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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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Lenguaje: | eng |
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2022
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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 & 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 & 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 |