Talks
This list includes 20 invited and 12 contributed presentations.
Invited Talks
- Neutron stars, mergers, and gravitational waves — XII International Conference on Nuclear Physics in Astrophysics, Cluj-Napoca (Romania, 2026)
- Persistent chiral dynamics without magnetic helicity: Implications for magnetars — Frontier Research in Astrophysics - V, Palermo (Italy, 2026)
- Neutron Star Physics Explored Through 3D Simulations — Astrophysical Fluid Dynamics Workshop, Escola d’Enginyeria de Barcelona (Spain, 2026)
- Magnetic Field Evolution in Neutron Stars: Effects of Superfluidity and Superconductivity — European COST Action CA24139 – SCALES: Vortex motion from laboratory to the stars, Warsaw (Poland, 2026)
- Magnetic field evolution in isolated neutron stars — Strong Gravity Seminar, Perimeter Institute (Canada, 2026)
- How helicity distribution shapes large-scale dipoles in magnetars — CITA Seminar, CITA (Canada, 2026)
- Descobrint la física de les estrelles de neutrons: una expedició en 3D a l'evolució magnetotèrmica en estrelles de neutrons aïllades amb MATINS — Fòrum IEEC 2025, Casa Convalescència (UAB), Barcelona (Spain, 2025)
- Origin of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal Simulations — Modern Equations of State and Spectroscopy in Neutron Star Matter, Alcala University (Spain, 2025)
- Magnetar Field Dynamics Shaped by Chiral Anomalies and Magnetic Helicity — Extreme Physics of Neutron Star Interiors, Princeton University, New Jersey (USA, 2025)
- Chiral Magnetic Instability in Neutron Star Crust: A Possible Origin of Magnetar Fields — Breaking New Ground in Supernova Physics 2025 (BNGSP25), Fukuoka University (Japan, 2025)
- Origin and Dynamics of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal Simulations — IReNA-INT Joint Workshop on Thermal and Magnetic Evolution, University of Washington, Washington (USA, 2024)
- Unveiling the Physics of Neutron Stars, a 3D expedition into MAgneto-Thermal evolution in Isolated Neutron Stars with MATINS — Frontier Workshop, Palermo (Italy, 2024)
- MATINS, The Magnetic Field Formalism — Astrophysics Seminar, Valencia University (Spain, 2023)
- MATINS, The Magnetic Field Formalism — Astrophysics Seminar, Nordita (Sweden, 2023)
- A new finite volume code for the evolution of magnetic field in three dimensions — AstroCoffee Seminar, Goethe University (Germany, 2022)
- A new finite volume code for the evolution of magnetic field in three dimensions — NucPhys Seminar, Ganil Facilities (France, 2022)
- The Influence of Crustal Physics in the Cooling of Neutron Stars — Hadronic, Nuclear & Atomic Physics Seminar, University of Barcelona (Spain, 2021)
- On the rate of crustal failures in young magnetars — Astrophysics Seminar, University of Alicante (Spain, 2021)
- On the rate of crustal failures in young magnetars — Stars & Compact Objects Meeting, Flatiron Institute, New York City (USA, 2020)
- Neutron stars equation of state and merging using the Metamodeling technique — Hadronic, Nuclear & Atomic Physics Seminar, University of Barcelona (Spain, 2019)
Contributed Talks
- Why some neutron stars become magnetars: chiral anomalies in the absence of magnetic helicity — NewAthena Rising, ICE-CSIC, Barcelona (Spain, 2026)
- Origin of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal Simulations — EAS annual Meeting, University College Cork (Ireland, 2025)
- Constraints on the dense matter equation of state from young and cold isolated neutron stars — International Conference on Quarks and Nuclear Physics, University of Barcelona (Spain, 2024)
- Understanding the dynamics of neutron star magnetic field through 3D magneto-thermal simulations — XMM-Newton Workshop, ESA Madrid (Spain, 2024)
- Young and cold neutron stars constraining the dense matter equation of state — Special Seminar, Institute of Space Sciences, Barcelona (Spain, 2024)
- The role of chiral magnetic effect and helicity in proto-neutron stars turbulent dynamo — Astrophysics Seminar, University of Alicante (Spain, 2024)
- A better understanding of the thermally emitting neutron stars via magneto-thermal evolution models — EAS Annual Meeting (Online, 2022)
- A new finite volume code for the evolution of magnetic field in three dimensions — Pharos Conference, La Sapienza University (Italy, 2022)
- A new finite-volume code for the magnetic field evolution of neutron stars in 3D — Pizza Seminar, Institute of Space Sciences, Barcelona (Spain, 2022)
- The influence of crustal physics in the cooling of a neutron star — IAU Symposium 363 (online, 2021)
- On the rate of crustal failures in young magnetars — Pizza Seminar, Institute of Space Sciences, Barcelona (Spain, 2020)
- Hot neutron rich nuclear matter studied with the BCPM nuclear energy density functional — Pharos Conference, Patras University (Canceled due to Covid-19) (Greece, 2020)