Massless composite particles and space-time description of gauge transformations

1983 ◽  
Vol 27 (10) ◽  
pp. 2348-2353
Author(s):  
D. Han ◽  
Y. S. Kim ◽  
D. Son
Keyword(s):  
Space Time ◽  
Composite Particles ◽  
Gauge Transformations ◽  
Time Description

scholarly journals The relativity of color

2015 ◽  
Vol 30 (35) ◽  
pp. 1550211 ◽  
Author(s):  
Paul D. Stack ◽  
Robert Delbourgo
Keyword(s):  
Space Time ◽  
Coordinate Transformations ◽  
Gauge Transformations ◽  
Time Property ◽  
Property Space ◽  
Lorentz Scalar ◽  
Color Property

By attaching three anticommuting Lorentz scalar (color) property coordinates to space–time, with an appropriate extended metric, we unify gravity with chromodynamics: gauge transformations then just correspond to coordinate transformations in the enlarged space–time-property space.

Space-time description of neutron spin echo spectrometry

1996 ◽  
Vol 229 (1) ◽  
pp. 1-17 ◽  
Author(s):  
R. Gähler ◽  
R. Golub ◽  
K. Habicht ◽  
T. Keller ◽  
J. Felber
Keyword(s):  
Spin Echo ◽  
Space Time ◽  
Neutron Spin ◽  
Neutron Spin Echo ◽  
Time Description

scholarly journals ON THE UNIQUENESS OF D = 11 INTERACTIONS AMONG A GRAVITON, A MASSLESS GRAVITINO AND A THREE-FORM II: THREE-FORM AND GRAVITINI

2008 ◽  
Vol 23 (30) ◽  
pp. 4841-4859 ◽  
Author(s):  
EUGEN-MIHĂIŢĂ CIOROIANU ◽  
EUGEN DIACONU ◽  
SILVIU CONSTANTIN SĂRARU
Keyword(s):  
Master Equation ◽  
Gauge Field ◽  
Space Time ◽  
Free Solution ◽  
Coupling Constant ◽  
Abelian Gauge ◽  
Gauge Transformations ◽  
Lorentz Covariance ◽  
Brst Cohomology ◽  
Chern Simons

The interactions that can be introduced between a massless Rarita–Schwinger field and an Abelian three-form gauge field in 11 space–time dimensions are analyzed in the context of the deformation of the "free" solution of the master equation combined with local BRST cohomology. Under the hypotheses of smoothness of the interactions in the coupling constant, locality, Poincaré invariance, Lorentz covariance, and the presence of at most two derivatives in the Lagrangian of the interacting theory (the same number of derivatives as in the free Lagrangian), we prove that there are neither cross-couplings nor self-interactions for the gravitino in D = 11. The only possible term that can be added to the deformed solution to the master equation is nothing but a generalized Chern–Simons term for the three-form gauge field, which brings contributions to the deformed Lagrangian, but does not modify the original, Abelian gauge transformations.

Space-Time Description of Hadrons. II

1970 ◽  
Vol 1 (2) ◽  
pp. 512-522 ◽  
Author(s):  
G. Domokos ◽  
S. Kovesi-Domokos ◽  
F. Mansouri
Keyword(s):  
Space Time ◽  
Time Description
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