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Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection

<!--HTML--><div><span>All of the three established pulsar timing arrays (NANOGrav, EPTA, PPTA), along with international pulsar timing array (IPTA) have now reported strong Bayesian evidence for a common-spectrum stochastic process in their latest data sets, with broad agreement in...

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Autor principal: Pol, Nihan
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:http://cds.cern.ch/record/2803303
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author Pol, Nihan
author_facet Pol, Nihan
author_sort Pol, Nihan
collection CERN
description <!--HTML--><div><span>All of the three established pulsar timing arrays (NANOGrav, EPTA, PPTA), along with international pulsar timing array (IPTA) have now reported strong Bayesian evidence for a common-spectrum stochastic process in their latest data sets, with broad agreement in the recovered spectral characteristics of this process. However, evidence for the quadrupolar Hellings &amp; Downs interpulsar correlations, which are characteristic of gravitational-wave signals, is not yet significant in any of these datasets. </span></div> <div><span>In this talk, I will review these results, and describe and quantify, through realistic simulations, the key milestones that pulsar timing arrays can be expected to achieve in the next few years.</span></div>
id cern-2803303
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2022
record_format invenio
spelling cern-28033032022-11-02T22:05:14Zhttp://cds.cern.ch/record/2803303engPol, NihanAstrophysics Milestones for Pulsar Timing Array Gravitational-wave DetectionAstrophysics Milestones for Pulsar Timing Array Gravitational-wave DetectionTH Cosmo Coffee<!--HTML--><div><span>All of the three established pulsar timing arrays (NANOGrav, EPTA, PPTA), along with international pulsar timing array (IPTA) have now reported strong Bayesian evidence for a common-spectrum stochastic process in their latest data sets, with broad agreement in the recovered spectral characteristics of this process. However, evidence for the quadrupolar Hellings &amp; Downs interpulsar correlations, which are characteristic of gravitational-wave signals, is not yet significant in any of these datasets. </span></div> <div><span>In this talk, I will review these results, and describe and quantify, through realistic simulations, the key milestones that pulsar timing arrays can be expected to achieve in the next few years.</span></div>oai:cds.cern.ch:28033032022
spellingShingle TH Cosmo Coffee
Pol, Nihan
Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title_full Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title_fullStr Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title_full_unstemmed Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title_short Astrophysics Milestones for Pulsar Timing Array Gravitational-wave Detection
title_sort astrophysics milestones for pulsar timing array gravitational-wave detection
topic TH Cosmo Coffee
url http://cds.cern.ch/record/2803303
work_keys_str_mv AT polnihan astrophysicsmilestonesforpulsartimingarraygravitationalwavedetection