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Isotopes of fluorine

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Although fluorine (F) has 18 known isotopes from 14F to 31F and one isomer (18mF), only one of these isotopes is stable, that is, fluorine-19; as such, it is a monoisotopic element. The longest-lived radioisotope is 18F with a half-life of 109.771 minutes. All other isotopes have half-lives under a minute, the majority under a second, making fluorine a mononuclidic element as well. The least stable isotope is 15F, whose half-life is 4.1 x 10−22 seconds, corresponding to a spectral linewidth of about 1 MeV. Only 14F has an unknown half-life.

Standard atomic mass: 18.9984032(5) u

Fluorine-18

The nuclide 18F is the radionuclide of fluorine with the longest half-life, 109.771 minutes, allowing it to serve commercially as an important source of positrons. Its major use is for the production of the radiopharmaceutical fludeoxyglucose for positron emission tomography scanning in medicine.

Like all positron-emissing radioisotopes, 18F also has a probability to decay by electron capture. In this case, 18F decays 96.86 (19)% of the time by beta plus (positron emission), and 3.14 (19)% by electron capture.[1]

Fluorine-19

Fluorine-19, the only stable isotope of fluorine. Its abundance is 100%; no other isotopes of fluorine exist in significant quantities. Its binding energy is 147801 keV. Fluorine-19 is NMR-active, so it is used in fluorine-19 NMR spectroscopy.

Fluorine-20

Fluorine-20, is one of the more unstable isotopes of fluorine. It has a half-life of 11.07 seconds and undergoes beta decay, transforming into its daughter nuclide 20Ne. Its specific radioactivity is 1.885 x 109 TBq/g and has a lifetime of 15.87 seconds.

Fluorine-21

Fluorine-21, as with fluorine-20, is also one of the more unstable isotopes of this element. It has a half-life of 4.158 seconds. It undergoes beta decay as well which leaves behind a daughter nuclei of 21Ne. Its specific radioactivity is 4.78 x 109 TBq/g.

Table

nuclide
symbol
Z(p) N(n)  
isotopic mass (u)
 
half-life decay mode(s)[2] daughter
isotope(s)[n 1]
nuclear
spin
representative
isotopic
composition
(mole fraction)
range of natural
variation
(mole fraction)
excitation energy
14F 9 5 14.03506(43)# p 13O 2-#
15F 9 6 15.01801(14) 410(60)×10−24 s
[1.0(2) MeV]
p 14O (1/2+)
16F 9 7 16.011466(9) 11(6)×10−21 s
[40(20) keV]
p 15O 0-
17F 9 8 17.00209524(27) 64.49(16) s β+ 17O 5/2+
18F[n 2] 9 9 18.0009380(6) 109.771(20) min β+ 18O 1+
18mF 1121.36(15) keV 162(7) ns 5+
19F 9 10 18.99840322(7) Stable 1/2+ 1.0000
20F 9 11 19.99998132(8) 11.163(8) s β 20Ne 2+
21F 9 12 20.9999490(19) 4.158(20) s β 21Ne 5/2+
22F 9 13 22.002999(13) 4.23(4) s β (89.0%) 22Ne 4+,(3+)
β, n (11.0%) 21Ne
23F 9 14 23.00357(9) 2.23(14) s β (86.0%) 23Ne (3/2,5/2)+
β, n (14.0%) 22Ne
24F 9 15 24.00812(8) 400(50) ms β (94.1%) 24Ne (1,2,3)+
β, n (5.9%) 23Ne
25F 9 16 25.01210(11) 50(6) ms β (76.0%) 25Ne (5/2+)#
β, n (24.0%) 24Ne
26F 9 17 26.01962(18) 9.6(8) ms β (68.0%) 26Ne 1+
β, n (32.0%) 25Ne
27F 9 18 27.02676(40) 4.9(2) ms β 27Ne 5/2+#
28F 9 19 28.03567(55)# <40 ns n 27F
29F 9 20 29.04326(62)# 2.6(3) ms β 29Ne 5/2+#
30F 9 21 30.05250(64)# <260 ns
31F 9 22 31.06043(64)# 1# ms [>260 ns] 5/2+#
  1. ^ Bold for stable isotopes
  2. ^ Has medicinal uses

Notes

  • Values marked # are not purely derived from experimental data, but at least partly from systematic trends. Spins with weak assignment arguments are enclosed in parentheses.
  • Uncertainties are given in concise form in parentheses after the corresponding last digits. Uncertainty values denote one standard deviation, except isotopic composition and standard atomic mass from IUPAC which use expanded uncertainties.

References

  • Isotope masses from:
    • G. Audi, A. H. Wapstra, C. Thibault, J. Blachot and O. Bersillon (2003). "The NUBASE evaluation of nuclear and decay properties" (PDF). Nuclear Physics A. 729: 3–128. Bibcode:2003NuPhA.729....3A. doi:10.1016/j.nuclphysa.2003.11.001.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  • Isotopic compositions and standard atomic masses from:
  • Half-life, spin, and isomer data selected from the following sources. See editing notes on this article's talk page.
  1. ^ [1] F-18 branching ratio for positron emission vs. EC
  2. ^ http://www.nucleonica.net/unc.aspx