Publisher： Edp Sciences
E-ISSN： 2100-014x|38|issue|17008-17008
ISSN： 2100-014x
Source： EPJ Web of Conference, Vol.38, Iss.issue, 2012-12, pp. : 17008-17008
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Abstract
Synthesis of iron group chemical elements is considered for the ultra-magnetized astrophysical plasma in supernovae. Maximum of nucleosynthesis products is shown to shift towards smaller mass numbers approaching titanium due to magnetic modification of nuclear structure. The results are corroborated with an excess of 44Ti revealed from the INTEGRAL mission data.
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