1962
DOI: 10.1002/prop.2180100302
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Zur Darstellungstheorie der inhomogenen Lorentzgruppe als Grundlage quantenmechanischer Kinematik

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Cited by 343 publications
(107 citation statements)
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“…It should be also noted that according to the Refs. [5][6][7]51,[54][55][56], the basic properties of the Riemann curvature tensor including the relevant results presented in Section 3.6, it would be concluded that the field strength tensor R ρσµν (i.e., the Riemann tensor) the in (1 + 3) space-time dimensions by general covariant massive (tensor) field Equation (71) (formulated solely with a column matrix of the type Ψ R (98-2)), represents a general covariant bispinor field of spin-2 particles (as a generalized massive formulation of the Einstein gravitational field equation). In a similar manner, according to the Refs.…”
Section: Showing That the Universe Could Be Realized Solely By The (1mentioning
confidence: 99%
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“…It should be also noted that according to the Refs. [5][6][7]51,[54][55][56], the basic properties of the Riemann curvature tensor including the relevant results presented in Section 3.6, it would be concluded that the field strength tensor R ρσµν (i.e., the Riemann tensor) the in (1 + 3) space-time dimensions by general covariant massive (tensor) field Equation (71) (formulated solely with a column matrix of the type Ψ R (98-2)), represents a general covariant bispinor field of spin-2 particles (as a generalized massive formulation of the Einstein gravitational field equation). In a similar manner, according to the Refs.…”
Section: Showing That the Universe Could Be Realized Solely By The (1mentioning
confidence: 99%
“…In a similar manner, according to the Refs. [5][6][7]51,[54][55][56], the field strength tensor F µν which is defined in (1 + 3) space-time dimensions by the general covariant massive (tensor) field Equation (72) (formulated solely by a column matrix of the type Ψ F (98-2)), and represents a general covariant bispinor field of spin-1 particles (representing new generalized massive formulations of the Maxwell's equations, and also Yang-Mills field equations). Furthermore, as it would be shown in Section 3.15, the general covariant field Equation (72) (representing the spin-1 boson fields coupling to the spin-1/2 fermionic currents) is also compatible with the SU(2) L ⊗U(2) R and SU(3) symmetry groups.…”
Section: Showing That the Universe Could Be Realized Solely By The (1mentioning
confidence: 99%
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“…The overlap coefficients with the tensor product of single particle states are Poincaré Clebsch-Gordan coefficients which can be found in ( [14][15][3] [16]). …”
Section: The Two-body Problemmentioning
confidence: 99%
“…As usual, the theory of RWE closely relates with higher spin formalisms. However, at present there is no a fully adequate formalism for description of higher-spin fields (all widely accepted higher-spin formalisms such as Rarita-Schwinger approach [27], BargmannWigner [5] and Gel'fand-Yaglom [13] multispinor theories, and also Joos-Weinberg 2(2j+1)-component formalism [19,39] have many intrinsic contradictions and difficulties). On the other hand, it is known that the study of RWE leads naturally to the fields which depend on both Minkowski space coordinates and some continuous variables corresponding to spin degrees of freedom [15,5,40,30].…”
Section: Introductionmentioning
confidence: 99%