Literature DB >> 23373917

Neutron matter at next-to-next-to-next-to-leading order in chiral effective field theory.

I Tews1, T Krüger, K Hebeler, A Schwenk.   

Abstract

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.

Year:  2013        PMID: 23373917     DOI: 10.1103/PhysRevLett.110.032504

Source DB:  PubMed          Journal:  Phys Rev Lett        ISSN: 0031-9007            Impact factor:   9.161


  1 in total

1.  Constraining neutron-star matter with microscopic and macroscopic collisions.

Authors:  Sabrina Huth; Peter T H Pang; Ingo Tews; Tim Dietrich; Arnaud Le Fèvre; Achim Schwenk; Wolfgang Trautmann; Kshitij Agarwal; Mattia Bulla; Michael W Coughlin; Chris Van Den Broeck
Journal:  Nature       Date:  2022-06-08       Impact factor: 69.504

  1 in total

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