Zobrazeno 1 - 10
of 15
pro vyhledávání: '"F D Lora-Clavijo"'
We measure the effects of non-isotropic thermal conduction on generation of solar chromospheric jets through numerical simulations carried out with the use of one fluid MHD code MAGNUS. Following the work of Srivastava et al. (2018), we consider the
Externí odkaz:
http://arxiv.org/abs/2011.02006
Autor:
J. M. Velásquez-Cadavid, J. A. Arrieta-Villamizar, F. D. Lora-Clavijo, O. M. Pimentel, J. E. Osorio-Vargas
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 82, Iss 2, Pp 1-12 (2022)
Abstract The radiation observed in quasars and active galactic nuclei is mainly produced by a relativistic plasma orbiting close to the black hole event horizon, where strong gravitational effects are relevant. The observational data of such systems
Externí odkaz:
https://doaj.org/article/63196ed11f644819b8b82d0df44d84b5
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:
A. Cruz-Osorio, F. D. Lora-Clavijo, F. S. Guzmán, H. A. Morales-Tecotl, L. A. Urena-Lopez, R. Linares-Romero, H. H. Garcia-Compean
Publikováno v:
AIP Conference Proceedings.
We solve numerically the wave equation on a fixed background space‐time corresponding to 1+1 Minkowski space‐time. In this case we use scri‐fixing conformal compactifications and solve the wave equation on the conformal space‐time. We draw sp
Publikováno v:
Astrophysical Journal; 7/10/2018, Vol. 861 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 7/20/2017, Vol. 844 Issue 1, p1-1, 1p
Publikováno v:
Journal of Physics: Conference Series; 2017, Vol. 831 Issue 1, p1-1, 1p
Publikováno v:
Classical & Quantum Gravity; 4/6/2017, Vol. 34 Issue 7, p1-1, 1p
Publikováno v:
Astrophysical Journal Supplement Series; Aug2015, Vol. 219 Issue 2, p1-1, 1p