N=1supergravity as a nonlinear realization

1992 ◽  
Vol 45 (12) ◽  
pp. 4545-4554 ◽  
Author(s):  
E. A. Ivanov ◽  
J. Niederle
Keyword(s):  
Nonlinear Realization

Nonlinear Realization

2004 ◽  
pp. 276-276
Author(s):  
Hideaki Aoyama ◽  
Anatoli Konechny ◽  
V. Lemes ◽  
N. Maggiore ◽  
M. Sarandy ◽  
...  
Keyword(s):  
Nonlinear Realization

scholarly journals Quaternionic structures, supertwistors and fundamental superspaces

2016 ◽  
Vol 13 (09) ◽  
pp. 1650113 ◽  
Author(s):  
Diego Julio Cirilo-Lombardo ◽  
Victor N. Pervushin
Keyword(s):  
Gravitational Field ◽  
Extended Supersymmetry ◽  
Irreducible Representations ◽  
Nonlinear Realization ◽  
Specific Construction

Superspace is considered as space of parameters of the supercoherent states defining the basis for oscillator-like unitary irreducible representations of the generalized superconformal group [Formula: see text] in the field of quaternions [Formula: see text]. The specific construction contains naturally the supertwistor one of the previous work by Litov and Pervushin [1] and it is shown that in the case of extended supersymmetry such an approach leads to the separation of a class of superspaces and its groups of motion. We briefly discuss this particular extension to the domain of quaternionic superspaces as nonlinear realization of some kind of the affine and the superconformal groups with the final end to include also the gravitational field [6] (this last possibility to include gravitation, can be realized on the basis of Ref. 12 where the coset [Formula: see text][Formula: see text] was used in the non supersymmetric case). It is shown that this quaternionic construction avoid some unconsistencies appearing at the level of the generators of the superalgebras (for specific values of [Formula: see text] and [Formula: see text]; [Formula: see text]) in the twistor one.

scholarly journals COMPACT STARS IN HADRON AND QUARK-HADRON MODELS

2010 ◽  
Vol 19 (08n10) ◽  
pp. 1455-1462 ◽  
Author(s):  
S. SCHRAMM ◽  
V. A. DEXHEIMER
Keyword(s):  
Phase Diagram ◽  
Neutron Star ◽  
Chiral Symmetry ◽  
Degrees Of Freedom ◽  
Dense Matter ◽  
Compact Stars ◽  
Chiral Symmetry Restoration ◽  
Hybrid Star ◽  
Nonlinear Realization ◽  
Model Approach

We investigate strongly interacting dense matter and neutron stars using a flavor-SU(3) approach based on a nonlinear realization of chiral symmetry. We study chiral symmetry restoration and the equation of state of stellar matter and determine neutron star properties using different sets of degrees of freedom. Finally, we include quarks in the model approach. We show the resulting phase diagram as well as hybrid star solutions for this model.

N=1 supergravity as a nonlinear realization. II. The general case

1994 ◽  
Vol 50 (10) ◽  
pp. 6318-6328 ◽  
Author(s):  
D. Maxera ◽  
J. Niederle
Keyword(s):  
Nonlinear Realization
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