A Massive-born Neutron Star with a Massive White Dwarf Companion
arXiv:1706.08060 · doi:10.3847/1538-4357/aa7bee
Abstract
We report on the results of a 4-year timing campaign of PSR~J2222, a 2.44-day binary pulsar with a massive white dwarf (WD) companion, with the Nançay, Effelsberg and Lovell radio telescopes. Using the Shapiro delay for this system, we find a pulsar mass and a WD mass . We also measure the rate of advance of periastron for this system, which is marginally consistent with the GR prediction for these masses. The short lifetime of the massive WD progenitor star led to a rapid X-ray binary phase with little () mass accretion onto the neutron star (NS); hence, the current pulsar mass is, within uncertainties, its birth mass; the largest measured to date. We discuss the discrepancy with previous mass measurements for this system; we conclude that the measurements presented here are likely to be more accurate. Finally, we highlight the usefulness of this system for testing alternative theories of gravity by tightly constraining the presence of dipolar radiation. This is of particular importance for certain aspects of strong-field gravity, like spontaneous scalarization, since the mass of PSR~J2222 puts that system into a poorly tested parameter range.
17 pages in journal format, 3 figures, 2 tables, accepted for publication in the Astrophysical Journal. Some references fixed and updated
References in corpus (16)
- The Confrontation between General Relativity and Experiment
- A Massive Pulsar in a Compact Relativistic Binary
- Masses, Radii, and Equation of State of Neutron Stars
- TEMPO2, a new pulsar timing package. I: Overview
- PSRCHIVE and PSRFITS An Open Approach to Radio Pulsar Data Storage and Analysis
- Pre-Supernova Evolution of Massive Single and Binary Stars
- An Ultraluminous X-ray Source Powered by An Accreting Neutron Star
- Tempo2, a new pulsar timing package. II: The timing model and precision estimates
- The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity
- The Landscape of the Neutrino Mechanism of Core-Collapse Supernovae: Neutron Star and Black Hole Mass Functions, Explosion Energies and Nickel Yields
- Formation of millisecond pulsars with CO white dwarf companions - II. Accretion, spin-up, true ages and comparison to MSPs with He white dwarf companions
- The relativistic pulsar-white dwarf binary PSR J1738+0333 I. Mass determination and evolutionary history
- Measuring pulse times of arrival from broadband pulsar observations
- A Massive Millisecond Pulsar in an Eccentric Binary
- A 1.05 Companion to PSR J2222-0137: The Coolest Known White Dwarf?
- Microarcsecond VLBI pulsar astrometry with PSRPI I. Two binary millisecond pulsars with white dwarf companions
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