Pith. sign in

REVIEW 2 cited by

Joint gravitational wave detection by TianQin and LISA

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2407.11293 v2 pith:6UQSCGCV submitted 2024-07-16 astro-ph.HE gr-qc

Alejandro Torres-Orjuela This is my paper · ORCID
classification astro-ph.HEgr-qc
keywords detectionimrisjointlisasgwbtianqinaccuracybinaries
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We study the detection accuracy of double white dwarfs (DWDs), stellar-mass black hole binaries (SBHBs), light and heavy intermediate mass ratio inspirals (IMRIs), extreme mass ratio inspirals (EMRIs), massive black hole binaries (MBHBs), and the stochastic gravitational wave background (SGWB) of astronomical origin for TianQin, LISA, and joint detection. We use a Fisher matrix analysis and consider for each source the averaged detection accuracy over a realistic range of parameters. We find that on average TianQin obtains more accurate parameter estimation for DWDs and light IMRIs, LISA for heavy IMRIs, EMRIs, MBHBs, and the galactic foreground of the SGWB, and both contribute similarly to the detection of SBHBs and the extra-galactic SGWB. Nevertheless, for all sources joint detection allows setting tighter constraints on most parameters highlighting its importance for future detection.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Gravitational Wave Signatures of Quasi-Periodic Eruptions: LISA Detection Prospects for RX J1301.9+2747

    astro-ph.HE 2025-08 conditional novelty 6.0 of 10

    Modeling quasi-periodic eruptions as eccentric EMRIs with disk impacts yields high-frequency tails and frequency shifts in GW waveforms, making RX J1301.9+2747 potentially detectable by LISA for orbiter masses above a...

  2. Detection of Intermediate-Mass Ratio Inspirals in Globular Clusters: Revealing the Brownian Motion with Gravitational Waves

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    Brownian motion from stellar encounters in globular clusters imprints Doppler and aberrational phase shifts on IMRI gravitational waves that should be detectable for most sources loud enough for TianQin, LISA, or AION to see.

Pith tools