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The Leonard E Parker Center for Gravitation, Cosmology and Astrophysics is supported by NASA, the National Science Foundation, UW-Milwaukee College of Letters and Science, and UW-Milwaukee Graduate School. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of these organizations.
Posted by Patrick Brady on December 28, 2011
The first direct detection of gravitational waves will be a watershed event in 21st century physics and astronomy. The scientific goals of the LSC rely on a substantial computational infrastructure, which spans astrophysical data analysis, detector and analysis middleware, software sustainability and computational hardware support. Initial LIGO has shown that cyber-infrastructure is as essential to gravitational-wave astronomy as the detectors themselves. It will not be possible to detect gravitational-wave sources, to study their properties, and to maximize the NSF's investment in LIGO without support for the enabling computational technologies. This award to develop and sustain Advanced LIGO's cyber-infrastructure will allow the LIGO Scientific Collaboration to be ready for the transformative new science that gravitational-wave observations will bring. The LDG research program will train students and postdocs to be experts in next-generation cyber-infrastructure, push the boundaries of LIGO's geographically distributed, locally-available computational data grid, and sustain the operation of this cyber-infrastructure to support LIGO's science mission. Collaborations with external partners (including Internet2, Globus, Condor and Pegasus) will have significant impact outside the LSC.