Binary White Dwarfs as Gravitational Wave Sources for LISA

arXiv:2607.17787 · astro-ph.SR, astro-ph.GA, astro-ph.HE · Submitted 2026-07-20 · Read on arXiv

Sreeta Roy, Surajit Kalita, Tomasz Bulik, Dorota Gondek-Rosińska

astro-ph.SR, astro-ph.GA, astro-ph.HE

Submitted: 2026-07-20

Comments: 13 pages with 5 figures and 2 tables; comments welcome

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Metallicity — 37× in this paper · explained in 3 episodes
• Population Synthesis — 10× in this paper · explained in 2 episodes
• Core — 8× in this paper · explained in 2 episodes
• Milky Way — 8× in this paper
• Accretion Efficiency — 4× in this paper · explained in 2 episodes
• Laser Interferometer Space Antenna — 3× in this paper
• Angular Momentum Loss — 1× in this paper · explained in 1 episode
• Anisotropy — 1× in this paper · explained in 3 episodes
• Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

• A Practical Theorem on Gravitational Wave Backgrounds

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