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Teleportation of an Arbitrary Two-Particle State by Two Partial Entangled Three-Particle GHZ States 被引量:6
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作者 DAIHong-Yi CHENPing-Xing LICheng-Zu 《Communications in Theoretical Physics》 SCIE CAS CSCD 2005年第5期799-802,共4页
We present a scheme for teleporting an unknown arbitrary two-particle state from a sender to either one of two receivers. The quantum channel is composed of two partial entangled three-particle GHZ states. An unknown ... We present a scheme for teleporting an unknown arbitrary two-particle state from a sender to either one of two receivers. The quantum channel is composed of two partial entangled three-particle GHZ states. An unknown arbitrary two-particle state can be perfectly teleported probabilistically if the sender performs two generalized Bell-state measurements and each receiver introduces an appropriate unitary transformation with the help of the other receiver's Hadamard operations and simple measurements. 展开更多
关键词 probabilistic teleportation arbitrary two-particle state unitary transformation Hadamard operation
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Single Boson Realizations of the Higgs Algebra 被引量:2
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作者 RUANDong WUChu SUNHong-Zhou 《Communications in Theoretical Physics》 SCIE CAS CSCD 2003年第1X期73-76,共4页
We obtained for the Higgs algebra three kinds of single boson realizations such as the unitary Holstein-Primakoff-like realization, the non-unitary Dyson-like realization, and the unitary Villain-like realization. Th... We obtained for the Higgs algebra three kinds of single boson realizations such as the unitary Holstein-Primakoff-like realization, the non-unitary Dyson-like realization, and the unitary Villain-like realization. The corre-sponding similarity transformations between the Holstein-Primakoff-like realizations and the Dyson-like realizations are given. 展开更多
关键词 希格斯介子代数 非线性角动量代数 玻色子 Higgs代数 多项式角动量代数 量子场论
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Energy of Gravitational Field of Static Spherically Symmetric Neutron Stars 被引量:1
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作者 WENDe-Hua CHENWei +3 位作者 WANGXian-Ju AIBao-Quan LIUGuo-Tao LIULiang-Gang 《Communications in Theoretical Physics》 SCIE CAS CSCD 2003年第5X期637-640,共4页
By using the Einstein-Tolman expression of the energy-momentum pseudo-tensor, the energy density of the gravitational field of the static spherically symmetric neutron stars is calculated in the Cartesian coordinate s... By using the Einstein-Tolman expression of the energy-momentum pseudo-tensor, the energy density of the gravitational field of the static spherically symmetric neutron stars is calculated in the Cartesian coordinate system.It is exciting that the energy density of gravitational field is positive and rational The xmmerical results of the energy density of gravitational field of neutron stars are calculated. For neutron stars with M=2M, the ratio of the energy density of gravitational field to the energy density of pure matters would be up to 0.54 at the surface. 展开更多
关键词 中子星 球对称 重力场能 能量密度 重力波
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