Benjamin Owen, Ph.D
Department of Physics and Astronomy
Phone: (806) 834-0231
ResearchI have been laying the foundations of gravitational wave astronomy since the days most people said it would never happen. I am one of very few people who has worked on all four types of signals (binary mergers, continuous waves, stochastic background, non-binary bursts), both theory and data analysis. LIGO's historic discoveries of binary mergers used my mathematical techniques for covering parameter space and evaluating waveform accuracy, and I have also worked on analytical and numerical waveforms. I discovered the most promising emission mechanisms for continuous waves, astrophysically guided many LIGO searches, and run big searches myself. Many types of LIGO burst searches bear my fingerprints, particularly searches for starquakes.
With binary merger detections becoming routine, I am focused on the yet undetected signals that define the new frontier. Continuous waves present the greatest mathematical and computational challenges, their searches are most affected by electromagnetic astronomy, and they can tell us uniquely about the microphysics of dense matter; so they are the type that gets most of my attention these days. I am also interested in all sorts of novel signals, particularly those involving neutron stars.
I am the head of observational data and computing for Cosmic Explorer, a planned improvement on LIGO.
Brief Bio2016 Special Breakthrough Prize (as part of the LIGO Scientific Collaboration)
2015 faculty at Texas Tech
2013 Fellow of the American Physical Society
2002 faculty at Penn State
2000 postdoc at University of Wisconsin - Milwaukee
1998 postdoc at Max Planck Institute for Gravitational Physics
1998 Clauser Prize for Doctoral Thesis of the Year, Caltech
1998 PhD from Caltech, Advisor: Kip Thorne
1993 BS from Sonoma State University
2021-now member of the Cosmic Explorer consortium
1997-2019 member of the LIGO Scientific Collaboration
- B. Rajbhandari, B. J. Owen, S. Caride, and R. Inta, "First search for gravitational waves from r-modes of the Crab pulsar," Phys. Rev. D 104, 122008 (2021)
- L. Lindblom and B. J. Owen, "Directed searches for continuous gravitational waves from twelve supernova remnants
in data from Advanced LIGO's second observing run," Phys. Rev. D 101, 083023 (2020)
- B. P. Abbott, et al. (LIGO Scientific Collaboration and Virgo Collaboration), "GW170817: Observation of Gravitational Waves From a Binary Neutron Star Inspiral," Phys. Rev. Lett. 119, 161101 (2017)
- B. P. Abbott, et al. (LIGO Scientific Collaboration and Virgo Collaboration), "Observation of gravitational waves from a binary black hole merger," Phys. Rev. Lett. 116, 061102 (2016)
- N. K. Johnson-McDaniel and B. J. Owen, "Maximum elastic deformations of relativistic stars," Phys. Rev. D 88, 044004 (2013)
- J. Abadie, et al. (LIGO Scientific Collaboration and Virgo Collaboration), "Search for gravitational wave bursts from six magnetars," Astrophys. J. 734, L35 (2011)
- L. Lindblom, B. J. Owen, and D. A. Brown, "Model waveform accuracy standards for gravitational wave data analysis," Phys. Rev. D 78, 124020 (2008)
- B. J. Owen, "Maximum elastic deformations of compact stars with exotic equations of state," Phys. Rev. Lett. 95, 211101 (2005)
- B. J. Owen, L. Lindblom, C. Cutler, B. F. Schutz, A. Vecchio, and N. Andersson, "Gravitational waves from hot young rapidly rotating neutron stars," Phys. Rev. D 58, 084020 (1998)
- B. J. Owen, "Search templates for gravitational waves from inspiraling binaries: Choice of template spacing," Phys. Rev. D 53, 6749 (1996)
Curriculum VitaeMy long form CV is available as a PDF.
Department of Physics and Astronomy
AddressTexas Tech University, Physics & Astronomy Department, Box 41051, Lubbock, TX 79409-1051
Phone806.742.3767 | Fax: 806.742.1182