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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...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
2013
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2013/10/001 http://cds.cern.ch/record/1546485 |
_version_ | 1780930124501221376 |
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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 |
record_format | invenio |
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 |