Is the Harrison-Zel’dovich spectrum coming back? ACT preference forns∼ 1 and its discordance with Planck

Author:

Giarè William123ORCID,Renzi Fabrizio4ORCID,Mena Olga5,Di Valentino Eleonora3ORCID,Melchiorri Alessandro26

Affiliation:

1. Galileo Galileo Institute for theoretical physics , Centro Nazionale INFN di studi avanzati, Largo Enrico Fermi 2, Firenze I-50125, Italy

2. INFN Sezione di Roma , P.le A. Moro 2, Roma I-00185, Italy

3. School of Mathematics and Statistics, University of Sheffield , Hounsfield Road, Sheffield S3 7RH, United Kingdom

4. Lorentz Institute for Theoretical Physics, Leiden University , PO Box 9506, Leiden NL-2300 RA, The Netherlands

5. IFIC, Universidad de Valencia-CSIC , Valencia E-46071, Spain

6. Physics Department, Università di Roma ‘La Sapienza’ , Ple Aldo Moro 2, Rome I-00185, Italy

Abstract

ABSTRACTThe Data Release 4 of the Atacama Cosmology Telescope (ACT) shows an agreement with an Harrison-Zel’dovich primordial spectrum (ns = 1.009 ± 0.015), introducing a tension with a significance of 99.3  per cent Confidence Level (CL) with the results from the Planck satellite. The discrepancy on the value of the scalar spectral index is neither alleviated with the addition of large scale structure information nor with the low multipole polarization data. We discuss possible avenues to alleviate the tension relying on either neglecting polarization measurements from ACT or in extending different sectors of the theory.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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