Evolutionary Period Changes for 25 X-ray Binaries and the Measurement of an Empirical Universal Law for Angular Momentum Loss in Accreting Binaries
Bradley E. Schaefer (Louisiana State University)

TL;DR
This study measures period changes in 77 X-ray binaries and cataclysmic variables to empirically derive a universal law for angular momentum loss, challenging existing theoretical models and providing a new predictive framework.
Contribution
It introduces an empirical universal law for angular momentum loss in accreting binaries, based on direct measurements, and tests the inadequacy of traditional magnetic braking models.
Findings
Most systems' AML predictions deviate by over an order of magnitude from models.
The derived AML law fits observed data across different binary classes.
Three distinct AML laws are proposed for different period ranges, forming a universal description.
Abstract
I measure and collect timings of phase markers (like eclipse times) for the orbits of 25 X-ray binaries (XRBs) so as to calculate the steady evolutionary period change (). I combine these with my observed measures from 52 cataclysmic variables (CVs). Further, I subtract out the contributions from gravitational radiation () and mass transfer (), deriving the period change from the residual unknown angular momentum loss (=--). I have measures for 77 XRBs and CVs, with these being direct measures of the driver of binary evolution. The venerable Magnetic Braking Model (MBM) of binary evolution has its most fundamental predictions tested, with most systems having predictions wrong by over one order-of-magnitude. Other proposed mechanisms to explain the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Stellar, planetary, and galactic studies · Pulsars and Gravitational Waves Research
