Neon-32 is a radioisotope of the chemical element neon, which has 22 neutrons in its atomic nucleus in addition to the element-specific 10 protons; the sum of the number of these atomic nucleus building blocks results in a mass number of 32. The very short-lived, only artificially produced, unstable and thus radioactive nuclide has no practical significance; the study of 32Ne is exclusively for academic purposes and experimental research.
Neon-32 belongs to a rare group of isotopes - the so-called exotic nuclei, whose atomic nuclei are strongly deformed. These nuclides are always on the verge of breaking apart because they contain too many or too few neutrons. However, their study is problematic because exotic nuclei are very difficult to produce and have a very short lifespan [cf. Doornenbal et al. 2009; Murray et al. 2019].
The first observation of the neutron-rich isotope was reported in 1990: According to this, neon-32 was created by fragmenting a tantalum sample with a 44 MeV/u beam of calcium-48 ions [1].
See also: List of individual Neon isotopes (and general data sources).
Half-life T½ = 3.5(9) ms respectively 3.5 × 10-3 seconds s.
| Decay mode | Daughter | Probability | Decay energy | γ energy (intensity) |
|---|---|---|---|---|
| β- | 32Na | 100 % | 18.360(500) MeV | |
| β-, n | 31Na | ? | 16.682(503) MeV | |
| β-, 2n | 30Na | ? |
| Z | Isotone N = 22 | Isobar A = 32 |
|---|---|---|
| 9 | 31F | |
| 10 | 32Ne | 32Ne |
| 11 | 33Na | 32Na |
| 12 | 34Mg | 32Mg |
| 13 | 35Al | 32Al |
| 14 | 36Si | 32Si |
| 15 | 37P | 32P |
| 16 | 38S | 32S |
| 17 | 39Cl | 32Cl |
| 18 | 40Ar | 32Ar |
| 19 | 41K | 32K |
| 20 | 42Ca | |
| 21 | 43Sc | |
| 22 | 44Ti | |
| 23 | 45V | |
| 24 | 46Cr | |
| 25 | 47Mn | |
| 26 | 48Fe | |
| 27 | 49Co | |
| 28 | 50Ni |
[1] - D. Guillemaud-Mueller, J. C. Jacmart, E. Kashy et al.:
Particle stability of the isotopes 26O and 32Ne in the reaction 44 MeV/nucleon 48Ca+Ta.
In: Physical Review C, 41, 937, (1990), DOI 10.1103/PhysRevC.41.937.
[2] - P. Doornenbal et al.:
Spectroscopy of 32Ne and the Island of Inversion.
In: Physical Review Letters, (2009), DOI 10.1103/PhysRevLett.103.032501.
[3] - I. Murray, M. MacCormick, D. Bazin et al.:
Spectroscopy of strongly deformed 32Ne by proton knockout reactions.
In: Physical Review C, 99, 011302(R), (2019), DOI 10.1103/PhysRevC.99.011302.
Last update: 2024-10-22
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