Project Grant 2409745
- This $3 million National Science Foundation project grant supports research and development activities critical to the success of gravitational-wave astronomy through the Laser Interferometer Gravitational-Wave Observatory (LIGO)-Virgo-KAGRA network. Funded under the Mathematical and Physical Sciences program, the University of Wisconsin-Milwaukee will deliver several data analysis elements for low-latency detection of transient gravitational waves from binary neutron star and black hole...
- This Project Grant award from the National Science Foundation (NSF) Directorate for Mathematical and Physical Sciences (CFDA 47.049) will advance the understanding of massive black hole binaries (MBHBs) and their role as multimessenger sources of gravitational waves (GWs) and X-ray emissions. The $510,590 award to the Georgia TECH Research Corporation will model the X-ray counterparts to the GW signals produced by inspiraling MBHBs. This work will lay the groundwork for observations, investigate...
- This $188,470 Project Grant awarded by the National Science Foundation (NSF) Division of Physics under the Mathematical and Physical Sciences program (CFDA 47.049) supports theoretical investigations into gravitational waves (GWs) emitted by extreme mass-ratio compact binaries. The research aims to develop improved mathematical models and computational techniques for analyzing GW signals that will be detected by the upcoming Laser Interferometer Space Antenna (LISA) mission. This work involves...
- The National Science Foundation (NSF) Directorate for Mathematical and Physical Sciences awarded a $337,029 Project Grant to Northwestern University for the "COLLABORATIVE RESEARCH: WOU-MMA: SEARCHES AFTER GRAVITATIONAL-WAVES USING ARIZONA'S OBSERVATORIES (SAGUARO)" project. The grant, which runs from September 1, 2023 to August 31, 2026, supports an electromagnetic observing campaign associated with gravitational wave detector observations. Key activities include comprehensive...
- This $150,000 federal Project Grant awarded by the National Science Foundation's (NSF) Mathematical and Physical Sciences program (CFDA 47.049) supports research conducted by Embry-Riddle Aeronautical University in two key areas: Detector characterization efforts to understand and mitigate the effects of Earth-based noise on the Laser Interferometer Gravitational-Wave Observatory (LIGO) interferometers, enabling more sensitive detection of gravitational waves. This includes near-real time...
- This federal Project Grant award, issued by the National Science Foundation (NSF) under the Mathematical and Physical Sciences (CFDA 47.049) program, will enhance existing search strategies and analysis capabilities for discovering and characterizing the coalescence of compact binary systems, such as black holes and neutron stars. The $200,000 award, with a performance period from August 1, 2024 to July 31, 2027, will fund four key activities: (i) extending multi-messenger Bayesian inference...
- This $628,695 National Science Foundation project grant supports research at Northwestern University to analyze gravitational wave data and infer astrophysical population properties. The university will characterize gravitational waves detected in the fourth observing run of the Laser Interferometer Gravitational-Wave Observatory to understand how black holes and neutron stars interact. Researchers will develop frameworks to analyze binary merger source populations, interpret observed...
- This $301,094 federal Project Grant award from the National Science Foundation's (NSF) Mathematical and Physical Sciences program (CFDA 47.049) supports research on neutron stars and gravitational waves. The main research activities include searches for continuous gravitational waves from young neutron stars, including R-mode oscillations of known pulsars and searches of supernova remnants for non-pulsing neutron stars. The award also contributes to searches for other signals like neutron star...
- This National Science Foundation (NSF) Project Grant award for $600,000 supports research in gravitational wave astrophysics at the Georgia Institute of Technology. The goal is to advance the detection, characterization, and interpretation of gravitational wave transients from compact binary mergers and other astrophysical sources using LIGO-VIRGO-KAGRA data. Key objectives include improving software infrastructure, mitigating noise impacts, and participating in the 4th LIGO observing run....
- This $374,699 federal Project Grant awarded by the National Science Foundation (NSF) Division of Astronomical Sciences under the Mathematical and Physical Sciences program (CFDA 47.049) will fund a 4-year collaborative research program led by investigators at Louisiana State University, Harvard University, University of Minnesota-Twin Cities, and University of Maryland, College Park. The research aims to improve the understanding of explosive transients in the distant universe by...
WOU-MMA: CONTINUOUS GRAVITATIONAL WAVES: FROM SEARCHING TO OBSERVING -MULTIMESSENGER ASTROPHYSICS (MMA) COMBINES DIFFERENT MEANS OF OBSERVATION SUCH AS ELECTROMAGNETIC AND GRAVITATIONAL WAVES (GWS), AS SEEN IN THE 2017 LIGO-VIRGO OBSERVATION OF A BINARY NEUTRON STAR INSPIRAL ASSOCIATED WITH A GAMMA-RAY BURST, FOLLOWED BY MULTIPLE OBSERVATIONS OF AN ELECTROMAGNETIC COUNTERPART. A PROMISING MMA TARGET IS THE LOW-MASS X-RAY BINARY (LMXB) SCORPIUS X-1, LONG STUDIED IN X-RAY, RADIO, AND OPTICAL. THIS BINARY STAR SYSTEM CONSISTS OF A NEUTRON STAR, AN EXTREMELY DENSE OBJECT MORE MASSIVE THAN THE SUN AND THE SIZE OF A CITY, TOGETHER WITH A LESS MASSIVE STAR, THE OUTER LAYERS OF WHICH ARE BEING PULLED ONTO THE NEUTRON STAR BY ITS GRAVITY. THE NEUTRON STAR IS BELIEVED TO BE SPINNING TENS TO HUNDREDS OF TIMES A SECOND AND IS ONE OF THE MOST PROMISING SOURCES OF LONG-LIVED GRAVITATIONAL WAVES. THE GOAL OF THIS PROJECT IS TO DETECT OR FURTHER CONSTRAIN THOSE WAVES, WHICH WILL BROADEN THE FIELD OF GRAVITATIONAL WAVE ASTRONOMY BEYOND THE SHORT-LIVED GW SIGNALS OBSERVED SO FAR BY LIGO AND VIRGO. THIS PROJECT WILL INVOLVE FACULTY, SCIENTIFIC STAFF, AND STUDENTS OF THE ROCHESTER INSTITUTE OF TECHNOLOGY, WHO WILL CONDUCT THE MOST SENSITIVE SEARCH EVER FOR GWS FROM SCO X-1 USING DATA FROM THE FOURTH AND FIFTH OBSERVING RUNS OF THE ADVANCED LIGO, ADVANCED VIRGO, AND KAGRA DETECTORS, PROBING THE RANGE OF PLAUSIBLE SIGNAL STRENGTHS OVER A WIDE RANGE OF FREQUENCIES, AND POSSIBLY LEADING TO THE FIRST OBSERVATION OF CONTINUOUS GRAVITATIONAL WAVES. THE PROGRAM WILL ALSO BE EXTENDED BY EXPANDING THE SEARCH TO OTHER LMXBS, IMPROVING THE VALIDATION OF POTENTIAL DETECTIONS, AND TRANSITIONING FROM A MODE OF SEARCHING ALL THE DATA OF A RUN AT ONCE TO ONGOING INCREMENTAL OBSERVATIONS. THE SEARCH FOR GWS FROM SCO X-1 IS CONSIDERED A HIGHEST PRIORITY BY THE LIGO SCIENTIFIC COLLABORATION, AND THIS GRANT WILL BE INSTRUMENTAL IN MAXIMIZING ITS SUCCESS. 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 NOT PLANNED FOR THIS AWARD.
Mod # | Description | ReasonForModification | Federal Obligation | Date |
|---|---|---|---|---|
| Not listed | $83.5k | 6/20/25 | ||
| Not listed | $111.4k | 6/28/24 |