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Optimal analysis of azimuthal features in the CMB

We present algorithms for searching for azimuthally symmetric features in CMB data. Our algorithms are fully optimal for masked all-sky data with inhomogeneous noise, computationally fast, simple to implement, and make no approximations. We show how to implement the optimal analysis in both Bayesian...

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Detalles Bibliográficos
Autores principales: Osborne, Stephen, Senatore, Leonardo, Smith, Kendrick
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2013/10/001
http://cds.cern.ch/record/1546485
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author Osborne, Stephen
Senatore, Leonardo
Smith, Kendrick
author_facet Osborne, Stephen
Senatore, Leonardo
Smith, Kendrick
author_sort Osborne, Stephen
collection CERN
description We present algorithms for searching for azimuthally symmetric features in CMB data. Our algorithms are fully optimal for masked all-sky data with inhomogeneous noise, computationally fast, simple to implement, and make no approximations. We show how to implement the optimal analysis in both Bayesian and frequentist cases. In the Bayesian case, our algorithm for evaluating the posterior likelihood is so fast that we can do a brute-force search over parameter space, rather than using a Monte Carlo Markov chain. Our motivating example is searching for bubble collisions, a pre-inflationary signal which can be generated if multiple tunneling events occur in an eternally inflating spacetime, but our algorithms are general and should be useful in other contexts.
id cern-1546485
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
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spelling cern-15464852019-09-30T06:29:59Zdoi:10.1088/1475-7516/2013/10/001http://cds.cern.ch/record/1546485engOsborne, StephenSenatore, LeonardoSmith, KendrickOptimal analysis of azimuthal features in the CMBAstrophysics and AstronomyWe present algorithms for searching for azimuthally symmetric features in CMB data. Our algorithms are fully optimal for masked all-sky data with inhomogeneous noise, computationally fast, simple to implement, and make no approximations. We show how to implement the optimal analysis in both Bayesian and frequentist cases. In the Bayesian case, our algorithm for evaluating the posterior likelihood is so fast that we can do a brute-force search over parameter space, rather than using a Monte Carlo Markov chain. Our motivating example is searching for bubble collisions, a pre-inflationary signal which can be generated if multiple tunneling events occur in an eternally inflating spacetime, but our algorithms are general and should be useful in other contexts.arXiv:1305.1970CERN-PH-TH-2013-094oai:cds.cern.ch:15464852013-05-10
spellingShingle Astrophysics and Astronomy
Osborne, Stephen
Senatore, Leonardo
Smith, Kendrick
Optimal analysis of azimuthal features in the CMB
title Optimal analysis of azimuthal features in the CMB
title_full Optimal analysis of azimuthal features in the CMB
title_fullStr Optimal analysis of azimuthal features in the CMB
title_full_unstemmed Optimal analysis of azimuthal features in the CMB
title_short Optimal analysis of azimuthal features in the CMB
title_sort optimal analysis of azimuthal features in the cmb
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1088/1475-7516/2013/10/001
http://cds.cern.ch/record/1546485
work_keys_str_mv AT osbornestephen optimalanalysisofazimuthalfeaturesinthecmb
AT senatoreleonardo optimalanalysisofazimuthalfeaturesinthecmb
AT smithkendrick optimalanalysisofazimuthalfeaturesinthecmb