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Projection Operator and Feynman Propagator for a Free Massive Particle of Arbitrary Spin
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作者 HUANGShi-Zhong ZHANGPeng-Fei +2 位作者 RUANTu-Nan ZHUYu-Can zhengzhi-peng 《Communications in Theoretical Physics》 SCIE CAS CSCD 2004年第3期405-418,共14页
Based on the solution to the Bargmann Wigner equations, a direct derivation of the projection operator and Feynman propagator for a free massive particle of arbitrary spin is worked out. The projection operator constr... Based on the solution to the Bargmann Wigner equations, a direct derivation of the projection operator and Feynman propagator for a free massive particle of arbitrary spin is worked out. The projection operator constructed by Behrends and Fronsdal is re-deduced and confirmed, and simplified in the case of half-integral spin, the general commutation rules and Feynman propagator with additional non-covariant terms for a free massive particle with any spin are derived, and explicit expressions for the propagators for spins 3/2, 2, 5/2, 3, 7/2, and 4 are provided. 展开更多
关键词 free massive particle arbitrary spin projection operator Feynman propagator
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Solution to the Cosmological Constant Problem by Gauge Theory of Gravity
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作者 WUNing GermanoResconi +3 位作者 zhengzhi-peng XUZhan ZHANGDa-Hua RIJANTu-Nan 《Communications in Theoretical Physics》 SCIE CAS CSCD 2003年第2X期253-256,共4页
Based on geometry picture of gravitational gauge theory, the cosmological constant is determined theoreti-cally. The cosmological constant is related to the average energy density of gravitational gauge field. Because... Based on geometry picture of gravitational gauge theory, the cosmological constant is determined theoreti-cally. The cosmological constant is related to the average energy density of gravitational gauge field. Because the energy density of gravltatlona] gauge field is negative, the cosmological constant is positive, which generates repulasive force on stars to make the expansion rate of the Universe accelerated. A rough estimation of it gives out its magnitude of the order of about 10^52m^-2, which is well consistent with experimental results. 展开更多
关键词 宇宙学常量 宇宙论 量子引力 广义相对论
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