Overview of stellar nucleosynthesis in explosive environments and recent experimental highlights

IF 2.6 3区 物理与天体物理 Q2 PHYSICS, NUCLEAR
H. Jayatissa, M. L. Avila, M. Alruwaili, M. Anastasiou, K. Bhatt, K. A. Chipps, C. Fougères, A. M. Laird, E. Lopez-Saavedra, K. E. Rehm, D. Santiago-Gonzalez
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引用次数: 0

Abstract

Explosive stellar environments such as neutron star mergers, supernovae and X-ray bursts contribute significantly to the synthesis of many chemical elements known in the universe. Understanding the underlying explosion mechanisms and stellar conditions, as well as the observed signatures of chemical elements at a variety of these sites require a considerable effort from the nuclear physics community. An overview of several explosive stellar environments have been summarized, along with brief highlights of recent experimental efforts to better constrain the nucleosynthesis from these environments using recent advances of rare isotope beam facilities and measurement techniques.

爆炸环境下恒星核合成的概述和最近的实验亮点
爆炸的恒星环境,如中子星合并、超新星和x射线爆发,对宇宙中已知的许多化学元素的合成做出了重大贡献。了解潜在的爆炸机制和恒星条件,以及在各种这些地点观察到的化学元素的特征,需要核物理学界付出相当大的努力。总结了几种爆炸性恒星环境的概况,并简要介绍了最近利用稀有同位素束设施和测量技术的最新进展更好地限制这些环境中核合成的实验努力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
The European Physical Journal A
The European Physical Journal A 物理-物理:核物理
CiteScore
5.00
自引率
18.50%
发文量
216
审稿时长
3-8 weeks
期刊介绍: Hadron Physics Hadron Structure Hadron Spectroscopy Hadronic and Electroweak Interactions of Hadrons Nonperturbative Approaches to QCD Phenomenological Approaches to Hadron Physics Nuclear and Quark Matter Heavy-Ion Collisions Phase Diagram of the Strong Interaction Hard Probes Quark-Gluon Plasma and Hadronic Matter Relativistic Transport and Hydrodynamics Compact Stars Nuclear Physics Nuclear Structure and Reactions Few-Body Systems Radioactive Beams Electroweak Interactions Nuclear Astrophysics Article Categories Letters (Open Access) Regular Articles New Tools and Techniques Reviews.
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