On Two-Component Wave Equations

1950 ◽  
Vol 77 (6) ◽  
pp. 844-845 ◽  
Author(s):  
F. Gürsey
Keyword(s):  
Wave Equations ◽  
Two Component ◽  
Component Wave

Two-Component Wave Equations

1949 ◽  
Vol 75 (10) ◽  
pp. 1609-1609 ◽  
Author(s):  
Herbert Jehle
Keyword(s):  
Wave Equations ◽  
Two Component ◽  
Component Wave

Remarks on the Two-Component Wave Equations for Massive Leptons

1974 ◽  
Vol 9 (3) ◽  
pp. 161-162 ◽  
Author(s):  
M Havlicek ◽  
P Exner
Keyword(s):  
Wave Equations ◽  
Two Component ◽  
Component Wave

Two-Component Wave Equations

1949 ◽  
Vol 76 (10) ◽  
pp. 1538-1538 ◽  
Author(s):  
J. Serpe
Keyword(s):  
Wave Equations ◽  
Two Component ◽  
Component Wave

Two-Component Wave Equations

1949 ◽  
Vol 76 (4) ◽  
pp. 568-568 ◽  
Author(s):  
C. W. Kilmister
Keyword(s):  
Wave Equations ◽  
Two Component ◽  
Component Wave

Infinite-Component Wave Equations and Mass Splittings Within SU(3) and SU(2) Multiplets

1972 ◽  
Vol 5 (9) ◽  
pp. 2327-2331 ◽  
Author(s):  
A. O. Barut ◽  
William Brink Monsma
Keyword(s):  
Wave Equations ◽  
Component Wave ◽  
Infinite Component

Comment on Finite-Component Wave Equations

1969 ◽  
Vol 187 (5) ◽  
pp. 2278-2279 ◽  
Author(s):  
MAYER HUMI ◽  
SHIMON MALIN
Keyword(s):  
Wave Equations ◽  
Component Wave

scholarly journals A local description of dark energy in terms of classical two-component massive spin-one uncharged fields on spacetimes with torsionful affinities

Open Physics ◽  
2015 ◽  
Vol 13 (1) ◽  
Author(s):  
Jorge G. Cardoso
Keyword(s):  
Dark Energy ◽  
Physical Properties ◽  
Gauge Group ◽  
Wave Equations ◽  
Wave Functions ◽  
Local Description ◽  
Massive Spin ◽  
Two Component ◽  
Curved Spacetimes ◽  
Component Spinor

AbstractIt is assumed that the two-component spinor formalisms for curved spacetimes that are endowed with torsionful affine connexions can supply a local description of dark energy in terms of classical massive spin-one uncharged fields. The relevant wave functions are related to torsional affine potentials which bear invariance under the action of the generalized Weyl gauge group. Such potentials are thus taken to carry an observable character and emerge from contracted spin affinities whose patterns are chosen in a suitable way. New covariant calculational techniques are then developed towards deriving explicitly the wave equations that supposedly control the propagation in spacetime of the dark energy background. What immediately comes out of this derivation is a presumably natural display of interactions between the fields and both spin torsion and curvatures. The physical properties that may arise directly fromthe solutions to thewave equations are not brought out.

Finite- and Infinite-Component Wave Equations

1969 ◽  
Vol 22 (18) ◽  
pp. 972-974 ◽  
Author(s):  
I. Gyuk ◽  
H. Umezawa
Keyword(s):  
Wave Equations ◽  
Component Wave ◽  
Infinite Component
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