Hugo García-Compean

Prof. Hugo García-Compean

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Research Focus & Metrics

Academic Career Length

33Years (1994-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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4 April 2002 in Physical Review Letters
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HGHugo García-Compean
Hugo García-Compean
OOO. Obregón
O. Obregón
CRCupatitzio Ramirez
Cupatitzio Ramirez
We propose a model for noncommutative quantum cosmology by means of a deformation of minisuperspace. For the Kantowski-Sachs metric we are able to find the exact wave function. We construct wave packets and show that new quantum states that “compete” to be the most probable state appear, in clear contrast with the commutative case. A tunneling process could be possible among these states.

21 August 2003 in Physical Review D
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HGHugo García-Compean
Hugo García-Compean
OOO. Obregón
O. Obregón
CRCupatitzio Ramirez
Cupatitzio Ramirez
MSM. Sabido
M. Sabido
Starting from a self-dual formulation of gravity, we obtain a noncommutative theory of pure Einstein theory in four dimensions. In order to do that, we use the Seiberg-Witten map. A procedure is outlined that allows one to find the solution of the noncommutative torsion constraint through the vanishing of the commutative one. Finally, the noncommutative corrections to the action are computed up to second order.

26 March 2021 in Journal of High Energy Physics
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ECErick Chacón
Erick Chacón
HGHugo García-Compean
Hugo García-Compean
ALAndrés Luna
Andrés Luna
RMRicardo Monteiro
Ricardo Monteiro
CWChris D. White
Chris D. White
The double copy relates scattering amplitudes and classical solutions in Yang-Mills theory, gravity, and related field theories. Previous work has shown that this has an explicit realisation in self-dual YM theory, where the equation of motion can be written in a form that maps directly to Plebański’s heavenly equation for self-dual gravity. The self-dual YM equation involves an area-preserving diffeomorphism algebra, two copies of which appear in the heavenly equation. In this paper, we show that this construction is a special case of a wider family of heavenly-type examples, by (i) performing Moyal deformations, and (ii) replacing the area-preserving diffeomorphisms with a less restricted algebra. As a result, we obtain a double-copy interpretation for hyper-Hermitian manifolds, extending the previously known hyper-Kähler case. We also introduce a double-Moyal deformation of the heavenly equation. The examples where the construction of Lax pairs is possible are manifestly consistent with Ward’s conjecture, and suggest that the classical integrability of the gravity-type theory may be guaranteed in general by the integrability of at least one of two gauge-theory-type single copies.

28 August 2003 in Physical Review D
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HGHugo García-Compean
Hugo García-Compean
OOO. Obregón
O. Obregón
CRCupatitzio Ramirez
Cupatitzio Ramirez
MSM. Sabido
M. Sabido
The possibility of noncommutative topological gravity arising in the same manner as Yang-Mills theory is explored. We use the Seiberg-Witten map to construct such a theory based on a SL(2,C) complex connection, from which the Euler characteristic and the signature invariant are obtained. Finally, we speculate on the description of noncommutative gravitational instantons, as well as noncommutative local gravitational anomalies.

23 November 2018 in Letters in Mathematical Physics
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MBMiriam Bocardo-Gaspar
Miriam Bocardo-Gaspar
HGHugo García-Compean
Hugo García-Compean
WZW. Zúñiga-Galindo
W. Zúñiga-Galindo

27 June 2011 in Physical Review D
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RCRubén Cordero
Rubén Cordero
HGHugo García-Compean
Hugo García-Compean
FTFrancisco J. Turrubiates
Francisco J. Turrubiates
The Weyl-Wigner-Groenewold-Moyal formalism of deformation quantization is applied to cosmological models in the minisuperspace. The quantization procedure is performed explicitly for quantum cosmology in a flat minisuperspace. The de Sitter cosmological model is worked out in detail and the computation of the Wigner functions for the Hartle-Hawking, Vilenkin and Linde wave functions are done numerically. The Wigner function is analytically calculated for the Kantowski-Sachs model in (non)commutative quantum cosmology and for string cosmology with dilaton exponential potential. Finally, baby universes solutions are described in this context and the Wigner function is obtained.