相关实验视频
Updated: Aug 11, 2026

09:50
Preparation and Reactivity of Gasless Nanostructured Energetic Materials
Published on: April 2, 2015
概括
自然存在的核可能是在恒星爆炸中形成的. 这些事件表明,大质量恒星是质量在20到62之间元素的起源.
科学领域:
- 核天体物理学 核天体物理学
- 恒星进化中的恒星演变
背景情况:
- 核合成描述了化学元素的产生.
- 了解元素的起源是天体物理学的一个基本问题.
研究的目的:
- 为自然存在的核的爆炸性起源提供证据.
- 假设特定质量范围内的核的起源 (20 <= A <= 62).
主要方法:
- 审查最近的核合成计算.
- 分析所需的物理条件 (温度,密度,膨胀率).
主要成果:
- 计算强烈支持自然发生的核的爆炸性起源.
- 物理条件表明,进化的大质量恒星是它们的祖先.
- 一个新的表格假设了具有20 <= A <= 62的原子核的起源.
结论:
- 大质量恒星中的爆炸事件是自然发生的核的可能来源.
- 这项研究为了解特定质量范围内的元素的起源提供了一个框架.
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 Stability
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
To hold positively charged protons together in the...
Nuclear Binding Energy
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound together;...
Nuclear Fission
Many heavier elements with smaller binding energies per nucleon can decompose into more stable elements that have intermediate mass numbers and larger binding energies per nucleon—that is, mass numbers and binding energies per nucleon that are closer to the “peak” of the binding energy graph near 56. Sometimes neutrons are also produced. This decomposition of a large nucleus into smaller pieces is called fission. The breaking is rather random with the formation of a large number of different...
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...

