This work aims to widen our knowledge about the pyrolysis,
and
catalytic pyrolysis of asphaltenes at low and high pressure through
experimental and simulation approaches. Experimentally, asphaltenes
were subjected to high-pressure thermogravimetric analysis obtaining
a pressure-dependent behavior. As pressure increases, asphaltene reactivity
is reduced by the retardation in the thermal cracking temperature
and increment of the coke amount deposition. The coke deposited follows
the order 0.084 MPa (8.0%) < 3.0 MPa (10.0%) < 6.0 MPa (11.0%).
When ceria-based nanoparticles were used for the catalytic thermal
cracking of asphaltenes, it was obtained that during the low-temperature
range (<250 °C), the amount of mass lost was 60, 45, and 38%
at 0.084, 3.0, and 6.0 MPa, respectively. The rest of the asphaltenes
are cracked in the high-temperature region (HTR), which means that
coke is not produced in the catalytic reaction regardless of the system
pressure. Molecular dynamic calculations were done based on the ReaxFF
potential to provide an atomistic description of asphaltene pyrolysis
at 0.084 and 6.0 MPa. The theoretical results were compared with those
obtained experimentally, achieving successful reproducibility. During
the LTR region, the asphaltene aggregate integrity remains without
significant changes, whereas most structural changes in the HTR were
obtained. The number of the species increases with the rising temperature,
obtaining at 0.084 MPa, 32, 1515, and 4065 species at 300, 450, and
550 °C, respectively, whereas at 6.0 MPa, 28, 589, and 867 species
at 300, 450, and 550 °C were obtained. The variety of the molecules
was found to be higher at 450 °C due to the breaking of a large
number of complex hydrocarbons. This result corroborates that asphaltenes
mainly react during HTR, and with increasing pressure, the rate of
reaction is negatively affected. The species are mainly found in the
form of reactive radicals such as CHO2 (carboxyl radical),
OH (hydroxyl radical), and CHO (aldehyde radical), and molecules of
CO2, H2O, CH2O, and CO are observed
as major O-containing gas products that account for most of the gas
phase.