Alpha nuclide

An alpha nuclide is a nuclide that consists of an integer number of alpha particles. Alpha nuclides have equal, even numbers of protons and neutrons; they are important in stellar nucleosynthesis since the energetic environment within stars is amenable to fusion of alpha particles into heavier nuclei.[1][2] Stable alpha nuclides, and stable decay products of radioactive alpha nuclides, are some of the most common metals in the universe.

Alpha nuclide is also shorthand for alpha radionuclide, referring to those radioactive isotopes that undergo alpha decay and thereby emit alpha particles.[3]

List of alpha nuclides

Alpha number	nuclide	Stable/radioactive	decay mode	half-life[4]	product(s) of decay (bold is stable)
1	⁴ ₂He	Stable
2	⁸ ₄Be	Radioactive	α	8.19(37)×10⁻¹⁷ s	⁴ ₂He
3	¹² ₆C	Stable
4	¹⁶ ₈O	Stable
5	²⁰ ₁₀Ne	Stable
6	²⁴ ₁₂Mg	Stable
7	²⁸ ₁₄Si	Stable
8	³² ₁₆S	Stable
9	³⁶ ₁₈Ar	Observationally Stable
10	⁴⁰ ₂₀Ca	Observationally Stable
11	⁴⁴ ₂₂Ti	Radioactive	EC	60.0(11) y	⁴⁴ ₂₁Sc → ⁴⁴ ₂₀Ca
12	⁴⁸ ₂₄Cr	Radioactive	β⁺	21.56(3) h	⁴⁸ ₂₃V → ⁴⁸ ₂₂Ti
13	⁵² ₂₆Fe	Radioactive	β⁺	8.275(8) h	⁵² ₂₅Mn → ⁵² ₂₄Cr
14	⁵⁶ ₂₈Ni	Radioactive	β⁺	6.075(10) d	⁵⁶ ₂₇Co → ⁵⁶ ₂₆Fe
15	⁶⁰ ₃₀Zn	Radioactive	β⁺	2.38(5) min	⁶⁰ ₂₉Cu → ⁶⁰ ₂₈Ni

The nuclear binding energy of alpha nuclides heavier than zinc-60 (beginning with germanium-64) is too large for them be formed by fusion processes. As of 2018, the heaviest known alpha nuclide is xenon-108.[5]

gollark: https://qph.fs.quoracdn.net/main-qimg-5b0690e302a38cf2a8068158199e7a21-c

gollark: https://www.quora.com/How-do-you-find-the-positive-integer-solutions-to-frac-x-y+z-+-frac-y-z+x-+-frac-z-x+y-4?share=1 is extremely.

gollark: I know of simple to pose problems with really hard solutions, but not the other way round.

gollark: Hmm. It seems to have realized that there is actually a really simple solution. Sad.

gollark: I could try using RIES for it.

References

Appenzeller; Harwit; Kippenhahn; Strittmatter; Trimble, eds. (1998). Astrophysics Library (3rd ed.). New York: Springer.
Carroll, Bradley W. & Ostlie, Dale A. (2007). An Introduction to Modern Stellar Astrophysics. Addison Wesley, San Francisco. ISBN 978-0-8053-0348-3.
John Avison (November 2014). The World of Physics. Nelson Thornes. pp. 397–. ISBN 978-0-17-438733-6.
Audi, G.; Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S. (2017). "The NUBASE2016 evaluation of nuclear properties" (PDF). Chinese Physics C. 41 (3): 030001. Bibcode:2017ChPhC..41c0001A. doi:10.1088/1674-1137/41/3/030001.
Auranen, K.; et al. (2018). "Superallowed α decay to doubly magic ¹⁰⁰Sn" (PDF). Physical Review Letters. 121 (18): 182501. doi:10.1103/PhysRevLett.121.182501. PMID 30444390.

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[Appenzeller-1] Appenzeller; Harwit; Kippenhahn; Strittmatter; Trimble, eds. (1998). Astrophysics Library (3rd ed.). New York: Springer.

[Ostlie-2] Carroll, Bradley W. & Ostlie, Dale A. (2007). An Introduction to Modern Stellar Astrophysics. Addison Wesley, San Francisco. ISBN 978-0-8053-0348-3.

[3] John Avison (November 2014). The World of Physics. Nelson Thornes. pp. 397–. ISBN 978-0-17-438733-6.

[NUBASE2016-4] Audi, G.; Kondev, F. G.; Wang, M.; Huang, W. J.; Naimi, S. (2017). "The NUBASE2016 evaluation of nuclear properties" (PDF). Chinese Physics C. 41 (3): 030001. Bibcode:2017ChPhC..41c0001A. doi:10.1088/1674-1137/41/3/030001.

[Xe108-5] Auranen, K.; et al. (2018). "Superallowed α decay to doubly magic ¹⁰⁰Sn" (PDF). Physical Review Letters. 121 (18): 182501. doi:10.1103/PhysRevLett.121.182501. PMID 30444390.