Gravitational form factors and mechanical properties of the nucleon in a meson dominance approach

We analyze the gravitational form factors and mechanical properties of the nucleon, focusing both on some general issues, as well as on modeling with meson dominance. We show that the lattice QCD results for the nucleon gravitational form factors at <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>m</a:mi><a:mi>π</a:mi></a:msub><a:mo>=</a:mo><a:mn>170</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi>MeV</a:mi></a:math>, available for spacelike momentum transfer squared up to 2 GeV, are explained in a natural way within the meson dominance approach. We carry out the proper Raman spin decomposition of the energy-momentum tensor and in each spin channel use a minimum number of resonances consistent with the perturbative QCD short-distance constraints. These constraints are related to the superconvergence sum rules, following from the asymptotic perturbative QCD falloff of the form factors. The value of the nucleon <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>D</c:mi></c:math>-term following from the fits is <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mo>−</e:mo><e:mn>3.0</e:mn><e:mo stretchy="false">(</e:mo><e:mn>4</e:mn><e:mo stretchy="false">)</e:mo></e:math>. Next, we obtain the two-dimensional transverse gravitational densities of the nucleon in the transverse coordinate <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mi>b</i:mi></i:math>. With the superconvergence sum rules, we derive new sum rules for these densities at the origin and for their derivatives, involving logarithmic weighting in the corresponding spectral density integrals. From analysis of the threshold behavior in the timelike region and the properties of the <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mi>π</k:mi><k:mi>π</k:mi><k:mo stretchy="false">→</k:mo><k:mi>N</k:mi><k:mover accent="true"><k:mi>N</k:mi><k:mo stretchy="false">¯</k:mo></k:mover></k:math> reaction, we infer the behavior of the transverse densities at asymptotically large coordinates. We also carry out the meson dominance analysis of the two- and three-dimensional mechanical properties of the nucleon (the pressure and stress) and explore their connection to the spectral densities via dispersion relations.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-08-13
DOI
https://doi.org/10.1103/ylml-mrlh
Citations
7
Primary Topic
Geochemistry and Geologic Mapping
Type
article
Field-Weighted Citation Impact
17.37
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article

Gravitational form factors and mechanical properties of the nucleon in a meson dominance approach

7 citations
Physical review. D/Physical review. D.
Geochemistry and Geologic Mapping
17.37
article

Gravitational form factors and mechanical properties of the nucleon in a meson dominance approach

article en
7 citations

Abstract

We analyze the gravitational form factors and mechanical properties of the nucleon, focusing both on some general issues, as well as on modeling with meson dominance. We show that the lattice QCD results for the nucleon gravitational form factors at <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:msub><a:mi>m</a:mi><a:mi>π</a:mi></a:msub><a:mo>=</a:mo><a:mn>170</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi>MeV</a:mi></a:math>, available for spacelike momentum transfer squared up to 2 GeV, are explained in a natural way within the meson dominance approach. We carry out the proper Raman spin decomposition of the energy-momentum tensor and in each spin channel use a minimum number of resonances consistent with the perturbative QCD short-distance constraints. These constraints are related to the superconvergence sum rules, following from the asymptotic perturbative QCD falloff of the form factors. The value of the nucleon <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"><c:mi>D</c:mi></c:math>-term following from the fits is <e:math xmlns:e="http://www.w3.org/1998/Math/MathML" display="inline"><e:mo>−</e:mo><e:mn>3.0</e:mn><e:mo stretchy="false">(</e:mo><e:mn>4</e:mn><e:mo stretchy="false">)</e:mo></e:math>. Next, we obtain the two-dimensional transverse gravitational densities of the nucleon in the transverse coordinate <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:mi>b</i:mi></i:math>. With the superconvergence sum rules, we derive new sum rules for these densities at the origin and for their derivatives, involving logarithmic weighting in the corresponding spectral density integrals. From analysis of the threshold behavior in the timelike region and the properties of the <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mi>π</k:mi><k:mi>π</k:mi><k:mo stretchy="false">→</k:mo><k:mi>N</k:mi><k:mover accent="true"><k:mi>N</k:mi><k:mo stretchy="false">¯</k:mo></k:mover></k:math> reaction, we infer the behavior of the transverse densities at asymptotically large coordinates. We also carry out the meson dominance analysis of the two- and three-dimensional mechanical properties of the nucleon (the pressure and stress) and explore their connection to the spectral densities via dispersion relations.

Physical review. D/Physical review. D.Vol. 112(5)
Jan Kochanowski University (PL), Universidad de Granada (ES), Institute of Nuclear Physics (UZ)
Openalex Percentile: Top 1%
Geochemistry and Geologic Mapping
17.37
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