Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory
arXiv:1206.0025 · doi:10.1103/PhysRevLett.110.032504
Abstract
Neutron matter presents a unique system for chiral effective field theory (EFT), because all many-body forces among neutrons are predicted to next-to-next-to-next-to-leading order (N3LO). We present the first complete N3LO calculation of the neutron matter energy. This includes the subleading three-nucleon (3N) forces for the first time and all leading four-nucleon (4N) forces. We find relatively large contributions from N3LO 3N forces. Our results provide constraints for neutron-rich matter in astrophysics with controlled theoretical uncertainties.
5 pages, 4 figures; improved version, 3N ring and 2pi-contact contributions corrected, conclusions unchanged; v3: minor changes, published version
References in corpus (7)
- Shapiro delay measurement of a two solar mass neutron star
- Chiral effective field theory and nuclear forces
- Improved nuclear matter calculations from chiral low-momentum interactions
- Constraints on neutron star radii based on chiral effective field theory interactions
- Subleading contributions to the chiral three-nucleon force I: long-range terms
- Improving the convergence of the chiral expansion for nuclear forces II: low phases and the deuteron
- Two-pion exchange three-nucleon potential: O(q^4) chiral expansion
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