一个中子星合并的无线电对应
G Hallinan1, A Corsi2, K P Mooley3
1Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA 91125, USA. gh@astro.caltech.edu.
概括
科学家探测到来自双中子恒星 (GW170817) 合并的无线电信号,揭示了合并的洞察力
科学领域:
- 天体物理学
- 多传递器天文学
- 引力波天文学
背景情况:
- 来自双中子星合并事件GW170817的引力波的检测提供了这种宇宙碰撞的第一个直接证据.
- 电磁辐射的同时检测证实了合并的位置在距离我们大约40兆帕塞克的星系NGC 4993中.
研究的目的:
- 调查GW170817合并事件的能源和环境背景.
- 识别和描述引力波事件的无线电对应物.
- 对合并后的结果进行区分.
主要方法:
- 在合并16天后出现的无线电对应源.
- 分析无线电辐射以诊断合并的能量和环境.
- 使用非常长的基线干扰测量 (VLBI) 来测量碎片的几何形状和角速度.
主要成果:
- 在GW170817事件发生16天后发现了无线电对应源.
- 观察到的无线电辐射与轴外超相对论喷射或轻微相对论喷射一致.
- 无线电光线曲线预计将在100天内区分这两种模型.
结论:
- 无线电对应器为了解二进制中子星合并的物理提供了至关重要的数据.
- 未来的观测将通过VLBI直接测量碎片的几何和角度速度.
- 这项研究强调了多信息天文学在解开极端宇宙事件的力量.
相关概念视频
Radioactivity and Nuclear Equations
18.3K
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...
18.3K
Nuclear Stability
20.5K
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...
To hold positively...
20.5K
Nuclear Fission
9.5K
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...
9.5K
Nuclear Fusion
33.2K
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...
33.2K
Nuclear Transmutation
12.9K
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...
12.9K
Atomic Nuclei: Nuclear Spin
5.1K
All atomic particles possess an intrinsic angular momentum, or 'spin'. Electrons, protons, and neutrons each have a spin value of ½, although protons and neutrons in nuclei may have higher half-integer spins owing to energetic factors.
Atomic nuclei have a net nuclear spin, , which can have an integer or half-integer value. In atomic nuclei, the spins of protons are paired against each other but not with neutrons, and vice versa. Consequently, an even number of protons does not contribute...
Atomic nuclei have a net nuclear spin, , which can have an integer or half-integer value. In atomic nuclei, the spins of protons are paired against each other but not with neutrons, and vice versa. Consequently, an even number of protons does not contribute...
5.1K


