Evolving LMXBs: CARB Magnetic Braking
K. X. Van, N. Ivanova

TL;DR
This paper introduces the CARB magnetic braking model, which improves the theoretical understanding of mass transfer in neutron star low-mass X-ray binaries, aligning predictions with observed data.
Contribution
The paper presents a new magnetic braking prescription, CARB, that incorporates recent insights into stellar magnetic fields and rotation, resolving previous discrepancies in LMXB evolution models.
Findings
CARB magnetic braking reproduces observed mass transfer rates.
The model aligns theory with observed orbital periods and mass ratios.
It agrees with donor star temperature measurements.
Abstract
The formation of low-mass X-ray binaries (LMXBs) is an ongoing challenge in stellar evolution. The important subset of LMXBs are the binary systems with a neutron star (NS) accretor. In NS LMXBs with non-degenerate donors, the mass transfer is mainly driven by magnetic braking. The discrepancies between the observed mass transfer (MT) rates and the theoretical models were known for a while. Theory predictions of the MT rates are too weak and differ by an order of magnitude or more. Recently, we showed that with the standard magnetic braking, it is not possible to find progenitor binary systems such that they could reproduce -- at any time of their evolution -- most of the observed persistent NS LMXBs. In this we present a modified magnetic braking prescription, CARB (Convection And Rotation Boosted). CARB magnetic braking combines two recent improvements in understanding…
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