What is the NSF Pire Award


"Partnerships for International Research and Education (PIRE) is an NSF-wide program that supports international activities across all NSF supported disciplines. The primary goal of PIRE is to support high quality projects in which advances in research and education could not occur without international collaboration. PIRE seeks to catalyze a higher level of international engagement in the U.S. science and engineering community."

"International partnerships are essential to addressing critical science and engineering problems. In the global context, U.S. researchers and educators must be able to operate effectively in teams with partners from different nations and cultural backgrounds. PIRE promotes excellence in science and engineering through international collaboration and facilitates development of a diverse, globally-engaged, U.S. science and engineering workforce."

More information about the National Science Foundation's PIRE program can be found at www.nsf.gov. An abstract for NANOGrav's PIRE award can be found at www.nsf.gov/awardsearch.

NANOGrav's goals for the PIRE Award


Mission
U.S. Researchers and students will join with foreign colleagues to direct gravitational wave detection, build a diverse community of researchers with international expertise, and lay the groundwork for gravitational wave studies in the next decade and beyond.
Goal One: Scienctific Knowledge
Advance new knowledge and discoveries at the frontiers of science while acheiving increased sensitivity to gravitational waves (GWs)
Goal Two: Education
Facilitate greater student and faculty preparation for and participation in the IPTA
Goal Three: Partnerships
Enable NANOGrav to establish collaborative relationship and operate effectively with IPTA members form different nations and cultural backgrounds
Goal Four: Institutional Capacity
Strenthen the capacity of our institutions to engage and benefit form IPTA research and education collaborations
Goal Five: Workforce Development
Develop a diverse, globally-engaged science workforce by catalyzing a higher level of international engagement by NANOGrav

What does the PIRE Award mean for NANOGrav Science?


Gravitational waves are a key prediction of Einstein’s theory of general relativity, but their influence has only been indirectly detected to date. Millisecond pulsars are rapidly rotating neutron stars that emit pulses of radio waves, similar to flashes of light from a lighthouse. Gravitational waves perturb the travel of these pulses from a pulsar to the Earth. Together with international collaborators, the U.S. investigators will use radio telescopes around the world to observe signals from dozens of pulsars over several years. This will enable the detection or placement of stringent limits on the existence of gravitational waves. The PIRE award will support many of the activities of the North American NanoHertz Observatory for Gravitational waves (NANOGrav) as well as provide essential resources for the International Pulsar Timing Array (IPTA), a collaboration with Australian, European, and Indian scientists. The direct detection of gravitational waves will open up a new window on the universe that will allow studies of black holes at the cores of massive galaxies and the earliest stages of the universe.

The PIRE program will foster international research collaboration and cooperation by (i) supporting postdoctoral researchers and graduate and undergraduate students at 10 U.S. institutions, (ii) funding yearly international science meetings, student workshops, and research and observing trips, (iii) providing infrastructure for communication, data storage, and data management, and (iv) establishing study abroad programs. These initiatives will broaden student horizons and enable U.S. researchers to collaborate more effectively with international colleagues in pursuit of this outstanding frontier of Einstein’s legacy.


Quarterly Newsletters


Lisa Kohne from SmartStart Educational Consulting Services serves as the external evaluator for the PIRE project. Evaluation results provide feedback to the PIRE leadership team to improve PIRE project activities. They also assess progress made towards achievement of project goals. Evaluation findings are based on surveys, evaluation forms, interviews, and focus group discussions. Quarterly evaluation reports and newsletters are available below.

Advisory Board


To assist us as we apply the funds from the NSF PIRE award we have enlisted a diverse advisory board. Their invaluable input will insure that we meet our goals and fulfill expectations.

Patrick Brady
University of Wisconsin-Milwaukee, is an expert on gravitation and the detection of gravitational waves with interferometers.
Joan Centrella
Goddard Space Flight Center, is an expert on numerical relativity in support of LIGO and is head of the Gravitational Astrophysics Laboratory at the Goddard Space Flight Center.
Marjorie Darrah
West Virginia University, is an Associate Professor of Mathematics at WVU and is an expert on integrating research into educational outreach.
Jim Moran
Harvard University, is chair of the astronomy department and an expert on studies of galaxies and black holes with radio and submillimeter arrays.
Christopher Plein
West Virginia University, is the Assistant Dean of the School of Applied Social Sciences and Chair of the Division of Public Administration at WVU and an expert on community organization and project management.
Richard Price
University of Texas at Brownsville, is a theoretical astrophysicist specializing in general relativity.