概括
沉重的宇宙射线核的流量比率在数十亿年的时间里保持了显著的一致性. 这表明来自宇宙辐射源的稳定元素组成,无论时间或位置在太阳系.
科学领域:
- 宇宙射线物理学的物理学.
- 核天体物理学 核天体物理学
- 星球科学 星球科学
背景情况:
- 宇宙射线提供了对天体物理过程和宇宙元素组成的洞察.
- 了解重型宇宙射线核的起源和变异对于天体物理模型至关重要.
研究的目的:
- 为了研究重型宇宙射线核流量比的时间和空间稳定性.
- 为了确定宇宙辐射源的元素组成是否在宇宙时间尺度上发生了变化.
主要方法:
- 分析石和月球样本以确定宇宙射线暴露年龄和核成分.
- 测量重核 (原子数30-40) 与铁组核 (原子数20-28),相对于重核的流量比.
- 通过不同动能 (30-2000 MeV/核子) 和太阳系距离 (1-3 AU) 的流量比较.
主要成果:
- 重型宇宙射线核 (Z=30-40) 与铁组核 (Z=20-28) 的流量比率显示出最小的变化.
- 几十亿年来,变化一直保持在 (1.3 +/- 0.6) x 10(-3) 之内.
- 没有观察到对时间,太阳系距离或运动能量的显著依赖.
结论:
- 宇宙辐射源的元素组成在数十亿年的时间里非常稳定.
- 这些发现表明,这些重型宇宙射线核的来源是持久的和统一的.
- 这种稳定性对理解银河系宇宙射线传播和源组成有重大影响.
相关概念视频
Atomic Mass
Atoms — and the protons, neutrons, and electrons that compose them — are extremely small. For example, a carbon atom weighs less than 2 × 10−23 g. When describing the properties of tiny objects such as atoms, we use appropriately small units of measure, such as the atomic mass unit (amu). The amu was originally defined based on hydrogen, the lightest element, then later in terms of oxygen. Since 1961, it has been defined with regard to the most abundant isotope of carbon, atoms of which are...
Atomic Radii and Effective Nuclear Charge
The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.
Radioactivity and Nuclear Equations
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
A nuclide of an element has a specific number of protons and...
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 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 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...


