Uncertainty quantification for proton–proton fusion in chiral effective field theory

B. Acharya, B. D. Carlsson, A. Ekström, C. Forssén, L. Platter

Research output: Contribution to journalArticlepeer-review

31 Scopus citations

Abstract

We compute the S-factor of the proton–proton (pp) fusion reaction using chiral effective field theory (χEFT) up to next-to-next-to-leading order (NNLO) and perform a rigorous uncertainty analysis of the results. We quantify the uncertainties due to (i) the computational method used to compute the pp cross section in momentum space, (ii) the statistical uncertainties in the low-energy coupling constants of χEFT, (iii) the systematic uncertainty due to the χEFT cutoff, and (iv) systematic variations in the database used to calibrate the nucleon–nucleon interaction. We also examine the robustness of the polynomial extrapolation procedure, which is commonly used to extract the threshold S-factor and its energy-derivatives. By performing a statistical analysis of the polynomial fit of the energy-dependent S-factor at several different energy intervals, we eliminate a systematic uncertainty that can arise from the choice of the fit interval in our calculations. In addition, we explore the statistical correlations between the S-factor and few-nucleon observables such as the binding energies and point-proton radii of 2,3H and 3He as well as the D-state probability and quadrupole moment of 2H, and the β-decay of 3H. We find that, with the state-of-the-art optimization of the nuclear Hamiltonian, the statistical uncertainty in the threshold S-factor cannot be reduced beyond 0.7%.

Original languageEnglish
Pages (from-to)584-589
Number of pages6
JournalPhysics Letters B
Volume760
DOIs
StatePublished - Sep 10 2016
Externally publishedYes

Funding

We would like to thank Thomas Papenbrock, Doron Gazit, and Laura Marcucci for useful discussions. We are highly obliged to Laura Marcucci for sending us data to benchmark our codes with, and for providing valuable comments on the manuscript. This work was supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under Contract No. DE-AC05-00OR22725 , the National Science Foundation under Grant No. PHY-1516077 , the European Research Council under the European Community's Seventh Framework Programme ( FP7/2007-2013 )/ ERC Grant No. 240603 , and the Swedish Foundation for International Cooperation in Research and Higher Education (STINT, Grant No. IG2012-5158 ). Computations were performed on resources provided by the Swedish National Infrastructure for Computing (SNIC) at the National Supercomputer Centre (NSC).

FundersFunder number
National Science FoundationPHY-1516077
U.S. Department of Energy
Office of Science
Nuclear PhysicsDE-AC05-00OR22725
Seventh Framework Programme1516077, 240603
Engineering Research Centers
European Research Council
Swedish Foundation for International Cooperation in Research and Higher EducationIG2012-5158
Seventh Framework Programme

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