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Extending the Observational Frequency Range for Gravitational Waves in a Pulsar Timing Array

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 نشر من قبل Chan Park
 تاريخ النشر 2021
  مجال البحث فيزياء
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 تأليف Chan Park




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We provide an observation method for gravitational waves using a pulsar timing array to extend the observational frequency range up to the rotational frequency of pulsars. For this purpose, we perform an analysis of a perturbed electromagnetic wave in perturbed spacetime from the field perspective. We apply the analysis to the received electromagnetic waves in a radio telescope, which partially composes the periodic electromagnetic pulse emitted by a pulsar. For simple observation, two frequency windows are considered. For each window, we propose gauge-invariant quantities and discuss their observations.



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