The progenitor of binary millisecond radio pulsar PSR J1713+0747 (Research Note)
Wen-Cong Chen, and Jorge A. Panei

TL;DR
This study models the evolutionary history of the binary millisecond pulsar PSR J1713+0747, supporting its origin from a low-mass X-ray binary with specific initial conditions, and compares predicted WD properties with observations.
Contribution
It provides detailed binary evolution models for PSR J1713+0747, confirming the LMXB origin hypothesis and estimating progenitor parameters consistent with observed data.
Findings
Progenitor was a low-mass X-ray binary with a 1.3-1.6 M_sun donor star.
Initial orbital period ranged from 2.40 to 4.15 days.
Predicted white dwarf temperature slightly higher than observed.
Abstract
PSR J1713+0747 is a binary system comprising millisecond radio pulsar with a spin period of 4.57 ms, and a low-mass white dwarf (WD) companion orbiting the pulsar with a period of 67.8 days. Using the general relativistic Shapiro delay, the masses of the WD and pulsar components were previously found to be and (68% confidence), respectively. Standard binary evolution theory suggests that PSR J1713+0747 evolved from a low-mass X-ray binary (LMXB). Here, we test this hypothesis. We used a binary evolution code and a WD evolution code to calculate evolutionary sequences of LMXBs that could result in binary millisecond radio pulsars such as PSR J1713+0747. During the mass exchange, the mass transfer is nonconservative. Because of the thermal and viscous instabilities developing in the accretion disk, the neutron star accretes only a small part…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · High-pressure geophysics and materials · Astrophysical Phenomena and Observations
