2026-09-18T20:52:12Zhttps://dspace.mit.edu/server/oai/requestoai:dspace.mit.edu:1721.1/327432022-01-13T07:54:41Zcom_1721.1_7582com_1721.1_7581col_1721.1_131024
Edmund Bertschinger.
Lam, Yukyam, 1982-
Massachusetts Institute of Technology. Dept. of Physics.
Massachusetts Institute of Technology. Department of Physics
2006-05-15T20:26:51Z
2006-05-15T20:26:51Z
2004
2004
http://hdl.handle.net/1721.1/32743
56730555
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.
Includes bibliographical references (p. 59-60).
According to the WMAP and earlier COBE observations, the Cosmic Microwave Background (CMB) anisotropy power on large angular scales appears to be significantly lower than predicted by the standard model of cosmology. We propose a scalar field model of the dark energy as a mechanism for suppressing low l multipoles through late-Universe evolution of metric fluctuations and the integrated Sachs-Wolfe (ISW) effect. We find that for a constant dark energy equation of state, theoretical predictions actually give a larger (instead of a desired smaller) value of the quadrupole and other low l multipoles.
by Yukyan Lam.
S.B.
60 p.
2117393 bytes
2118894 bytes
application/pdf
application/pdf
eng
Massachusetts Institute of Technology
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.
http://dspace.mit.edu/handle/1721.1/7582
Physics.
Dark energy and CMB anisotropy
Dark energy and Cosmic Microwave Background anisotropy
Thesis
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