Zobrazeno 1 - 10
of 36
pro vyhledávání: '"H. H. Garcia-Compean"'
Autor:
Yuri Bonder, Daniel Sudarsky, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
In this work we show that the spin pendulum techniques developed by the E\:{o}t-Wash group could be used to put very stringent bounds on the free parameters of a Lorentz invariant phenomenological model of quantum gravity. The model is briefly descri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::794de1d0970af9147024102a2d75a265
http://arxiv.org/abs/1003.5245
http://arxiv.org/abs/1003.5245
Autor:
K. Kanakoglou, C. Daskaloyannis, A. Herrera-Aguilar, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
The mathematical structure of a mixed paraparticle system (combining both parabosonic and parafermionic degrees of freedom) commonly known as the Relative Parabose Set, will be investigated and a braided group structure will be described for it. A ne
Autor:
Celia Escamilla-Rivera, Octavio Obregón, Luis Arturo Ureña-López, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
We study the case of a supersymmetric FRW model in a flat space in the superfield formulation. Some exact solutions of the model are found and we provide a range of possible applications in the evolution of the Universe at early times for two scalar
Autor:
J. P. Cruz-Pérez, J. A. González, F. S. Guzmán, F. D. Lora-Clavijo, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
In this academic work, we present a comparison between the Smoothed Particles Hydrodynamics (SPH) method and the standard finite differences (FD). As the test case for this comparison we use the Sod shock tube. In order to deal with the shock waves w
Autor:
F. D. Lora-Clavijo, J. A. González, F. S. Guzmán, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
We present the accretion of a phantom scalar field into a black hole for various scalar field potentials in the full non-linear regime. Our results are based on the use of numerical methods and show that for all the cases studied the black hole's app
Autor:
H. Vargas-Rodriguez, R. A. Gonzalez-Silva, L. I. Lopez Benitez, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
An exact solution of the Einstein‐Maxwell’s field equations is presented. This solution describes an axisymmetric charged dust distribution, with NUT rotation, in the presence of an electromagnetic field of the pure magnetic type. In the comoving
Autor:
Lizbeth M. Fernández, L. Arturo Ureña-López, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
In this paper we study the evolution of a scalar field falling into a static black hole, for which we consider Eddington‐Finkelstein coordinates. For both the massless and massive cases, we find that dispersion depends upon the mean wave number k0
Autor:
Gastón de los Santos, Román Linares, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
We review the canonical analysis of Maxwell’s theory in five dimensions (5D). In the first part we summarize the canonical analysis of the free theory in Minkowski space‐time. As is well known the theory has two first class constraints and theref
Publikováno v:
AIP Conference Proceedings.
We analyze the possibilities that the methods of statistical mechanics could offer us in the context of precision tests. The properties of a Bose‐Einstein condensate in a Lorentz violating scenario, characterized by a deformation in the dispersion
Autor:
Daniel Sudarsky, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
We discuss here a not very well advertised problem afflicting the standard inflationary account of the origin of structure in the universe as the result of the, so called, quantum fluctuations of the inflaton field. We will show that such account is