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Nitrogen-13

From Wikipedia, the free encyclopedia
Isotope of nitrogen
Nitrogen-13, 13N
General
Symbol13N
Namesnitrogen-13, 13N, N-13
Protons(Z)7
Neutrons(N)6
Nuclide data
Half-life(t1/2)9.97 min
Parent isotopes13O (β+)
Decay modes
Decay modeDecay energy (MeV)
β+1.2003
Isotopes of nitrogen
Complete table of nuclides

Nitrogen-13 (13N) is aradioisotope ofnitrogen used inpositron emission tomography (PET). It has ahalf-life of a little under ten minutes, so it must be made at the PET site. Acyclotron may be used for this purpose.

Nitrogen-13 is used to tagammonia molecules for PETmyocardial perfusion imaging.

Production

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Nitrogen-13 is used in medical PET imaging in the form of13N-labelled ammonia. It can be produced with a medical cyclotron, using a target of pure water with a trace amount of ethanol. The reactants are oxygen-16 (present as H2O) and a proton, and the products are nitrogen-13 and an alpha particle (helium-4).

1H +16O →13N +4He

The proton must be accelerated to have total energy greater than 5.66 MeV. This is the threshold energy for this reaction,[1] as it isendothermic (i.e., the mass of the products is greater than the reactants, so energy needs to be supplied which is converted to mass). For this reason, the proton needs to carry extraenergy to induce thenuclear reaction.

The energy difference is actually 5.22 MeV, but if the proton only supplied this energy, the reactants would be formed with nokinetic energy. Asmomentum must beconserved, the true energy that needs to be supplied by the proton is given by:

K=(1+m/M)|E|{\displaystyle K=(1+m/M)|E|}

wherem{\displaystyle m} is the mass of4He andM{\displaystyle M} is the mass of13N ; thereforem/M0.308{\displaystyle m/M\approx 0.308}. The presence of ethanol (at a concentration of ~5mM) in aqueous solution allows the convenient formation of ammonia as nitrogen-13 is produced. Other routes of producing13N-labelled ammonia exist, some of which facilitate co-generation of other light radionuclides for diagnostic imaging.[2][3]

The N-13 role in the CNO cycle.

Nitrogen-13 plays a significant role in theCNO cycle, which is the dominant source of energy inmain-sequence stars more massive than 1.5 times themass of theSun.[4]

Lightning may have a role in the production of nitrogen-13.[5][6]

External links

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References

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  1. ^Islam, M. R.; Beni, M. S.; Ng, C; et al. (2022)."Proton range monitoring using13N peak for proton therapy applications".PLOS ONE.17 (2): e0263521-1–e0263521-18.doi:10.1371/journal.pone.0263521.PMC 8846528.PMID 35167589.
  2. ^Biricova, Veronika; Kuruc, Jozef (2007)."Synthesis of the radiopharmaceuticals for positron emission tomography". U.S. Department of Energy, Office of Scientific and Technical Information. Retrieved4 August 2022.
  3. ^Yokell, Daniel L.; Rice, Peter A.; Neelamegam, Ramesh; El Fakhri, Georges (13 May 2020)."Development, validation and regulatory acceptance of improved purification and simplified quality control of [13N] Ammonia".EJNMMI Radiopharm Chem.5 (11): 11.doi:10.1186/s41181-020-00097-7.PMC 7221112.PMID 32405797.
  4. ^Phillips, A.C. (1994).The Physics of Stars. John Wiley & Sons.ISBN 0-471-94057-7.
  5. ^"Lightning, with a chance of antimatter".Phys.org. ScienceX. November 22, 2017. RetrievedNovember 24, 2017.The gamma rays emitted in lightning have enough energy to knock a neutron out of atmospheric nitrogen
  6. ^Castelvecchi, Davide (November 22, 2017)."Lightning makes new isotopes".Nature.doi:10.1038/nature.2017.23033. RetrievedNovember 29, 2017.


Lighter:
nitrogen-12
Nitrogen-13 is an
isotope ofnitrogen
Heavier:
nitrogen-14
Decay product of:
oxygen-13(electron capture)
Decay chain
of nitrogen-13
Decays to:
carbon-13(EC)
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