An apparent positive relation between spin and orbital angular momentum in X-ray binaries
Zhen Yan, Wenda Zhang, Wenfei Yu

TL;DR
This study finds a positive correlation between black hole spin and orbital parameters in X-ray binaries, suggesting accretion as a key mechanism in spinning up compact objects and explaining the bimodal distribution of black hole spins.
Contribution
It reveals a bimodal distribution of black hole spins and establishes a positive relation between spin and orbital parameters across different XRB types, indicating diverse accretion histories.
Findings
Bimodal distribution of BH spin parameters centered at ~0.17 and 0.83.
Positive correlation between spin and orbital period/separation.
Different accretion histories inferred for low and high spin BHs.
Abstract
The origin of current angular momentum (AM) of the black hole (BH) in X-ray binary (XRB) is still unclear, which is related with the birth and/or the growth of the BH. Here we collect the spin parameters measured in BH XRBs and find an apparent bimodal distribution centered at 0.17 and 0.83. We find a positive relation between the spin parameter and the orbital period/orbital separation through combining distinct XRB categories, including neutron star (NS) low-mass X-ray binaries (LMXBs), Roche-lobe overflow (RLOF) BH XRBs and wind-fed BH XRBs. It seems that the AM of the compact star and the binary orbit correlates by combining the different XRB systems. These positive relations imply that accretion process is a common mechanism for spinning up the compact star in these diverse XRB systems. We infer that the low and high spin BH XRBs may experience different evolution…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Mechanics and Biomechanics Studies · Geophysics and Sensor Technology
