Abstract
We present a computational approach to infinite nuclear matter employing Hartree-Fock theory, many-body perturbation theory and coupled cluster theory. These lectures are closely linked with those of Chaps. 9, 10 and 11 and serve as input for the correlation functions employed in Monte Carlo calculations in Chap. 9, the in-medium similarity renormalization group theory of dense fermionic systems of Chap. 10 and the Green’s function approach in Chap. 11 We provide extensive code examples and benchmark calculations, allowing thereby an eventual reader to start writing her/his own codes. We start with an object-oriented serial code and end with discussions on strategies for porting the code to present and planned high-performance computing facilities.
Original language | English |
---|---|
Title of host publication | Lecture Notes in Physics |
Publisher | Springer Verlag |
Pages | 293-399 |
Number of pages | 107 |
DOIs | |
State | Published - 2017 |
Publication series
Name | Lecture Notes in Physics |
---|---|
Volume | 936 |
ISSN (Print) | 0075-8450 |
Funding
We are much indebted to Carlo Barbieri, Scott Bogner, Alex Brown, David Dean, Heiko Hergert, Dean Lee, Titus Morris, Thomas Papenbrock, Nathan Parzuchowski, Piotr Piecuch and Fei Yuan for many discussions on many-body theory. Computational resources were provided by Michigan State University and the Norwegian Notur project (Supercomputing grant NN2977K). This work was supported by NSF Grant No. PHY-1404159 (Michigan State University), by the Oce of Nuclear Physics, U.S. Department of Energy, under grants DE-FG02-96ER40963, DE-SC0008499 (NUCLEI SciDAC collaboration) and the Field Work Proposal ERKBP57 at Oak Ridge National Laboratory (ORNL). This research used also resources of the Oak Ridge Leadership Computing Facility located at ORNL, which is supported by the Office of Science of the Department of Energy under Contract No. DE-AC05-00OR22725. This manuscript has been authored by UT-Battelle, LLC under Contract No. DE-AC05-00OR22725 with the U.S. Department of Energy. The U.S. Government retains a nonexclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for U.S. Government purposes. The views and conclusions contained herein are those of the authors and should not be interpreted as necessarily representing the official policies or endorsements, either expressed or implied, of the U.S. Government or any U.S. Government agency. The Department of Energy will provide public access to these results of federally sponsored research in accordance with the DOE Public Access Plan.