papers

Publications (35)

astro-ph.HE2021

Gravitational Wave Signals from Two-Dimensional Core-Collapse Supernova Models with Rotation and Magnetic Fields

Rylan Jardine, Jade Powell, Bernhard Müller

We investigate the impact of rotation and magnetic fields on the dynamics and gravitational wave emission in 2D core-collapse supernova simulations with neutrino transport. We simu…

astro-ph.HE2021

Detecting and reconstructing gravitational waves from the next Galactic core-collapse supernova in the Advanced Detector Era

Marek Szczepanczyk, Javier Antelis, Michael Benjamin +17

We performed a detailed analysis of the detectability of a wide range of gravitational waves derived from core-collapse supernova simulations using gravitational-wave detector nois…

gr-qc2020

Core-Collapse Supernova Gravitational-Wave Search and Deep Learning Classification

Alberto Iess, Elena Cuoco, Filip Morawski +1

We describe a search and classification procedure for gravitational waves emitted by core-collapse supernova (CCSN) explosions, using a convolutional neural network (CNN) combined…

astro-ph.IM2016

Classification methods for noise transients in advanced gravitational-wave detectors II: performance tests on Advanced LIGO data

Jade Powell, Alejandro Torres-Forné, Ryan Lynch +5

The data taken by the advanced LIGO and Virgo gravitational-wave detectors contains short duration noise transients that limit the significance of astrophysical detections and redu…

astro-ph.HE2017

Inferring the core-collapse supernova explosion mechanism with three-dimensional gravitational-wave simulations

Jade Powell, Marek Szczepanczyk, Ik Siong Heng

A detection of a core-collapse supernova signal with an Advanced LIGO and Virgo gravitational-wave detector network will allow us to measure astrophysical parameters of the source.…

astro-ph.HE2026

Reconstructing Core-Collapse Supernova Gravitational-Wave Signals with Transdimensional Bayesian Inference

Hayden Chapman, Jade Powell, Nir Guttman +2

Core-collapse supernovae (CCSNe) are promising future sources of gravitational waves for current and next-generation observatories. Reconstructing CCSN gravitational-wave signals i…

astro-ph.HE2024

An Optically Targeted Search for Gravitational Waves emitted by Core-Collapse Supernovae during the Third Observing Run of Advanced LIGO and Advanced Virgo

Marek J. Szczepańczyk, Yanyan Zheng, Javier M. Antelis +35

We present the results from a search for gravitational-wave transients associated with core-collapse supernovae observed optically within 30 Mpc during the third observing run of A…

astro-ph.IM2019

Reconstructing Gravitational Wave Core-Collapse Supernova Signals with Dynamic Time Warping

Sofia Suvorova, Jade Powell, Andrew Melatos

Core-collapse supernovae (CCSNe) are a potential source for ground-based gravitational wave detectors, as their predicted emission peaks in the detectors' frequency band. Typical s…

astro-ph.HE2021

The final core collapse of pulsational pair instability supernovae

Jade Powell, Bernhard Müller, Alexander Heger

We present 3D core-collapse supernova simulations of massive Pop-III progenitor stars at the transition to the pulsational pair instability regime. We simulate two progenitor model…

astro-ph.HE2025

Gravitational waves from core-collapse supernovae with no electromagnetic counterparts

Jade Powell, Bernhard Müller

Core-collapse supernovae (CCSNe) are regularly observed electromagnetically, prompting targetted searches for their gravitational-wave emission. However, there are scenarios where…

gr-qc2021

The SPIIR online coherent pipeline to search for gravitational waves from compact binary coalescences

Qi Chu, Manoj Kovalam, Linqing Wen +16

This paper presents the SPIIR pipeline used for public alerts during the third advanced LIGO and Virgo observation run (O3 run). The SPIIR pipeline uses infinite impulse response (…

astro-ph.IM2018

Bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy

Gregory Ashton, Moritz Huebner, Paul D. Lasky +18

Bayesian parameter estimation is fast becoming the language of gravitational-wave astronomy. It is the method by which gravitational-wave data is used to infer the sources' astroph…

gr-qc2025

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

astro-ph.HE2019

The impact of pair-instability mass loss on the binary black hole mass distribution

Simon Stevenson, Matthew Sampson, Jade Powell +4

A population of binary black hole mergers has now been observed in gravitational waves by Advanced LIGO and Virgo. The masses of these black holes appear to show evidence for a pil…

astro-ph.HE2020

Three-dimensional core-collapse supernova simulations of massive and rotating progenitors

Jade Powell, Bernhard Müller

We present three-dimensional simulations of the core-collapse of massive rotating and non-rotating progenitors performed with the general relativistic neutrino hydrodynamics code C…

astro-ph.IM2023

Generating transient noise artifacts in gravitational-wave detector data with generative adversarial networks

Jade Powell, Ling Sun, Katinka Gereb +2

Transient noise glitches in gravitational-wave detector data limit the sensitivity of searches and contaminate detected signals. In this Paper, we show how glitches can be simulate…

astro-ph.IM2019

Astrophysics with core-collapse supernova gravitational wave signals in the next generation of gravitational wave detectors

Vincent Roma, Jade Powell, Ik Siong Heng +1

The next generation of gravitational wave detectors will improve the detection prospects for gravitational waves from core-collapse supernovae. The complex astrophysics involved in…

astro-ph.HE2025

Strategy for identifying Vera C. Rubin Observatory kilonova candidates for targeted gravitational-wave searches

Simon Stevenson, Anais Möller, Jade Powell

Since the observation of the binary neutron star merger GW170817 and the associated kilonova AT2017gfo, the next joint gravitational-wave/optical kilonova has been highly anticipat…

astro-ph.HE2024

Determining the core-collapse supernova explosion mechanism with current and future gravitational-wave observatories

Jade Powell, Alberto Iess, Miquel Llorens-Monteagudo +5

Gravitational waves are emitted from deep within a core-collapse supernova, which may enable us to determine the mechanism of the explosion from a gravitational-wave detection. Pre…

astro-ph.HE2016

Inferring the core-collapse supernova explosion mechanism with gravitational waves

Jade Powell, Sarah E. Gossan, Joshua Logue +1

A detection of a core-collapse supernova (CCSN) gravitational-wave (GW) signal with an Advanced LIGO and Virgo detector network may allow us to measure astrophysical parameters of…

astro-ph.HE2026

The deci-Hz gravitational wave signal from the collapse of rotating very massive stars

Bailey Sykes, Jade Powell, Bernhard Müller +1

We calculate the gravitational wave signal from the collapse of a rotating 300 star at the upper end of the pair-instability regime. The large-scale asymmetries that deve…

astro-ph.HE2020

Enhancing Gravitational-Wave Science with Machine Learning

Elena Cuoco, Jade Powell, Marco Cavaglià +23

Machine learning has emerged as a popular and powerful approach for solving problems in astrophysics. We review applications of machine learning techniques for the analysis of grou…

astro-ph.HE2025

The minimum neutron star mass in neutrino-driven supernova explosions

Bernhard Müller, Alexander Heger, Jade Powell

Supernova theory has struggled to explain the lightest known neutron star candidate with an accurate mass determination, the companion in the eccentric comp…

astro-ph.HE2019

Gravitational Wave Emission from 3D Explosion Models of Core-Collapse Supernovae with Low and Normal Explosion Energies

Jade Powell, Bernhard Müller

Understanding gravitational wave emission from core-collapse supernovae will be essential for their detection with current and future gravitational wave detectors. This requires a…

astro-ph.HE2023

Gravitational Waves from a Core g-Mode in Supernovae as Probes of the High-Density Equation of State

Pia Jakobus, Bernhard Müller, Alexander Heger +5

Using relativistic supernova simulations of massive progenitor stars with a quark-hadron equation of state (EoS) and a purely hadronic EoS, we identify a distinctive feature in the…

astro-ph.HE2022

Inferring Astrophysical Parameters of Core-Collapse Supernovae from their Gravitational-Wave Emission

Jade Powell, Bernhard Müller

Nearby core-collapse supernovae (CCSNe) are powerful multi-messenger sources for gravitational-wave, neutrino and electromagnetic telescopes as they emit gravitational waves in the…

astro-ph.HE2026

Impact of the nuclear equation of state on the explodability of massive stars

Jade Powell, Bernhard Müller

In recent years, astrophysical observations have placed tight constraints on key properties of the nuclear equation of state (EoS). Using 93 two-dimensional simulations for three d…

astro-ph.HE2024

The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields

Jade Powell, Bernhard Müller

Gravitational waveform predictions from 3D simulations of explosions of non-rotating massive stars with no magnetic fields have been extensively studied. However, the impact of mag…

astro-ph.IM2015

Classification methods for noise transients in advanced gravitational-wave detectors

Jade Powell, Daniele Trifiro, Elena Cuoco +2

Noise of non-astrophysical origin will contaminate science data taken by the Advanced Laser Interferometer Gravitational-wave Observatory (aLIGO) and Advanced Virgo gravitational-w…

astro-ph.HE2025

The DAWES review: Gravitational-wave burst astrophysics

Jade Powell, Paul D. Lasky

Over a hundred gravitational-wave signals have now been detected from the mergers of black holes and neutron stars, but other sources of gravitational waves have not yet been disco…

astro-ph.HE2019

Unmodelled Clustering Methods for Gravitational Wave Populations of Compact Binary Mergers

Jade Powell, Simon Stevenson, Ilya Mandel +1

The mass and spin distributions of compact binary gravitational-wave sources are currently uncertain due to complicated astrophysics involved in their formation. Multiple sub-popul…

astro-ph.IM2018

Parameter Estimation and Model Selection of Gravitational Wave Signals Contaminated by Transient Detector Noise Glitches

Jade Powell

The number of astrophysical sources detected by Advanced LIGO and Virgo is expected to increase as the detectors approach their design sensitivity. Gravitational wave detectors are…

astro-ph.HE2024

Nucleosynthesis in the Innermost Ejecta of Magnetorotational Supernova Explosions in 3-dimensions

Shuai Zha, Bernhard Müller, Jade Powell

Core-collapse supernova (CCSN) explosions powered by rotation and magnetic fields present an interesting astrophysical site for nucleosynthesis that potentially contributes to the…

gr-qc2023

Open data from the third observing run of LIGO, Virgo, KAGRA and GEO

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1741

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data…

astro-ph.HE2023

Three dimensional magnetorotational core-collapse supernova explosions of a 39 solar mass progenitor star

Jade Powell, Bernhard Mueller, David R. Aguilera-Dena +1

We perform three-dimensional simulations of magnetorotational supernovae using a progenitor star with two different initial magnetic field strengths of G…