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A Borromean nucleus is an atomic nucleus comprising three bound components in which any subsystem of two components is unbound. [1] This has the consequence that if one component is removed, the remaining two comprise an unbound resonance, so that the original nucleus is split into three parts. [2]

The name is derived from the Borromean rings, a system of three linked rings in which no pair of rings is linked. [2]

Examples of Borromean nuclei

Many Borromean nuclei are light nuclei near the nuclear drip lines that have a nuclear halo and low nuclear binding energy. For example, the nuclei 6
, 11
, and 22
each possess a two- neutron halo surrounding a core containing the remaining nucleons. [2] [3] These are Borromean nuclei because the removal of either neutron from the halo will result in a resonance unbound to one- neutron emission, whereas the dineutron (the particles in the halo) is itself an unbound system. [1] Similarly, 17
is a Borromean nucleus with a two-proton halo; both the diproton and 16
are unbound. [4]

Additionally, 9
is a Borromean nucleus comprising two alpha particles and a neutron; [3] the removal of any one component would produce one of the unbound resonances 5
, 5
, or 8

Several Borromean nuclei such as 9
and the Hoyle state (an excited resonance in 12
) play an important role in nuclear astrophysics. Namely, these are three-body systems whose unbound components (formed from 4
) are intermediate steps in the triple-alpha process; this limits the rate of production of heavier elements, for three bodies must react nearly simultaneously. [3]

Borromean nuclei consisting of more than three components can also exist. These also lie along the drip lines; for instance, 8
is a five-body Borromean system with a four-neutron halo. [5] It is also possible that nuclides produced in the alpha process (such as 12
and 16
) may be clusters of alpha particles, having a similar structure to Borromean nuclei. [2]

As of 2012, the heaviest known Borromean nucleus is 29
. [6] Heavier species along the neutron drip line have since been observed; these and undiscovered heavier nuclei along the drip line are also likely to be Borromean nuclei with varying numbers (3, 5, 7, or more) of bodies. [5]

See also


  1. ^ a b Id Betan, R. M. (2017). "Cooper pairs in the Borromean nuclei 6He and 11Li using continuum single particle level density". Nuclear Physics A. 959: 147–148. arXiv: 1701.08099. Bibcode: 2017NuPhA.959..147I. doi: 10.1016/j.nuclphysa.2017.01.004. S2CID  119243017.
  2. ^ a b c d Manton, N.; Mee, N. (2017). "Nuclear Physics". The Physical World: An Inspirational Tour of Fundamental Physics. Oxford University Press. pp. 387–389. doi: 10.1093/oso/9780198795933.003.0012. ISBN  978-0-19-879611-4. LCCN  2017934959.
  3. ^ a b c Vaagen, J. S.; Gridnev, D. K.; Heiberg-Andersen, H.; et al. (2000). "Borromean Halo Nuclei" (PDF). Physica Scripta. T88 (1): 209–213. Bibcode: 2000PhST...88..209V. doi: 10.1238/Physica.Topical.088a00209. S2CID  121095106.
  4. ^ Oishi, T.; Hagino, K.; Sagawa, H. (2010). "Diproton correlation in the proton-rich Borromean nucleus 17Ne". Physical Review C. 82 (6): 066901–1–066901–6. arXiv: 1007.0835. doi: 10.1103/PhysRevC.82.069901.
  5. ^ a b Riisager, K. (2013). "Halos and related structures". Physica Scripta. 2013 (14001): 014001. arXiv: 1208.6415. Bibcode: 2013PhST..152a4001R. doi: 10.1088/0031-8949/2013/T152/014001. S2CID  119290542.
  6. ^ Gaudefroy, L.; Mittig, W.; Orr, N. A.; et al. (2012). "Direct Mass Measurements of 19B, 22C, 29F, 31Ne, 34Na and Other Light Exotic Nuclei". Physical Review Letters. 109 (20): 202503–1–202503–5. arXiv: 1211.3235. doi: 10.1103/PhysRevLett.109.202503. PMID  23215476. S2CID  21166319.