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Jae Hyung Yee - One of the best experts on this subject based on the ideXlab platform.
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scalar field theory in κ Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of U(igl(4,R)), the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional κ-Minkowski Spacetime. The action in momentum space turns out to differ only in the integration measure from the commutative theory.
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Differential structure on the κ-Minkowski Spacetime from twist
Physics Letters B, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Abstract We study four-dimensional κ-Minkowski Spacetime constructed by the twist deformation of U ( igl ( 4 , R ) ) . We demonstrate that the differential structure of such twist-deformed κ-Minkowski Spacetime is closed in four dimensions contrary to the construction of κ-Poincare bicovariant calculus which needs an extra fifth dimension. Our construction holds in arbitrary dimensional Spacetimes.
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Differential structure on κ-Minkowski Spacetime realized as module of twisted Weyl algebra
Physics Letters B, 2009Co-Authors: Hyeong-chan Kim, Jae Hyung YeeAbstract:Abstract The differential structure on the κ -Minkowski Spacetime from Jordanian twist of Weyl algebra is constructed, and it is shown to be closed in 4-dimensions in contrast to the conventional formulation. Based on this differential structure, we have formulated a scalar field theory in this κ -Minkowski Spacetime.
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Scalar Field theory in $\kappa$-Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of $U(igl(4,R))$, the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional $\kappa$-Minkowski Spacetime. The action in momentum space turns out to differ only in integration measure from the commutative theory.
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Casimir energy of a spherical shell in $\kappa-$Minkowski Spacetime
Journal of the Korean Physical Society, 2008Co-Authors: Hyeong-chan Kim, Chaiho Rim, Jae Hyung YeeAbstract:We study the Casimir energy of a spherical shell of radius $a$ in $\kappa$-Minkowski Spacetime for a complex field with an asymmetric ordering and obtain the energy up to $O(1/\kappa^2)$. We show that the vacuum breaks particle and anti-particle symmetry if one requires the spectra to be consistent with the blackbody radiation at the commutative limit.
Hyeong-chan Kim - One of the best experts on this subject based on the ideXlab platform.
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Braided Statistics from Abelian Twist in κ-Minkowski Spacetime
Modern Physics Letters A, 2010Co-Authors: Hyeong-chan Kim, Youngone Lee, Chaiho RimAbstract:κ-deformed commutation relation between quantum operators is constructed via Abelian twist deformation in κ-Minkowski Spacetime. The commutation relation is written in terms of universal R-matrix satisfying braided statistics. The equal-time commutator function vanishes in this framework.
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scalar field theory in κ Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of U(igl(4,R)), the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional κ-Minkowski Spacetime. The action in momentum space turns out to differ only in the integration measure from the commutative theory.
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Differential structure on the κ-Minkowski Spacetime from twist
Physics Letters B, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Abstract We study four-dimensional κ-Minkowski Spacetime constructed by the twist deformation of U ( igl ( 4 , R ) ) . We demonstrate that the differential structure of such twist-deformed κ-Minkowski Spacetime is closed in four dimensions contrary to the construction of κ-Poincare bicovariant calculus which needs an extra fifth dimension. Our construction holds in arbitrary dimensional Spacetimes.
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Differential structure on κ-Minkowski Spacetime realized as module of twisted Weyl algebra
Physics Letters B, 2009Co-Authors: Hyeong-chan Kim, Jae Hyung YeeAbstract:Abstract The differential structure on the κ -Minkowski Spacetime from Jordanian twist of Weyl algebra is constructed, and it is shown to be closed in 4-dimensions in contrast to the conventional formulation. Based on this differential structure, we have formulated a scalar field theory in this κ -Minkowski Spacetime.
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Scalar Field theory in $\kappa$-Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of $U(igl(4,R))$, the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional $\kappa$-Minkowski Spacetime. The action in momentum space turns out to differ only in integration measure from the commutative theory.
Chaiho Rim - One of the best experts on this subject based on the ideXlab platform.
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Braided Statistics from Abelian Twist in κ-Minkowski Spacetime
Modern Physics Letters A, 2010Co-Authors: Hyeong-chan Kim, Youngone Lee, Chaiho RimAbstract:κ-deformed commutation relation between quantum operators is constructed via Abelian twist deformation in κ-Minkowski Spacetime. The commutation relation is written in terms of universal R-matrix satisfying braided statistics. The equal-time commutator function vanishes in this framework.
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scalar field theory in κ Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of U(igl(4,R)), the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional κ-Minkowski Spacetime. The action in momentum space turns out to differ only in the integration measure from the commutative theory.
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Differential structure on the κ-Minkowski Spacetime from twist
Physics Letters B, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Abstract We study four-dimensional κ-Minkowski Spacetime constructed by the twist deformation of U ( igl ( 4 , R ) ) . We demonstrate that the differential structure of such twist-deformed κ-Minkowski Spacetime is closed in four dimensions contrary to the construction of κ-Poincare bicovariant calculus which needs an extra fifth dimension. Our construction holds in arbitrary dimensional Spacetimes.
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Scalar Field theory in $\kappa$-Minkowski Spacetime from twist
Journal of Mathematical Physics, 2009Co-Authors: Hyeong-chan Kim, Chaiho Rim, Youngone Lee, Jae Hyung YeeAbstract:Using the twist deformation of $U(igl(4,R))$, the linear part of the diffeomorphism, we define a scalar function and construct a free scalar field theory in four-dimensional $\kappa$-Minkowski Spacetime. The action in momentum space turns out to differ only in integration measure from the commutative theory.
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Casimir energy of a spherical shell in $\kappa-$Minkowski Spacetime
Journal of the Korean Physical Society, 2008Co-Authors: Hyeong-chan Kim, Chaiho Rim, Jae Hyung YeeAbstract:We study the Casimir energy of a spherical shell of radius $a$ in $\kappa$-Minkowski Spacetime for a complex field with an asymmetric ordering and obtain the energy up to $O(1/\kappa^2)$. We show that the vacuum breaks particle and anti-particle symmetry if one requires the spectra to be consistent with the blackbody radiation at the commutative limit.
Kentaroh Yoshida - One of the best experts on this subject based on the ideXlab platform.
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yang baxter deformations of Minkowski Spacetime
Journal of High Energy Physics, 2015Co-Authors: Takuya Matsumoto, Domenico Orlando, Susanne Reffert, Junichi Sakamoto, Kentaroh YoshidaAbstract:We study Yang-Baxter deformations of 4D Minkowski Spacetime. The Yang-Baxter sigma model description was originally developed for principal chiral models based on a modified classical Yang-Baxter equation. It has been extended to coset curved spaces and models based on the usual classical Yang-Baxter equation. On the other hand, for flat space, there is the obvious problem that the standard bilinear form degenerates if we employ the familiar coset Poincare group/Lorentz group. Instead we consider a slice of AdS5 by embedding the 4D Poincare group into the 4D conformal group SO(2, 4) . With this procedure we obtain metrics and B-fields as Yang-Baxter deformations which correspond to well-known configurations such as T-duals of Melvin backgrounds, Hashimoto-Sethi and Spradlin-Takayanagi-Volovich backgrounds, the T-dual of Grant space, pp-waves, and T-duals of dS4 and AdS4. Finally we consider a deformation with a classical r-matrix of Drinfeld-Jimbo type and explicitly derive the associated metric and B-field which we conjecture to correspond to a new integrable system.
Hideki Ishihara - One of the best experts on this subject based on the ideXlab platform.
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Exactly solvable strings in Minkowski Spacetime
Classical and Quantum Gravity, 2010Co-Authors: Hiroshi Kozaki, Tatsuhiko Koike, Hideki IshiharaAbstract:We study the integrability of the equations of motion for the Nambu–Goto strings with a cohomogeneity-one symmetry in Minkowski Spacetime. A cohomogeneity-one string has a world surface which is tangent to a Killing vector field. By virtue of the Killing vector, the equations of motion reduce to the geodesic equation in the orbit space. Cohomogeneity-one strings are classified into seven classes (types I to VII). We investigate the integrability of the geodesic equations for all the classes and find that the geodesic equations are integrable. For types I to VI, the integrability comes from the existence of Killing vectors on the orbit space which are the projections of Killing vectors on Minkowski Spacetime. For type VII, the integrability is related to a projected Killing vector and a nontrivial Killing tensor on the orbit space. We also find that the geodesic equations of all types are exactly solvable, and show the solutions.
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exactly solvable strings in Minkowski Spacetime
arXiv: General Relativity and Quantum Cosmology, 2009Co-Authors: Hiroshi Kozaki, Tatsuhiko Koike, Hideki IshiharaAbstract:We study the integrability of the equations of motion for the Nambu-Goto strings with a cohomogeneity-one symmetry in Minkowski Spacetime. A cohomogeneity-one string has a world surface which is tangent to a Killing vector field. By virtue of the Killing vector, the equations of motion can be reduced to the geodesic equation in the orbit space. Cohomogeneity-one strings are classified into seven classes (Types I to VII). We investigate the integrability of the geodesic equations for all the classes and find that the geodesic equations are integrable. For Types I to VI, the integrability comes from the existence of Killing vectors on the orbit space which are the projections of Killing vectors on Minkowski Spacetime. For Type VII, the integrability is related to a projected Killing vector and a nontrivial Killing tensor on the orbit space. We also find that the geodesic equations of all types are exactly solvable, and show the solutions.