Difference between revisions of "An Electronic Radiation of Blackbody: Cosmic Electron Background"
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==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. | + | 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:Cosmology]] | + | [[Category:Scientific Paper|electronic radiation blackbody cosmic electron background]] |
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| + | [[Category:Cosmology|electronic radiation blackbody cosmic electron background]] | ||
Latest revision as of 19:17, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | An Electronic Radiation of Blackbody: Cosmic Electron Background |
| Author(s) | Jian-Miin Liu |
| Keywords | {{{keywords}}} |
| Published | 2008 |
| Journal | ArXiv |
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.
