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Calcium-48

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Isotope of calcium "Ca-48" redirects here. The term may also refer to California's 48th congressional district.
Calcium-48, Ca
A glass container with 2 g of
CaCO
3
General
SymbolCa
Namescalcium-48, 48Ca, Ca-48
Protons (Z)20
Neutrons (N)28
Nuclide data
Natural abundance0.187%
Half-life (t1/2)(6.4
−0.6
−0.9) × 10 a
Isotope mass47.952534(4) Da
Isotopes of calcium
Complete table of nuclides

Calcium-48 is a scarce isotope of calcium containing 20 protons and 28 neutrons. It makes up 0.187% of natural calcium by mole fraction. Although it is unusually neutron-rich for such a light nucleus, its beta decay is extremely hindered, and so the only radioactive decay pathway that it has been observed to undergo is the extremely rare process of double beta decay. Its half-life is about 64 billion billion (6.4×10) years, so for all practical purposes it can be treated as stable. One factor contributing to this unusual stability is that 20 and 28 are both magic numbers, making Ca a "doubly magic" nucleus.

Since Ca is both practically stable and neutron-rich, it is a valuable starting material for the production of new nuclei in particle accelerators, both by fragmentation and by fusion reactions with other nuclei, for example in the discoveries of the heaviest five elements on the periodic table, from flerovium to oganesson (atomic numbers 114 through 118). Heavier nuclei generally require a greater fraction of neutrons for maximum stability, so neutron-rich starting materials are necessary.

Ca is the lightest nucleus known to undergo double beta decay and the only one simple enough to be analyzed with the sd nuclear shell model. It also releases more energy (4.27 MeV) than any other double beta decay candidate. These properties make it an interesting probe of nuclear structure models and a promising candidate in the ongoing search for neutrinoless double beta decay.

See also

References

  1. Coursey, J. S.; D. J. Schwab; R. A. Dragoset (February 2005). "Atomic Weights and Isotopic Compositions". NIST Physical Reference Data. Retrieved 2006-10-27.
  2. Arnold, R.; et al. (NEMO-3 Collaboration) (2016). "Measurement of the double-beta decay half-life and search for the neutrinoless double-beta decay of Ca with the NEMO-3 detector". Physical Review D. 93 (11): 112008. arXiv:1604.01710. Bibcode:2016PhRvD..93k2008A. doi:10.1103/PhysRevD.93.112008.
  3. Notani, M.; et al. (2002). "New neutron-rich isotopes, Ne, Na and Si, produced by fragmentation of a 64A MeV Ca beam". Physics Letters B. 542 (1–2): 49–54. Bibcode:2002PhLB..542...49N. doi:10.1016/S0370-2693(02)02337-7.
  4. Oganessian, Yu. Ts.; et al. (October 2006). "Synthesis of the isotopes of elements 118 and 116 in the Cf and Cm + Ca fusion reactions". Physical Review C. 74 (4): 044602. Bibcode:2006PhRvC..74d4602O. doi:10.1103/PhysRevC.74.044602.
  5. Balysh, A.; et al. (1996). "Double Beta Decay of Ca". Physical Review Letters. 77 (26): 5186–5189. arXiv:nucl-ex/9608001. Bibcode:1996PhRvL..77.5186B. doi:10.1103/PhysRevLett.77.5186. PMID 10062737.
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