Project Grant 2609790
- This Project Grant from the National Science Foundation's Mathematical and Physical Sciences program, totaling $173,064, supports research at Barry University from July 1, 2022 to June 30, 2024. The awardee, Barry University, will construct new particle physics models to solve outstanding problems in dark matter, matter-antimatter asymmetry, and neutrino masses. These models can be tested using gravitational wave experiments to gain insight into the very early universe before one trillionth of a...
- The National Science Foundation (NSF) awarded a $900,000 Project Grant to the University of Florida to conduct research supporting future gravitational-wave observatories under the NSF's "Windows on the Universe" Big Idea program. The research aims to contribute improvements to current LIGO detectors as well as develop technologies for third-generation gravitational-wave observatories. Key focus areas include high-power optical isolation, laser modulation, and suspension simulations...
- 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, valued at $660,000.00, was issued by the National Science Foundation (NSF) under the Mathematical and Physical Sciences (CFDA 47.049) federal grant program. The award supports research at the University of Florida on wide-ranging searches for gravitational wave sources using the Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors. The research aims to advance scientific understanding of relativistic astrophysical systems, black holes, neutron stars, and...
- This $210,000 Project Grant awarded by the National Science Foundation (CFDA 47.049 - Mathematical and Physical Sciences) supports research by the University of Virginia to advance gravitational wave physics and astrophysics. The key goals are to: (i) Compute persistent gravitational wave signals from binary black hole mergers using new conservation law models, and assess their detection prospects. (ii) Improve modeling of the gravitational wave memory effect to better understand its...
- This Project Grant award from the National Science Foundation (NSF) Mathematical and Physical Sciences (CFDA 47.049) program provides $139,844 to American University to develop and characterize AlGaAs coatings for gravitational-wave detectors. The goal is to improve the mirrors used in the Laser Interferometer Gravitational-Wave Observatory (LIGO) to enable more frequent and sensitive detection of gravitational waves, which can help advance our understanding of the universe and test theories...
- The University of Florida was awarded a $719,999 Project Grant from the National Science Foundation to conduct searches for gravitational wave transients from September 1, 2021 through August 31, 2024. The grant was awarded under the NSF's Mathematical and Physical Sciences program (CFDA 47.049), which supports progress in these scientific fields and enhances understanding of major problems facing the nation. Specifically, the University will use the funding to analyze data for the Laser...
- This National Science Foundation (NSF) Project Grant, awarded under the Mathematical and Physical Sciences Program (CFDA 47.049), is providing $100,000 to support the development and characterization of AlGaAs coatings for LIGO gravitational-wave detectors. The goal is to improve the mirrors in the laser-based LIGO system, enabling more frequent and higher quality observations of gravitational wave events. This research will help advance the understanding of the universe, including mysteries...
- 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 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....
RUI: PROBING GAUGE EXTENSIONS OF THE STANDARD MODEL WITH PRIMORDIAL GRAVITATIONAL WAVES -THIS AWARD FUNDS THE RESEARCH ACTIVITIES OF PROFESSOR BARTOSZ FORNAL AT BARRY UNIVERSITY, MIAMI, FL. THE FIRST DETECTION OF GRAVITATIONAL WAVES BY THE LASER INTERFEROMETER GRAVITATIONAL-WAVE OBSERVATORY (LIGO) IN 2015 MARKED THE BEGINNING OF A NEW ERA IN GRAVITATIONAL WAVE ASTRONOMY. ALTHOUGH THUS FAR ONLY SIGNALS FROM BLACK HOLE AND NEUTRON STAR MERGERS HAVE BEEN OBSERVED, MANY COSMOLOGICAL PROCESSES THAT OCCURRED WITHIN A FRACTION OF A SECOND AFTER THE BIG BANG ARE EXPECTED TO HAVE PRODUCED A STOCHASTIC GRAVITATIONAL-WAVE SIGNAL CONTINUOUSLY PASSING THROUGH US TODAY, CARRYING INFORMATION ABOUT THE PHYSICS AT THE EARLIEST TIMES. THIS PRIMORDIAL GRAVITATIONAL-WAVE BACKGROUND MAY HOLD THE KEY TO DISCOVERING THE FUNDAMENTAL LAWS GOVERNING NATURE AT THE HIGHEST ENERGIES, UNDERSTANDING HOW MATTER IN THE UNIVERSE CAME TO DOMINATE OVER ANTIMATTER, AND UNCOVERING THE NATURE OF DARK MATTER. AS A RESULT, RESEARCH IN THIS AREA ADVANCES THE NATIONAL INTEREST BY PROMOTING THE PROGRESS OF SCIENCE IN ONE OF ITS MOST FUNDAMENTAL DIRECTIONS: THE DISCOVERY AND UNDERSTANDING OF NEW PHYSICAL LAW. IN HIS RESEARCH, PROFESSOR FORNAL WILL DEVELOP NEW STRATEGIES FOR USING GRAVITATIONAL-WAVE OBSERVATIONS TO TEST PARTICLE-PHYSICS THEORIES WITH EXTENDED SYMMETRIES AT HIGH ENERGIES THAT ADDRESS OUTSTANDING QUESTIONS IN FUNDAMENTAL PHYSICS. THIS PROJECT IS ALSO ENVISIONED TO HAVE SIGNIFICANT BROADER IMPACTS. PROFESSOR FORNAL WILL INVOLVE UNDERGRADUATE STUDENTS IN HIS RESEARCH, PROVIDING THEM WITH THE NECESSARY SKILLS AND EXPERIENCE TO BECOME FUTURE RESEARCHERS. THEY WILL PRESENT THEIR RESEARCH RESULTS AT CONFERENCES AND MEETINGS OF THE AMERICAN PHYSICAL SOCIETY, PROVIDING VALUABLE OPPORTUNITIES FOR SCIENTIFIC EXCHANGE AND CAREER DEVELOPMENT. PROFESSOR FORNAL WILL ALSO DEVELOP NEW COURSE CURRICULA BASED ON THE RESULTS OF THIS RESEARCH, AS WELL AS CONDUCT OUTREACH ACTIVITIES AT LOCAL SCHOOLS AND ORGANIZE EVENTS FOR THE GENERAL PUBLIC. MORE TECHNICALLY, PROFESSOR FORNAL AND HIS STUDENTS WILL INVESTIGATE GRAVITATIONAL WAVE SIGNATURES OF EARLY-UNIVERSE SYMMETRY-BREAKING PHASE TRANSITIONS WITHIN THE FRAMEWORK OF WELL-MOTIVATED BEYOND-STANDARD MODEL THEORIES WITH EXTENDED GAUGE STRUCTURES. PARTICULAR ATTENTION WILL BE GIVEN TO ADDITIONAL SPECTRAL FEATURES ARISING FROM DOMAIN-WALL ANNIHILATION AND SYMMETRY-RESTORING PHASE TRANSITIONS DURING REHEATING. THE RESEARCH WILL ENCOMPASS MODELS WITH GAUGED BARYON AND LEPTON NUMBER, GRAND UNIFICATION, AND GAUGED FLAVOR SYMMETRIES. THE MODELS CONSIDERED WILL ACCOMMODATE DARK MATTER, EXPLAIN THE MATTER-ANTIMATTER ASYMMETRY OF THE UNIVERSE, INCLUDE MECHANISMS FOR GENERATING NEUTRINO MASSES, AND SHED LIGHT ON THE REHEATING EPOCH. THE PREDICTED SIGNALS WILL BE EXPLORED THROUGH MULTI-MESSENGER ASTROPHYSICAL OBSERVATIONS, CREATING NEW SYNERGIES BETWEEN PARTICLE PHYSICS, GRAVITATIONAL-WAVE ASTRONOMY, AND ASTROPHYSICS WHILE HELPING GUIDE THE OPTIMAL DESIGN OF FUTURE GRAVITATIONAL-WAVE DETECTORS. 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 | $80.0k | 8/10/26 |