Gabriela González

Boyd Professor
| PhD: 1995 - Syracuse University |
| Email: gonzalez@lsu.edu |
| Phone: 225-578-0468 |
| Office: 271-B Nicholson Hall, Tower Dr., Baton Rouge, LA 70803-4001 |
Research Interests
Experimental General Relativity
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.
Select Publications
- "Observation of Gravitational Waves from a Binary Black Hole Merger", B.P. Abbott et al. (LIGO Scientific and Virgo Collaborations) Phys. Rev. Lett. 116 (2016) 6, 061102
- "GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral", B.P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Phys. Rev. Lett. 119 (2017) 16, 161101
- "LIGO Detector Characterization in the Second and Third Observing Runs", D. Davis et al., Class. Quantum Grav. 38 135014 (2021)
- "Noise in the LIGO Livingston gravitational wave observatory due to trains", J. Glanzer et al., Class.Quant. Grav. 40 19, 195015 (2023)
- "Reducing Scattered Light in LIGO's Third Observing Run", S. Soni et al., Class. Quantum Grav. 38 025016 (2021)