Quantum field theory of scalar cosmological perturbations
Name
62627132-MIT.pdf
Description
Full printable version
Size
1.98 MB
Format
Adobe PDF
Checksum (MD5)
cb2dcb3562dc526a9562ce201c9bb8ae
Author(s)
Tassev, Svetlin Valentinov
Advisor(s)
Edmund Bertschinger.
Date Issued
2005
Publisher
Massachusetts Institute of Technology
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.
Description
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2005.
Includes bibliographical references (leaf 55).
Subjects
Physics.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Terms of Use
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.
Persistent DSpace Link