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Boson star superradiance
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作者 He-Yu Gao Paul M.Saffin +2 位作者 Yi-Jie Wang Qi-Xin Xie Shuang-Yong Zhou 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS CSCD 2024年第6期69-78,共10页
Recently,it has been realized that in some systems internal space rotation can induce energy amplification for scattered waves,similar to rotation in real space.In particularly,it has been shown that energy extraction... Recently,it has been realized that in some systems internal space rotation can induce energy amplification for scattered waves,similar to rotation in real space.In particularly,it has been shown that energy extraction is possible for a Q-ball,a stationary non-topological soliton that is coherently rotating in its field space.In this paper,we generalize the analysis to the case of boson stars,and show that the same energy extraction mechanism still works for boson stars. 展开更多
关键词 SUPERRADIANCE boson star field space rotation
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Effects of Gravitational Correction on Neutron Stars with Antikaon Condensation
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作者 丁文波 侯佳为 +5 位作者 戚湛强 鄂姗姗 特木尔巴根 刘广洲 喻孜 赵恩广 《Communications in Theoretical Physics》 SCIE CAS CSCD 2016年第6期772-776,共5页
Effects of gravitational correction through the introduction of U bosons on neutron stars with antikaon condensation are studied in the relativistic mean field theory. How the global properties of neutron stars, redsh... Effects of gravitational correction through the introduction of U bosons on neutron stars with antikaon condensation are studied in the relativistic mean field theory. How the global properties of neutron stars, redshift and the momentum of inertia are modified by gravitational correction and antikaon condensation are discussed here. Results show that antikaon condensation can occur at the core of pulsar PSR J1614-2230. Gravitational correction and antikaon condensation influence each other, and when coupling constant of U bosons and baryons becomes very high, effects of antikaon condensation almost vanish. Moreover, both the redshift and the momentum of inertia of neutron stars are sensitive to the constant of U bosons. Combining with observation data, we can provide a further constraint on coupling constant of U bosons. 展开更多
关键词 neutron stars gravitational correction antikaon condensation U bosons
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