Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/125067
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Type: | Journal article |
Title: | Magnetic polarizability of the nucleon using a Laplacian mode projection |
Author: | Bignell, R. Kamleh, W. Leinweber, D. |
Citation: | Physical Review D, 2020; 101(9):094502-1-094502-17 |
Publisher: | American Physical Society |
Issue Date: | 2020 |
ISSN: | 2470-0010 2470-0029 |
Statement of Responsibility: | Ryan Bignell, Waseem Kamleh, and Derek Leinweber |
Abstract: | Conventional hadron interpolating fields, which utilize gauge-covariant Gaussian smearing, are ineffective in isolating ground state nucleons in a uniform background magnetic field. There is evidence that residual Landau-mode physics remains at the quark level, even when QCD interactions are present. In this work, quark-level projection operators are constructed from the SU(3)×U(1) eigenmodes of the two-dimensional lattice Laplacian operator associated with Landau modes. These quark-level modes are formed from a periodic finite lattice where both the background field and strong interactions are present. Using these eigenmodes, quark-propagator projection operators provide the enhanced hadronic energy-eigenstate isolation necessary for calculation of nucleon energy shifts in a magnetic field. The magnetic polarizability of both the proton and neutron is calculated using this method on the 323×64 dynamical QCD lattices provided by the PACS-CS Collaboration. A chiral effective-field theory analysis is used to connect the lattice QCD results to the physical regime, obtaining magnetic polarizabilities of βp=2.79(22)( +13−18)×10−4 fm3 and βn=2.06(26)( +15−20)×10−4 fm3, where the numbers in parentheses describe statistical and systematic uncertainties. |
Rights: | Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP³. |
DOI: | 10.1103/PhysRevD.101.094502 |
Grant ID: | http://purl.org/au-research/grants/arc/LE190100021 http://purl.org/au-research/grants/arc/LE160100051 http://purl.org/au-research/grants/arc/DP140103067 http://purl.org/au-research/grants/arc/DP150103164 http://purl.org/au-research/grants/arc/DP190102215 http://purl.org/au-research/grants/arc/DP190100297 |
Published version: | http://dx.doi.org/10.1103/physrevd.101.094502 |
Appears in Collections: | Aurora harvest 4 Physics publications |
Files in This Item:
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hdl_125067.pdf | Published version | 1.56 MB | Adobe PDF | View/Open |
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