The half-lives of Al26m, Cl34, Co54 and Cu58
References (17)
- et al.
Nuclear Physics
(1965) - et al.
Nuclear Physics
(1962) - et al.
Nuclear Physics
(1958) - et al.
Nuclear Physics
(1958) - et al.
Physica
(1958) - et al.
Phys. Lett.
(1962) Phys. Lett.
(1964)- et al.
Phys. Rev.
(1978)
Cited by (26)
The Mg isotope composition of presolar silicate grains from red giant stars
2014, Geochimica et Cosmochimica ActaCitation Excerpt :Production of 26Al and that of its daughter isotope 26Mg via the Mg–Al reaction chain [more precisely via 25Mg(p,γ)26Al(β+)26Mg] occurs during H-burning (Arnould et al., 1999; Mowlavi and Meynet, 2000; Karakas and Lattanzio, 2003). 26Al produced during H-burning is present in two states, the ground state (∼80%; Iliadis et al., 2010) and an isomeric state (∼20%), with different half-lifes (705,000 years and 6.37 s, respectively (Freeman et al., 1965; Norris et al., 1983). Thus, the actual increase in the surface abundance of 26Al and 26Mg does not only depend on the rate of proton capture on 25Mg but also on the rate of proton capture on 26Al [26Al(p,γ)27Si(β+)27Al] and 26Mg [26Mg(p,γ)27Al] in the H-burning shell as well as on the efficiency of material transport from the site of previous H-burning to the stellar surface during dredge up events.
Nuclear Data Sheets for A = 34
2012, Nuclear Data SheetsNuclear Data Sheets for A = 58
2010, Nuclear Data SheetsNuclear data sheets for <sup>58</sup> Cu*
1999, Nuclear Data SheetsNuclear data sheets for A = 58
1997, Nuclear Data SheetsNuclear Data Sheets update for A=58. Last evaluation: L. K. Peker Nuclear Data Sheets 42, 457 (1984)
1990, Nuclear Data Sheets
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