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Inferring three-nucleon couplings from multi-messenger neutron-star observations
Rahul Somasundaram1,2, Isak Svensson3,4,5, Soumi De6
1Department of Physics, Syracuse University, Syracuse, NY, USA. rsomasundaram@lanl.gov.
This study links neutron star observations to nuclear physics, constraining three-nucleon interactions in dense matter. Future observations promise even tighter constraints on these fundamental couplings.
Area of Science:
- Nuclear Physics
- Astrophysics
- Theoretical Physics
Background:
- Understanding nucleon interactions in dense matter is crucial for nuclear physics.
- Effective field theories are key for low-energy nuclear interactions.
- The applicability of these theories within neutron stars remains an open question.
Purpose of the Study:
- Develop a framework to infer three-nucleon couplings from neutron star observations.
- Connect microscopic quantum field theory couplings to macroscopic astrophysical data.
- Test consistency between terrestrial and astrophysical measurements of nuclear interactions.
Main Methods:
- Developed a novel framework for inferring three-nucleon couplings.
- Applied the framework to LIGO/Virgo event GW170817 and Neutron Star Interior Composition Explorer (NICER) data.
- Utilized chiral effective field theory for describing nuclear interactions.
Main Results:
- Established direct constraints on three-nucleon couplings in dense matter.
- Demonstrated the potential of future neutron star merger observations for stringent coupling constraints.
- Showcased a method to link microscopic couplings to macroscopic neutron star properties.
Conclusions:
- Successfully connected quantum field theory couplings to astrophysical observations.
- Provided a pathway to test consistency between low-energy nuclear couplings from different data sources.
- Highlighted the power of astrophysical observations in constraining fundamental nuclear physics.
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