Chilean university with parallel research groups in cosmological simulation and mathematical logic, participating in large intercontinental MSCA researcher exchange networks.
Universidad Andrés Bello is a Chilean private university that brings research capacity in two distinct fundamental disciplines to international collaborations: computational astrophysics and the mathematical foundations of computer science. Their astrophysics researchers work on large-scale simulations of galaxy formation, dark matter distribution, and cosmological dynamics using high-performance computing. A separate research group works on the theoretical end of computing — mathematical logic, computable analysis over infinite data structures, and the computational complexity of exact real-number arithmetic. As a Latin American partner in European researcher exchange networks, UNAB serves as a host institution for visiting scientists and a bridge connecting EU research programs with South American scientific communities.
LACEGAL (2017–2022) placed UNAB within a Latin American–Chinese–European network for galaxy formation simulations, dark matter modeling, and cosmological data analysis using HPC infrastructure.
CID (2017–2023) involved UNAB researchers in computable analysis, exact real-number computation, descriptive set theory, and program extraction — foundational work in the mathematics of computation.
LACEGAL explicitly lists HPC and data science among its research methods, indicating UNAB contributes computational infrastructure or expertise to large-scale simulation pipelines.
CID covers topology and dynamical systems as part of its computable analysis framework, suggesting mathematical depth in continuous and structural analysis within UNAB's CS group.
Both projects entered the H2020 record in 2017 simultaneously, so the apparent shift from astrophysics keywords to theoretical CS keywords does not reflect a genuine change in direction over time — it reflects two parallel and independent research groups within the same university operating in entirely different domains. UNAB has not visibly evolved its focus between the early and late periods of H2020; rather, it has maintained two separate specialist tracks that happened to enter EU collaboration networks in the same year. This simultaneous breadth across cosmological simulation and abstract mathematics suggests a multi-faculty institution with no single dominant research identity in European projects.
With both research tracks active since 2017, no growth in project count, and no coordinator role taken on, UNAB shows no signal of building toward independent EU project leadership — they appear to be a stable but peripheral host for MSCA researcher exchanges rather than an organization expanding its European research footprint.
UNAB participates exclusively as a third party in both projects, meaning they host visiting researchers or provide supporting resources without holding formal consortium membership or receiving direct EC funding. Both projects are large MSCA-RISE staff exchange networks — a scheme designed for researcher mobility rather than joint R&D — which means UNAB's role is primarily as a receiving institution for European and Chinese scientists. This pattern suggests that working with UNAB means engaging their local research environment and network access rather than co-leading a research agenda.
UNAB sits within two large international research networks that together span 36 unique partner organizations across 22 countries, reflecting the broad geographic design of MSCA-RISE consortia rather than UNAB's own bilateral relationship-building. Their network reach extends to Europe, China, and Latin America, but these connections are mediated through the consortium structure rather than independently developed partnerships.
As one of the very few Chilean universities appearing in the H2020 database, UNAB offers European consortia a documented entry point into Latin American scientific networks — particularly relevant for astrophysics projects that benefit from southern hemisphere observatory access and for theoretical CS groups seeking intercontinental academic exchange. Their unusual combination of cosmological simulation capacity and abstract mathematical logic expertise in a single institution makes them an atypical partner profile: two separate specialist groups with no obvious overlap, which can be an asset for broad consortia needing diverse nodes. However, their third-party status in both projects provides limited evidence of independent research leadership, and their value to future partners depends heavily on which faculty group the collaboration targets.
