Magnetic structure of light nuclei from lattice QCD
Lattice QCD with background magnetic fields is used to calculate the magnetic moments and magnetic polarizabilities of the nucleons and of light nuclei with A ≤ 4, along with the cross section for the M1 transition np → dγ, at the flavor SU(3)-symmetric point where the pion mass is m[subscript π] ∼...
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American Physical Society
2015
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Online Access: | http://hdl.handle.net/1721.1/100451 https://orcid.org/0000-0002-0400-8363 |
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author | Chang, Emmanuel Detmold, William Orginos, Kostas Savage, Martin J. Tiburzi, Brian C. Beane, Silas R. Parreno, Assumpta |
author2 | Massachusetts Institute of Technology. Center for Theoretical Physics |
author_facet | Massachusetts Institute of Technology. Center for Theoretical Physics Chang, Emmanuel Detmold, William Orginos, Kostas Savage, Martin J. Tiburzi, Brian C. Beane, Silas R. Parreno, Assumpta |
author_sort | Chang, Emmanuel |
collection | MIT |
description | Lattice QCD with background magnetic fields is used to calculate the magnetic moments and magnetic polarizabilities of the nucleons and of light nuclei with A ≤ 4, along with the cross section for the M1 transition np → dγ, at the flavor SU(3)-symmetric point where the pion mass is m[subscript π] ∼ 806 MeV. These magnetic properties are extracted from nucleon and nuclear energies in six uniform magnetic fields of varying strengths. The magnetic moments are presented in a recent article [S. Beane et al., Phys. Rev. Lett. 113, 252001 (2014)]. For the charged states, the extraction of the polarizability requires careful treatment of Landau levels, which enter nontrivially in the method that is employed. The nucleon polarizabilities are found to be of similar magnitude to their physical values, with β[subscript p] = 5.22([+0.66 over -0.45])(0.23) × 10[superscript -4] fm[superscript 3] and β[subscript n] = 1.253([+0.056 over -0.067])(0.055) × 10[superscript -4] fm[superscript 3], exhibiting a significant isovector component. The dineutron is bound at these heavy quark masses, and its magnetic polarizability, β[subscript nn] = 1.872([+0.121 over -0.113])(0.082) × 10[superscxript -4] fm[superscript 3], differs significantly from twice that of the neutron. A linear combination of deuteron scalar and tensor polarizabilities is determined by the energies of the j[subscript z] = ±1 deuteron states and is found to be β[subscript d,±1] = 4.4([+1.6 over -1.5])(0.2) × 10[superscript -4] fm[superscript 3]. The magnetic polarizabilities of the three-nucleon and four-nucleon systems are found to be positive and similar in size to those of the proton, β[subscript 3]subscript He] = 5.4([+2.2 over -2.1])(0.2) × 10[superscript -4] fm[superscript 3], β[subscript 3]subscript H] = 2.6(1.7)(0.1) × 10[superscript -4] fm[superscript 3], and β[subscript 4]subscript He] = 3.4([+2.0 over -1.9])(0.2) × 10[superscript -4] fm[superscript 3]. Mixing between the j[subscript z] = 0 deuteron state and the spin-singlet np state induced by the background magnetic field is used to extract the short-distance two-nucleon counterterm, [bar over L][subscript 1], of the pionless effective theory for NN systems (equivalent to the meson-exchange current contribution in nuclear potential models) that dictates the cross section for the np → dγ process near threshold. Combined with previous determinations of NN scattering parameters, this enables an ab initio determination of the threshold cross section at these unphysical masses. |
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spelling | mit-1721.1/1004512022-09-27T17:51:09Z Magnetic structure of light nuclei from lattice QCD Chang, Emmanuel Detmold, William Orginos, Kostas Savage, Martin J. Tiburzi, Brian C. Beane, Silas R. Parreno, Assumpta Massachusetts Institute of Technology. Center for Theoretical Physics Massachusetts Institute of Technology. Department of Physics Detmold, William Lattice QCD with background magnetic fields is used to calculate the magnetic moments and magnetic polarizabilities of the nucleons and of light nuclei with A ≤ 4, along with the cross section for the M1 transition np → dγ, at the flavor SU(3)-symmetric point where the pion mass is m[subscript π] ∼ 806 MeV. These magnetic properties are extracted from nucleon and nuclear energies in six uniform magnetic fields of varying strengths. The magnetic moments are presented in a recent article [S. Beane et al., Phys. Rev. Lett. 113, 252001 (2014)]. For the charged states, the extraction of the polarizability requires careful treatment of Landau levels, which enter nontrivially in the method that is employed. The nucleon polarizabilities are found to be of similar magnitude to their physical values, with β[subscript p] = 5.22([+0.66 over -0.45])(0.23) × 10[superscript -4] fm[superscript 3] and β[subscript n] = 1.253([+0.056 over -0.067])(0.055) × 10[superscript -4] fm[superscript 3], exhibiting a significant isovector component. The dineutron is bound at these heavy quark masses, and its magnetic polarizability, β[subscript nn] = 1.872([+0.121 over -0.113])(0.082) × 10[superscxript -4] fm[superscript 3], differs significantly from twice that of the neutron. A linear combination of deuteron scalar and tensor polarizabilities is determined by the energies of the j[subscript z] = ±1 deuteron states and is found to be β[subscript d,±1] = 4.4([+1.6 over -1.5])(0.2) × 10[superscript -4] fm[superscript 3]. The magnetic polarizabilities of the three-nucleon and four-nucleon systems are found to be positive and similar in size to those of the proton, β[subscript 3]subscript He] = 5.4([+2.2 over -2.1])(0.2) × 10[superscript -4] fm[superscript 3], β[subscript 3]subscript H] = 2.6(1.7)(0.1) × 10[superscript -4] fm[superscript 3], and β[subscript 4]subscript He] = 3.4([+2.0 over -1.9])(0.2) × 10[superscript -4] fm[superscript 3]. Mixing between the j[subscript z] = 0 deuteron state and the spin-singlet np state induced by the background magnetic field is used to extract the short-distance two-nucleon counterterm, [bar over L][subscript 1], of the pionless effective theory for NN systems (equivalent to the meson-exchange current contribution in nuclear potential models) that dictates the cross section for the np → dγ process near threshold. Combined with previous determinations of NN scattering parameters, this enables an ab initio determination of the threshold cross section at these unphysical masses. United States. Dept. of Energy (Early Career Research Award DE-SC001049) 2015-12-21T15:08:00Z 2015-12-21T15:08:00Z 2015-12 2015-08 2015-12-09T23:00:05Z Article http://purl.org/eprint/type/JournalArticle 1550-7998 1550-2368 http://hdl.handle.net/1721.1/100451 Chang, Emmanuel, William Detmold, Kostas Orginos, Assumpta Parreno, Martin J. Savage, Brian C. Tiburzi, and Silas R. Beane. "Magnetic structure of light nuclei from lattice QCD." Phys. Rev. D 92, 114502 (December 2015). © 2015 American Physical Society https://orcid.org/0000-0002-0400-8363 en http://dx.doi.org/10.1103/PhysRevD.92.114502 Physical Review D Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. American Physical Society application/pdf American Physical Society American Physical Society |
spellingShingle | Chang, Emmanuel Detmold, William Orginos, Kostas Savage, Martin J. Tiburzi, Brian C. Beane, Silas R. Parreno, Assumpta Magnetic structure of light nuclei from lattice QCD |
title | Magnetic structure of light nuclei from lattice QCD |
title_full | Magnetic structure of light nuclei from lattice QCD |
title_fullStr | Magnetic structure of light nuclei from lattice QCD |
title_full_unstemmed | Magnetic structure of light nuclei from lattice QCD |
title_short | Magnetic structure of light nuclei from lattice QCD |
title_sort | magnetic structure of light nuclei from lattice qcd |
url | http://hdl.handle.net/1721.1/100451 https://orcid.org/0000-0002-0400-8363 |
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