Dr Simone Scaringi simone.scaringi@durham.ac.uk
Associate Professor
Cataclysmic variables are a key population of gravitational wave sources for LISA
Scaringi, S; Breivik, K; Littenberg, T B; Knigge, C; Groot, P J; Veresvarska, M
Authors
K Breivik
T B Littenberg
C Knigge
P J Groot
Martina Veresvarska martina.veresvarska@durham.ac.uk
PGR Student Doctor of Philosophy
Abstract
The gravitational wave (GW) signals from the Galactic population of cataclysmic variables (CVs) have yet to be carefully assessed. Here, we estimate these signals and evaluate their significance for Laser Interferometer Space Antenna (LISA). First, we find that at least three known systems are expected to produce strong enough signals to be individually resolved within the first four years of LISA’s operation. Secondly, CVs will contribute significantly to the LISA Galactic binary background, limiting the mission’s sensitivity in the relevant frequency band. Third, we predict a spike in the unresolved GW background at a frequency corresponding to the CV minimum orbital period. This excess noise may impact the detection of other systems near this characteristic frequency. Fourth, we note that the excess noise spike amplitude and location associated with Pmin ∼ 80 min can be used to measure the CV space density and period bounce location with complementary and simple GW biases compared to the biases and selection effects plaguing samples selected from electromagnetic signals. Our results highlight the need to explicitly include the Galactic CV population in the LISA mission planning, both as individual GW sources and generators of background noise, as well as the exciting prospect of characterising the CV population through their GW emission.
Citation
Scaringi, S., Breivik, K., Littenberg, T. B., Knigge, C., Groot, P. J., & Veresvarska, M. (2023). Cataclysmic variables are a key population of gravitational wave sources for LISA. Monthly Notices of the Royal Astronomical Society: Letters, 525(1), L50-L55. https://doi.org/10.1093/mnrasl/slad093
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 4, 2023 |
Online Publication Date | Jul 6, 2023 |
Publication Date | 2023-10 |
Deposit Date | Aug 17, 2023 |
Publicly Available Date | Aug 17, 2023 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Electronic ISSN | 1745-3933 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 525 |
Issue | 1 |
Pages | L50-L55 |
DOI | https://doi.org/10.1093/mnrasl/slad093 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://durham-repository.worktribe.com/output/1720511 |
Files
Published Journal Article
(976 Kb)
PDF
Licence
http://creativecommons.org/licenses/by/4.0/
Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/
Copyright Statement
© The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
You might also like
Burst-induced spin variations in the accreting magnetic white dwarf PBC J0801.2–4625
(2024)
Journal Article
Evolution of spin in the intermediate polar CC sculptoris
(2024)
Journal Article
The Peculiar Bursting Nature of CP Pup
(2024)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search