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Abreu, L. M.*; Gubler, P.; Khemchandani, K. P.*; Martnez Torres, A.*; Hosaka, Atsushi
Physics Letters B, 860, p.139175_1 - 139175_7, 2025/01
Times Cited Count:1 Percentile:0.00(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:1 Percentile:63.95(Astronomy & Astrophysics)Fujikawa, 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:5 Percentile:77.95(Astronomy & Astrophysics)Lechner, 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:5 Percentile:77.95(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:11 Percentile:92.67(Astronomy & Astrophysics)no abstracts in English
Akaishi, Takaya; Hashimoto, Tadashi; Tanida, Kiyoshi; 35 of others*
Physics Letters B, 845, p.138128_1 - 138128_4, 2023/10
Times Cited Count:1 Percentile:28.72(Astronomy & Astrophysics)Nakayama, Katsumasa*; Suzuki, Kei
Physics Letters B, 843, p.138017_1 - 138017_7, 2023/08
Times Cited Count:6 Percentile:62.61(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 CdAs
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.
Chen, 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:7 Percentile:83.07(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.
Wang, 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:4 Percentile:62.61(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.
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:48.20(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:48.20(Astronomy & Astrophysics)Revel, 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:62.61(Astronomy & Astrophysics)no abstracts in English
Aikawa, Shu*; Hashimoto, Tadashi; Tanida, Kiyoshi; 73 of others*
Physics Letters B, 837, p.137637_1 - 137637_8, 2023/02
Times Cited Count:8 Percentile:74.14(Astronomy & Astrophysics)Huang, H.*; Zhang, W. Q.*; Andreyev, A. N.; Liu, Z.*; Seweryniak, D.*; Li, Z. H.*; Guo, C. Y.*; Barzakh, A. E.*; Van Duppen, P.*; Andel, B.*; et al.
Physics Letters B, 833, p.137345_1 - 137345_8, 2022/10
Times Cited Count:1 Percentile:18.70(Astronomy & Astrophysics)Zhang, W. Q.*; Andreyev, A. N.; Liu, Z.*; Seweryniak, D.*; Huang, H.*; Li, Z. H.*; Li, J. G.*; Guo, C. Y.*; 34 of others*
Physics Letters B, 829, p.137129_1 - 137129_7, 2022/06
Times Cited Count:6 Percentile:68.58(Astronomy & Astrophysics)Koiwai, Takuma*; Wimmer, K.*; Doornenbal, P.*; Obertelli, A.*; Barbieri, C.*; Duguet, T.*; Holt, J. D.*; Miyagi, Takayuki*; Navrtil, P.*; Ogata, Kazuyuki*; et al.
Physics Letters B, 827, p.136953_1 - 136953_7, 2022/04
Times Cited Count:6 Percentile:68.58(Astronomy & Astrophysics)no abstracts in English
Maruyama, Tomoyuki*; Baha Balantekin, A.*; Cheoun, M.-K.*; Kajino, Toshitaka*; Kusakabe, Motohiko*; Mathews, G. J.*
Physics Letters B, 824, p.136813_1 - 136813_8, 2022/01
Times Cited Count:6 Percentile:54.93(Astronomy & Astrophysics)Meng, Q.*; Harada, Masayasu*; Hiyama, Emiko; Hosaka, Atsushi; Oka, Makoto
Physics Letters B, 824, p.136800_1 - 136800_5, 2022/01
Times Cited Count:30 Percentile:97.23(Astronomy & Astrophysics)Spectrum of the doubly heavy tetraquarks, , is studied in a constituent quark model. Four-body problem is solved in a variational method where the real scaling technique is used to identify resonant states above the fall-apart decay thresholds. In addition to the two bound states that were reported in the previous study we have found several narrow resonant states above the
and
thresholds. Their structures are studied and are interpreted by the quark dynamics. A narrow resonance with spin-parity
is found to be a mixed state of a compact tetraquark and a
scattering state. This is driven by a strong color Coulombic attraction between the
quarks. Negative-parity excited resonances with
,
and
form a triplet under the heavy-quark spin symmetry. It turns out that they share a similar structure to the
-mode of a singly heavy baryon as a result of the strongly attractive correlation for the doubly heavy diquark.
Kitamura, Noritaka*; Wimmer, K.*; Poves, A.*; Shimizu, Noritaka*; Tostevin, J. A.*; Bader, V. M.*; Bancroft, C.*; Barofsky, D.*; Baugher, T.*; Bazin, D.*; et al.
Physics Letters B, 822, p.136682_1 - 136682_7, 2021/11
Times Cited Count:9 Percentile:64.85(Astronomy & Astrophysics)no abstracts in English
Tonev, D.*; De Angelis, G.*; Deloncle, I.*; Orlandi, R.; 27 of others*
Physics Letters B, 821, p.136603_1 - 136603_6, 2021/10
Times Cited Count:5 Percentile:52.80(Astronomy & Astrophysics)