Spectral analysis of microwave background perturbations induced by cosmic strings

dc.contributor.authorPerivolaropoulos, Leandrosen
dc.date.accessioned2015-11-24T18:35:08Z
dc.date.available2015-11-24T18:35:08Z
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/17048
dc.rightsDefault Licence-
dc.titleSpectral analysis of microwave background perturbations induced by cosmic stringsen
heal.abstractUsing a simple analytic model based on seed superposition we obtain the spectrum of microwave background perturbations induced by cosmic strings on all angular scales larger than about 2 armin. We assume standard recombination in an Einstein de Sitter universe with $h=1/2$ and study the fluctuation spectrum along a great circle in the sky. Doppler and potential perturbations on the last scattering surface (Sachs-Wolfe effect) are shown to dominate over post-recombination perturbations on scales smaller than about 2 degrees. Using a filter function corresponding to the COBE experiment we obtain an effective power spectrum index $n_{eff}\simeq 1.35$ in good agreement with the recently announced second year COBE data showing $n_{eff}\simeq 1.5$. The only free parameter ($G\mu$) of the string model is fixed by normalizing on the COBE detection leading to $G\mu=1.6$. Other parameters (e.g. the {\it rms} string velocity) are fixed by comparing with string simulations. Using these parameter values we compare the {\it rms} temperature fluctuations $({{\Delta T}\over T})_{\it rms}$ predicted for ongoing experiments (Tenerife, SP91, MAX, OVRO etc) with detections and with the corresponding predictions of inflationary models.en
heal.accesscampus-
heal.fullTextAvailabilityTRUE-
heal.journalNameAstrophys.J.en
heal.journalTypepeer reviewed-
heal.publicationDate1995-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.typejournalArticle-
heal.type.elΆρθρο Περιοδικούel
heal.type.enJournal articleen

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