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arXiv 0811.4650astro-ph
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来自“塌缩”的核合成产额

Nucleosynthetic Yields from "Collapsars"

Gabriel Rockefeller, Christopher L. Fryer, Patrick Young, Michael Bennett, Steven Diehl, Falk Herwig, Raphael Hirschi, Aimee Hungerford, Marco Pignatari, Georgi… 展开作者

Gabriel Rockefeller, Christopher L. Fryer, Patrick Young, Michael Bennett, Steven Diehl, Falk Herwig, Raphael Hirschi, Aimee Hungerford, Marco Pignatari, Georgios Magkotsios, Francis X. Timmes

摘要:

伽马射线暴的“超新星”引擎利用普通超新星的失败和黑洞的形成作为其能量来源。在这里,我们提出的第一个三维模拟的结果,一个大质量的恒星坍缩到一个黑洞,包括随后的吸积和爆炸。爆炸显着不同的轴对称的情况下获得的二维模拟,这对核合成产量的重要后果。我们比较的核合成产额的超新星。计算产量从三维爆炸需要新的策略后处理核合成,我们讨论NuGrid的三维产量计划。

英文摘要:

The "collapsar" engine for gamma-ray bursts invokes as its energy source the failure of a normal supernova and the formation of a black hole. Here we present the results of the first three-dimensional simulation of the collapse of a massive star down to a black hole, including the subsequent accretion and explosion. The explosion differs significantly from the axisymmetric scenario obtained in two-dimensional simulations; this has important consequences for the nucleosynthetic yields. We compare the nucleosynthetic yields to those of hypernovae. Calculating yields from three-dimensional explosions requires new strategies in post-process nucleosynthesis; we discuss NuGrid's plan for three-dimensional yields.

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