- Research Article
- 10.1088/1674-1056/ae50de
Revisit the orbital period and eccentricity distribution: implications on the multiple origins for double neutron stars
- Mar 12, 2026
- Chinese Physics B
- Yiyan Yang
Abstract Double neutron-star (DNS) systems are key compact-binary laboratories for testing gravitational waves and general relativity. It is highly necessary for research on the origin and evolutionary pathways of the DNS system. The Extreme Deconvolution Method, based on a Gaussian mixture model, is applied to an updated sample of 33 DNS pairs,which might provide a clue for understanding the DNS formation scenarios. The result of the Bayesian Information Criterion (BIC) confirms the bimodality of the DNS in the orbital periodeccentricity plane, which can be attributed to different formation mechanisms. 14 DNS systems with low eccentricities and orbital periods shorter than 1 day originated from low-energy electron capture supernovae, which merge within the Hubble time. 18 DNS systems exhibiting longer orbital periods and higher eccentricities are formed through core collapse supernova explosions. Based on 13 DNS systems with precisely measured component masses, the merger timescales are calculated, and it is found that most DNSs with orbital periods shorter than 1 day are expected to merge within the Hubble time. This result provides further constraints on the DNS merger rate within the Galaxy.
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