An Electronic Radiation of Blackbody: Cosmic Electron Background: Difference between revisions
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{{Infobox paper | {{Infobox paper | ||
| title = An Electronic Radiation of Blackbody: Cosmic Electron Background | | title = An Electronic Radiation of Blackbody: Cosmic Electron Background | ||
| url = [http://arxiv.org/abs/0802.3464 Link to paper] | |||
| author = [[Jian-Miin Liu]] | | author = [[Jian-Miin Liu]] | ||
| keywords = radiation, electron | |||
| published = 2008 | | published = 2008 | ||
| journal = [[ArXiv]] | | journal = [[ArXiv]] | ||
}} | }} | ||
'''Read the full paper''' [http://arxiv.org/abs/0802.3464 here] | |||
==Abstract== | ==Abstract== | ||
The Universe owns the electronic radiation of blackbody at temperature 2.725 K, which we call the cosmic electron background. We calculate its radiation spectrum. The energy distribution of number density of electrons in the cosmic electron background becomes zero as energy goes to both zero and infinity. It has one maximum peak near the energy level of 10**(-23) J.[[Category:Scientific Paper]] | The Universe owns the electronic radiation of blackbody at temperature 2.725 K, which we call the cosmic electron background. We calculate its radiation spectrum. The energy distribution of number density of electrons in the cosmic electron background becomes zero as energy goes to both zero and infinity. It has one maximum peak near the energy level of 10**(-23) J. | ||
[[Category:Scientific Paper|electronic radiation blackbody cosmic electron background]] | |||
[[Category:Cosmology]] | [[Category:Cosmology|electronic radiation blackbody cosmic electron background]] | ||
Latest revision as of 07:26, 21 July 2026
| Scientific Paper | |
|---|---|
| Title | An Electronic Radiation of Blackbody: Cosmic Electron Background |
| Read in full | Link to paper |
| Author(s) | Jian-Miin Liu |
| Keywords | radiation, electron |
| Published | 2008 |
| Journal | ArXiv |
Read the full paper here
Abstract
The Universe owns the electronic radiation of blackbody at temperature 2.725 K, which we call the cosmic electron background. We calculate its radiation spectrum. The energy distribution of number density of electrons in the cosmic electron background becomes zero as energy goes to both zero and infinity. It has one maximum peak near the energy level of 10**(-23) J.