We contribute to the solution of equilibrium, stability, and transport of
magnetically confined plasmas in the context of controlled nuclear fusion
research. Specifically, our investigation focuses on mechanisms that can
enhance plasma confinement in toroidal devices, such as tokamaks and
stellarators.
We conduct studies on astrophysical fluids, focusing on various types of
jets: jets associated with gamma-ray bursts, jets from young and evolved
stars, and jets in stellar binary systems. We also study other
astrophysical fluids, including supernova remnants, turbulent molecular
clouds, galactic-scale flows (such as winds from star formation, and mass
redistribution within galaxies), photoionized regions, and interactions
between exoplanets and stellar winds and their magnetic fields. To carry
out these studies, we develop computational codes for fluid dynamics
(newtonian and relativistic hydrodynamics andmagnetohydrodynamics,
radiative transport, and chemical kinetics). We also create analytic
models and conduct observational work using both ground-based and orbital
telescopes.
• Spectroscopy Experiments with Alkali Atoms
and X-ray Absorption Studies
The interaction processes between atomic systems and laser radiation fields are studied with the aim of developing experimental quantum control tools,
both in thermal atomic vapours and in clouds of cold atoms confined in magneto-optical traps. The precision spectroscopy techniques developed enable
the manipulation of the internal and motional degrees of freedom of atoms. The research includes the production of Rydberg states through multiphoton
excitation processes, with the goal of developing quantum technologies such as electromagnetic radiation sensors in the terahertz range. Additionally,
the effects of intensity structure, polarization, phase, and orbital angular momentum of a light beam on the probability of inducing transitions that
are forbidden under the electric dipole approximation are investigated. The primary motivation of this research is the creation of novel quantum control
methods for atomic states. The group also studies the structure of highly correlated materials containing transition metals using resonant X-ray
absorption and inelastic soft X-ray scattering (RIXS). In addition, to contribute to the advance of quantum technologies in Mexico through the
implementation of quantum metrology and high-precision spectroscopy systems, the development of high-precision quantum sensors based on matter-wave
interferometry techniques, specifically an atomic gravimeter, is also a research goal of the department.
We conduct experimental research in astrobiology, to study some of the
most important physicochemical processes in chemical evolution leading to
the abiotic formation of organic compounds in terrestrial environments.
Additionally, similar processes that may occur in extraterrestrial
locations within our solar system, such as Mars and the icy moons Titan,
Europa, and Enceladus, are examined. Furthermore, the research aims to
contribute to quantitative chemical analysis techniques that can be used
in space exploration missions.
We carry out theoretical studies on planetary atmospheres, planetary
habitability conditions, and remote detection of life on exoplanets.
Additionally, we conduct experimental research on the physical and
chemical characteristics of protoplanetary disks and meteorite
components.
• Radiolysis and Thermolysis in Prebiotic Chemistry
Research is conducted on radiolysis and thermolysis of compounds relevant
to prebiotic chemistry, including radiation-induced reactions in frozen
aqueous systems and the effects of radiation on solids such as alkali
halides with rare-earth impurities. Additional studies focus on changes in
the properties of irradiated solids, surface phenomena, and applications
of solid-state properties to chemical evolution and dosimetry.