Magnetic Wind From a Massive White Dwarf Merger: References

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15 May 2024

This paper is available on arxiv under CC 4.0 license.

Authors:

(1) Yici Zhong, Department of Physics, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan;

(2) Kazumi Kashiyama, Research Center for the Early Universe, Graduate School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan and Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU,WPI), The University of Tokyo, Chiba 277-8582, Japan;

(3) Shinsuke Takasao, Department of Earth and Space Science, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan;

(4) Toshikazu Shigeyama, Research Center for the Early Universe (RESCEU), School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan and Department of Astronomy, School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan;

(5) Kotaro Fujisawa, Research Center for the Early Universe (RESCEU), School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan and Department of Liberal Arts, Tokyo University of Technology, Ota-ku, Tokyo 144-0051, Japan.

Abstract and Intro

Setup

Result

Summary and Discussion

Appendix

A. Dual Energy Formalism

B. Convergence of Results

C. Change of the Mass Loss Rate in MHD Regime

References

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Figure 6. Parameter dependence of the ratio between time-averaged mass loss rate after turning on the magnetic fields M˙ MHD and the value for pressure-driven wind M˙ HD on surface magnetic field B∗ and WD spin frequency Ω∗.

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