Cosmic string signatures in anisotropies of the cosmic microwave background

We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the light of current high-resolution observations from the BOOMERanG, MAXIMA and DA...

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Autores principales: Gangui, A., Pogosian, L., Winitzki, S.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_13876473_v46_n11_p681_Gangui
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spelling todo:paper_13876473_v46_n11_p681_Gangui2023-10-03T16:12:31Z Cosmic string signatures in anisotropies of the cosmic microwave background Gangui, A. Pogosian, L. Winitzki, S. Bispectrum Cosmic microwave background radiation Cosmic strings We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the light of current high-resolution observations from the BOOMERanG, MAXIMA and DASI collaborations. Upcoming megapixel experiments will have the potential to look for non-Gaussian features in the CMB temperature maps with unprecedented accuracy. We therefore devote the last part of this review to treat the non-Gaussianity of the microwave background and present a method for computation of the bispectrum from simulated string realizations. © 2002 Elsevier Science B.V. All rights reserved. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_13876473_v46_n11_p681_Gangui
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Bispectrum
Cosmic microwave background radiation
Cosmic strings
spellingShingle Bispectrum
Cosmic microwave background radiation
Cosmic strings
Gangui, A.
Pogosian, L.
Winitzki, S.
Cosmic string signatures in anisotropies of the cosmic microwave background
topic_facet Bispectrum
Cosmic microwave background radiation
Cosmic strings
description We briefly review certain aspects of cosmic microwave background anisotropies as generated in passive and active models of structure formation. We then focus on cosmic strings based models and discuss their status in the light of current high-resolution observations from the BOOMERanG, MAXIMA and DASI collaborations. Upcoming megapixel experiments will have the potential to look for non-Gaussian features in the CMB temperature maps with unprecedented accuracy. We therefore devote the last part of this review to treat the non-Gaussianity of the microwave background and present a method for computation of the bispectrum from simulated string realizations. © 2002 Elsevier Science B.V. All rights reserved.
format JOUR
author Gangui, A.
Pogosian, L.
Winitzki, S.
author_facet Gangui, A.
Pogosian, L.
Winitzki, S.
author_sort Gangui, A.
title Cosmic string signatures in anisotropies of the cosmic microwave background
title_short Cosmic string signatures in anisotropies of the cosmic microwave background
title_full Cosmic string signatures in anisotropies of the cosmic microwave background
title_fullStr Cosmic string signatures in anisotropies of the cosmic microwave background
title_full_unstemmed Cosmic string signatures in anisotropies of the cosmic microwave background
title_sort cosmic string signatures in anisotropies of the cosmic microwave background
url http://hdl.handle.net/20.500.12110/paper_13876473_v46_n11_p681_Gangui
work_keys_str_mv AT ganguia cosmicstringsignaturesinanisotropiesofthecosmicmicrowavebackground
AT pogosianl cosmicstringsignaturesinanisotropiesofthecosmicmicrowavebackground
AT winitzkis cosmicstringsignaturesinanisotropiesofthecosmicmicrowavebackground
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