Please use this identifier to cite or link to this item: http://dspace.mediu.edu.my:8181/xmlui/handle/123456789/8381
Title: Evolution of perturbations in a domain wall cosmology
Issue Date: 1-Jun-2013
Publisher: Sociedade Brasileira de Física
Description: A fluid of domain walls may have an effective equation of state p w = -<img id="_x0000_i1026" src="../../../img/revistas/bjp/v33n4/a39img01.gif" align=absbottom>rhow. This equation of state is qualitatively in agreement with the supernova type Ia observations. We exploit a cosmological model where the matter content is given by a dust fluid and a domain wall fluid. The process of formation of galaxies is essentially preserved. On the other hand, the behaviour of the density contrast in the ordinary fluid is highly altered when domain walls begin to dominate the matter content of the Universe. This domain wall phase occurs at relative recent era, and its possible consequences are discussed, specially concerning the Sachs-Wolfe effect.
URI: http://koha.mediu.edu.my:8181/jspui/handle/123456789/8381
Other Identifiers: http://www.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332003000400039
http://www.doaj.org/doaj?func=openurl&genre=article&issn=01039733&date=2003&volume=33&issue=4&spage=834
Appears in Collections:Physics and Astronomy

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