The DOI matches its Crossref record; 25 of the 25 references it cites were found in a registry or an index.
Neutron Matter at Next-to-Next-to-Next-to-Leading Order in Chiral Effective Field Theory
Open accessAbstract
Neutron matter presents a unique system for chiral effective field theory because all many-body forces among neutrons are predicted to next-to-next-to-next-to-leading order (N(3)LO). We present the first complete N(3)LO calculation of the neutron matter energy. This includes the subleading three-nucleon forces for the first time and all leading four-nucleon forces. We find relatively large contributions from N(3)LO three-nucleon forces. Our results provide constraints for neutron-rich matter in astrophysics with controlled theoretical uncertainties.
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Cites
A two-solar-mass neutron star measured using Shapiro delay
Demorest, P. B., Pennucci, T., Ransom, S. M., Roberts, M. S. E., & Hessels, J. W. T. (2010) · Nature · doi:10.1038/nature09466 · Cited by 3,905
Equation of state of nucleon matter and neutron star structure
Akmal, A., Pandharipande, V. R., & Ravenhall, D. G. (1998) · Physical Review C · doi:10.1103/physrevc.58.1804 · Cited by 2,493
Modern theory of nuclear forces
Epelbaum, E., Hammer, H.-W., & Meißner, U.-G. (2009) · Reviews of Modern Physics · doi:10.1103/revmodphys.81.1773 · Cited by 1,883
Chiral effective field theory and nuclear forces
Machleidt, R., & Entem, D. R. (2011) · Physics Reports · doi:10.1016/j.physrep.2011.02.001 · Cited by 1,612
Accurate charge-dependent nucleon-nucleon potential at fourth order of chiral perturbation theory
Entem, D. R., & Machleidt, R. (2003) · Physical Review C · doi:10.1103/physrevc.68.041001 · Cited by 1,574
The two-nucleon system at next-to-next-to-next-to-leading order
Epelbaum, E., Glöckle, W., & Meißner, U.-G. (2005) · Nuclear Physics A · doi:10.1016/j.nuclphysa.2004.09.107 · Cited by 666
Improved nuclear matter calculations from chiral low-momentum interactions
Hebeler, K., Bogner, S. K., Furnstahl, R. J., Nogga, A., & Schwenk, A. (2011) · Physical Review C · doi:10.1103/physrevc.83.031301 · Cited by 585
Self-citationNuclear energy density optimization
Kortelainen, M., Lesinski, T., Moré, J., Nazarewicz, W., Sarich, J., Schunck, N., Stoitsov, M. V., & Wild, S. (2010) · Physical Review C · doi:10.1103/physrevc.82.024313 · Cited by 509
From low-momentum interactions to nuclear structurePreprint
Bogner, S. K., Furnstahl, R. J., & Schwenk, A. (2010) · Cited by 472
Self-citationMaximum mass and radius of neutron stars, and the nuclear symmetry energy
Gandolfi, S., Carlson, J., & Reddy, S. (2012) · Physical Review C · doi:10.1103/physrevc.85.032801 · Cited by 453
Metadata
- Authors
- Tews, I., Krüger, T., Hebeler, K., & Schwenk, A.
- Venue
- Physical Review Letters
- Publisher
- American Physical Society (APS)
- Published
- 2013-01-15
- Volume
- 110
- Issue
- 3
- Pages
- 032504-032504
- ISSN
- 0031-9007 (ISSN-L)
- 1079-7114
- OpenAlex
- W2169076560
- Cited by
- 409
- References
- 25
- FWCI
- 19.03
- Type
- journal article
- Language
- en
- Open access
- green
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- Tews, I., Krüger, T., Hebeler, K., & Schwenk, A. (2013). Neutron Matter at Next-to-Next-to-Next-to-Leading Order in Chiral Effective Field Theory. Physical Review Letters. https://doi.org/10.1103/physrevlett.110.032504
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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