This repository is an active, evolving research codebase spanning the full duration of a PhD (2025--2030). Although every effort is made to keep the code correct and well-documented, some parts may be unfinished, outdated, or in the process of being reworked. Earlier versions of some codes have been deliberately preserved for bookkeeping purposes -- they may contain naive approaches or undeveloped ideas that could still prove useful later. No guarantee of correctness (or more precisely, of completeness) is implied for any file in this repository.
This repository collects most of the analysis and simulation codes developed during my PhD at IFGW -- Instituto de Física Gleb Wataghin, Universidade Estadual de Campinas (Unicamp), within the ALICE collaboration at CERN.
The central physics goal is to search for local
The O2Physics tasks that run inside the ALICE Hyperloop framework live in a separate repository and are not included here.
(For those, look at my fork at cmuncinelli/O2Physics!)
| Folder | Description |
|---|---|
vorticity_hydro/ |
Hydrodynamic and PYTHIA-based toy models for |
pythia_runs/ |
PYTHIA8 and PYTHIA Angantyr generator codes with FastJet integration. Produces zero-polarization MC reference samples for the ring observable analysis. |
RingPol_RAW_LocalHelpers/ |
Local analysis framework for the ring polarization observable. Includes tools for downloading, processing, and analyzing both raw AOD and Hyperloop derived data. |
LambdaV0Radius_QA/ |
Quality assurance study for systematic effects related to the V0 decay radius in |
ToyModels/ |
Collection of Toy Models to estimate and understand spurious polarization effects introduced by kinematic cuts and detector asymmetries. |
O2PhysicsTools/ |
Memory cleaning scripts and tools for linting+formatting code before submitting PRs to the central repository. |
IC_helper_tasks/ |
Utility scripts written to support undergraduate research students. |
archive/ |
Some older code that never made it into the central repository of O2Physics. Stored here for bookkeeping some old ideas that may come in hand. |
Some scripts contain hardcoded paths such as /home/cicero/ or references to cluster nodes (e.g. jarvis*). These reflect the original computing environment at Unicamp and should be adapted to your local setup.
This work is supported by the Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP).
I would like to acknowledge the people of the state of São Paulo, whose public investment in science makes research like this possible -- even when its impact is not immediately visible. I am sincerely grateful for that support and trust.
This research is carried out at the Instituto de Física Gleb Wataghin (IFGW), at the Universidade Estadual de Campinas (Unicamp).