Email this article Low-Mass Neutron Stars with Rotation
- Authors: Yudin A.V.1,2, Razinkova T.L.1, Blinnikov S.I.1,3
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Affiliations:
- Institute for Theoretical and Experimental Physics
- “Kurchatov Institute” National Research Center
- Kavli IPMU
- Issue: Vol 45, No 12 (2019)
- Pages: 847-854
- Section: Article
- URL: https://journal-vniispk.ru/1063-7737/article/view/191725
- DOI: https://doi.org/10.1134/S1063773719120077
- ID: 191725
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Abstract
The properties of low-mass neutron stars with rigid rotation are considered. The possible evolution paths of such stars in a close binary system with mass transfer are calculated. The properties of the gamma-ray burst GRB 170817A interpreted in terms of the stripping model, a natural ingredient of which is the explosion of a low-mass neutron star—a binary component, are briefly discussed.
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About the authors
A. V. Yudin
Institute for Theoretical and Experimental Physics; “Kurchatov Institute” National Research Center
Author for correspondence.
Email: yudin@itep.ru
Russian Federation, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; pl. Kurchatova 1, Moscow, 123182
T. L. Razinkova
Institute for Theoretical and Experimental Physics
Email: yudin@itep.ru
Russian Federation, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259
S. I. Blinnikov
Institute for Theoretical and Experimental Physics; Kavli IPMU
Email: yudin@itep.ru
Russian Federation, ul. Bolshaya Cheremushkinskaya 25, Moscow, 117259; Kashiwa
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