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書目名稱Gravity, Gauge Theories and Quantum Cosmology影響因子(影響力)




書目名稱Gravity, Gauge Theories and Quantum Cosmology影響因子(影響力)學(xué)科排名




書目名稱Gravity, Gauge Theories and Quantum Cosmology網(wǎng)絡(luò)公開度




書目名稱Gravity, Gauge Theories and Quantum Cosmology網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Gravity, Gauge Theories and Quantum Cosmology被引頻次




書目名稱Gravity, Gauge Theories and Quantum Cosmology被引頻次學(xué)科排名




書目名稱Gravity, Gauge Theories and Quantum Cosmology年度引用




書目名稱Gravity, Gauge Theories and Quantum Cosmology年度引用學(xué)科排名




書目名稱Gravity, Gauge Theories and Quantum Cosmology讀者反饋




書目名稱Gravity, Gauge Theories and Quantum Cosmology讀者反饋學(xué)科排名

fatty-streak

Path Integralsm law to law, there is a common characteristic shared by most of them: they are all derivable from a principle of stationary action. Let us begin by examining this principle in the context of the oldest established laws of physics: the laws of motion. We consider the simple example of a point partic

LAPSE

altruism

Gauge Fieldsdifficulty, viz. that of divergences in the perturbation expansion. We have two ways of dealing with this difficulty: (i) analyse the theory nonperturbatively or (ii) confine ourselves to only those theories which are perturbatively renormalizable.

冷淡一切

General Theory of Relativityered well established since the days of Newton. Einstein had been led to special relativity from considerations of symmetry, from the deduction that Maxwell’s equations of electromagnetic theory were invariant under Lorentz transformations (and not under Galilean transformations). Observational cons

凹室

凹室

CHAFE

FUME

Quantum Conformal Fluctuations geometrodynamics. In the present chapter we shall first examine how . can be formulated with the help of Feynman’s path integral formalism. The sketchy survey of other approaches to quantum gravity in the previous chapter will have convinced the reader that the problem is not simple, whatever means

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