2607948
Project Grant
Overview
Grant Description
THE NANOGRAV PHYSICS FRONTIERS CENTER -THIS AWARD TO THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES (NANOGRAV) SUPPORTS THEIR GOAL OF CHARACTERIZING THE LOW-FREQUENCY GRAVITATIONAL-WAVE (GW) UNIVERSE THROUGH RADIO TIMING OBSERVATIONS OF PRECISE CELESTIAL CLOCKS CALLED MILLISECOND PULSARS. NANOGRAV HAS ALREADY DISCOVERED THE TELLTALE SPATIAL CORRELATIONS AMONG PULSE ARRIVAL TIMES EXPECTED FROM A STOCHASTIC BACKGROUND OF GWS. THIS BACKGROUND IS LIKELY TO HAVE A SIGNIFICANT CONTRIBUTION FROM THE SUPERMASSIVE BLACK HOLE BINARIES FORMED WHEN GALAXIES MERGE. FUTURE NANOGRAV MEASUREMENTS OF THE PROPERTIES OF THE STOCHASTIC BACKGROUND WILL PLACE UNIQUE CONSTRAINTS ON THE GROWTH AND EVOLUTION OF GALAXIES THROUGH COSMIC TIME. THERE MAY ALSO BE BACKGROUND CONTRIBUTIONS FROM MORE EXOTIC SOURCES SUCH AS COSMIC STRINGS, PHASE TRANSITIONS IN THE EARLY UNIVERSE, AND RELIC GWS FROM INFLATION; DETECTING ANY OF THESE WOULD BE TRANSFORMATIVE AND COULD DRAMATICALLY CHANGE OUR UNDERSTANDING OF THE UNIVERSE. THIS AWARD WILL ENABLE NANOGRAV TO CONSTRUCT A MORE SENSITIVE DATA SET THAT WILL ALLOW CONSTRAINTS ON THE ORIGIN OF THIS STOCHASTIC BACKGROUND, AND SEARCHES FOR INDIVIDUAL SUPERMASSIVE BLACK HOLE BINARIES, WHOSE DETECTION WILL HERALD A NEW ERA OF MULTI-MESSENGER NANOHERTZ GW ASTROPHYSICS. THIS WORK REQUIRES THE SYNERGY OF EXPERTS IN GRAVITATIONAL PHYSICS, DATA ANALYSIS, AND ASTROPHYSICS COMING TOGETHER IN A COLLABORATIVE ENVIRONMENT. IN ADDITION TO MONITORING A KNOWN LIST OF MILLISECOND PULSARS, NANOGRAV ROUTINELY DISCOVERS NEW MSPS TO ADD TO THEIR STUDY. NANOGRAV OBSERVATIONS ALSO ENABLE HIGH-IMPACT SYNERGISTIC SCIENCE, INCLUDING CONSTRAINING THE DENSE MATTER EQUATION OF STATE, MAKING DYNAMICAL TESTS OF GENERAL RELATIVITY, FURTHER UNDERSTANDING THE IONIZED INTERSTELLAR MEDIUM, AND DISCOVERING EXOTIC NEUTRON STAR SYSTEMS AND RADIO TRANSIENTS. NANOGRAV REACHES LARGE NUMBERS OF THE GENERAL PUBLIC THROUGH EXHIBITS AND TALKS, AS WELL AS A GROWING SOCIAL MEDIA PRESENCE. AN ASSOCIATED STUDENT RESEARCH PROGRAM, NANOGRAV STARS, REACHES MORE THAN 100 UNDERGRADUATE STUDENTS EVERY YEAR, AND THE PULSAR SCIENCE COLLABORATORY INVOLVES HUNDREDS OF MIDDLE AND HIGH SCHOOL STUDENTS AND THEIR TEACHERS. THIS AWARD IS SUPPORTED BY THE PHYSICS SECTION AND THE ASTRONOMICAL SCIENCES SECTION WITHIN THE MATHEMATICAL AND PHYSICAL SCIENCES DIRECTORATE. 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.- SUBAWARDS ARE PLANNED FOR THIS AWARD.
Funding Goals
THE GOAL OF THIS FUNDING OPPORTUNITY, "DIVISION OF PHYSICS: INVESTIGATOR-INITIATED RESEARCH PROJECTS", IS IDENTIFIED IN THE LINK: HTTPS://WWW.NSF.GOV/PUBLICATIONS/PUB_SUMM.JSP?ODS_KEY=NSF23615
Grant Program (CFDA)
Awarding / Funding Agency
Place of Performance
Morgantown,
West Virginia
26505-6315
United States
Geographic Scope
Single Zip Code
Related Opportunity
West Virginia University Research Corporation was awarded
NANOGrav: Low-Frequency GW Universe Characterization
Project Grant 2607948
worth $5,950,041
from the Division of Physics in June 2026 with work to be completed primarily in Morgantown West Virginia United States.
The grant
has a duration of 1 year 5 months and
was awarded through assistance program 47.049 Mathematical and Physical Sciences.
The Project Grant was awarded through grant opportunity Division of Physics: Investigator-Initiated Research Projects.
Status
(Ongoing)
Last Modified 6/3/26
Period of Performance
6/1/26
Start Date
11/30/27
End Date
Funding Split
$6.0M
Federal Obligation
$0.0
Non-Federal Obligation
$6.0M
Total Obligated
Activity Timeline
Additional Detail
Award ID FAIN
2607948
SAI Number
None
Award ID URI
SAI EXEMPT
Awardee Classifications
For-Profit Organization (Other Than Small Business)
Awarding Office
490301 DIVISION OF PHYSICS
Funding Office
490301 DIVISION OF PHYSICS
Awardee UEI
M7PNRH24BBM8
Awardee CAGE
4B983
Performance District
WV-02
Senators
Joe Manchin
Shelley Capito
Shelley Capito
Modified: 6/3/26