马射线爆发:积累的余光影响,祖先线索和前景
1Department of Astronomy and Astrophysics, Pennsylvania State University, University Park, PA 16803, USA. pmeszaros@astro.psu.edu
概括
马射线爆发 (GRBs) 是每天检测到的强烈的宇宙闪光,超过所有其他来源. 最近的发现揭示了它们的余光,宿主星系和与恒星形成的联系,进步了我们对这些天体物理奥秘的理解.
科学领域:
- 天体物理学 天体物理学
- 高能天文学 高能天文学
背景情况:
- 马射线爆发 (GRBs) 是短暂而强大的马射线闪光,每天可以检测到.
- 在发射过程中,GRBs在发射过程中超过了所有其他天体马射线来源.
研究的目的:
- 总结一下最近在GRB研究中的重大进展.
- 突出新问题和现场正在进行的辩论.
主要方法:
- 观测天文学,包括X射线,光学和无线电光后探测.
- 在宇宙学距离上识别GRB宿主星系.
- 分析GRB与恒星形成区域和超新星的关联.
主要成果:
- 发现缓慢消失的X射线,光学和无线电余光.
- 在显著的宇宙距离上识别 GRB 的宿主星系.
- 证据将GRB与恒星形成区域和潜在的超新星联系起来.
结论:
- GRB后照辐射是由相对论火球冲击模型解释的.
- 进步已经开辟了关于GRB发动机,原始发动机和环境影响的新研究途径.
- 在天体物理学中,GRB仍然是一个深刻的团,关于其起源和相关现象的争论仍在进行中.
更多相关视频
09:18Laser-heating and Radiance Spectrometry for the Study of Nuclear Materials in Conditions Simulating a Nuclear Power Plant Accident
Published on: December 14, 2017
06:28Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
Published on: January 30, 2020
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:
Biological Effects of Radiation
All radioactive nuclides emit high-energy particles or electromagnetic waves. When this radiation encounters living cells, it can cause heating, break chemical bonds, or ionize molecules. The most serious biological damage results when these radioactive emissions fragment or ionize molecules. For example, α and β particles emitted from nuclear decay reactions possess much higher energies than ordinary chemical bond energies. When these particles strike and penetrate matter, they produce ions...
Radiation: Applications
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...
Generating Electromagnetic Radiations
The German physicist Heinrich Hertz (1857–1894) was the first to generate and detect certain types of electromagnetic waves in the laboratory. Starting in 1887, he performed a series of experiments that confirmed the existence of electromagnetic waves and verified that they travel at the speed of light. Hertz used an alternating-current RLC (resistor-inductor-capacitor) circuit that resonated at a known frequency and connected it to a loop of wire. High voltages induced across the gap in the...
Positron Emission Tomography
Positron emission tomography (PET) is a medical imaging technique involving radiopharmaceuticals — substances that emit short-lived radiation. Although the first PET scanner was introduced in 1961, it took 15 more years before radiopharmaceuticals were combined with the technique and revolutionized its potential.
One of the main requirements of a PET scan is a positron-emitting radioisotope, which is produced in a cyclotron and then attached to a substance used by the part of the body being...
One of the main requirements of a PET scan is a positron-emitting radioisotope, which is produced in a cyclotron and then attached to a substance used by the part of the body being...
Absorption of Radiation
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
