Neutron Stars: Connecting Fundamental Physics to Astrophysical ObservationsTheoretical Physics Seminar, Autonomous University of Madrid, Spain
2026
Neutron stars, mergers, and gravitational wavesXII International Conference on Nuclear Physics in Astrophysics, Cluj-Napoca, Romania
Magnetic Field Evolution in Neutron Stars: Effects of Superfluidity and SuperconductivityEuropean COST Action CA24139 – SCALES: Superfluid Condensates in Astrophysics and Laboratory Experiments, Coimbra, Portugal
Neutron Star Physics Explored Through 3D SimulationsAstrophysical Fluid Dynamics Workshop, Escola d’Enginyeria de Barcelona, Spain
Magnetic Field Evolution in Neutron Stars: Effects of Superfluidity and SuperconductivityEuropean COST Action CA24139 – SCALES: Vortex motion from laboratory to the stars, Warsaw, Poland
Magnetic field evolution in isolated neutron starsStrong Gravity Seminar, Perimeter Institute, Canada
How helicity distribution shapes large-scale dipoles in magnetarsCITA Seminar, CITA, Canada
2025
Descobrint la física de les estrelles de neutrons: una expedició en 3D a l'evolució magnetotèrmica en estrelles de neutrons aïllades amb MATINSFòrum IEEC 2025, Casa Convalescència (UAB), Barcelona, Spain
Origin of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal SimulationsModern Equations of State and Spectroscopy in Neutron Star Matter, Alcala University, Spain
Magnetar Field Dynamics Shaped by Chiral Anomalies and Magnetic HelicityExtreme Physics of Neutron Star Interiors, Princeton University, New Jersey, USA
Chiral Magnetic Instability in Neutron Star Crust: A Possible Origin of Magnetar FieldsBreaking New Ground in Supernova Physics 2025 (BNGSP25), Fukuoka University, Japan
2024
Origin and Dynamics of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal SimulationsIReNA-INT Joint Workshop on Thermal and Magnetic Evolution, University of Washington, Washington, USA
Unveiling the Physics of Neutron Stars, a 3D expedition into MAgneto-Thermal evolution in Isolated Neutron Stars with MATINSFrontier Workshop, Palermo, Italy
2023
MATINS, The Magnetic Field FormalismAstrophysics Seminar, Valencia University, Spain
MATINS, The Magnetic Field FormalismAstrophysics Seminar, Nordita, Sweden
2022
A new finite volume code for the evolution of magnetic field in three dimensionsAstroCoffee Seminar, Goethe University, Germany
A new finite volume code for the evolution of magnetic field in three dimensionsNucPhys Seminar, Ganil Facilities, France
2021
The Influence of Crustal Physics in the Cooling of Neutron StarsHadronic, Nuclear & Atomic Physics Seminar, University of Barcelona, Spain
On the rate of crustal failures in young magnetarsAstrophysics Seminar, University of Alicante, Spain
2020
On the rate of crustal failures in young magnetarsStars & Compact Objects Meeting, Flatiron Institute, New York City, USA
2019
Neutron stars equation of state and merging using the Metamodeling techniqueHadronic, Nuclear & Atomic Physics Seminar, University of Barcelona, Spain
Contributed Talks
2026
The physics of neutron starsPencil Code User Meeting 2026, Alicante, Spain
Origin of magnetar magnetic fields: Insights from 3D magneto-thermal simulationsX-ray Universe 2026, XMM-Newton, Elche, Spain
Why some neutron stars become magnetars: chiral anomalies in the absence of magnetic helicityNewAthena Rising, ICE-CSIC, Barcelona, Spain
2025
Origin of Magnetar Magnetic Fields: Insights from 3D Magneto-Thermal SimulationsEAS annual Meeting, University College Cork, Ireland
2024
Constraints on the dense matter equation of state from young and cold isolated neutron starsInternational Conference on Quarks and Nuclear Physics, University of Barcelona, Spain
Understanding the dynamics of neutron star magnetic field through 3D magneto-thermal simulationsXMM-Newton Workshop, ESA Madrid, Spain
Young and cold neutron stars constraining the dense matter equation of stateSpecial Seminar, Institute of Space Sciences, Barcelona, Spain
The role of chiral magnetic effect and helicity in proto-neutron stars turbulent dynamoAstrophysics Seminar, University of Alicante, Spain
2022
A better understanding of the thermally emitting neutron stars via magneto-thermal evolution modelsEAS Annual Meeting, Online
A new finite volume code for the evolution of magnetic field in three dimensionsPharos Conference, La Sapienza University, Italy
A new finite-volume code for the magnetic field evolution of neutron stars in 3DPizza Seminar, Institute of Space Sciences, Barcelona, Spain
2021
The influence of crustal physics in the cooling of a neutron starIAU Symposium 363, online
2020
On the rate of crustal failures in young magnetarsPizza Seminar, Institute of Space Sciences, Barcelona, Spain
Hot neutron rich nuclear matter studied with the BCPM nuclear energy density functionalPharos Conference, Patras University (Canceled due to Covid-19), Greece
