arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 1208.1328nucl-thastro-ph.SRhep-latnucl-ex
收藏

霍伊尔态的结构和转动

Structure and rotations of the Hoyle state

Evgeny Epelbaum, Hermann Krebs, Timo Lähde, Dean Lee, Ulf-G. Meißner

摘要:

被称为“霍伊尔态”的12 C核的激发态构成了核物理学中最有趣、最困难和最及时的挑战之一,因为它在通过三个α粒子聚变产生碳的过程中发挥着关键作用。红巨星。在这封信中,我们提出了从头晶格计算解开的霍伊尔状态的结构,以及一个低洼的自旋-2旋转激发的证据。对于~(12)C基态和第一激发自旋为2的态,我们发现α团簇是一种紧凑的三角形构型。对于Hoyle态和第二个自旋为2的激发态,我们发现α团簇的构型为“横臂”或钝角三角形。我们还计算了12 C的低激发态之间的电磁跃迁率。

英文摘要:

The excited state of the 12C nucleus known as the "Hoyle state" constitutes one of the most interesting, difficult and timely challenges in nuclear physics, as it plays a key role in the production of carbon via fusion of three alpha particles in red giant stars. In this letter, we present ab initio lattice calculations which unravel the structure of the Hoyle state, along with evidence for a low-lying spin-2 rotational excitation. For the 12C ground state and the first excited spin-2 state, we find a compact triangular configuration of alpha clusters. For the Hoyle state and the second excited spin-2 state, we find a "bent-arm" or obtuse triangular configuration of alpha clusters. We also calculate the electromagnetic transition rates between the low-lying states of 12C.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

↑