Projetos

 

#35 projectos disponíveis

Probing the nature of the neutrino: search for neutrinoless double beta decay with the LUX-ZEPLIN detector
Neutrinoless double beta (0vBB) decay is one of the most interesting topics in modern particle physics. Its observation would be proof of new physics beyond the Standard Model (SM), showing that neutrinos are their own antiparticles (Majorana particles), and violation of lepton number conservation — hinting that leptons play a part in the matter/antimatter asymmetry. The LUX-ZEPLIN (LZ) experiment uses the largest dual-phase (liquid/gas) xenon TPC ever built, with 7 tonnes of active target, and was primarily designed to search for direct interactions of dark matter with baryonic matter. Operating since 2021 in the Sanford Underground Research Facility (SURF, SD, USA), 1.5 km below ground to protect it from cosmic rays and installed inside a large water tank to shield it from environmental radioactivity, the inner region of the detector is an extremely low background laboratory that can be used to search for other rare event processes, such as 0vBB decay in 136Xe. In this project the student will participate in the ongoing analyses of the available LZ data to search for this process, becoming familiar with the interesting physics involved in the decay and the operational details of the detector, and learn how to explore the recorded data.

Grupo : DarkMatter
Local : Coimbra
Supervisor(s) : Alexandre Lindote / Paulo Brás
Email : alex@lip.pt
Vagas : 1
Duração/Datas : July to September


A neutrino observatory for geosciences
Due to their different properties, each elementary particle is useful for getting different information. The SNO+ detector in Canada measures neutrinos produced by the Uranium and Thorium decays in the Earth crust and mantle, as done previously only from Japan and Italy. SNO+ is located 2000 m underground to avoid noise from cosmic ray muons, but still a few muons can reach it every hour, which can be used to map the shielding between the detector and the surface. Based on simple models and inspired by real data, we want to explore what both neutrinos and muons are already telling us, and estimate how much time we need to understand more of their messages about the Earth.

Grupo : Neutrinos
Local : Lisboa
Supervisor(s) : Sofia Andringa
Email : sofia@lip.pt
Vagas : 2
Duração/Datas : flexible


Análise de dados com a experiência Alpha Magnetic Spectrometer (AMS-02) instalada na ISS
A experiência Alpha Magnetic Spectrometer (AMS-02) é um detetor de física de partículas de alta precisão instalado a bordo da Estação Espacial Internacional desde 2011. Projetado para operar no ambiente de radiação cósmica do espaço, o AMS-02 combina um íman permanente de 0,15 T com múltiplos subsistemas de deteção (detectores de silício, de tempo de voo, calorímetro eletromagnético, TRD e RICH) para medir com rigor sem precedentes o fluxo, a carga e a massa dos raios cósmicos, desde o hidrogénio até ao ferro. A sua missão científica visa a procura de antimatéria, a deteção indireta de matéria escura através da análise de espectros de partículas carregadas, e o estudo da propagação e aceleração de raios cósmicos na Galáxia. Neste contexto, o detetor de efeito de Cherenkov RICH desempenha um papel fundamental: fornece medições de velocidade com resolução acima de 0.1%, permitindo a separação de isótopos. A medida das observáveis físicas como a velocidade, momento linear, carga eléctrica e energia, depende diretamente de algoritmos avançados de reconstrução, e de correções várias e alinhamento geométrico contínuo. É exatamente nesta interface entre física e análise de dados que o trabalho de estágio se insere. O estágio de verão dá a oportunidade de contribuires diretamente para a melhoria da performance da análise de dados de AMS-02, através do desenvolvimento de uma das seguintes tarefas: - Reconstrução de eventos Cherenkov num radiador plástico: analisarás padrões de luz gerados por partículas cósmicas, aprendendo a extrair informação física a partir de sinais reais de deteção. - Optimização da resolução de velocidade: desenvolverás métodos estatísticos e computacionais para eliminar dependências com o tempo, temperatura, posição de impacto da partícula, etc., elevando a precisão intrínseca do detetor. - Estudo de desalinhamento traço–detetor RICH: investigarás o eventual desalignamento geométrico entre o plano de deteção do detector RICH e detector de traços, que afeta a reconstrução de velocidade. - Identificação de isótopos cósmicos: desenvolverás um método de separação de isótopos com templates de massa analíticos. O estágio vai-te permitir trabalhar com dados reais ou simulados, ferramentas de análise modernas (ROOT, Python, C++) e aprofundares as ligações entre o conhecimento adquirido na Universidade com as actividades de investigação.

Grupo : AMS
Local : Lisboa
Supervisor(s) : Fernando Barão
Email : fernando.barao@tecnico.ulisboa.pt
Vagas : 3
Duração/Datas : 1-31 Julho


Coincident detection of neutrinos and charm hadrons with SND@LHC and ATLAS
Neutrinos were observed for the first time in 1957 by Reines and Cowan, confirming Paulis 1931 prediction. In the nearly seven decades since this discovery, dozens of neutrino experiments have been conducted which have made decisive contributions towards our understanding of the relationship between the three generations of fermions, the origin of mass, and the inner workings of the Sun. However, none of these experiments has ever detected the production and interaction of a neutrino in a single event. The Scattering and Neutrino Detector at the Large Hadron Collider (SND@LHC) is located 480 m away from the ATLAS detector where proton-proton collisions take place. Neutrinos resulting from these collisions travel undisturbed through the material between the collision point and the SND@LHC detector, where they have a 1 in a billion chance of interacting. In this project, the coincident detection of neutrinos in SND@LHC and charm hadrons in ATLAS will be explored. Preliminary results indicate that over 1000 coincident events will occur during the high-luminosity phase of the LHC. Simulated data will be used to develop strategies for efficiently identifying the production of neutrinos in ATLAS proton-proton collision events, while reducing backgrounds. The use of machine learning algorithms to achieve this task will be explored.

Grupo : SHiP/SND@LHC
Local : Lisboa
Supervisor(s) : Cristóvão Vilela, Nuno Leonardo
Email : c.vilela@cern.ch
Vagas : 2
Duração/Datas : Flexible


Data-driven validation of the ProtoDUNE-Vertical Drift geometry using calibration systems
Data-driven validation of the ProtoDUNE-Vertical Drift geometry using calibration systems

Grupo : Neutrinos
Local : Lisboa
Supervisor(s) : José Maneira, Cristóvão Vilela, Joana Vences
Email : joanavences@lip.pt
Vagas : 1
Duração/Datas : Julh-Ago


Electron neutrino observation at the LHC
While copious amounts of neutrinos are produced in the Large Hadron Collider (LHC) at CERN, none had been directly observed until recently. In 2023, two experiments, SND@LHC and FASER, announced the first direct detection of the muon neutrino at the LHC. This result is a milestone in experimental particle physics, opening the door to a rich new program of neutrino measurements at colliders, which will elucidate topics ranging from proton structure to flavour symmetry in the Standard Model of particle physics. Identifying the flavour (electron, muon or tau) of the detected neutrinos is a key requirement to achieve the SND@LHC goals. This project is focused on the SND@LHC electron neutrino analysis, which uses a binned-likelihood fit to the data. Simulated electron neutrino interactions will be used to optimise the analysis parameters, and the expected precision of electron neutrino measurements with the full SND@LHC dataset will be estimated.

Grupo : SHiP/SND@LHC
Local : Lisboa
Supervisor(s) : Cristóvão Vilela, Nuno Leonardo
Email : c.vilela@cern.ch
Vagas : 2
Duração/Datas : Flexible


Exploring the Inner Structure of Ultra-High-Energy Air Showers with AugerPrime
Cosmic rays are high-energy particles arriving at Earth from outer space. When the most energetic of these particles hit the atmosphere, they create enormous cascades of secondary particles, known as air showers, that spread over many square kilometers. While scientists have learned a great deal about these showers, what happens at their very core—close to where the cascade is most intense—remains largely unknown. In this project, we will explore this unexplored region using data from the Pierre Auger Observatory, the world’s largest cosmic-ray detector. We will focus on a particularly dense part of the detector array (SD-433) and take advantage of recent upgrades (AugerPrime), which include new sensors capable of measuring extremely large particle densities near the shower axis. The student will work with real experimental data to study how particles are distributed at the center of these showers and compare the results with computer simulations. This project offers a unique opportunity to engage with cutting-edge research, learn data analysis techniques used in astroparticle physics, and contribute to our understanding of fundamental particle interactions at energies far beyond those accessible in human-made accelerators. Requirements: This project is intended for undergraduate students in Physics with prior experience in programming (preferably C++ and/or Python). The internship is designed to be carried out in person in Lisbon.

Grupo : Auger
Local : Lisboa
Supervisor(s) : Ruben Conceição, Milton Freitas
Email : ruben@lip.pt
Vagas : 2
Duração/Datas : June to September (exact dates to be agreed upon with supervisors)


Muography in archeology
Muons created in the atmosphere by cosmic rays can cross tens of meters of rocks, in straight lines and losing energy slowly until they stop (and decay). They can be used to create a muography, an image just like in radiography but in a larger scale. This method has revealed, for example, a secret chamber inside a pyramid in Egypt. In Portugal we tested it by imaging a geological fault from a mining gallery. We now plan to muograph the signs of roman mining in Aljustrel, imaging hiden vertical accesses or small horizontal galleries from below. In this summer project, the idea is to adapt and extend methods previously developed to this new scenario, and to test them on simulations of these and other structures in the mine. This is a fundamental step to plan a measuring campaign in the near future. The internship can be done in Lisbon or Braga

Grupo : MuTom
Local : Lisboa
Supervisor(s) : Sofia Andringa and Raul Sarmento
Email : sofia@lip.pt
Vagas : 2
Duração/Datas : flexible


Sistema de monitorização da temperatura dos detectores de SWGO
SWGO (Southern Wide-field Gamma-ray Observatory) é um projeto internacional para construir uma rede de detectores de raios gama de grande campo de visão no hemisfério Sul, com o objetivo de monitorizar o céu no intervalo de energias TeV-PeV. SWGO usará arrays de tanques de água instrumentados com fotomultiplicadores para detectar a radiação Cherenkov produzida por chuveiros atmosféricos, oferecendo uma capacidade de operação contínua e alta sensibilidade, complementando os observatórios existentes no hemisfério Norte. A monitorização da temperatura em tanques de água usados como detectores de raios gamma cósmicos é crucial por várias razões: - estabilidade do sinal: variações de temperatura alteram propriedades físicas da água (densidade, índice de refração), afetando a propagação da luz Cherenkov e, consequentemente, a resposta dos fotomultiplicadores - alteração da eficiência de detecção e a forma do pulso. - calibração e linearidade: photo-sensores e eletrónica associada (PMTs, bases, cabos) têm ganho e ruído dependentes da temperatura. - precisão temporal: diferenças térmicas podem alterar tempos de propagação dos fotões, degradando resolução temporal necessária para reconstrução de eventos e rejeição de fundo. - operacionalidade e durabilidade: ciclos térmicos extremos aceleram degradação de materiais, vedantes e componentes eletrónicos. SWGO está previsto ser instalado em Pampa La Bola, no Atacama Astronomical Park (região de Antofagasta, Chile), a cerca de 4770 m de altitude; o sítio fica perto de San Pedro de Atacama e de instalações como o ALMA. Do ponto de vista das condições térmicas, a sua altitute elevada implica um ar rarefeito e grande amplitude térmica diária (grandes variações de temperatura entre dia e noite). Existe por isso o risco de congelação parcial da água dos tanques. O congelamento parcial expande água e pode causar a ruptura mecânica do tanque. No quadro da participação do LIP na experiência, o grupo é responsável pelo modelo termodinâmico capaz de prever as variações de temperatura interna da água e pela instalação de um sistema de monitorização da temperatura dos tanques que permita validar o modelo. O sistema inclui um conjunto de sensores de temperatura (PT100) a serem instalados no interior do tanque de água (topo, meio, fundo), uma placa de aquisição de dados e ainda um micro-computador capaz de realizar as leituras de temperatura em intervalos regulares de tempo e registá-las num ficheiro binário. O sistema de monitorização inclui um software servidor-cliente em desenvolvimento que permite ao micro-computador gerir em paralelo as diferentes tarefas: 1) leitura das temperaturas registadas pelos sensores de forma regular e escrita em ficheiro diário (UTC), 2) gerir os pedidos de acesso dos clientes aos registos de temperatura. A aplicação cliente deverá ser capaz de aceder remotamente aos registos de temperatura e afixá-las graficamente usando um sistema como por exemplo o GRAfana. Este sistema será instalado dentro de alguns meses conjuntamente com o protótipo do tanque de água, no Chile. O projecto de estágio permitirá aos estudantes participarem no desenvolvimento do sistema de monitorização e na calibração dos sensores de temperatura. Complementarmente, os estudantes terão contacto com o conceito de uma experiência de deteção de raios-gamma e com as suas várias etapas de desenvolvimento.

Grupo : SWGO
Local : Lisboa
Supervisor(s) : Fernando Barão, Mário Pimenta
Email : fernando.barao@tecnico.ulisboa.pt
Vagas : 2
Duração/Datas : 1-31/Julho


Enhancing 3D Visualization tools for the Pierre Auger Collaboration
The Pierre Auger Observatory relies on advanced visualization tools to communicate its science, support education, and facilitate collaboration among researchers. In particular, interactive 3D visualization plays a key role in public outreach, helping diverse audiences engage with cosmic-ray physics. As the Observatory continues to expand, with new detector systems and increasing volumes of data, these tools must evolve to accurately represent the full experimental infrastructure and accommodate new scientific requirements. This project focuses on improving and extending the Pierre Auger Collaborations 3D visualization framework by incorporating recently deployed detectors, enhancing data integration capabilities, and developing new features to better support both scientific and educational applications. The resulting upgrades will strengthen the utility of these tools across outreach, teaching, and research, ensuring they remain an effective platform for exploring and presenting the Observatorys work.

Grupo : Auger
Local : Minho
Supervisor(s) : Henrique Carvalho, Raul Sarmento
Email : hcarvalho@lip.pt
Vagas : 2
Duração/Datas : June / July


Simulation of an experimental setup for calibrations in Auger Phase II
The Pierre Auger Observatory operates the largest detector in the world for the study of ultra-high-energy cosmic rays. The observatory was upgraded with new electronics and detectors and recently entered in Phase II with measurements planned up to 2035. This project consists in the simulation of an experimental setup used for the calibration of the new scintillator surface detectors of Auger.

Grupo : Auger
Local : Minho
Supervisor(s) : Raul Sarmento
Email : raul@lip.pt
Vagas : 2
Duração/Datas : Mostly July


Assembly and Characterization of an RPC Detector for Muon Tomography Applications
Within the framework of the TOMAR project (Muon Tomography Applied with Resistive Plate Chambers), which aims to develop a muon tomograph based on RPC technology capable of producing high-resolution images at low cost and with potential applications in sectors such as civil engineering, infrastructure, mining, and security, the interns will actively participate in the assembly and characterization of one of the first detector planes of the telescope under development. Throughout this process, they will gain direct hands-on experience with the operation of a particle detector, acquiring an integrated understanding of its different components, from front-end amplification electronics to the data acquisition system. This experience will provide solid practical training in scientific instrumentation, along with insight into the technological challenges associated with the development of advanced detection systems.

Grupo : RPC
Local : Coimbra
Supervisor(s) : Alberto Blanco
Email : alberto@lip.pt
Vagas : 5
Duração/Datas : June to September


Caracterização do Tracker de Raios Gama da Missão THOR a bordo do Space Rider da ESA, em função da temperatura
Em 2028, o grupo i-Astro lançará a bordo do Space Rider, um novo veículo reutilizável da ESA, o mini-observatório THOR (TGF and High-energy astrophysics Observatory for gamma-Rays on board the Space Rider) financiada pelo Programa PRODEX da ESA (PEA No. 4000141332), baseado em sensores de CdTe e Si para a observação do Universo no domínio dos raios gama. Pretende-se neste trabalho estudar o potencial de observação durante um voo de dois meses em órbita baixa. O aluno deverá contribuir para desenvolver o instrumento científico principal da missão THOR, o tracker de raios gama constituído por 3 planos de CdTe, em particular, deverá contribuir para os estudos de calibração do sistema em função da temperatura, bem como avaliar a eficiência de deteção e a resolução em energia. O aluno deverá operar e adaptar um programa de análise de dados, que permite ler dados de um instrumento científico e realizar análises de eficiência de deteção e resolução em energia. Em cada medida será alterada a temperatura de operação do sistema de deteção e traçar curvas de calibração, usando fontes de radiação (alfa e gama) propriedade do LIP. Os resultados obtidos serão incluídos no manual de instruções de calibração do instrumento THOR para a 1ª fase do voo do Space Rider.

Grupo : i-Astro
Local : Coimbra
Supervisor(s) : Alexandre Trindade & Rui Silva
Email : alexandre.trindade@lip.pt
Vagas : 3
Duração/Datas : entre junho e setembro - A combinar com o aluno datas precisas


Determinação da velocidade de deriva de eletrões em detetores de CdTe
Neste estágio, os alunos serão integrados numa equipa de investigação, na área de instrumentação para o espaço. A equipa de investigação está, neste momento, fortemente envolvida num projeto europeu com a ESA numa missão em que um vai-vém espacial não tripulado – Space Rider, colocará em órbita no ano de 2028, um dos nossos detetores de radiação de estado sólido. O trabalho consiste na utilização de detetores de radiação de estado sólido semelhantes aos da missão. Depois de uma introdução/revisão teórica do funcionamento dos diferentes tipos de detetores de radiação, os alunos vão ter a oportunidade de operar estes detetores. Com os dados recolhidos vão aprender a identificar a natureza da radiação incidente bem como a avaliar a energia e direção de incidência. O trabalho servirá para dar mais um pequeno contributo para a missão, com a caracterização dos detetores, nomeadamente na determinação da velocidade de deriva dos eletrões e a sua dependência na temperatura, usando o traço deixado (depósito de energia) na deteção de muões. Além das competências adquiridas com a utilização dos detetores, no decorrer do estágio os alunos irão também aprender ou reforçar os seus conhecimentos de técnicas de vácuo, manuseamento de gases e de eletrónica nuclear.

Grupo : i-Astro
Local : Coimbra
Supervisor(s) : Alexandre Trindade & Afonso Marques
Email : alexandre.trindade@lip.pt
Vagas : 3
Duração/Datas : entre junho e setembro - A combinar com os alunos datas precisas


From Bonner Spheres to a Single Smart Detector Approach for Neutron Field Characterisation
This internship, hosted by the Neutron Detectors Group at LIP in Coimbra, Portugal, focuses on the development and simulation of a novel neutron spectrometer design. Neutron detection plays a vital role across a wide range of applications, from nuclear safety and material analysis to medical physics techniques such as boron neutron capture therapy (BNCT). The project centers on evaluating an innovative detector concept based on neutron Resistive Plate Chambers (nRPCs) interspersed with a high-density polyethylene moderator, proposed as a more efficient alternative to the conventional Bonner Sphere Spectrometer, a well-established but time-consuming multi-detector method for characterising neutron energy fields. The students will be introduced to Monte Carlo simulation toolkits ANTS3 and Geant4, to model and optimise both the novel detector and the Bonner Sphere system (used as a benchmark), alongside hands-on experimental work including data acquisition and processing. By the end of the internship, students are expected to present their results at the LIP Summer Student Internship Workshop, and submit an internal technical note to be published on the LIP website.

Grupo : nDet
Local : Coimbra
Supervisor(s) : Luís Margato and Andrey Morozov
Email : margato@lip.pt
Vagas : 2
Duração/Datas : 1-2 months, flexible


Improvements to the OPGI prototype configuration for planning new experimental beam measurements
Proton therapy (PT) is expanding worldwide due to its ability to deliver a highly conformal dose to the irradiated target. However, several factors can compromise this conformality, leading to undesirable situations that are suspected to correlate with tumor recurrence. In this context, various approaches have been proposed for the in vivo monitoring of PT dose delivery and for verification of the proton beam range. One such approach is based on the detection of orthogonal prompt gamma rays produced by proton–nucleus interactions within the body. At LIP, we developed a small three-channel prototype, which was tested under proton beam irradiation conditions in Delft, the Netherlands. The main objectives of this work are: (1) to analyze the experimentally acquired data using MATLAB software; and (2) to investigate, through GEANT4 simulations, potential optimizations to be implemented in a new experimental campaign using proton and/or X-ray beams.

Grupo : ORimag
Local : Coimbra
Supervisor(s) : Hugo Simões
Email : hugo.simoes@lip.pt
Vagas : 2
Duração/Datas : June to September (exact dates to be agreed upon with supervisor)


Building a network of AI agents to test hypotheses in social physics
n the Social Physics and Complexity research group we use quantitative models tested in digital data to understand human behaviour and develop tools that benefit society https://socialcomplexity.eu/. Large Language Models (LLMs) and multi-modal generative artificial intelligence models have infiltrated all aspects of society and their influence is only expected to grow. However, they are black boxes in that their outputs cannot be understood from first principles in a trivial way. It is thus important that we understand and predict their behaviour in different situations. Furthermore, as LLMs are trained on human-generated data to mimic human interactions, they offer an experimental platform for developing and testing new mechanistic models of behavior. Indeed, LLMs are increasingly being leveraged in computational social science [1], particularly for understanding specific aspects of human interaction (e.g., [2, 3]). While LLMs are not expected to behave identically to humans, we can compare their textual outputs with empirical observations. This approach offers an advantage over traditional agent-based models, as we dont need to parameterize every aspect of their interactions, allowing for the testing of more complex hypotheses. At SPAC, we want to build an artificial social network where we are able to fully customize agent behaviour as well as adapt it to use different model architectures. The students participating in this internship will create a functional prototype of this network and run a pilot experiment. References [1] Ziems, C., Held, W., Shaikh, O., Chen, J., Zhang, Z., & Yang, D. (2024). Can large language models transform computational social science?. Computational Linguistics, 50(1), 237-291. https://direct.mit.edu/coli/article/50/1/237/118498 [2] Jia, F., Ye, Z., Lai, S., Shu, K., Gu, J., Bibi, A., ... & Chen, C. (2024). Can large language model agents simulate human trust behavior?. Advances in neural information processing systems, 37, 15674-15729. https://proceedings.neurips.cc/paper_files/paper/2024/hash/1cb57fcf7ff3f6d37eebae5becc9ea6d-Abstract-Conference.html [3] Ashery, A. F., Aiello, L. M., & Baronchelli, A. (2025). Emergent social conventions and collective bias in LLM populations. Science Advances, 11(20), eadu9368. https://www.science.org/doi/full/10.1126/sciadv.adu9368

Grupo : SPAC
Local : Lisboa
Supervisor(s) : Lilia Perfeito
Email : lperfeito@lip.pt
Vagas : 2
Duração/Datas : June and July 2026


Cooking quantum dots for particle detection
Scintillating materials, which emit light when traversed by ionizing radiation, are one of the main tools for particle detection. In particular, liquid scintillators have long been used for large-scale detectors such as those used for neutrino and dark matter experiments. Typical liquids consist of organic scintillator compounds in solvent, which pose environmental risks, or noble elements kept at cryogenic temperatures, which pose logistical challenges. This project will explore the use of carbon quantum dots to produce water-based scintillating solutions that are a promising and environmentally safe technology to overcome the main challenges in the liquid scintillator detector state-of-the-art. Carbon quantum dots will be synthesized from household items such as sugar, used coffee grounds or orange juice using a microwave oven. Several solutions will be prepared and their fluorescence will be assessed under UV light. The most promising solutions will then be exposed to a radioactive source and their response to ionizing radiation will be measured with photomultiplier tubes as used in particle physics experiments. The students will prepare the carbon quantum dot solutions, take data in LIP’s scintillating materials laboratory in Lisbon, and analyse the data to quantify the sensitivity of water-based carbon quantum dot solutions to ionizing radiation.

Grupo : Neutrinos
Local : Lisboa
Supervisor(s) : Sofia Andringa, Cristóvão Vilela
Email : c.vilela@cern.ch
Vagas : 2
Duração/Datas : Flexible


Electronics - Development for the BoneOscopy and FLASHGuard Projects
N/A

Grupo : Particles4Health
Local : Lisboa
Supervisor(s) : Gonçalo Ribeiro e Gonçalo Roriz
Email : gmribeiro@lip.pt
Vagas : 0
Duração/Datas : n/A


Experimental Validation of the FLASHGuard Prototype Using an Sr-90 Source
This work focuses on the experimental testing and validation of the FLASHGuard prototype. The project is centered on the use of an already developed and instrumented system, aiming to assess its performance under controlled laboratory conditions. The prototype is designed to ensure reliable data acquisition, high system responsiveness, and safe operation. A key objective is the validation of the system using a Strontium-90 (Sr-90) radioactive source, enabling controlled evaluation of its behavior under radiation exposure. The experimental campaign will support the analysis of system responsiveness, robustness, and measurement consistency. The results are expected to contribute to the verification of the FLASHGuard concept and provide insights for future improvements.

Grupo : Particles4Health
Local : Lisboa
Supervisor(s) : Gonçalo Roriz & Pedro Assis
Email : goncalororiz@tecnico.ulisboa.pt
Vagas : 1
Duração/Datas : 06/07-31/07


Geant4 Simulation Study of new variants of the FLASHGuard Project
This project presents a preliminary Geant4 simulation study aimed at characterizing and optimizing the spatial resolution of a novel detector concept developed within the FLASHGuard Project for beam monitoring in FLASH radiotherapy (RT). The work involves the complete definition, implementation, and validation of a comprehensive simulation framework, including detector geometry, material properties, optical photon transport, and realistic readout modelling. The study focuses on quantifying the detector’s spatial resolution as a function of key design parameters and irradiation conditions, with the goal of identifying optimal configurations. In addition, a dedicated case study is performed using a Laser Wakefield Acceleration (LWFA) beam, incorporating a realistic phase-space description to evaluate detector performance under the beam’s distinctive characteristics. Reconstruction strategies are assessed and performance metrics are defined to systematically evaluate detector response. The outcomes of this work include simulation-driven design guidelines and recommendations to support the next development phase of the FLASHGuard device. Overall, this study provides valuable insights into detector optimization and feasibility for emerging ultrahigh-dose-rate beams, contributing to ongoing advancements in FLASH RT beam monitoring.

Grupo : Particles4Health
Local : Lisboa
Supervisor(s) : Gonçalo Ribeiro & Pedro Assis
Email : gmribeiro@lip.pt
Vagas : 1
Duração/Datas : 21/07-7/09


Instrumentation Development for the FLASHGuard Advanced Radiotherapy Monitoring Project
Development in the FLASHGuard Advanced Radiotherapy Monitoring Project

Grupo : Particles4Health
Local : Lisboa
Supervisor(s) : Manuel Ratola & Pedro Assis
Email : manuelratola22@tecnico.ulisboa.pt
Vagas : 1
Duração/Datas : 21/07-7/09


Optical Fibre Instrumentation R&D for the AntiMatter-OTech Detector
This project focuses on the development of optical fibre instrumentation for the AntiMatter-OTech detector, an innovative LiquidO-based antineutrino detector being built in Lisbon to monitor nuclear reactors non-invasively. Before construction, the detector’s optical readout systems require extensive prototyping and testing, and the student will contribute to optimizing the fibre instrumentation, evaluating different optical fibre technologies, and developing systems to validate fibre readout during detector assembly. The project will be developed in LIPs Laboratory of Optics and Scintillating Materials and integrated within the AntiMatter-OTech consortium.

Grupo : LOMaC
Local : Lisboa
Supervisor(s) : Rute Pedro and Agostinho Gomes
Email : rute@lip.pt
Vagas : 3
Duração/Datas : July to September


Optical Instrumentation for the TileCal/ALLEGRO detector at the Future Circular Collider
This project supports the development of optical-based particle detectors for future collider experiments, focusing on the ALLEGRO detector concept proposed for the Future Circular Collider (FCC-ee). The work involves the optical characterisation of new plastic scintillator materials for the high-granularity hadronic calorimeter prototype and studies of scintillator–fibre coupling to optimize light collection efficiency and detector performance.

Grupo : LOMaC
Local : Lisboa
Supervisor(s) : Rute Pedro and Agostinho Gomes
Email : rute@lip.pt
Vagas : 2
Duração/Datas : July to September


Particle tracks reconstruction using passive dosimeters - a path towards cell level dosimetry
In the past few months, we have been irradiating a type of dosimeters called FNTDs (https://doi.org/10.1063/1.3576173). The dosimeters were irradiated with alpha particles (target: dosimeter) and neutrons (target: HDPE+dosimeter). After irradiation, information is stored in the dosimeter in displaced electrons trapped in the band gap. The stored information is related to dosimetric quantities. The most common dosimeters use thermoluminescence (TL) or optically stimulated luminescence (OSL). FNTDs, fantastically, can track particles, and the tracks can be associated with a quantity called LET, most relevant for micro- and nano- dosimetry, which means looking at the cell-level scale. The FNTD readout uses confocal microscopy (CFM) to collect segments that make the particle tracks. CFM readout, besides selecting wavelength ranges for excitation/readout, works by defining several focal planes (with a width of the order of tenths of micrometre) along the dosimeters thickness and recording the hotspots. The measured tracks correspond to or are associated with the LET of particles crossing the dosimeter volume. For a particle crossing the volume, this results in a correlation between the different recorded CFM planes. The commonly used SW is Fiji (https://imagej.net/software/fiji/). Would you be interested in reviewing a set of images collected for these dosimeters. The goal is to review the images and collect all the information on existing tracks: geometric and intensity. In the end, you will have defined a methodology to deal with these images that we can use for dosimeter readout in future irradiations.

Grupo : ATLAS
Local : Lisboa
Supervisor(s) : Cristiana Rodrigues (cristiana@lip.pt), Joao Gentil Saraiva (gentil@lip.pt)
Email : gentil@lip.pt
Vagas : 1
Duração/Datas : N/A


The Science Behind the Low-cost Production of Sapphires for Dosimetric Applications
Hadron therapy has emerged as one of the most promising forms of radiation therapy, offering exceptional precision in targeting tumors while minimizing damage to surrounding healthy tissue. Yet, despite major technological advances, current treatment planning still relies heavily on macroscopic absorbed-dose metrics. These do not fully capture how energy is deposited at the microscopic and nanoscopic scales where biological damage actually occurs. To unlock the full therapeutic potential of hadron therapy, new microscale dosimetry tools are needed, tools capable of linking physical dose deposition to the biological response of individual cells. At LIP, ongoing research focuses on developing micro/nanodosimetric techniques and detectors with improved spatial resolution. These efforts aim to bridge the gap between physical radiation interactions and radiobiological effects. Passive dosimeters are essential tools in radiation protection and dosimetry, enabling accurate monitoring of radiation exposure over time, memorizing this information in their inner structure for post-processing and not requiring any data acquisition system during exposure. Among passive dosimetry methods, Thermoluminescence (TL) and Optically Stimulated Luminescence (OSL) stand out. Materials such as carbon-doped sapphire (Al2O3:C) are widely used due to their excellent luminescent properties. However, the search for improved or application-specific materials is an active and exciting research frontier. This internship offers the opportunity to contribute directly to this field by exploring the growth and characterization of doped and undoped Al2O3 crystals produced using a novel method. These crystals will be evaluated for their potential use in luminescence-based dosimetry. The crystals will be synthesized using the flux method, where a volatile flux is evaporated at a constant temperature, significantly below the melting point of the material, to gradually bring the solution into a supersaturated state and promote crystal formation. The student will engage in the following tasks: Growth of Al2O3 crystals (doped and undoped) using the flux method; Preparation and handling of crystal samples for characterizations; Chemical/Elemental characterization using X-Ray Fluorescence (XRF) or other methods; Structural analysis via X-ray Diffraction (XRD); Optical analysis using UV-Vis spectroscopy; Luminescence characterization using the RISO DA-20 TL/OSL Reader at C2TN; Data analysis, interpretation, and documentation of results. These techniques will help determine dopant incorporation, crystal purity, and lattice structure, key factors influencing luminescence performance. This proposal arises from a collaboration between LIP and C2TN, leveraging the expertise available in both research units. By the end of the internship, the student is expected to: Gain hands-on experience in laboratory work; Understand the principles and applications of solid-state synthesis and crystal growth.

Grupo : RADART
Local : Lisboa
Supervisor(s) : Cristiana Rodrigues, João Gentil
Email : cristiana@lip.pt
Vagas : 1 or 2
Duração/Datas : Adjustable and discussed with students from June to early September (probable stop in August due to Holidays but remote work may proceed)


Development of a low cost plastic scintillator based cosmic ray detector for outreach applications
Detection of cosmic ray muons is one of the simplest demonstrations that can be made for high school students. LIP already has a successful program based on the reproduction of the Hesse experiment using a detector based on a Geiger counter. This project aims to expand the portfolio, by implementing a low cost detector based on plastic scintillator, that can be used as an evolution of the previous experiment. The goal is to develop a compact detector, including the eletronics, as well as additional sensors, to allow for continuous data acquisition and detector monitoring.

Grupo : LIP - Geral
Local : Minho
Supervisor(s) : Nuno Barros
Email : barros@lip.pt
Vagas : 1
Duração/Datas : 1/6 - 14/08


Simulation of a new photon detector design for neutrino detectors
The ARAPUCA family of detectors have been developed and deployed with great success in various high energy neutrino physics experiments. These detectors are able to separate the light emitted from particle interactions into two groups, separating the less abundant, but directional Cherenkov emission component from the dominant, isotropic liquid scintillator component. The goal to this project is to initiate study to expand this technology to detectors using liquid scintillator. The goal is to develop a Geant4 based simulation of a setup that will permit to characterize different aspects of the detector, and carry out a study of different detector approaches to guide the design of the setup to be assembled.

Grupo : Neutrinos
Local : Minho
Supervisor(s) : Nuno Barros, José Maneira
Email : barros@lip.pt
Vagas : 1
Duração/Datas : 1/6 - 14/08


Exploring extreme QCD matter with heavy flavour at the LHC
This project focuses on one of the hallmarks of Quantum Chromodynamics (QCD): hadronization, the non-perturbative process by which color charges, the quarks and the gluons, transform into color-neutral hadrons. Despite its central role in strong-interaction physics, the dynamics governing hadron formation remains only partially understood, making precision studies of heavy-flavor production especially valuable. The student will investigate B-meson production in proton–proton (pp) collisions using Run 3 data collected by the CMS experiment at the Large Hadron Collider. Production yields will be measured as functions of key kinematic variables, such as transverse momentum and rapidity, as well as event-activity observables, including charged-particle multiplicity and collision centrality. These measurements provide a sensitive probe of the interplay between perturbative heavy-quark production and the subsequent non-perturbative hadronization stage. The work will employ modern data-analysis techniques, combining maximum-likelihood fitting methods with machine-learning approaches for signal extraction, background suppression, and efficiency optimization. A central objective is the determination of b-quark fragmentation fractions: the probabilities that a bottom quark hadronizes into different beauty-hadron species. Their ratios, kinematic dependences, and possible modifications with event environment will be studied with high precision. These results establish an important benchmark for understanding heavy-ion collisions (PbPb), where a deconfined medium known as the quark–gluon plasma (QGP) is created. Comparing pp and PbPb systems will help reveal how the QGP influences heavy quark hadronization, providing new insight into both confinement dynamics and the properties of strongly interacting matter under extreme conditions.

Grupo : CMS
Local : Lisboa
Supervisor(s) : Henrique Legoinha, Nuno Leonardo
Email : nuno.leonardo@cern.ch
Vagas : 2
Duração/Datas : June - August


Investigating the Flavor Anomalies in B-meson Decays at the LHC
The Standard Model (SM) of particle physics provides a very accurate description of the fundamental particles and their interactions. However, several experimental results in the decays of B hadrons showed clear deviations from its predictions, making these processes an exciting environment to search for signs of new physics. Among them, the decay of the B0 meson into a K*0 and a pair of muons stands out as a powerful probe, thanks to the rich structure of its angular distributions. In this project, the student will work with data collected by the Compact Muon Solenoid experiment at the Large Hadron Collider during the recent Run-3 data taking. The goal is to reconstruct B0 → K*0 μμ decay candidates and to perform an angular analysis by producing accurate models and fitting them to the observed distributions. These tasks will be accomplished with the use of advanced computational tools, including machine learning techniques and software for statistical analysis. The student will be integrated into an active research team and will gain hands-on experience with real experimental data, developing both practical skills and a deeper understanding of how precision measurements at the LHC can reveal physics beyond the Standard Model.

Grupo : CMS
Local : Lisboa
Supervisor(s) : Alessio Boletti, Nuno Leonardo
Email : alessio.boletti@cern.ch
Vagas : 2
Duração/Datas : Between end of June to beginning of September (with some degree of flexibility, exact dates can be agreed)


Search for New Phenomena using Anomaly Detection in the ATLAS/LHC Experiment
This project explores the use of anomaly detection techniques, including auto-encoders and Deep SVDD, to search for signs of phenomena beyond the Standard Model in data from the ATLAS experiment at CERN’s Large Hadron Collider. Unlike traditional searches that target specific theoretical models, this approach aims to identify rare, non-Standard-Model-like events in a model-independent way by training deep neural networks on known physics processes. The analysis focuses on events with boosted jets and missing transverse momentum, using both simulated and real collision data, while benchmark new physics signals are employed to validate the methods. The project will be integrated into the ATLAS Portuguese group and in the ATLAS collaboration team analysing Monojet events.

Grupo : ATLAS
Local : Lisboa
Supervisor(s) : Rute Pedro, Annalisa Berti, Inês Moreira
Email : rute@lip.pt
Vagas : 1
Duração/Datas : July to September


From Thermal Phase Transitions to Gauge Extensions: Optimising Gravitational Wave Signals in U(1) Models
The early Universe may have undergone first-order phase transitions capable of generating stochastic backgrounds of gravitational waves, potentially observable by future experiments such as LISA. The strength and duration of these transitions are typically characterised by the parameters α (the released vacuum energy) and β/H (the inverse duration rate of the transition), which together determine the amplitude and shape of the resulting gravitational wave spectrum. In this project, students will first study a simplified finite-temperature scalar potential, the coupled fluid-scalar field model (CFF), identifying the parametric conditions that maximise α and minimise β/H, thereby enhancing the gravitational wave signal. Particular emphasis will be placed on understanding the roles of the cubic thermal term, the scalar self-coupling, and the temperature scale associated with symmetry breaking. Building on this analytic understanding, the project will establish a direct correspondence between the toy CFF model parameters and those of a minimal U(1)′ gauge extension of the Standard Model. In this framework, the cubic term responsible for the phase transition barrier arises from thermal gauge boson effects, allowing the optimisation criteria derived in the toy model to be mapped onto physically meaningful parameters such as the gauge coupling, scalar quartic interaction, and symmetry-breaking scale. The final goal is to identify regions of parameter space in U(1)′ models that lead to strong and long-lasting phase transitions, and therefore to potentially observable gravitational wave signals. This provides a concrete illustration of how theoretical particle physics models can be constrained, and potentially discovered, through cosmological observations.

Grupo : Pheno
Local : Minho
Supervisor(s) : António Morais
Email : amorais@lip.pt
Vagas : 3
Duração/Datas : 01/06/2026 - 31/09/2026


Exploring heavy mesons
Hadrons are composite systems of quarks and antiquarks that interact through the strong interaction, which is mediated by the exchange of gluons. This interaction is so strong that single quarks cannot be separated from other quarks, a phenomenon known as confinement. It is not yet known how exactly confinement arises from the fundamental quark and gluon interactions, but one can study effective models to learn about its properties. A particular kind of hadrons are called mesons, most of which can be understood as bound states of one quark and one antiquark. The objective of this internship project is to explore how details of the interaction between quarks and antiquarks influence the masses and the internal structure of mesons. We will focus on studying heavy mesons, where relativistic effects, most importantly spin-dependent interactions, are expected to be small enough to be treated perturbatively. By varying the strengths of these interactions, their relative importance in the theoretical descriptions of observables can be assessed. This is a theory project with a strong computational component, so experience with programming in languages like Mathematica, Fortran, C++ or Python is necessary. Candidates should also have a decent knowledge of quantum mechanics, including the quantum treatment of spin and orbital angular momentum, as well as of special relativity. Familiarity with the Dirac equation would be a plus.

Grupo : NPStrong
Local : Lisboa
Supervisor(s) : Alfred Stadler, Elmar Biernat
Email : stadler@lip.pt
Vagas : 3
Duração/Datas : Dates are flexible. We could start sometime in June and continue until the end of July in person at LIP. Occasional remote meetings during August would also be possible, if needed. Participation in person in the internship workshop at the beginning of September is expected.


R-Matrix Analysis of Nuclear Reactions with AZURE2
Nuclear reactions are at the heart of both clean fusion energy and emerging, targeted cancer treatments. This internship focuses on the nuclear reactions of protons with Boron-11 relevant to Ion Beam Analysis—a technique to study wall materials for future fusion reactors—and to Proton-Boron Capture Therapy in medicine. Students will analyze existing experimental data using AZURE2. This open-source code is based on R-matrix theory, a quantum-mechanical framework for modeling low-energy nuclear reactions. The two students selected for this project will familiarize themselves with the fundamentals of nuclear reactions, R-matrix theory, and the AZURE2 code, they will configure and run AZURE2, and compile input data from IAEA nuclear databases, including separation energies, spin-parity assignments, and the energies and widths of excited states of the compound nucleus for several reaction channels. The objective of this internship is to fit existing cross-section data using AZURE2. Evaluating data using R-matrix theory is essential for quantifying uncertainties and making reliable extrapolations. High-quality cross-sections are critical for advancing Ion Beam Analysis in nuclear fusion research and for quantifying the localized, high-LET alpha-particle dose boost in Proton-Boron Capture Therapy. Candidate Requirements: a solid foundation in quantum mechanics, basic understanding of nuclear physics, and prior experience in programming and data handling is highly beneficial.

Grupo : NPStrong
Local : Lisboa
Supervisor(s) : Elmar Biernat, Alfred Stadler
Email : elmar@lip.pt
Vagas : 2
Duração/Datas : Dates are flexible. We could start sometime in June and continue until the end of July in person at LIP. Occasional remote meetings during August would also be possible, if needed. Participation in person in the internship workshop at the beginning of September is expected.


Tensor Networks for in-medium particle dynamics
Quantum Chromodynamics predicts that at extreme temperatures and densities, matter enters a deconfined state in which quarks and gluons are quasi-free — the Quark-Gluon Plasma (QGP), a phase that filled the universe during its first microsecond. Such conditions are recreated at the LHC in ultra-relativistic heavy-ion collisions, making these collisions a unique laboratory for studying the primordial liquid. Jets - collimated sprays of particles produced by hard scatterings - are ideal probes: their interactions with the QGP imprint characteristic modifications on jet observables, from which the mediums properties can be inferred. Quantitative comparison with experiment requires a precise theoretical description of how QCD partons propagate and radiate inside a background medium.The underlying formalism was formulated nearly 30 years ago by BDMPS-Z, and several problems have remained long-standing given the complexity of the evolution equations. Solving them beyond the simplest approximations quickly runs into a dimensionality wall, making grid-based numerical methods impractical. This internship will explore computational methods that can potentially be used to address these limitations. The main direction is for the candidates to explore Tensor Networks, which exploits low-rank structure to represent and evolve high-dimensional functions with storage and cost that scale linearly rather than exponentially in the number of dimensions. A secondary direction, depending on the candidates interests, is the construction of neural-network surrogates for fast, inline evaluation of these high-dimensional objects in Monte Carlo simulations, and a quantitative comparison of the two approaches. The selected candidates will gain hands-on experience with a modern computational toolkit alongside exposure to the theoretical foundations of jet quenching. These skills are directly transferable to many areas of computational physics where high-dimensional problems and the need for efficient numerical methods are central concerns. Meetings with the supervisor will mostly be online, with possible exceptions.

Grupo : Pheno
Local : Lisboa
Supervisor(s) : Marco Leitão
Email : mleitao@lip.pt
Vagas : 3
Duração/Datas : Flexible. From June to September