An Electronic Radiation of Blackbody: Cosmic Electron Background - Revision history

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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.[[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.

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	[[Category:Cosmology]]		[[Category:Cosmology]]

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{{Infobox paper
| title = An Electronic Radiation of Blackbody: Cosmic Electron Background
| author = [[Jian-Miin Liu]]
| 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.[[Category:Scientific Paper]]

[[Category:Cosmology]]