Award Abstract # 2116686
Nuclear Physics from Multi-Messenger Mergers (NP3M)

NSF Org: PHY
Division Of Physics
Recipient: UNIVERSITY OF TENNESSEE
Initial Amendment Date: July 30, 2021
Latest Amendment Date: August 21, 2025
Award Number: 2116686
Award Instrument: Cooperative Agreement
Program Manager: Bogdan Mihaila
bmihaila@nsf.gov
 (703)292-8235
PHY
 Division Of Physics
MPS
 Directorate for Mathematical and Physical Sciences
Start Date: August 1, 2021
End Date: July 31, 2026 (Estimated)
Total Intended Award Amount: $3,250,000.00
Total Awarded Amount to Date: $3,250,000.00
Funds Obligated to Date: FY 2021 = $1,250,000.00
FY 2022 = $2,000,000.00
History of Investigator:
  • William Hix (Principal Investigator)
    raph@utk.edu
  • Charles Horowitz (Co-Principal Investigator)
  • Duncan Brown (Co-Principal Investigator)
  • Claudia Ratti (Co-Principal Investigator)
  • David Radice (Co-Principal Investigator)
  • Andrew Steiner (Former Principal Investigator)
Recipient Sponsored Research Office: University of Tennessee Knoxville
201 ANDY HOLT TOWER
KNOXVILLE
TN  US  37996-0001
(865)974-3466
Sponsor Congressional District: 02
Primary Place of Performance: University of Tennessee Knoxville
1 Circle Park
Knoxville
TN  US  37996-0003
Primary Place of Performance
Congressional District:
02
Unique Entity Identifier (UEI): FN2YCS2YAUW3
Parent UEI: LXG4F9K8YZK5
NSF Program(s): WoU-Windows on the Universe: T,
PHYSICS AT THE INFO FRONTIER,
NUCLEAR THEORY
Primary Program Source: 01002425DB NSF RESEARCH & RELATED ACTIVIT
01002122DB NSF RESEARCH & RELATED ACTIVIT

01002223DB NSF RESEARCH & RELATED ACTIVIT

01002324DB NSF RESEARCH & RELATED ACTIVIT

01002526DB NSF RESEARCH & RELATED ACTIVIT

01002223DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 7569, 7483, 069Z
Program Element Code(s): 107y00, 755300, 128500
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.049

ABSTRACT

The goal of the Nuclear Physics from Multi-Messenger Mergers (NP3M) Focus Research Hub is to create a national effort in nuclear physics and astrophysical simulations to systematically probe the properties of hot and dense strongly interacting matter with multi-messenger observations of neutron stars. Neutron star mergers probe the nature of matter at densities and temperatures far beyond those present in atomic nuclei. The NP3M Hub will form a new interdisciplinary collaboration across nuclear physics, astrophysics, and gravitational-wave physics to drive the coordinated advances in each of these sub-fields needed to interpret observations. The NP3M Hub will develop theoretical models of dense and hot matter to connect multi-messenger observations of neutron stars to the underlying merger dynamics by means of numerical simulations. Hub members will lead a coordinated effort to study the impact of theoretical uncertainties in the nuclear physics and the numerical modeling on the prediction of multi-messenger signals from merging neutron stars (end-to-end). They will lead a parallel effort to back propagate observational constraints to nuclear physics, connecting astronomical observations with laboratory results.

The Nuclear Physics of Multi-Messenger Mergers (NP3M) collaboration is comprised of researchers across the US and aims to understand how atomic nuclei and the interactions between neutrons and protons impact the merger of two neutron stars. The evolution of neutron stars, the compact stellar objects which are the final stage in the evolution of stars between about 8 and 20 times the mass of the sun, is controlled by nuclear physics. Some neutron stars in our universe are created in pairs, and these pairs of neutron stars eventually merge in a cataclysmic event which emits gravitational waves, neutrinos, and photons, creating either a more massive neutron star or a black hole. These mergers are the likely origin of a significant fraction of the atomic nuclei heavier than iron which are present on earth. This grant supports the training of early-career scientists who will work on different aspects of this problem. The NP3M hub will create pages and videos that discuss how any new discoveries in multi-messenger astronomy impact nuclear astrophysics. The hub will develop a curriculum on nuclear physics and multi-messenger astronomy for K-12 educators, and host two summer schools that will educate students in hub-related science.

This project advances the objectives of "Windows on the Universe: the Era of Multi-Messenger Astrophysics", one of the 10 Big Ideas for Future NSF Investments.

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.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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(Showing: 1 - 10 of 58)
Cusinato, Marco and Guercilena, Federico Maria and Perego, Albino and Logoteta, Domenico and Radice, David and Bernuzzi, Sebastiano and Ansoldi, Stefano "Neutrino emission from binary neutron star mergers: characterising light curves and mean energies" The European Physical Journal A , v.58 , 2022 https://doi.org/10.1140/epja/s10050-022-00743-5 Citation Details
Camilletti, Alessandro and Chiesa, Leonardo and Ricigliano, Giacomo and Perego, Albino and Lippold, Lukas Chris and Padamata, Surendra and Bernuzzi, Sebastiano and Radice, David and Logoteta, Domenico and Guercilena, Federico Maria "Numerical relativity simulations of the neutron star merger GW190425: microphysics and mass ratio effects" Monthly Notices of the Royal Astronomical Society , v.516 , 2022 https://doi.org/10.1093/mnras/stac2333 Citation Details
Camilletti, Alessandro and Perego, Albino and Guercilena, Federico_Maria and Bernuzzi, Sebastiano and Radice, David "Geometric and thermodynamic characterization of binary neutron star accretion discs" Physical Review D , v.109 , 2024 https://doi.org/10.1103/PhysRevD.109.063023 Citation Details
Curtis, Sanjana and Mösta, Philipp and Wu, Zhenyu and Radice, David and Roberts, Luke and Ricigliano, Giacomo and Perego, Albino "r -process nucleosynthesis and kilonovae from hypermassive neutron star post-merger remnants" Monthly Notices of the Royal Astronomical Society , v.518 , 2022 https://doi.org/10.1093/mnras/stac3128 Citation Details
Saito, Yukiya and Dillmann, I. and Krücken, R. and Mumpower, M_R and Surman, R. "Uncertainty quantification of mass models using ensemble Bayesian model averaging" Physical Review C , v.109 , 2024 https://doi.org/10.1103/PhysRevC.109.054301 Citation Details
Somasundaram, R and Lynn, J E and Huth, L and Schwenk, A and Tews, I "Maximally local two-nucleon interactions at fourth order in delta-less chiral effective field theory" Physical Review C , v.109 , 2024 https://doi.org/10.1103/PhysRevC.109.034005 Citation Details
Suleiman, Lami and Oertel, Micaela and Mancini, Marco "Modified Urca neutrino emissivity at finite temperature" Physical Review C , v.108 , 2023 https://doi.org/10.1103/PhysRevC.108.035803 Citation Details
Suleiman, Lami and Read, Jocelyn "Quasiuniversal relations in the context of future neutron star detections" Physical Review D , v.109 , 2024 https://doi.org/10.1103/PhysRevD.109.103029 Citation Details
Sur, Ankan and Cook, William and Radice, David and Haskell, Brynmor and Bernuzzi, Sebastiano "Long-term general relativistic magnetohydrodynamics simulations of magnetic field in isolated neutron stars" Monthly Notices of the Royal Astronomical Society , v.511 , 2022 https://doi.org/10.1093/mnras/stac353 Citation Details
Ujevic, Maximiliano and Somasundaram, Rahul and Dietrich, Tim and Margueron, Jerome and Tews, Ingo "What Can We Learn about the Unstable Equation-of-state Branch from Neutron Star Mergers?" The Astrophysical Journal Letters , v.962 , 2024 https://doi.org/10.3847/2041-8213/ad2072 Citation Details
Wu, Zhenyu and Ricigliano, Giacomo and Kashyap, Rahul and Perego, Albino and Radice, David "Radiation hydrodynamics modelling of kilonovae with SNEC" Monthly Notices of the Royal Astronomical Society , v.512 , 2022 https://doi.org/10.1093/mnras/stac399 Citation Details
(Showing: 1 - 10 of 58)

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