used as one of the standard NPDFs for a long time. In the similar way, we studied global
analyses of longitudinally polarized PDFs [19] and fragmentation functions [20], and created
useful codes for calculating them at given x and Q
2
.
[16] Determination of nuclear parton distributions,
M. Hirai, S. Kumano, and M. Miyama, Phys. Rev. D 64 (2001) 034003.
[17] Nuclear parton distribution functions and their uncertainties,
M. Hirai, S. Kumano, and T.-H. Nagai, Phys. Rev. C 70 (2004) 044905.
[18] Determination of nuclear parton distribution functions and their uncertainties in next-to
-leading order, M. Hirai, S. Kumano, and T.-H. Nagai, Phys. Rev. C 76 (2007) 065207.
[19] Global analyses of polarized PDFs: Y. Goto et al., Phys. Rev. D 62 (2000) 034017;
M. Hirai, S. Kumano, and N. Saito, Phys. Rev. D 69 (2004) 054021; D 74 (2006) 014015;
M. Hirai and S. Kumano, Nucl. Phys. B 813 (2009) 106.
[20] Global analyses of fragmentation functions: M. Hirai, S. Kumano, T.-H. Nagai, and
K. Sudoh, Phys. Rev. D 75 (2007) 094009; M. Hirai, H. Kawamura, S. Kumano, and
K. Saito, PTEP 2016 (2016) 113B04; N. Sato et al., Phys. Rev. D 94 (2016) 114004.
Gravitational form factors of a hadron
Since gravitational interactions are too weak to be measured in microscopic systems, the
measurement of the gravitational form factors used to be considered impossible for hadrons and
nuclei. However, we know generalized parton distributions (GPDs) and generalized distribution
amplitudes (GDAs) contain matrix elements of energy-momentum tensor, which is a source of
gravity within a hadron. Here, the GDAs are s-t crossed quantities of the GPDs, so that they
could be called timelike GPDs. The spacelike GPDs are measured in virtual Compton scattering
at lepton-accelerator facilities, but it is also possible to investigate them by using exclusive
hadron reactions at hadron-accelerator facilities [21]. We extracted the gravitational form factors
for the first time from actual experimental measurements [22]. In our work, we extracted the
GDAs, which are s-t crossed quantities of the GPDs, from cross-section measurements of hadron-
pair production process γ
∗
γ → π
0
π
0
at KEKB. The GDAs were expressed by a number of
parameters and they were determined from the data of γ
∗
γ → π
0
π
0
. The timelike gravitational
form factors Θ
1
and Θ
2
were obtained from our GDAs, and they were converted to the spacelike
ones by the dispersion relation. From the spacelike Θ
1
and Θ
2
, gravitational densities of the
pion were calculated. Then, we obtained the mass (energy) radius and the mechanical (pressure
and shear force) radius from Θ
2
and Θ
1
, respectively. They were calculated as
√
⟨r
2
⟩
mass
=
0.32 ∼ 0.39 fm, whereas the mechanical radius was larger
√
⟨r
2
⟩
mech
= 0.82 ∼ 0.88 fm. This is
the first report on the gravitational radius of a hadron from actual experimental measurements
[22]. It is interesting to find the possibility that the gravitational mass and mechanical radii
could be different from the experimental charge radius
√
⟨r
2
⟩
charge
= 0.672 ± 0.008 fm for the
charged pion. Gravitational physics used to be considered as a field on macroscopic world.
However, we showed that it is p ossible to investigate it in the microscopic level in terms of
fundamental particles of quarks and gluons. In future, we expect much progress on origin of
hadron masses and internal hadron pressures in terms of quark and gluon degrees of freedom.
This work together with our studies on the gluon transversity [23] was selected one of highlight
research results of KEK in the annual report of 2019.
[21] GPDs at hadron-accelerator facilities: S. Kumano, M. Strikman, and K. Sudoh,
Phys. Rev. D 80 (2009) 074003; T. Sawada et al., Phys. Rev. D 93 (2016) 114034.
[22] Hadron tomography by generalized distribution amplitudes in pion-pair production process
γ
∗
γ → π
0
π
0
and gravitational form factors for pion, S. Kumano, Qin-Tao Song, and
O. V. Teryaev, Phys. Rev. D 97 (2018) 014020.
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