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RhZhang, J. Z.*; Chen, Z. Q.*; Qu, T.*; Wang, Y. K.*; Li, Z. H.*; Orlandi, R.; 62 of others*
Physics Letters B, 873, p.140144_1 - 140144_9, 2026/02
Fujii, Daisuke; Tanaka, Mitsuru*
Physics Letters B, 870, p.139872_1 - 139872_7, 2025/11
We investigate how the QCD scale anomaly contributes to the internal pressure structure of hadrons, employing the decomposition of the energy-momentum tensor into its trace and traceless parts. By utilizing recent model-independent results for gravitational form factors, we analyze the pressure distributions of both pions and nucleons in the instant form and the light-front form. Our analysis reveals that, in all examined cases, the confining pressure is predominantly driven by the scale anomaly. This indicates that the dominance of the scale anomaly in generating internal pressure is a robust and universal feature, regardless of the specific hadron, theoretical model, or form used in the analysis.
Nguyen, T. H. T.; Sanami, Toshiya*; Yamazaki, Hirohito*; Iwamoto, Nobuyuki; Itoga, Toshiro*; Kirihara, Yoichi; Lee, E.*; Sugihara, Kenta*; Miyamoto, Shuji*; Hashimoto, Satoshi*; et al.
Physics Letters B, 870, p.139900_1 - 139900_8, 2025/11
Fujii, Daisuke; Nakayama, Katsumasa*; Suzuki, Kei
Physics Letters B, 868, p.139758_1 - 139758_6, 2025/09
The Lifshitz formula has long served as a foundational framework for analyzing the Casimir effect under finite-temperature conditions. In this work, we extend its applicability to situations involving finite chemical potential, thereby incorporating quantum field contributions beyond thermal effects. We illustrate the broad utility of the resulting generalized formula by exploring characteristic features of the Casimir effect across a variety of setups, including different boundary conditions, temperature regimes, spatial dimensionalities, and chemical potential imbalances. This extended framework is particularly relevant to systems such as dense quark matter and Dirac/Weyl semimetals, where the chemical potential functions as a tunable parameter that influences the Casimir force.
Fe; Extending the shears mechanism to the
shell orbitalBasu, S.*; Mukherjee, G.*; Utsuno, Yutaka; 32 of others*
Physics Letters B, 868, p.139642_1 - 139642_5, 2025/09
Times Cited Count:1 Percentile:70.48(Astronomy & Astrophysics)no abstracts in English
Fujii, Daisuke; Kawaguchi, Mamiya*; Tanaka, Mitsuru*
Physics Letters B, 866, p.139559_1 - 139559_7, 2025/07
Times Cited Count:4 Percentile:99.08(Astronomy & Astrophysics)We investigate the confining pressure inside the nucleon and the associated gravitational form factor, known as the D-term, within a skyrmion based on the scale-invariant chiral perturbation theory. In this approach, the effects of scale symmetry breaking are incorporated through the coupling of a scalar meson field to the scale anomaly, following the low-energy theorem. Utilizing the decomposition of the nucleon's energy-momentum tensor, we clarify how the scale anomaly components contribute to the internal pressure. Our analysis reveals that the gluon-induced scale anomaly predominantly governs the confining pressure. Compared to the result in the chiral limit of conventional chiral perturbation theory, this approach yields a total pressure profile more consistent with lattice QCD data. Furthermore, the pressure due to the gluonic anomaly extends over a wide spatial region, leading to a significant contribution to the D-term.
Kim, H.*; Gubler, P.; Sasaki, Chihiro*
Physics Letters B, 866, p.139577_1 - 139577_4, 2025/07
correlation functionAbreu, L. M.*; Gubler, P.; Khemchandani, K. P.*; Mart
nez Torres, A.*; Hosaka, Atsushi
Physics Letters B, 860, p.139175_1 - 139175_7, 2025/01
Times Cited Count:3 Percentile:87.29(Astronomy & Astrophysics)Li, P. J.*; Utsuno, Yutaka; Yoshida, Kazuki; 85 of others*
Physics Letters B, 855, p.138828_1 - 138828_11, 2024/08
Times Cited Count:3 Percentile:67.20(Astronomy & Astrophysics)
condensed state in
Mg using the
C+
C scatteringFujikawa, Y.*; Kawabata, T.*; Adachi, S.*; Hirose, Kentaro; Makii, Hiroyuki; Nishio, Katsuhisa; Orlandi, R.; Suzaki, Fumi; 13 of others*
Physics Letters B, 848, p.138384_1 - 138384_6, 2024/01
Times Cited Count:8 Percentile:82.79(Astronomy & Astrophysics)
SbLechner, S.*; Miyagi, Takayuki*; Xu, Z. Y.*; Bissell, M. L.*; Blaum, K.*; Cheal, B.*; Devlin, C. S.*; Garcia Ruiz, R. F.*; Ginges, J. S. M.*; Heylen, H.*; et al.
Physics Letters B, 847, p.138278_1 - 138278_9, 2023/12
Times Cited Count:9 Percentile:87.30(Astronomy & Astrophysics)no abstracts in English
Meng, Q.*; Hiyama, Emiko*; Oka, Makoto*; Hosaka, Atsushi; Xu, C.*
Physics Letters B, 846, p.138221_1 - 138221_6, 2023/11
Times Cited Count:14 Percentile:93.67(Astronomy & Astrophysics)no abstracts in English
H hypernucleus using in-flight
He
H reactionAkaishi, Takaya; Hashimoto, Tadashi; Tanida, Kiyoshi; 35 of others*
Physics Letters B, 845, p.138128_1 - 138128_4, 2023/10
Times Cited Count:1 Percentile:19.07(Astronomy & Astrophysics)
Ca cast doubt on a doubly magic
CaChen, S.*; Browne, F.*; Doornenbal, P.*; Lee, J.*; Obertelli, A.*; Tsunoda, Yusuke*; Otsuka, Takaharu*; Chazono, Yoshiki*; Hagen, G.*; Holt, J. D.*; et al.
Physics Letters B, 843, p.138025_1 - 138025_7, 2023/08
Times Cited Count:9 Percentile:82.79(Astronomy & Astrophysics)Gamma decays were observed in
Ca and
Ca following quasi-free one-proton knockout reactions from
Sc. For
Ca, a
ray transition was measured to be 1456(12) keV, while for
Ca an indication for a transition was observed at 1115(34) keV. Both transitions were tentatively assigned as the
decays. A shell-model calculation in a wide model space with a marginally modified effective nucleon-nucleon interaction depicts excellent agreement with experiment for
level energies, two-neutron separation energies, and reaction cross sections, corroborating the formation of a new nuclear shell above the N = 34 shell. Its constituents, the
and
orbitals, are almost degenerate. This degeneracy precludes the possibility for a doubly magic
Ca and potentially drives the dripline of Ca isotopes to
Ca or even beyond.
Ne at the transition into the island of inversion; Detailed structure study of
NeWang, H.*; Yasuda, Masahiro*; Kondo, Yosuke*; Nakamura, Takashi*; Tostevin, J. A.*; Ogata, Kazuyuki*; Otsuka, Takaharu*; Poves, A.*; Shimizu, Noritaka*; Yoshida, Kazuki; et al.
Physics Letters B, 843, p.138038_1 - 138038_9, 2023/08
Times Cited Count:5 Percentile:65.61(Astronomy & Astrophysics)Detailed
-ray spectroscopy of the exotic neon isotope
Ne has been performed using the one-neutron removal reaction from
Ne. Based on an analysis of parallel momentum distributions, a level scheme with spin-parity assignments has been constructed for
Ne and the negative-parity states are identified for the first time. The measured partial cross sections and momentum distributions reveal a significant intruder p-wave strength providing evidence of the breakdown of the N = 20 and N = 28 shell gaps. Only a weak, possible f-wave strength was observed to bound final states. Large-scale shell-model calculations with different effective interactions do not reproduce the large p-wave and small f-wave strength observed experimentally, indicating an ongoing challenge for a complete theoretical description of the transition into the island of inversion along the Ne isotopic chain.
Nakayama, Katsumasa*; Suzuki, Kei
Physics Letters B, 843, p.138017_1 - 138017_7, 2023/08
Times Cited Count:8 Percentile:82.79(Astronomy & Astrophysics)The Casimir effect is a quantum phenomenon induced by the zero-point energy of relativistic fields confined in a finite-size system. This effect for photon fields has been studied for a long time, while the realization of counterparts for fermion fields in Dirac/Weyl semimetals is an open question. We theoretically demonstrate the typical properties of the Casimir effect for relativistic electron fields in Dirac/Weyl semimetals and show the results from an effective Hamiltonian for realistic materials such as Cd
As
and Na
Bi. We find an oscillation of the Casimir energy as a function of the thickness of the thin film, which stems from the existence of Dirac/Weyl nodes in momentum space. Experimentally, such an effect can be observed in thin films of semimetals, where the thickness dependence of thermodynamic quantities is affected by the Casimir energy.
Sun, L. J.*; Fry, C.*; Davids, B.*; Esker, N.*; Wrede, C.*; Smallcombe, J.; 27 of others*
Physics Letters B, 839, p.137801_1 - 137801_8, 2023/04
Times Cited Count:2 Percentile:34.66(Astronomy & Astrophysics)Xia, C.-J.*; Maruyama, Toshiki; Yasutake, Nobutoshi*; Tatsumi, Toshitaka*; Zhang, Y.-X.*
Physics Letters B, 839, p.137769_1 - 137769_5, 2023/04
Times Cited Count:2 Percentile:57.29(Astronomy & Astrophysics)
Ne at the boundary of the island of inversionRevel, A.*; Wu, J.*; Iwasaki, Hironori*; Ash, J.*; Bazin, D.*; Brown, B. A.*; Chen, J.*; Elder, R.*; Farris, P.*; Gade, A.*; et al.
Physics Letters B, 838, p.137704_1 - 137704_7, 2023/03
Times Cited Count:3 Percentile:47.61(Astronomy & Astrophysics)no abstracts in English
measured in
reactionsAikawa, Shu*; Hashimoto, Tadashi; Tanida, Kiyoshi; 73 of others*
Physics Letters B, 837, p.137637_1 - 137637_8, 2023/02
Times Cited Count:11 Percentile:83.94(Astronomy & Astrophysics)