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北川 俊作*; 徳永 陽; 酒井 宏典; 神戸 振作; 他11名*
Journal of the Physical Society of Japan, 93(12), p.123701_1 - 123701_5, 2024/11
被引用回数:2 パーセンタイル:53.15(Physics, Multidisciplinary)We report the re-measurement of the -axis spin susceptibility component in an early-stage sample of the spin-triplet superconductor UTe
with the transition temperature of
= 1.6 K. Using Knight-shift measurements along the
axis and at a 10-degree tilt from the
axis towards the
axis, we accurately determined the
-axis component without directly measuring the
-axis Knight shift. The experiment reveals that the previously reported absence of the reduction in Knight shift is attributed to the missing of signal from the superconducting region and to the detection of residual signals from the non-superconducting region instead.
雨森 道紘*; 土屋 晴文; Tibet AS Collaboration*; 他116名*
Astrophysical Journal, 954(2), p.200_1 - 200_7, 2023/09
被引用回数:5 パーセンタイル:56.22(Astronomy & Astrophysics)Gamma rays from HESS J1849-000, a middle-aged TeV pulsar wind nebula (PWN), are observed by the Tibet air shower array and the muon detector array. The detection significance of gamma rays reaches and
levels above 25 TeV and 100 TeV, respectively. The energy spectrum measured between 40 TeV
E
320 TeV for the first time is described with a simple power-law function of dN/dE =
. The gamma-ray energy spectrum from the sub-TeV to sub-PeV ranges including the results of previous studies can be modeled with the leptonic scenario, Inverse Compton Scattering by high-energy electrons accelerated by the PWN of PSR J1849-0001, but the scenario requires sophisticated theoretical modeling. On the other hand, the gamma-ray energy spectrum can be simply modeled with the hadronic scenario in which gamma rays are generated from the decay of neutral pions produced by collisions between accelerated cosmic-ray protons and the ambient molecular cloud found in the gamma-ray emitting region. The cutoff energy of cosmic-ray protons
is estimated at
, suggesting that protons are accelerated up to the PeV energy range. Our study proposes that HESS J1849-000 should be further investigated as a new candidate for a Galactic PeV cosmic-ray accelerator, or "PeVatron".
小杉 美央子*; 齊藤 英治; 吉川 貴史*; 他11名*
APL Materials (Internet), 11(8), p.081106_1 - 081106_6, 2023/08
被引用回数:1 パーセンタイル:14.50(Nanoscience & Nanotechnology)Strontium titanate [SrTiO (STO)], a perovskite oxide with an extremely high gate-tunable dielectric constant (
) due to quantum paraelectric phases, is attracting considerable attention for yielding various physical phenomena when two-dimensional (2D) layers are integrated. Superconductivity is such a typical phenomenon. However, the influence of the STO substrates on enhancing transition temperatures (
) for (atomically) thin 2D flakes attached to them has been rarely investigated. Here, we report gate-tunable and gradual four-terminal resistance drops with critical onset
(
) and scanning tunneling spectroscopy (STS) spectra in devices comprising thin TaS
flakes attached on monolayer hexagonal boron nitride (hBN) spacer/STO substrates. Observation of STS spectra confirms the presence of local superconducting gaps. (similar to 1.5 meV) with transition
(
three-times higher than previous reports of
under absent pressure and strong position dependence of
. Depending on
on back gate voltages (
) and magnetic fields, there is a strong correlation between
and the onset
of superconductivity, implying an enhancement of approximately five times compared with the previous highest-onset
values without pressure as the applied
increases. The high onset
and. are discussed based on screening of the long-range Coulomb interaction (CI) due to the high-
of SrTiO
, while the short-ranged CI remains strong in the 2D limit, causing the superconductivity. Using a monolayer hBN/SrTiO
substrate with
opens doors to
enhancement in thin superconducting layers integrated on it and wide application due to the solid-state high-
substrates.
Mastromarco, M.*; Amaducci, S.*; Colonna, N.*; 木村 敦; 他118名*
European Physical Journal A, 58(8), p.147_1 - 147_13, 2022/08
被引用回数:6 パーセンタイル:63.01(Physics, Nuclear)The U(n,f) cross section was measured in a wide energy range (18 meV - 170 keV) at the n_TOF facility at CERN, relative to
Li(n,t) and
B(n,
) standard reactions, with a setup based on a stack of six samples and six silicon detectors placed in the neutron beam. A resonance analysis has been performed up to 200 eV, with the code SAMMY. A good agreement, within 0.5%, is found on average between the new results and the latest evaluated data files ENDF/B-VIII.0 and JEFF-3.3, as well as with respect to the broad group average fission cross section established in the framework of the standard working group of IAEA. However, some discrepancies, of up to 4%, are still present in some specific energy regions.
Jia, S.*; 谷田 聖; Belle Collaboration*; 他211名*
Physical Review Letters, 128(8), p.081804_1 - 081804_9, 2022/02
被引用回数:2 パーセンタイル:29.32(Physics, Multidisciplinary)We search for a light Higgs boson () decaying into a
or
pair in the radiative decays of
. The production of
mesons is tagged by
transitions, using 158 million
events accumulated with the Belle detector at the KEKB asymmetric energy electron-positron collider. No significant
signals in the mass range from the
or
threshold to 9.2 GeV/
are observed. We set the upper limits at 90% credibility level (C.L.) on the product branching fractions for
and
varying from
to
. Our results represent an approximately twofold improvement on the current world best upper limits for the
production. For
, the upper limits on the product branching fractions for
and
are at the same level as the world average limits, and vary from
to
. The upper limits at 90% C.L. on the Yukawa coupling
and mixing angle
are also given.
雨森 道紘*; 土屋 晴文; Tibet AS Collaboration*; 他111名*
Physical Review Letters, 127(3), p.031102_1 - 031102_6, 2021/07
被引用回数:20 パーセンタイル:82.10(Physics, Multidisciplinary)We report observations of gamma-ray emissions with energies in the 100-TeV energy region from the Cygnus region in our Galaxy. Two sources are significantly detected in the directions of the Cygnus OB1 and OB2 associations. Based on their positional coincidences, we associate one with a pulsar PSR J2032 + 4127 and the other mainly with a pulsar wind nebula PWN G75.2 + 0.1, with the pulsar moving away from its original birthplace situated around the centroid of the observed gamma-ray emission. This work would stimulate further studies of particle acceleration mechanisms at these gamma-ray sources.
Kim, S. H.*; 市川 裕大; 佐甲 博之; 長谷川 勝一; 早川 修平*; 七村 拓野*; 佐藤 進; 谷田 聖; 吉田 純也; 他11名*
Nuclear Instruments and Methods in Physics Research A, 940, p.359 - 370, 2019/10
被引用回数:5 パーセンタイル:41.86(Instruments & Instrumentation)We have developed a gas electron multiplier (GEM)-based time projection chamber (TPC) for the H-dibaryon search experiment at J-PARC. High-rate beam particles enter a TPC gas volume of approximately 0.2 m
, in a direction perpendicular to the electric field. A long-rectangular hollow section is located inside the TPC volume to accommodate a diamond target. We commissioned the TPC using 230 MeV protons with beam rates of up to 1 MHz. The TPC data acquisition system collected 5768 pad signals in full readout mode, with almost 100% efficiency, at a preset trigger rate of 230 Hz. We operated the TPC in an Ar/CH
gas mixture (90/10) without a magnetic field. The spatial resolutions on the pad plane are measured to be 400-700
m, which correspond to 230-300
m in a magnetic field of 1 T. We confirmed high tracking capability at beam rates of up to 1 MHz.
Amaducci, S.*; 原田 秀郎; 木村 敦; 他118名*
European Physical Journal A, 55(7), p.120_1 - 120_19, 2019/07
被引用回数:23 パーセンタイル:87.47(Physics, Nuclear)n_TOF施設にて、熱から170keVの中性子エネルギー領域において、U(n, f)断面積を測定した。
Li(n, t)および
B(n,
)標準断面積に対する相対測定により、1.5%という系統的不確かさで測定値を得た。本測定には、6層からなるサンプルと6台のSi検出器を用いた。9
18keVエネルギー領域において、本測定結果は、最近の評価済み核データであるENDF/B-VIII.0およびJEFF3.3の評価値が、約5%過大評価であることを示した。高分解能測定の結果、keV領域で、共鳴構造を観測した。本測定より、7.8
11eVのエネルギー範囲の断面積の積分値について、249.7
1.4(統計的不確かさ)
0.94(系統的不確かさ)b
eVという結果を得た。この結果は、最近確立された標準値247.5
3b
eVを支持するものである。
Mastromarco, M.*; Manna, A.*; Aberle, O.*; Andrzejewski, J.*; 原田 秀郎; 木村 敦; n_TOF Collaboration*; 他116名*
European Physical Journal A, 55(1), p.9_1 - 9_20, 2019/01
被引用回数:27 パーセンタイル:90.17(Physics, Nuclear)Neutron capture cross section measurements on Gd and
Gd were performed using the time-of-flight technique at the n_TOF facility at CERN on isotopically enriched samples. The measurements were carried out in the n TOF experimental area EAR1, at 185m from the neutron source, with an array of 4 C
D
liquid scintillation detectors. At a neutron kinetic energy of 0.0253eV, capture cross sections of 62.2(2.2) and 239.8(8.4) kilobarn have been derived for
Gd and
Gd, respectively, with up to 6% deviation relative to values presently reported in nuclear data libraries, but consistent with those values within 1.6 standard deviations. A resonance shape analysis has been performed in the resolved resonance region up to 181eV and 307eV, respectively for
Gd and
Gd, where on average, resonance parameters have been found in good agreement with evaluations. Above these energies and up to 1keV, the observed resonance-like structure of the cross section has been analysed and characterised. From a statistical analysis of the observed neutron resonances we deduced: neutron strength function of 2.01(28)
10
and 2.17(41)
10
; average total radiative width of 106.8(14)meV and 101.1(20)meV and s-wave resonance spacing 1.6(2)eV and 4.8(5)eV for n +
Gd and n +
Gd systems, respectively.
Sandilya, S.*; 谷田 聖; Belle Collaboration*; 他211名*
Physical Review D, 98(7), p.071101_1 - 071101_8, 2018/10
被引用回数:5 パーセンタイル:25.37(Astronomy & Astrophysics)We have searched for the lepton-flavor-violating decay using a data sample of 711 fb
that contains
pairs. The data were collected near the
resonance with the Belle detector at the KEKB asymmetric-energy
collider. No signals were observed, and we set 90% confidence level upper limits on the branching fractions of
,
, and, for both decays combined,
. These are the most stringent limits on these decays to date.
Aidala, C.*; 長谷川 勝一; 今井 憲一; 佐甲 博之; 佐藤 進; 谷田 聖; PHENIX Collaboration*; 他311名*
Physical Review Letters, 120(6), p.062302_1 - 062302_8, 2018/02
被引用回数:54 パーセンタイル:90.53(Physics, Multidisciplinary)Recently, multiparticle-correlation measurements of relativistic He
Au,
Pb, and even
collisions have shown surprising collective signatures. Here we present beam-energy-scan measurements of 2-, 4-, and 6-particle angular correlations in
Au collisions at
=200, 62.4, 39, and 19.6 GeV. We also present measurements of 2- and 4-particle angular correlations in
Au collisions at
=200 GeV. We find the 4-particle cumulant to be real-valued for
Au collisions at all four energies. We also find that the 4-particle cumulant in
Au has the opposite sign as that in
Au, indicating that the correlations are geometrical and therefore collective in origin. Further we find that the 6-particle cumulant agrees with the 4-particle cumulant in
Au collisions at 200 GeV, which indicates that nonflow effects are subdominant and provides strong evidence of collectivity.
Lerendegui-Marco, J.*; Guerrero, C.*; 原田 秀郎; 木村 敦; n_TOF Collaboration*; 他115名*
EPJ Web of Conferences, 146, p.11045_1 - 11045_4, 2017/09
被引用回数:1 パーセンタイル:58.47(Nuclear Science & Technology)軽水炉及び高速炉でのMOX燃料利用にあたり、高精度の中性子捕獲断面積及び核分裂断面積が必要とされており、NEAの専門家会合WPEC-26の報告書によれば、特にPuの中性子捕獲断面積について、500eVから500keVのエネルギー領域に対して7
12%の精度が必要とされている。しかしながら、keV領域の測定値としては、不確かさが約35%と大きな1970年代のデータしかこの40年間存在しなかった。本論文では、n_TOF施設の第1実験室において測定実験を実施し、取得したデータを解析して得られた個々の中性子共鳴パラメータ及びその平均値について暫定結果を示す。
Guerrero, C.*; Lerendegui-Marco, J.*; Domingo-Pardo, C.*; 原田 秀郎; 木村 敦; n_TOF Collaboration*; 他113名*
EPJ Web of Conferences, 146, p.01007_1 - 01007_4, 2017/09
被引用回数:1 パーセンタイル:58.47(Nuclear Science & Technology)The neutron capture cross section of several key unstable isotopes acting as branching points in the s-process are crucial for stellar nucleosynthesis studies, but they are very challenging to measure due to the difficult production of sufficient sample material, the high activity of the resulting samples, and the actual (n,) measurement, for which high neutron fluxes and effective background rejection capabilities are required. Capture cross section of
Pm and
Tm have been measured for time-of-flight measurements at the CERN n_TOF facility using the 19 and 185m beam lines. Activation experiments on the same
Pm and
Tm targets with a high-intensity 30 keV quasi-Maxwellian flux of neutrons will be performed using the SARAF accelerator and the Liquid-Lithium Target (LiLiT) in order to extract the corresponding Maxwellian Average Cross Section (MACS). The status of these experiments and preliminary results will be presented and discussed as well.
Chiaveri, E.*; Aberle, O.*; Andrzejewski, J.*; 原田 秀郎; 木村 敦; n_TOF Collaboration*; 他111名*
EPJ Web of Conferences, 146, p.03001_1 - 03001_4, 2017/09
被引用回数:2 パーセンタイル:75.43(Nuclear Science & Technology)The CERN n_TOF neutron beam facility is characterized by a very high instantaneous neutron flux, excellent TOF resolution at the 185m long flight path (EAR-1), low intrinsic background and coverage of a wide range of neutron energies, from thermal to a few GeV. The overall efficiency of the experimental program and the range of possible measurements has been expanded with the construction of a second experimental area (EAR-2), located 20m on the vertical of the n_TOF spallation target. This upgrade, which benefits from a neutron flux 30 times higher than in EAR-1, provides a substantial extension in measurement capabilities, opening the possibility to collect data on neutron cross-section of isotopes with short half-lives or available in very small amounts. We will discuss the innovative features of the EAR-2 neutron beam that make possible to perform very challenging measurements on short-lived radioisotopes or sub-mg samples, out of reach up to now at other neutron facilities around the world. Finally, the future perspectives of the facility will be presented.
Lerendegui-Marco, J.*; Corts-Giraldo, M. A.*; Guerrero, C.*; 原田 秀郎; 木村 敦; n_TOF Collaboration*; 他114名*
EPJ Web of Conferences, 146, p.03030_1 - 03030_4, 2017/09
被引用回数:0 パーセンタイル:0.00(Nuclear Science & Technology)Monte Carlo (MC) simulations are an essential tool to determine fundamental features of a neutron beam, such as the neutron flux or the ray background, that sometimes can not be measured or at least not in every position or energy range. Until recently, the most widely used MC codes in this field had been MCNPX and FLUKA. However, the Geant4 toolkit has also become a competitive code for the transport of neutrons after the development of the native Geant4 format for neutron data libraries, G4NDL. In this context, we present the Geant4 simulations of the neutron spallation target of the n TOF facility at CERN, done with version 10.1.1 of the toolkit. The first goal was the validation of the intra-nuclear cascade models implemented in the code using, as benchmark, the characteristics of the neutron beam measured at the first experimental area (EAR1), especially the neutron flux and energy distribution, and the time distribution of neutrons of equal kinetic energy, the so-called Resolution Function. The second goal was the development of a Monte Carlo tool aimed to provide useful calculations for both the analysis and planning of the upcoming measurements at the new experimental area (EAR2) of the facility.