Erratum: Supersymmetry algebra of antisymmetric tensors with Green-Schwarz mechanisms

1990 ◽  
Vol 42 (8) ◽  
pp. 2947-2947
Author(s):  
M. Bodner ◽  
M. Villasante
2005 ◽  
Vol 20 (01) ◽  
pp. 99-128 ◽  
Author(s):  
B. B. DEO ◽  
L. MAHARANA

A string in four dimensions is constructed by supplementing it with 44 Majorana fermions. The later are represented by 11 vectors in the bosonic representation SO (D-1,1). The central charge is 26. The fermions are grouped in such a way that the resulting action is worldsheet supersymmetric. The energy–momentum and current generators satisfy the super-Virasoro algebra. GSO projections are necessary for proving modular invariance. Space–time supersymmetry algebra is deduced and is substantiated for specific modes of zero mass. The symmetry group of the model can descend to the low energy standard model group SU (3)× SU L(2)× U Y(1) through the Pati–Salam group.


2005 ◽  
Vol 627 (1-4) ◽  
pp. 217-223 ◽  
Author(s):  
A. Pahlavan ◽  
S. Rouhani ◽  
M.V. Takook

2008 ◽  
Vol 372 (38) ◽  
pp. 5955-5958 ◽  
Author(s):  
Azmi Ali Altıntaṣ ◽  
Metin Arık

2000 ◽  
Vol 15 (29) ◽  
pp. 1801-1811 ◽  
Author(s):  
HAJI AHMEDOV ◽  
ÖMER F. DAYI

Non-Abelian fractional supersymmetry algebra in two dimensions is introduced utilizing Uq(sl(2,ℝ)) at roots of unity. Its representations and the matrix elements are obtained. The dual of it is constructed and the corepresentations are studied. Moreover, a differential realization of the non-Abelian fractional supersymmetry generators is given in the generalized superspace defined by two commuting and two generalized Grassmann variables. An invariant action under the fractional supersymmetry transformations is given.


1990 ◽  
Vol 68 (12) ◽  
pp. 1377-1381
Author(s):  
D. G. C. McKeon

The Bjorken–Johnson–Low technique is used to compute the equal time anticommutator of the spinor currents associated with the supersymmetry of a two-dimensional Wess–Zumino model containing a Majorana spinor, a scalar, and an auxiliary field. Operator regularization is used to compute radiative effects as this does not explicitly break the supersymmetry present in the classical Lagrangian. We find that the spinor current is not conserved, and that the algebra of the generators of the supersymmetry transformation is altered. This is analogous to what has been found in theories with a classical axial gauge symmetry.


1989 ◽  
Vol 220 (4) ◽  
pp. 569-575 ◽  
Author(s):  
R. Casalbuoni ◽  
S. De Curtis ◽  
D. Dominici ◽  
F. Feruglio ◽  
R. Gatto

1978 ◽  
Vol 31 (6) ◽  
pp. 461 ◽  
Author(s):  
PD Jarvis

The space-time Poincare algebra is extended by introducing a four-spinor generator whose components satisfy certain trilinear parafermi commutation relations. The spin content of the irreducible multiplets is analysed in the massive and massless cases, and weight diagrams constructed, for arbitrary order p of the parastatistics. The supersymmetry algebra of Wess and Zumino, and of Salam and Strathdee, is exhibited as the special case of order p = 1 in this formulation.


2006 ◽  
Vol 18 (03) ◽  
pp. 329-347 ◽  
Author(s):  
P. A. HORVÁTHY

The dynamical (super)symmetries for various monopole systems are reviewed. For a Dirac monopole, non-smooth Runge–Lenz vector can exist; there is, however, a spectrum-generating conformal o(2,1) dynamical symmetry that extends into osp(1/1) or osp(1/2) for spin 1/2 particles. Self-dual 't Hooft–Polyakov-type monopoles admit an su(2/2) dynamical supersymmetry algebra, which allows us to reduce the fluctuation equation to the spin 0 case. For large r, the system reduces to a Dirac monopole plus a suitable inverse-square potential considered before by McIntosh and Cisneros, and by Zwanziger in the spin 0 case, and to the "dyon" of D'Hoker and Vinet for spin 1/2. The asymptotic system admits a Kepler-type dynamical symmetry as well as a "helicity-supersymmetry" analogous to the one Biedenharn found in the relativistic Kepler problem. Similar results hold for the Kaluza–Klein monopole of Gross–Perry–Sorkin. For the magnetic vortex, the N = 2 supersymmetry of the Pauli Hamiltonian in a static magnetic field in the plane combines with the o(2) × o(2,1) bosonic symmetry into an o(2) × osp(1/2) dynamical superalgebra.


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