在放射性超新星气体中碳的凝结
D D Clayton1, W Liu, A Dalgarno
1Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-1911, USA.
概括
超新星化学通过分解一氧化碳产生碳尘,使得尘埃的形成速度比它更快.
科学领域:
- 宇宙化学 宇宙化学
- 天体化学是天体化学.
- 恒星进化 恒星进化
背景情况:
- 超新星是重元素和尘埃合成的关键地点.
- 一氧化碳 (CO) 的形成通常限制了恒星外流中的自由碳原子的可用性.
- 在石中发现的太阳前颗粒为早期太阳系条件提供了洞察力.
研究的目的:
- 研究在膨胀超新星中导致含碳分子和尘埃形成的化学过程.
- 通过数值来解决控制这些物种丰度的方程.
- 探索放射性物质对碳化学和尘埃形成的影响.
主要方法:
- 控制物种丰度的化学运动方程的数值解.
- 扩张超新星内部化学模型.
- 分析放射性活动中能量电子的作用.
主要成果:
- 来自超新星放射性的能量电子解离CO分子,释放出自由的碳原子.
- 这一过程增加了可用于尘埃形成的碳原子供应.
- 碳尘通过结合增长的速度快于通过氧化破坏的速度.
结论:
- 超新星内部可以成为碳尘的重要来源.
- 能量电子的二氧化碳解离是使尘埃形成成为可能的关键机制.
- 这一发现改变了对前太阳碳固体起源的理解.
相关概念视频
Types of Radioactivity
The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Nuclear Fusion
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Nuclear Transmutation
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed protons being...
¹³C NMR: ¹H–¹³C Decoupling
The probability of having two carbon-13 atoms next to each other is negligible because of the low natural abundance of carbon-13. Consequently, peak splitting due to carbon-carbon spin-spin coupling is not observed in spectra. However, protons up to three sigma bonds away split the carbon signal according to the n+1 rule, resulting in complicated spectra.
A broadband decoupling technique is used to simplify these complex, sometimes overlapping, signals. Broadband decoupling relies on a...
A broadband decoupling technique is used to simplify these complex, sometimes overlapping, signals. Broadband decoupling relies on a...
Atomic Emission Spectroscopy: Overview
Atomic emission spectroscopy (AES) is an analytical technique used to determine the elemental composition of a sample by analyzing the light emitted from excited atoms. In AES, atoms in a sample are excited to higher energy levels by thermal energy from high-temperature sources, such as plasma, arcs, or sparks. When these excited atoms return to lower energy states, they emit light at specific wavelengths characteristic of each element. The resulting atomic emission spectrum, which consists of...
Atomic Emission Spectroscopy: Lab
AES is a powerful analytical technique, especially effective when used with plasma sources, producing abundant spectra in characteristic emission lines. The Inductively Coupled Plasma (ICP), in particular, yields superior quantitative analytical data due to its high stability, low noise, low background, and minimal interferences under optimal experimental conditions. However, newer air-operated microwave sources are emerging as promising alternatives that could be more cost-effective than...


