pith. machine review for the scientific record. sign in

arxiv: 1311.1657 · v2 · submitted 2013-11-07 · 🌌 astro-ph.CO

Recognition: unknown

Planck intermediate results. XVI. Profile likelihoods for cosmological parameters

Planck Collaboration: P. A. R. Ade , N. Aghanim , M. Arnaud , M. Ashdown , J. Aumont , C. Baccigalupi , A. J. Banday , R. B. Barreiro
show 174 more authors
J. G. Bartlett E. Battaner K. Benabed A. Benoit-L\'evy J.-P. Bernard M. Bersanelli P. Bielewicz J. Bobin A. Bonaldi J. R. Bond F. R. Bouchet C. Burigana J.-F. Cardoso A. Catalano A. Chamballu H. C. Chiang P. R. Christensen D. L. Clements S. Colombi L. P. L. Colombo F. Couchot F. Cuttaia L. Danese R. J. Davis P. De Bernardis A. De Rosa G. de Zotti J. Delabrouille C. Dickinson J. M. Diego H. Dole S. Donzelli O. Dor\'e M. Douspis X. Dupac T. A. En{\ss}lin H. K. Eriksen F. Finelli O. Forni M. Frailis E. Franceschi S. Galeotta S. Galli K. Ganga M. Giard Y. Giraud-H\'eraud J. Gonz\'alez-Nuevo K. M. G\'orski A. Gregorio A. Gruppuso F. K. Hansen D. Harrison S. Henrot-Versill\'e C. Hern\'andez-Monteagudo D. Herranz S. R. Hildebrandt E. Hivon M. Hobson W. A. Holmes A. Hornstrup W. Hovest K. M. Huffenberger A. H. Jaffe T. R. Jaffe W. C. Jones M. Juvela E. Keih\"anen R. Keskitalo T. S. Kisner R. Kneissl J. Knoche L. Knox M. Kunz H. Kurki-Suonio G. Lagache A. L\"ahteenm\"aki J.-M. Lamarre A. Lasenby R. Leonardi A. Liddle M. Liguori P. B. Lilje M. Linden-V{\o}rnle M. L\'opez-Caniego P. M. Lubin J. F. Mac\'ias-P\'erez B. Maffei D. Maino N. Mandolesi M. Maris P. G. Martin E. Mart\'inez-Gonz\'alez S. Masi M. Massardi S. Matarrese P. Mazzotta A. Melchiorri L. Mendes A. Mennella M. Migliaccio S. Mitra M.-A. Miville-Desch\^enes A. Moneti L. Montier G. Morgante D. Munshi J. A. Murphy P. Naselsky F. Nati P. Natoli F. Noviello D. Novikov I. Novikov C. A. Oxborrow L. Pagano F. Pajot D. Paoletti F. Pasian O. Perdereau L. Perotto F. Perrotta V. Pettorino F. Piacentini M. Piat E. Pierpaoli D. Pietrobon S. Plaszczynski E. Pointecouteau G. Polenta L. Popa G. W. Pratt J.-L. Puget J. P. Rachen R. Rebolo M. Reinecke M. Remazeilles C. Renault S. Ricciardi T. Riller I. Ristorcelli G. Rocha C. Rosset G. Roudier B. Rouill\'e d'Orfeuil J. A. Rubi\~no-Mart\'in B. Rusholme M. Sandri M. Savelainen G. Savini L. D. Spencer M. Spinelli J.-L. Starck F. Sureau D. Sutton A.-S. Suur-Uski J.-F. Sygnet J. A. Tauber L. Terenzi L. Toffolatti M. Tomasi M. Tristram M. Tucci G. Umana L. Valenziano J. Valiviita B. Van Tent P. Vielva F. Villa L. A. Wade B. D. Wandelt M. White D. Yvon A. Zacchei A. Zonca
Authors on Pith no claims yet
classification 🌌 astro-ph.CO
keywords planckresultsbayesiancombinationconfidencecosmologicalfrequentistinclusion
0
0 comments X
read the original abstract

We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Minuit). This allows a refinement of the Lambda-cdm best-fit solution with respect to previously-released results, and the construction of frequentist confidence intervals using profile likelihoods. The agreement with the cosmological results from the Bayesian framework is excellent, demonstrating the robustness of the Planck results to the statistical methodology. We investigate the inclusion of neutrino masses, where more significant differences may appear due to the non-Gaussian nature of the posterior mass distribution. By applying the Feldman--Cousins prescription, we again obtain results very similar to those of the Bayesian methodology. However, the profile-likelihood analysis of the CMB combination (Planck+WP+highL) reveals a minimum well within the unphysical negative-mass region. We show that inclusion of the Planck CMB-lensing information regularizes this issue, and provide a robust frequentist upper limit $M_\nu < 0.26 eV$ ($95%$ confidence) from the CMB+lensing+BAO data combination.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements

    astro-ph.CO 2024-11 accept novelty 6.0

    DESI DR1 full-shape clustering yields Ω_m = 0.2962 ± 0.0095 and σ_8 = 0.842 ± 0.034 in flat ΛCDM, tightening to H_0 = 68.40 ± 0.27 km/s/Mpc with CMB and DESY3, while favoring w_0 > -1, w_a < 0 and limiting neutrino ma...

  2. Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape

    astro-ph.CO 2025-03 conditional novelty 5.0

    DESI DR2 BAO and full-shape data plus CMB yield ∑m_ν < 0.0642 eV (95% CL) under ΛCDM, in 3σ tension with oscillation lower limits, relaxed to <0.163 eV in w0waCDM.