1, the number of protons decreases by 1, and the [[atomic mass]] number remains unchanged. By changing the number of protons, electron capture transforms the [[nuclide]] into a new [[chemical element|element]]. The atom moves into an [[excited state]] with the inner shell missing an electron. When transiting to the ground state, the atom will emit an [[X-ray|X-ray photon]] and/or [[Auger electrons]].
  
 
: <math>\mathrm{p}^+  + \mathrm{e}^- \rightarrow\mathrm{n} + {\nu}_e \,</math>
 
: <math>\mathrm{p}^+  + \mathrm{e}^- \rightarrow\mathrm{n} + {\nu}_e \,</math>
  
examples:  
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Additional examples:  
 
::{| width="50%"
 
::{| width="50%"
 
| <math>\mathrm{{}^{26}_{13}Al}+\mathrm{e}^- \rightarrow\mathrm{{}^{26}_{12}Mg}+{\nu}_e</math>
 
| <math>\mathrm{{}^{26}_{13}Al}+\mathrm{e}^- \rightarrow\mathrm{{}^{26}_{12}Mg}+{\nu}_e</math>
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Radioactive isotopes which decay by pure electron capture can, in theory, be inhibited from radioactive decay if they are fully [[ion]]ized ("stripped" is sometimes used to describe such ions). It is hypothesized that such elements, if formed by the [[r-process]] in exploding [[supernova]]e, are ejected fully ionized and so do not undergo radioactive decay as long as they do not encounter electrons in outer space. Anomalies in elemental distributions are thought to be partly a result of this effect on electron capture.
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Around the elements in the middle of the [[Periodic Table]], isotopes that are lighter than stable isotopes of the same element tend to decay through electron capture, while isotopes heavier than the stable ones decay with a process called [[negative beta decay]]. A good example of this effect would be silver, as its light isotopes use electron capture and the heavier ones decay by negative beta emission.
  
[[Chemical bonds]] can also affect the rate of electron capture to a small degree (generally less than 1%) depending on the proximity of electrons to the nucleus.[http://www.nature.com/news/2004/040913/pf/040913-24_pf.html]
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== Inhibition of electron capture ==
  
Around the elements in the middle of the periodic table, isotopes that are lighter than stable isotopes of the same element tend to decay through electron capture, while isotopes heavier than the stable ones decay with a process called [[negative beta decay]]. A good example of this effect would be silver, as its light isotopes use electron capture and the heavier ones decay by negative beta emission.
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Radioactive isotopes that decay by pure electron capture can, in theory, be inhibited from radioactive decay if they are fully [[ion]]ized ("stripped" is sometimes used to describe such ions). It is hypothesized that such elements, if formed by the [[r-process]] in exploding [[supernova]]e, are ejected fully ionized and so do not undergo radioactive decay as long as they do not encounter electrons in outer space. Anomalies in elemental distributions are thought to be partly a result of this effect on electron capture.
  
 
== See also ==
 
== See also ==

Revision as of 13:35, 25 October 2007


Nuclear physics
CNO Cycle.svg
Radioactive decay
Nuclear fission
Nuclear fusion

Electron capture (sometimes called Inverse Beta Decay) is a decay mode for isotopes that will occur when there are too many protons in the nucleus of an atom and insufficient energy to emit a positron; however, it continues to be an inviable decay mode for radioactive isotopes that can decay by positron emission. If the energy difference between the parent atom and the daughter atom is less than 1.022 MeV, positron emission is forbidden and electron capture is the sole decay mode.

Examples and explanation

Consider, for example, rubidium-83, which will decay to krypton-83 solely by electron capture (the energy difference is about 0.9 MeV).

In this case, one of the orbital electrons, usually from the K or L electron shell (K-electron capture, also K-capture, or L-electron capture, L-capture), is captured by a proton in the nucleus, forming a neutron and a neutrino. Since the proton is changed to a neutron, the number of neutrons increases by 1, the number of protons decreases by 1, and the atomic mass number remains unchanged. By changing the number of protons, electron capture transforms the nuclide into a new element. The atom moves into an excited state with the inner shell missing an electron. When transiting to the ground state, the atom will emit an X-ray photon and/or Auger electrons.

Additional examples:

Around the elements in the middle of the Periodic Table, isotopes that are lighter than stable isotopes of the same element tend to decay through electron capture, while isotopes heavier than the stable ones decay with a process called negative beta decay. A good example of this effect would be silver, as its light isotopes use electron capture and the heavier ones decay by negative beta emission.

Inhibition of electron capture

Radioactive isotopes that decay by pure electron capture can, in theory, be inhibited from radioactive decay if they are fully ionized ("stripped" is sometimes used to describe such ions). It is hypothesized that such elements, if formed by the r-process in exploding supernovae, are ejected fully ionized and so do not undergo radioactive decay as long as they do not encounter electrons in outer space. Anomalies in elemental distributions are thought to be partly a result of this effect on electron capture.

See also

References
ISBN links support NWE through referral fees

  • Krane, Kenneth S., and David Halliday. 1988. Introductory Nuclear Physics. New York: Wiley. ISBN 047180553X.
  • Martin, Brian. 2006. Nuclear and Particle Physics: An Introduction. Hoboken, NJ: Wiley. ISBN 0470025328.
  • Poenaru, D. N. 1996. Nuclear Decay Modes. Fundamental and Applied Nuclear Physics Series. Philadelphia: Institute of Physics. ISBN 0750303387.
  • Seiden, Abraham. 2004. Particle Physics: A Comprehensive Introduction. San Francisco, CA: Addison Wesley. ISBN 0805387366.
  • Tipler, Paul and Ralph Llewellyn. 2002. Modern Physics. 4th ed. New York, NY: W.H. Freeman. ISBN 0-7167-4345-0.
  • Turner, James E. 1995. Atoms, Radiation, and Radiation Protection. 2nd ed. New York: Wiley. ISBN 0471595810.

External links

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