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Modeling features in the redshift-space halo power spectrum with perturbation theory
We study the ability of perturbative models with effective field theory contributions and infra-red resummation to model the redshift space clustering of biased tracers in models where the linear power spectrum has “features”—either imprinted during inflation or induced by non-standard expansion his...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2020
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2020/11/035 http://cds.cern.ch/record/2747945 |