Another supersymmetric extension of local Lorentz symmetry in the vierbein formalism of Einstein gravity

1989 ◽  
Vol 41 (4) ◽  
pp. 637-643
Author(s):  
M. Abe
1989 ◽  
Vol 04 (11) ◽  
pp. 2837-2859
Author(s):  
M. ABE ◽  
N. NAKANISHI

The locally [Formula: see text]-symmetric extension of the vierbein formalism of the Einstein gravity is systematically reconstructed. The superconnection is defined by the requirement that the vierbein supermultiplet and the [Formula: see text] “vielbein” one have vanishing supercovariant derivatives. By using the superconnection, the globally super-invariant gauge-fixing Lagrangian density and the corresponding FP-ghost one are explicitly constructed. Then the theory is shown to be invariant under the extended BRS symmetry corresponding to the local [Formula: see text] symmetry.


1990 ◽  
Vol 05 (17) ◽  
pp. 3277-3334 ◽  
Author(s):  
MITSUO ABE

The supersymmetric extension of local Lorentz symmetry in the vierbein formalism is presented in detail. In contrast to supergravity, this new supersymmetry is purely internal, that is, totally irrelevant to general coordinate transformations. Because of its non-Poincaré nature, the degrees of freedom of bosons and fermions need not be equal and it is unnecessary to introduce gravitino. Instead, it is important to introduce a new type of nonlinear realization, called “ξ-field realization”. The Einstein Lagrangian density is trivially superinvariant and the Dirac theory can be supersymmetrized. A globally superinvariant gauge-fixing plus FP-ghost Lagrangian density is constructed in the BRS-invariant way. In the simplest case, canonical quantization is explicitly carried out and unitarity is proved. It is shown that the manifestly covariant canonical formalism of quantum gravity is extended to the supersymmetric form without spoiling its beauty in contrast to supergravity. This supersymmetric theory provides a natural link between quantum gravity and gauge theory; its implies that the chiral gauge group should be SO (N).


1989 ◽  
Vol 04 (11) ◽  
pp. 2765-2777 ◽  
Author(s):  
HIROAKI KANNO

Using the frame matrix representation of the Grassmann manifold, we derive a nonlinear realization of the general linear group. We show that its super-extension reproduces the ξ-field which appears in the recent work on a supersymmetric extension of local Lorentz symmetry by Abe and Nakanishi. This clarifies the geometrical meaning of the ξ-field and we discuss its properties on the basis of this interpretation. The similarity of this ξ-field and the vierbein field is pointed out.


2021 ◽  
Vol 964 ◽  
pp. 115312
Author(s):  
A. Kehagias ◽  
H. Partouche ◽  
B. de Vaulchier
Keyword(s):  

2021 ◽  
Vol 2021 (4) ◽  
Author(s):  
Tadashi Takayanagi ◽  
Takahiro Uetoko

Abstract In this paper we provide a Chern-Simons gravity dual of a two dimensional conformal field theory on a manifold with boundaries, so called boundary conformal field theory (BCFT). We determine the correct boundary action on the end of the world brane in the Chern-Simons gauge theory. This reproduces known results of the AdS/BCFT for the Einstein gravity. We also give a prescription of calculating holographic entanglement entropy by employing Wilson lines which extend from the AdS boundary to the end of the world brane. We also discuss a higher spin extension of our formulation.


2020 ◽  
Vol 2020 (3) ◽  
Author(s):  
Shamik Banerjee ◽  
Sudip Ghosh ◽  
Pranjal Pandey ◽  
Arnab Priya Saha
Keyword(s):  

2021 ◽  
Vol 2021 (8) ◽  
Author(s):  
Yusuke Yamada

Abstract We investigate supersymmetry (SUSY) breaking scenarios where both SUSY and Lorentz symmetry are broken spontaneously. For concreteness, we propose models in which scalar fluid or vector condensation breaks Lorentz symmetry and accordingly SUSY. Then, we examine whether such scenarios are viable for realistic model buildings. We find, however, that the scalar fluid model suffers from several issues. Then, we extend it to a vector condensation model, which avoids the issues in the scalar fluid case. We show that accelerated expansion and soft SUSY breaking in matter sector can be achieved. In our simple setup, the soft SUSY breaking is constrained to be less than $$ \mathcal{O}(100)\mathrm{TeV} $$ O 100 TeV from the constraints on modification of gravity.


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