File:Big bang inflation vs standardmodel.png
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Size of this preview: 313 × 599 pixels. Other resolutions: 125 × 240 pixels | 496 × 950 pixels.
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[edit]The image shows how with constant light speed, a much compact pre-inflated universe would have allowed thermal evenning out of the cosmic microwave background radiation (CMBR). Given such compactness, light (i.e., information) could have easily 'ran' back and forth, allowing thermal equilibrium to set in.
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[edit]Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
This file is licensed under the Creative Commons Attribution-Share Alike 3.0 Unported license. | ||
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This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 14:07, 5 May 2006 | 496 × 950 (156 KB) | Cosmocurio (talk | contribs) | The image shows how with constant light speed, a much compact pre-inflated universe would have allowed thermal evenning out of the cosmic microwave background radiation (CMBR). Given such compactness, light (i.e., information) could have easily 'ran' back |
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