核心崩超新星中的不对称性来自卡西欧佩亚A中放射性44Ti的地图
B W Grefenstette1, F A Harrison1, S E Boggs2
1Cahill Center for Astrophysics, 1216 East California Boulevard, California Institute of Technology, Pasadena, California 91125, USA.
Nature
|February 21, 2014
概括
在Cassiopeia A中绘制放射性的地图揭示了核心崩超新星中的低模式对流动不稳定性. 这一发现挑战了对称和双极爆炸模型,为恒星残余形成提供了新的见解.
科学领域:
- 天体物理学 天体物理学
- 核天体物理学 核天体物理学
- 超新星残留物 超新星残留物
背景情况:
- 核心崩超新星模拟需要不对称性,但它的形式各不相同.
- 放射性-44 (44Ti) 的分布痕迹爆炸不对称.
- 卡西奥佩亚A (Cas A) 是一个年轻的残余物,已检测到但未成像的44Ti.
研究的目的:
- 在Cas A中对44Ti的光谱属性进行空间映射和分析.
- 用44Ti分布来研究Cas A的爆炸不对称性.
- 为了协调观察到的44Ti和铁X射线发射相关性.
主要方法:
- 在Cas A.中44Ti排放的空间映射.
- 对44Ti属性的光谱分析.
- 观察到的44Ti分布与理论爆炸模型的比较.
主要成果:
- 报告了在Cas A中观察到的44Ti分布.
- 空间分布排除了对称爆炸和快速旋转的原始模型.
- 提供了核心崩超新星中低模式对流动不稳定的证据.
结论:
- 这项研究提供了强有力的证据,证明核崩超新星中低模式对流动不稳定性.
- 观察到的44Ti分布挑战了现有的恒星爆炸不对称性的模型.
- 这项工作为超新星爆炸和残留物形成的动态提供了新的见解.
相关概念视频
Atomic Nuclei: Nuclear Spin State Population Distribution
2.6K
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
2.6K
Gravitation Between Spherically Symmetric Masses
1.5K
The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.
1.5K
Nuclear Fission
12.9K
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...
12.9K
Nuclear Fusion
35.2K
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...
35.2K
Atomic Emission Spectroscopy: Overview
4.3K
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...
4.3K
Nuclear Stability
24.3K
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...
To hold positively charged protons together...
24.3K


