Gabriela González
Professor
Physics & Astronomy
Louisiana State University
United States of America
Biography
Gabriela is currently a professor in the physics and astronomy department at Louisiana State University (LSU). In addition to teaching, she works with the nearby Laser Interferometer Gravitational-Wave Observatory (LIGO) in Livingston, Louisiana. Gabriela pursued her passion for physics at the University of Cordoba, where she completed her "Licienciatura," a degree similar to a master’s degree in the U.S. After that, Gabriela moved to Syracuse University for her Ph.D., which focused on Brownian motion and gravitational waves. Gabriela studied a way to predict thermal noise which could "drown out" the gravitational wave’s extremely small signal. Thus, being able to predict thermal noise becomes important whenever physicists study gravitational waves.
Research Interest
Prof. González research interest is in the detection of gravitational waves with interferometric detectors, such as the one in the LIGO Livingston Observatory, in Livingston, LA. She has published several papers on the specific predictions of Brownian motion as a limiting sources to the detectors' sensitivity. She was a founding member of the LIGO Scientific Collaboration, and has participated intensely in the commissioning of the LIGO detector at the Livingston Observatory since joining LSU in 2001, in issues related to alignment sensing and control. Her group is very involved in the instrumental characterization and calibration of the data collected in the data-taking Science Runs performed by the LIGO Scientific Collaboration (LSC). From 2000 to 2007, she co-led one of the four data analysis groups in the Collaboration, dedicated to the search of gravitational waves generated by binary systems of compact objects (neutron stars or black holes) in the final inspiraling stage before coalescence. In 2008-2011, she led the LSc detector characterization working group. In 2011, she was elected as the LSC spokesperson.
Publications
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Improved analysis of GW150914 using a fully spin-precessing waveform Model B. P. Abbott et al. [LIGO Scientific and Virgo Collaborations]. Phys. Rev. X 6, 041014 (2016)
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Binary Black Hole Mergers in the first Advanced LIGO Observing Run B. P. Abbott et al. [LIGO Scientific and Virgo Collaborations], Phys. Rev. X 6, 041015 (2016)
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The basic physics of the binary black hole merger GW150914 B. P. Abbott et al. [LIGO Scientific and Virgo Collaborations]. Annalen Phys. (2016).