Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys

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dc.contributor.authorBallardini, Mario
dc.contributor.authorMurgia, Riccardo
dc.contributor.authorBaldi, Marco
dc.date.accessioned2021-02-17T09:52:53Z
dc.date.available2021-02-17T09:52:53Z
dc.date.issued2020
dc.description.abstractGalaxy surveys are an important probe for superimposed oscillations on the primordial power spectrum of curvature perturbations, which are predicted in several theoretical models of inflation and its alternatives. In order to exploit the full cosmological information in galaxy surveys it is necessary to study the matter power spectrum to fully non-linear scales. We therefore study the non-linear clustering in models with superimposed linear and logarithmic oscillations to the primordial power spectrum by running high-resolution darkmatter-only N-body simulations. We fit a Gaussian envelope for the non-linear damping of superimposed oscillations in the matter power spectrum to the results of the N-body simulations for k . 0.6 h/Mpc at 0 ≤ z ≤ 5 with an accuracy below the percent. We finally use this fitting formula to forecast the capabilities of future galaxy surveys, such as Euclid and Subaru, to probe primordial oscillation down to non-linear scales alone and in combination with the information contained in CMB anisotropies.en_US
dc.identifier.citationBallardini, M. et al. (2020). Non-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveys. Journal of Cosmology and Astroparticle Physics, 2020(04)en_US
dc.identifier.uri10.1088/1475-7516/2020/04/030
dc.identifier.urihttp://hdl.handle.net/10566/5943
dc.language.isoenen_US
dc.publisherIOP Publishing Ltden_US
dc.subjectCosmological parameters from LSSen_US
dc.subjectGalaxy clustersen_US
dc.subjectPhysics of the early universeen_US
dc.subjectPower spectrumen_US
dc.subjectGalaxy surveysen_US
dc.titleNon-linear damping of superimposed primordial oscillations on the matter power spectrum in galaxy surveysen_US
dc.typeArticleen_US

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