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BOOMERanG constraints on primordial non-Gaussianity from analytical Minkowski functionals

Natoli, P. and Bock, J. J. and Lange, A. E. (2010) BOOMERanG constraints on primordial non-Gaussianity from analytical Minkowski functionals. Monthly Notices of the Royal Astronomical Society, 408 (3). pp. 1658-1665. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200129-140653790

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Abstract

We use Minkowski functionals (MFs) to constrain a primordial non-Gaussian contribution to the cosmic microwave background intensity field as observed in the 150- and 145-GHz BOOMERanG maps from the 1998 and 2003 flights, respectively, performing for the first time a joint analysis of the two data sets. A perturbative expansion of the MF formulae in the limit of a weakly non-Gaussian field yields analytical formulae, derived by Hikage et al., which can be used to constrain the coupling parameter f_(NL) without the need for non-Gaussian simulations. We find −770 < f_(NL) < 500 at 95 per cent CL, significantly improving the previous constraints by De Troia et al. on the BOOMERanG 2003 data set. These are the best f_(NL) limits to date for suborbital probes.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1111/j.1365-2966.2010.17228.xDOIArticle
https://arxiv.org/abs/0905.4301arXivDiscussion Paper
ORCID:
AuthorORCID
Bock, J. J.0000-0002-5710-5212
Additional Information:© 2010 The Authors. Journal compilation © 2010 RAS. Accepted 2010 June 21. Received 2010 May 18; in original form 2009 June 2. Published: 19 October 2010. The BOOMERanG team gratefully acknowledges support from the CIAR, CSA and NSERC in Canada; Agenzia Spaziale Italiana, University La Sapienza and Programma Nazionale Ricerche in Antartide in Italy; PPARC and the Leverhulme Trust in the UK and NASA (awards NAG5-9251 and NAG5-12723) and NSF (awards OPP-9980654 and OPP-0407592) in the USA. Additional support for detector development was provided by CIT and JPL. Field, logistical and flight support were supplied by USAP and NSBF. This research used resources at NERSC, supported by the DOE under Contract No. DE-AC03-76SF00098, and CASPUR (Rome, Italy; special thanks are due to M. Botti and F. Massaioli). We also acknowledge partial support from ASI Contract I/016/07/0 ‘COFIS’ and ASI Contract Planck LFI activity of Phase E2. Some of the results in this paper have been derived using the HEALPIX package (Górski et al. 2005). CH acknowledges support from the Particle Physics and Astronomy Research Council grant number PP/C501692/1 and a JSPS (Japan Society for the Promotion of Science) fellowship. We thank an anonymous referee for useful suggestions.
Funders:
Funding AgencyGrant Number
Canadian Institute for Advanced Research (CIFAR)UNSPECIFIED
Canadian Space Agency (CSA)UNSPECIFIED
Natural Sciences and Engineering Research Council of Canada (NSERC)UNSPECIFIED
Agenzia Spaziale Italiana (ASI)I/016/07/0
University La SapienzaUNSPECIFIED
Programma Nazionale Ricerche in Antartide (PNRA)UNSPECIFIED
Particle Physics and Astronomy Research Council (PPARC)PP/C501692/1
Leverhulme TrustUNSPECIFIED
NASANAG5-9251
NASANAG5-12723
NSFOPP-9980654
NSFOPP-0407592
CaltechUNSPECIFIED
JPLUNSPECIFIED
Department of Energy (DOE)DE-AC03-76SF00098
Japan Society for the Promotion of Science (JSPS)UNSPECIFIED
Subject Keywords:methods: analytical, methods: statistical, early Universe, cosmic background radiation, cosmology: observations
Issue or Number:3
Record Number:CaltechAUTHORS:20200129-140653790
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200129-140653790
Official Citation:P. Natoli, G. De Troia, C. Hikage, E. Komatsu, M. Migliaccio, P. A. R. Ade, J. J. Bock, J. R. Bond, J. Borrill, A. Boscaleri, C. R. Contaldi, B. P. Crill, P. de Bernardis, G. de Gasperis, A. de Oliveira-Costa, G. Di Stefano, E. Hivon, T. S. Kisner, W. C. Jones, A. E. Lange, S. Masi, P. D. Mauskopf, C. J. MacTavish, A. Melchiorri, T. E. Montroy, C. B. Netterfield, E. Pascale, F. Piacentini, G. Polenta, S. Ricciardi, G. Romeo, J. E. Ruhl, M. Tegmark, M. Veneziani, N. Vittorio, BOOMERanG constraints on primordial non-Gaussianity from analytical Minkowski functionals, Monthly Notices of the Royal Astronomical Society, Volume 408, Issue 3, November 2010, Pages 1658–1665, https://doi.org/10.1111/j.1365-2966.2010.17228.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100994
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:29 Jan 2020 22:16
Last Modified:29 Jan 2020 22:16

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