“Etragalactic background light”的版本间差异

来自Shiyin's note
跳到导航 跳到搜索
无编辑摘要
无编辑摘要
 
第3行: 第3行:


*The extragalactic background light (EBL), defined here as the emission in the 0.1–1000 μm wavelength region, is one of the fundamental observational quantities in cosmology. It comprises the integrated light from resolved and unresolved extragalactic sources, and the light from any truly diffuse background, excluding the cosmic microwave background (CMB). It is therefore the repository of all energy released by nuclear and gravitational processes since the epoch of recombination. A significant fraction of this radiation is shifted by cosmic expansion and by absorption and reradiation by dust into infrared (IR) wavelengths.
*The extragalactic background light (EBL), defined here as the emission in the 0.1–1000 μm wavelength region, is one of the fundamental observational quantities in cosmology. It comprises the integrated light from resolved and unresolved extragalactic sources, and the light from any truly diffuse background, excluding the cosmic microwave background (CMB). It is therefore the repository of all energy released by nuclear and gravitational processes since the epoch of recombination. A significant fraction of this radiation is shifted by cosmic expansion and by absorption and reradiation by dust into infrared (IR) wavelengths.

==Cosmic Optical Background==
*[https://arxiv.org/abs/2407.06273]用 New Horizons上的一个仪器(可以有效避免黄道光)Long-Range Reconnaissance Imager (LORRI)测的

2024年7月10日 (三) 01:55的最新版本

  • 简单模型
arXiv 1712.06579
  • The extragalactic background light (EBL), defined here as the emission in the 0.1–1000 μm wavelength region, is one of the fundamental observational quantities in cosmology. It comprises the integrated light from resolved and unresolved extragalactic sources, and the light from any truly diffuse background, excluding the cosmic microwave background (CMB). It is therefore the repository of all energy released by nuclear and gravitational processes since the epoch of recombination. A significant fraction of this radiation is shifted by cosmic expansion and by absorption and reradiation by dust into infrared (IR) wavelengths.

Cosmic Optical Background

  • [1]用 New Horizons上的一个仪器(可以有效避免黄道光)Long-Range Reconnaissance Imager (LORRI)测的