activity
20182020
collaborators

5 papers

astro-ph.HE2020

Evolution of gas disc-embedded intermediate mass ratio inspirals in the LISA band

A. Derdzinski, D. D'Orazio, P. Duffell +2

Among the potential milliHz gravitational wave (GW) sources for the upcoming space-based interferometer LISA are extreme- or intermediate-mass ratio inspirals (EMRI/IMRIs). These e…

astro-ph.SR2019

Circumbinary Disks: Accretion and Torque as a Function of Mass Ratio and Disk Viscosity

Paul C. Duffell, Daniel D'Orazio, Andrea Derdzinski +4

Using numerical hydrodynamics calculations and a novel method for densely sampling parameter space, we measure the accretion and torque on a binary system from a circumbinary disk.…

astro-ph.HE2019

Astro2020 Science White Paper: A Shocking Shift in Paradigm for Classical Novae

Laura Chomiuk, Elias Aydi, Aliya-Nur Babul +10

The discovery of GeV gamma-rays from classical novae has led to a reassessment of these garden-variety explosions, and highlighted their importance for understanding radiative shoc…

astro-ph.HE2019

Multimessenger science opportunities with mHz gravitational waves

John Baker, Zoltán Haiman, Elena Maria Rossi +32

LISA will open the mHz band of gravitational waves (GWs) to the astronomy community. The strong gravity which powers the variety of GW sources in this band is also crucial in a num…

astro-ph.HE2018

Probing gas disc physics with LISA: simulations of an intermediate mass ratio inspiral in an accretion disc

A. Derdzinski, D. D'Orazio, P. Duffell +2

The coalescence of a compact object with a supermassive black hole (SMBH) produces mHz gravitational waves (GWs) detectable by the future Laser Interf…