We dedicate our efforts to study Superconducting qubits and circuit QED, Quantum many-body systems, Driven-dissipative quantum systems, Light-matter interaction in low-dimensional systems, Quantum Information
2006-2010 PhD in Astronomy and Astrophysics, University of Manchester, UK
2003-2005 Magíster en Astronomía, Universidad de Chile
1998-2002 Licenciatura en Ciencia m/Física, Universidad de Chile
Línea de investigación:
Astrofísica de estrellas de neutrones. Pulsar timing. Física espacial. Física de la magnetósfera terrestre.
Actividad:
Mi línea principal de investigación son los pulsares. Usamos datos tomados con radio telescopios o satélites de rayos-X para estudiar cómo rotan y qué procesos físicos alteran su rotación. De esta manera aprendemos sobre lo que ocurre dentro y fuera de los pulsares.
Desde hace poco he estado también trabajando en Física espacial. En particular, hemos estado usado datos tomados en la magnetósfera terrestre para estudiar cómo se distribuye la eneregía entre las partículas y los efectos de la turbulencia en el transporte de energía en la cola de la magnetósfera.
2023-RCM Modeling of Bubble Injections Into the Inner Magnetosphere: Spectral Properties of Plasma Sheet Particles-Journal of Geophysical Research: Space Physics-https://doi.org/10.1029/2022JA030673
2023-Formation of the Outer Radiation Belt: Adiabatic Effect and Stochastic Acceleration-Springer Proceedings in Earth and Environmental Sciences-https://doi.org/10.1007/978-3-031-40728-4_23
2023-A new small glitch in Vela discovered with a hidden Markov model-Monthly Notices of the Royal Astronomical Society-https://doi.org/10.1093/mnras/stad1335
2022-VLA proper motion constraints on the origin, age, and potential magnetar future of PSR J1734-3333-Astronomy and Astrophysics-https://doi.org/10.1051/0004-6361/202142598
2022-Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run-Astrophysical Journal-https://doi.org/10.3847/1538-4357/ac6ad0
2022-Timing Six Energetic Rotation-powered X-Ray Pulsars, Including the Fast-spinning Young PSR J0058-7218 and Big Glitcher PSR J0537-6910-Astrophysical Journal-https://doi.org/10.3847/1538-4357/ac8743
2022-Spontaneous Magnetic Fluctuations and Collisionless Regulation of Turbulence in the Earth's Magnetotail-Astrophysical Journal-https://doi.org/10.3847/1538-4357/ac33a2
2021-Ion Kappa Distribution Parameters in the Magnetosphere of the Earth at Geocentric Distances Smaller Than 20 RE During Quiet Geomagnetic Conditions-Journal of Geophysical Research-https://doi.org/10.1029/2021JA029409
2021-Influence of MHD Turbulence on Ion Kappa Distributions in the Earth's Plasma Sheet as a Function of Plasma β Parameter-Frontiers in Astronomy and Space Sciences-https://doi.org/10.3389/fspas.2021.647121
2021-Constraints from LIGO O3 Data on Gravitational-wave Emission Due to R-modes in the Glitching Pulsar PSR J0537-6910-Astrophysical Journal Letters-https://doi.org/10.3847/2041-8213/abffcd
2021-Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910-Astrophysical Journal, Supplement Series-https://doi.org/10.3847/1538-4365/abdec9
2021-On the Relation between Kappa Distribution Functions and the Plasma Beta Parameter in the Earth's Magnetosphere: THEMIS Observations-Astrophysical Journal-https://doi.org/10.3847/1538-4357/ac0d52
2021-Corrigendum: Small glitches and other rotational irregularities of the Vela pulsar (Astronomy and Astrophysics (2021) 647 (A25) DOI: 10.1051/0004-6361/202039044)-https://doi.org/10.1051/0004-6361/202039044e
2020-Proper motion, spectra, and timing of PSR J1813-1749 using Chandra and NICER-Monthly Notices of the Royal Astronomical Society-https://doi.org/10.1093/mnras/staa2653
2020-Return of the Big Glitcher: NICER timing and glitches of PSR J0537-6910-Monthly Notices of the Royal Astronomical Society-https://doi.org/10.1093/mnras/staa2640
La física espacial se dedica a la comprensión de los procesos fundamentales en el sistema viento solar-magnetosfera-ionosfera (SVSMI) basados en la física de plasmas. Se espera que avances en esta área mejoren nuestra comprensión del espacio y genere mejor pronóstico del clima espacial, un área crítica de investigación tanto en Chile como en el mundo, ya que nuestra sociedad depende cada vez más de la tecnología espacial.
We dedicate our efforts to understand the underlying difficulties in science education, in special in the Chilean and Latin American framework, taking into account aspects as socioeconomic distribution and gender equality. In this context, we implement and quantify different strategies at institutional, teacher formation and student level to contribute close the gap in science education.
