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Blue perturbation spectra from inflation
We investigate inflationary models leading to density perturbations with a spectral index $n>1$ (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
1994
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.50.4835 http://cds.cern.ch/record/543018 |
| _version_ | 1780898360380620800 |
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| author | Mollerach, Silvia Matarrese, Sabino Lucchin, Francesco |
| author_facet | Mollerach, Silvia Matarrese, Sabino Lucchin, Francesco |
| author_sort | Mollerach, Silvia |
| collection | CERN |
| description | We investigate inflationary models leading to density perturbations with a spectral index $n>1$ (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such as those measured by COBE, and that required to give bulk motions and structures on the $\sim 50~h^{-1}$ Mpc scale. |
| id | cern-543018 |
| institution | Organización Europea para la Investigación Nuclear |
| language | eng |
| publishDate | 1994 |
| record_format | invenio |
| spelling | cern-5430182023-03-14T19:27:16Zdoi:10.1103/PhysRevD.50.4835http://cds.cern.ch/record/543018engMollerach, SilviaMatarrese, SabinoLucchin, FrancescoBlue perturbation spectra from inflationAstrophysics and AstronomyWe investigate inflationary models leading to density perturbations with a spectral index $n>1$ (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such as those measured by COBE, and that required to give bulk motions and structures on the $\sim 50~h^{-1}$ Mpc scale.We investigate inflationary models leading to density perturbations with a spectral index $n>1$ (``blue spectra"). These perturbation spectra may be useful to simultaneously account for both the amount of ultra large-scale power required to fit cosmic microwave background anisotropies, such as those measured by COBE, and that required to give bulk motions and structures on the $\sim 50h~{-1}$ Mpc scale.astro-ph/9309054oai:cds.cern.ch:5430181994 |
| spellingShingle | Astrophysics and Astronomy Mollerach, Silvia Matarrese, Sabino Lucchin, Francesco Blue perturbation spectra from inflation |
| title | Blue perturbation spectra from inflation |
| title_full | Blue perturbation spectra from inflation |
| title_fullStr | Blue perturbation spectra from inflation |
| title_full_unstemmed | Blue perturbation spectra from inflation |
| title_short | Blue perturbation spectra from inflation |
| title_sort | blue perturbation spectra from inflation |
| topic | Astrophysics and Astronomy |
| url | https://dx.doi.org/10.1103/PhysRevD.50.4835 http://cds.cern.ch/record/543018 |
| work_keys_str_mv | AT mollerachsilvia blueperturbationspectrafrominflation AT matarresesabino blueperturbationspectrafrominflation AT lucchinfrancesco blueperturbationspectrafrominflation |