Evidence for an inflationary phase transition from the LSS and CMB anisotropy data

In the light of the recent Boomerang and Maxima observations of the CMB which show an anomalously low second acoustic peak, we reexamine the prediction by Adams et al (1997) that this would be the consequence of a 'step' in the primordial spectrum induced by a spontaneous symmetry breaking...

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Main Authors: Barriga, J, Gaztanaga, E, Santos, MG, Sarkar, S
Format: Conference item
Published: 2000
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author Barriga, J
Gaztanaga, E
Santos, MG
Sarkar, S
author_facet Barriga, J
Gaztanaga, E
Santos, MG
Sarkar, S
author_sort Barriga, J
collection OXFORD
description In the light of the recent Boomerang and Maxima observations of the CMB which show an anomalously low second acoustic peak, we reexamine the prediction by Adams et al (1997) that this would be the consequence of a 'step' in the primordial spectrum induced by a spontaneous symmetry breaking phase transition during primordial inflation. We demonstrate that a deviation from scale-invariance around $k\sim0.1h$~Mpc$^{-1}$ can simultaneously explain both the feature identified earlier in the APM galaxy power spectrum as well the recent CMB anisotropy data, with a baryon density consistent with the BBN value. Such a break also allows a good fit to the data on cluster abundances even for a critical density matter-dominated universe with zero cosmological constant.
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spelling oxford-uuid:9c3bfc3f-9b21-4c78-b323-0805b42a9d152022-03-27T00:34:34ZEvidence for an inflationary phase transition from the LSS and CMB anisotropy dataConference itemhttp://purl.org/coar/resource_type/c_5794uuid:9c3bfc3f-9b21-4c78-b323-0805b42a9d15Symplectic Elements at Oxford2000Barriga, JGaztanaga, ESantos, MGSarkar, SIn the light of the recent Boomerang and Maxima observations of the CMB which show an anomalously low second acoustic peak, we reexamine the prediction by Adams et al (1997) that this would be the consequence of a 'step' in the primordial spectrum induced by a spontaneous symmetry breaking phase transition during primordial inflation. We demonstrate that a deviation from scale-invariance around $k\sim0.1h$~Mpc$^{-1}$ can simultaneously explain both the feature identified earlier in the APM galaxy power spectrum as well the recent CMB anisotropy data, with a baryon density consistent with the BBN value. Such a break also allows a good fit to the data on cluster abundances even for a critical density matter-dominated universe with zero cosmological constant.
spellingShingle Barriga, J
Gaztanaga, E
Santos, MG
Sarkar, S
Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title_full Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title_fullStr Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title_full_unstemmed Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title_short Evidence for an inflationary phase transition from the LSS and CMB anisotropy data
title_sort evidence for an inflationary phase transition from the lss and cmb anisotropy data
work_keys_str_mv AT barrigaj evidenceforaninflationaryphasetransitionfromthelssandcmbanisotropydata
AT gaztanagae evidenceforaninflationaryphasetransitionfromthelssandcmbanisotropydata
AT santosmg evidenceforaninflationaryphasetransitionfromthelssandcmbanisotropydata
AT sarkars evidenceforaninflationaryphasetransitionfromthelssandcmbanisotropydata