Titlebook: Quantum Mechanics of Fundamental Systems 1; Claudio Teitelboim Book 1988 Springer Science+Business Media New York 1988 mechanics.nuclear p

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書目名稱Quantum Mechanics of Fundamental Systems 1影響因子(影響力)




書目名稱Quantum Mechanics of Fundamental Systems 1影響因子(影響力)學科排名




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書目名稱Quantum Mechanics of Fundamental Systems 1網絡公開度學科排名




書目名稱Quantum Mechanics of Fundamental Systems 1被引頻次




書目名稱Quantum Mechanics of Fundamental Systems 1被引頻次學科排名




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書目名稱Quantum Mechanics of Fundamental Systems 1年度引用學科排名




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書目名稱Quantum Mechanics of Fundamental Systems 1讀者反饋學科排名

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enchant

Update on Anomalous Theories,with these.] As a consequence, the symmetry current, whose classical conservation is assured by Noether’s theorem, ceases to be conserved after quantization. We call such a current . it possesses an ., and the coupling of gauge fields to this current becomes problematical [1].

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The Gravitational Path Integral and Critical Dimensions of Linear and Nonlinear Locally Supersymmet parameter and in this way the Noether current enters in the Ward identities. For local symmetries with external gauge fields one can make a local classical gauge transformation, but if the gauge fields are dynamical, one must instead consider the rigid BRST symmetry of the quantum action.

dragon

Grassmannian Space-Time Structure as an Origin of Gauge Symmetries, local coordinates {. ., .}, where . and . are a pair of Grassmannian coordinates with no spinorial charge, constitute a very intriguing phenomenon. In this framework, the BRST and anti-BRST operators are naturally introduced as exterior differential operators along the unphysical coordinates . and

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呼吸

Toward a Complete Theory for Unconventional Vacua,d notion if we try to work in a bounded or a curved space-time, or if we use accelerated observers. In these cases infinite new vacuum notion must be defined; and we must deal with unconventional vacua. In this chapter we introduce a reasonable vacuum definition in all the cases where we deal with n

motor-unit

Some Properties of the Solutions of the Back-Reaction Problem,ese equations [1], which rule the dynamic of the space-time metric, have a source term that is the renormalized expectation value of the energy-momentum tensor. The computation of this last object as a function of the metric is a rather difficult task that has been performed only in a few cases.