Formation of extremely low-mass white dwarf binaries undergoing enhanced angular momentum loss
Ziqi Zhao, Zhenwei Li, Zhengwei Liu, Hailiang Chen, Hongwei Ge, Xiangcun Meng, Dengkai Jiang, Xuefei Chen, Zhanwen Han

TL;DR
This study models the formation of extremely low-mass white dwarf binaries with enhanced angular momentum loss, successfully explaining observed shorter orbital periods than previous theories.
Contribution
It introduces a model with increased angular momentum loss during mass transfer, accounting for observed properties of ELM WD binaries not explained by earlier models.
Findings
Enhanced AML shifts the WD mass-orbital period relation downward.
The model reproduces most observed ELM WD binary systems.
Structural differences in WDs affect their mass-radius relation.
Abstract
Extremely low-mass white dwarfs (ELM WDs) are helium (He) WDs with masses below , mainly formed through binary interaction. ELM WD binaries typically are formed from two channels, namely the stable Roche lobe overflow (RLOF) channel and the common envelope ejection channel. For ELM WD binaries produced from RLOF channel, the ELM WD mass has a strong correlation with the orbital period, i.e., the so-called WD mass-orbital period relation. However, the observations in the ELM Survey show that the orbital periods of ELM WD binaries from the RLOF channel are typically shorter than the theoretically predicted values. Extra angular momentum loss (AML) may be needed to explain such a phenomenon. In this work, we assumed that part of the transferred mass from the donor is lost at the outer Lagrangian point and simulated the formation of ELM WD binaries. Enhanced AML enables…
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