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Continuous Gravitational Waves from Magnetized White Dwarfs: Quantifying the Detection Plausibility by LISA

  • Authors: Mayusree Das, Banibrata Mukhopadhyay, Tomasz Bulik

Mayusree Das et al 2025 The Astrophysical Journal 995 .

  • Provider: AAS Journals

Caption: Figure 4.

Top panel: decay of ν (red solid) and χ (blue dashed) as functions of time for initial ν = 0.05 Hz, χ = 3 for a toroidally dominated WD—WD1+BP ( ﹩{B}_{max}^{{\rm{Toroidal}}}=4\times 1{0}^{13}﹩ G, ﹩{B}_{p}^{{\rm{Poloidal}}}=8\times 1{0}^{8}﹩ G) with a magnetosphere. For the same WD, the middle panel shows the variation of luminosities, and the bottom panel shows GW strain decay with time.

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