| dc.contributor.advisor | Edmund Bertschinger. | en_US |
| dc.contributor.author | Tassev, Svetlin Valentinov | en_US |
| dc.contributor.other | Massachusetts Institute of Technology. Dept. of Physics. | en_US |
| dc.date.accessioned | 2006-05-15T20:38:22Z | |
| dc.date.available | 2006-05-15T20:38:22Z | |
| dc.date.copyright | 2005 | en_US |
| dc.date.issued | 2005 | en_US |
| dc.identifier.uri | http://hdl.handle.net/1721.1/32906 | |
| dc.description | Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2005. | en_US |
| dc.description | Includes bibliographical references (leaf 55). | en_US |
| dc.description.abstract | Using canonical quantization we show that the spectrum of the scalar cosmological fluctuations as calculated until now is not correct. We derive the correct expression for the spectrum, and show that our correct treatment alleviates the fine-tuning problem in inflation. | en_US |
| dc.description.statementofresponsibility | by Svetlin Valentinov Tassev. | en_US |
| dc.format.extent | 55 leaves | en_US |
| dc.format.extent | 2075486 bytes | |
| dc.format.extent | 2076563 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | eng | en_US |
| dc.publisher | Massachusetts Institute of Technology | en_US |
| dc.rights | M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. | en_US |
| dc.rights.uri | http://dspace.mit.edu/handle/1721.1/7582 | |
| dc.subject | Physics. | en_US |
| dc.title | Quantum field theory of scalar cosmological perturbations | en_US |
| dc.type | Thesis | en_US |
| dc.description.degree | S.B. | en_US |
| dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | |
| dc.identifier.oclc | 62627132 | en_US |
