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Research Spending & Results

Award Detail

Awardee:UNIVERSITY OF CONNECTICUT
Doing Business As Name:University of Connecticut
PD/PI:
  • Chiara M Mingarelli
  • (860) 486-4915
  • chiara.mingarelli@uconn.edu
Award Date:08/02/2021
Estimated Total Award Amount: $ 313,139
Funds Obligated to Date: $ 313,139
  • FY 2021=$313,139
Start Date:08/15/2021
End Date:07/31/2024
Transaction Type:Grant
Agency:NSF
Awarding Agency Code:4900
Funding Agency Code:4900
CFDA Number:47.049
Primary Program Source:040100 NSF RESEARCH & RELATED ACTIVIT
Award Title or Description:Collaborative Research: An Empirical Blueprint for the Gravitational-Wave Background
Federal Award ID Number:2106552
DUNS ID:614209054
Parent DUNS ID:004534830
Program:STELLAR ASTRONOMY & ASTROPHYSC
Program Officer:
  • Hans Krimm
  • (703) 292-2761
  • hkrimm@nsf.gov

Awardee Location

Street:438 Whitney Road Ext.
City:Storrs
State:CT
ZIP:06269-1133
County:Storrs Mansfield
Country:US
Awardee Cong. District:02

Primary Place of Performance

Organization Name:University of Connecticut
Street:196A Auditorium Road
City:Storrs
State:CT
ZIP:06269-3046
County:Storrs Mansfield
Country:US
Cong. District:02

Abstract at Time of Award

Orbiting supermassive black holes in the centers of galaxies are thought to produce very low frequency gravitational waves that could be detected by careful timing of the arrival of radio pulses from pulsars through the ongoing pulsar timing array project. It is expected that the combined signals from many of these systems will produce a background noise that may soon be detectable by pulsar timing arrays. This project will use a new method based on observations of accreting supermassive black holes to provide an estimate of the strength of this background noise as well as it's distribution in gravitational wave frequencies. The project will use this new method to provide a framework for determining the history of the growth of supermassive black holes once the background noise is detected. The project will also create a Pulsar Search Collaboratory hub in New Jersey and New York that will involve high school students in the search for pulsars using real data. This award advances the goals of the Windows on the Universe Big Idea. The project will use observations of quasar luminosity functions at different redshifts combined with local observations of dual Active Galactic Nuclei to build an empirically-based model of the cosmological distribution of supermassive black hole binaries that will contribute to the stochastic gravitational wave background expected to be detected in pulsar timing array observation. This approach is complementary to the existing approach that is based on galaxy merger simulations. The new approach will determine key physical parameters that can be constrained through detection of the gravitational wave background. The project will also create a Pulsar Search Collaboratory hub in New Jersey and New York. The Pulsar Search Collaboratory is a long-standing NSF supported program that allows high schools students to search for pulsars with real radio data. It is a low-barrier way for students to experience science and scientific discovery. This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

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