Boron-8 is a radioisotope of the chemical element boron, which, in addition to the element-specific 5 protons, has 3 neutrons in the atomic nucleus, resulting in the mass number 8. The very short-lived, unstable and therefore radioactive nuclide, which can only be produced artificially, has no practical significance; the study of 8B serves exclusively academic purposes and experimental research.
The proton-rich isotope was first described in 1950 as a product of the irradiation of 10BF3 with protons (32 MeV) [1].
The 8B nucleus is of great interest for astrophysics, for example, as it is the main source of solar neutrinos with energies above 2 MeV; the boron neutrinos are far fewer in number, but their much higher energy makes detection easier. The β+/EE decay α spectrum occurring for this nuclide has been studied in detail on numerous occasions [3,4].
The nucleus of the proton-rich nuclide 8B is believed to have a 1-proton halo structure.
See also: list of Boron isotopes.
Half-life T½ = 771.17(94) ms respectively 7.7117 × 10-1 seconds s.
Decay mode | Daughter | Probability | Decay energy | γ energy (intensity) |
---|---|---|---|---|
EC β+ | 8Be | 100 % | 17.9798(10) MeV | |
β+, α | 4He |
A newer and more precise value for the half-life was published in 2020 and adopted here [5]. The older value of T1/2 = 0.770(3) s can be found in the relevant literature.
Boron-8 does not occur as a natural decay product of other radioisotopes; Corresponding starting nuclides are not known.
In stellar nucleosynthesis, the nuclide 8B occurs in the proton-proton III branch (p-p chain, T > 23 x 10 6 °C) to:
3He + 4He → 7Be + γ; + 1.56 MeV,
7Be + 1H → 8B + γ + 0.14 MeV.
This reaction plays an important role in nuclear astrophysics and has a direct impact on both the high-energy component of solar neutrinos [3].
Z | Isotone N = 3 | Isobar A = 8 |
---|---|---|
1 | 4H | |
2 | 5He | 8He |
3 | 6Li | 8Li |
4 | 7Be | 8Be |
5 | 8B | 8B |
6 | 9C | 8C |
7 | 10N | |
8 | 11O |
[1] - Luis W. Alvarez:
Three New Delayed Alpha-Emitters of Low Mass.
In: Physical Review, 80, 519, (1950), DOI 10.1103/PhysRev.80.519.
[2] - G. A. Korolev, A. V. Dobrovolsky, A. G. Inglessi et al.:
Halo structure of 8B determined from intermediate energy proton elastic scattering in inverse kinematics.
In: Physics Letters B, 780, 200-204, (2018), DOI 10.1016/j.physletb.2018.03.013.
[3] - R. Buompane et al.:
Test measurement of 7Be(p,γ)8B with the recoil mass separator ERNA.
In: The European Physical Journal A, 54, 92, (2018), DOI 10.1140/epja/i2018-12522-6.
[4] - S. Viñals et al.:
The experiments to determine the electron capture and β-decay of 8B into the highly excited states of 8Be.
In: Journal of Physics: Conference Series, 1643, 012130, (2020), DOI 10.1088/1742-6596/1643/1/012130.
[5] - S. Viñals et al.:
The Most Accurate Determination of the 8B Half-life.
In: Acta Physica Polonica B, 51, 3, (2020), DOI 10.5506/APhysPolB.51.717.
[6] - J. C. Zamora et al.:
Direct fusion measurement of the 8B proton-halo nucleus at near-barrier energies.
In: Physics Letters B, 816, 136256, (2021), DOI 10.1016/j.physletb.2021.136256.
Last update: 2024-10-24
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