Please use this identifier to cite or link to this item:
https://olympias.lib.uoi.gr/jspui/handle/123456789/16405Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Perivolaropoulos, L. | en |
| dc.date.accessioned | 2015-11-24T18:30:55Z | - |
| dc.date.available | 2015-11-24T18:30:55Z | - |
| dc.identifier.issn | 0920-5632 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16405 | - |
| dc.rights | Default Licence | - |
| dc.subject | large-scale structure | en |
| dc.subject | cold dark matter | en |
| dc.subject | density-fluctuations | en |
| dc.subject | galaxy formation | en |
| dc.subject | gravitational-radiation | en |
| dc.subject | microwave-anisotropy | en |
| dc.subject | expanding universe | en |
| dc.subject | vortex scattering | en |
| dc.subject | abelian higgs | en |
| dc.subject | domain-walls | en |
| dc.title | The rise and fall of the cosmic string theory for cosmological perturbations | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | <Go to ISI>://000230192000016 | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2005 | - |
| heal.abstract | The cosmic string theory for cosmological fluctuations is a good example of healthy scientific progress in cosmology. It is a well defined physically motivated model that has been tested by cosmological observations and has been ruled out as a primary source of primordial fluctuations. Until about fifteen years ago, the cosmic string theory of cosmological perturbations provided one of the two physically motivated candidate theories for the generation of primordial perturbations. The cosmological data that appeared during the last decade have been compared with the well defined predictions of the theory and have ruled out cosmic strings as a primary source of primordial cosmological perturbations. Since cosmic strings are predicted to form after inflation in a wide range of microphysical theories (including supersymmetric and fundamental string theories) their observational bounds may serve a source of serious constraints for these theories. This is a pedagogical review of the historical development, the main predictions of the cosmic string theory and the constraints that have been imposed on it by cosmological observations. Recent lensing events that could be attributed to lighter cosmic strings are also discussed. | en |
| heal.journalName | Nuclear Physics B-Proceedings Supplements | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) - ΦΥΣ | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| perivolaropoulos-2005-The rise and fall of the cosmic string theory for cosmological perturbations.pdf | 365.29 kB | Adobe PDF | View/Open Request a copy |
This item is licensed under a Creative Commons License
