Forward Modelling the O3a GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions

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Title

Forward Modelling the O3a GW transient mass distributions with BPASS by varying compact remnant mass and SNe kick prescriptions

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The University of Auckland Library

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ResearchSpace@Auckland

Description

We present forward modelling from the \textsc{bpass} code suite of the population of observed gravitational wave (GW) transients reported by the LIGO/VIRGO consortium (LVC) during the first half of their third observing run (O3a). Specifically, we predict the expected chirp mass and mass ratio distributions for GW transients, taking account of detector sensitivity to determine how many events should have been detected by the current detector network in O3a. We investigate how these prediction...

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Research paper

Research format

Journal article

Creator

Ghodla, Sohan / Zeist, Wouter GJ van / Eldridge, JJ / Stevance, Héloïse F / Stanway, Elizabeth R

URL

https://hdl.handle.net/2292/57584

Related subjects

astro-ph.HE / astro-ph.SR / gr-qc

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