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1. Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass composition

Author

Telescope Array Collaboration, Abbasi, R. U., Abe, Y., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cheon, B. G., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashida, N., He, H., Hibi, R., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawakami, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, S. W., Kimura, Y., Komae, I., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Mizuno, K., Murakami, M., Myers, I., Nagataki, S., Nakai, K., Nakamura, T., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Onishi, M., Ohoka, H., Okazaki, N., Oku, Y., Okuda, T., Omura, Y., Ono, M., Oshima, A., Oshima, H., Ozawa, S., Park, I. H., Park, K. Y., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rott, C., Rubtsov, G. I., Ryu, D., Sagawa, H., Saito, R., Sakaki, N., Sako, T., Sakurai, N., Sato, D., Sato, K., Sato, S., Sekino, K., Shah, P. D., Shibata, N., Shibata, T., Shikita, J., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Stokes, B. T., Stroman, T. A., Takagi, Y., Takahashi, K., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Udo, S., Urban, F., Warren, D., Wong, T., Yamazaki, K., Yashiro, K., Yoshida, F., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We report an estimation of the injected mass composition of ultra-high energy cosmic rays (UHECRs) at energies higher than 10 EeV. The composition is inferred from an energy-dependent sky distribution of UHECR events observed by the Telescope Array surface detector by comparing it to the Large Scale Structure of the local Universe. In the case of negligible extra-galactic magnetic fields the results are consistent with a relatively heavy injected composition at E ~ 10 EeV that becomes lighter up to E ~ 100 EeV, while the composition at E > 100 EeV is very heavy. The latter is true even in the presence of highest experimentally allowed extra-galactic magnetic fields, while the composition at lower energies can be light if a strong EGMF is present. The effect of the uncertainty in the galactic magnetic field on these results is subdominant., Comment: 8 pages, 3 figures, accepted for publication in PRL

Published
2024

2. Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope Array

Author

Telescope Array Collaboration, Abbasi, R. U., Abe, Y., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cheon, B. G., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashida, N., He, H., Hibi, R., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawakami, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, S. W., Kimura, Y., Komae, I., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Mizuno, K., Murakami, M., Myers, I., Nagataki, S., Nakai, K., Nakamura, T., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Onishi, M., Ohoka, H., Okazaki, N., Oku, Y., Okuda, T., Omura, Y., Ono, M., Oshima, A., Oshima, H., Ozawa, S., Park, I. H., Park, K. Y., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rott, C., Rubtsov, G. I., Ryu, D., Sagawa, H., Saito, R., Sakaki, N., Sako, T., Sakurai, N., Sato, D., Sato, K., Sato, S., Sekino, K., Shah, P. D., Shibata, N., Shibata, T., Shikita, J., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Stokes, B. T., Stroman, T. A., Takagi, Y., Takahashi, K., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Udo, S., Urban, F., Warren, D., Wong, T., Yamazaki, K., Yashiro, K., Yoshida, F., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

We use a new method to estimate the injected mass composition of ultrahigh cosmic rays (UHECRs) at energies higher than 10 EeV. The method is based on comparison of the energy-dependent distribution of cosmic ray arrival directions as measured by the Telescope Array experiment (TA) with that calculated in a given putative model of UHECR under the assumption that sources trace the large-scale structure (LSS) of the Universe. As we report in the companion letter, the TA data show large deflections with respect to the LSS which can be explained, assuming small extra-galactic magnetic fields (EGMF), by an intermediate composition changing to a heavy one (iron) in the highest energy bin. Here we show that these results are robust to uncertainties in UHECR injection spectra, the energy scale of the experiment and galactic magnetic fields (GMF). The assumption of weak EGMF, however, strongly affects this interpretation at all but the highest energies E > 100 EeV, where the remarkable isotropy of the data implies a heavy injected composition even in the case of strong EGMF. This result also holds if UHECR sources are as rare as $2 \times 10^{-5}$ Mpc$^{-3}$, that is the conservative lower limit for the source number density., Comment: 18 pages, 11 figures, accepted for publication in PRD

Published
2024

3. Benefits of use, and tolerance of, medium-chain triglyceride medical food in the management of Japanese patients with Alzheimer’s disease: a prospective, open-label pilot study

Author

Ohnuma T, Toda A, Kimoto A, Takebayashi Y, Higashiyama R, Tagata Y, Ito M, Ota T, Shibata N, and Arai H

Subjects
Alzheimer’s disease, medium-chain triglycerides, ketone, cognitive function, apolipoprotein E epsilon 4, Geriatrics, RC952-954.6
Abstract

Tohru Ohnuma, Aiko Toda, Ayako Kimoto, Yuto Takebayashi, Ryoko Higashiyama, Yuko Tagata, Masanobu Ito, Tsuneyoshi Ota, Nobuto Shibata, Heii Arai Department of Psychiatry, Juntendo University Alzheimer’s Disease Project, Faculty of Medicine, Juntendo University, Tokyo, Japan Objectives: This is the first clinical trial of this type in Japan, designed to analyze two important aspects of Alzheimer’s disease (AD) management using medium-chain triglycerides. Axona was administered for 3 months (40 g of powder containing 20 g of caprylic triglycerides). We used an indurating, four-step dose-titration method (from 10 to 40 g per day) for 7 days before the trial, and examined the tolerance and adverse effects of this intervention. We also investigated its effect on cognitive function in mild-to-moderate AD patients.Patients and methods: This was a clinical intervention in 22 Japanese patients with sporadic AD at a mild-to-moderate stage (ten females, 12 males), mean age (± standard deviation) 63.9 (±8.5) years, Mini-Mental State Examination (MMSE) score, 10–25, seven patients were ApoE4-positive. During Axona administration, we examined changes in cognitive function by obtaining MMSE and AD assessment-scale scores. Intolerance and serum ketone concentrations were also examined.Results: The tolerance of Axona was good, without severe gastrointestinal adverse effects. Axona did not improve cognitive function in our sample of AD patients, even in those patients without the ApoE4 allele. However, some ApoE4-negative patients with baseline MMSE score ≥14 showed improvement in their cognitive functions.Conclusion: The modified dose-titration method, starting with a low dose of Axona, decreased gastrointestinal adverse effects in Japanese patients. Axona might be effective for some relatively mildly affected patients with AD (with cognitive function MMSE score of ≥14 and lacking the ApoE4 allele). Keywords: Alzheimer’s disease, medium-chain triglycerides, ketone, cognitive function, apolipoprotein E epsilon 4

Published
2016

4. Lessons learned after three years of SPIDER operation and the first MITICA integrated tests

Author

Marcuzzi, D., Toigo, V., Boldrin, M., Chitarin, G., Bello, S. Dal, Grando, L., Luchetta, A., Pasqualotto, R., Pavei, M., Serianni, G., Zanotto, L., Agnello, R., Agostinetti, P., Agostini, M., Aprile, D., Barbisan, M., Battistella, M., Berton, G., Bigi, M., Brombin, M., Candela, V., Candeloro, V., Canton, A., Casagrande, R., Cavallini, C., Cavazzana, R., Cordaro, L., Cruz, N., Palma, M. Dalla, Dan, M., De Lorenzi, A., Delogu, R., De Muri, M., De Nardi, M., Denizeau, S., Fadone, M., Fellin, F., Ferro, A., Gaio, E., Gasparrini, C., Gnesotto, F., Jain, P., La Rosa, A., Lopez-Bruna, D., Lorenzini, R., Maistrello, A., Manduchi, G., Manfrin, S., Marconato, N., Mario, I., Martini, G., Milazzo, R., Patton, T., Peruzzo, S., Pilan, N., Pimazzoni, A., Poggi, C., Pomaro, N., Pouradier-Duteil, B., Recchia, M., Rigoni-Garola, A., Rizzetto, D., Rizzolo, A., Santoro, F., Sartori, E., Segalini, B., Shepherd, A., Siragusa, M., Sonato, P., Sottocornola, A., Spada, E., Spagnolo, S., Spolaore, M., Taliercio, C., Tinti, P., Tomsič, P., Trevisan, L., Ugoletti, M., Valente, M., Valisa, M., Veronese, F., Vignando, M., Zaccaria, P., Zagorski, R., Zaniol, B., Zaupa, M., Zuin, M., Cavenago, M., Boilson, D., Rotti, C., Decamps, H., Geli, F., Sharma, A., Veltri, P., Zacks, J., Simon, M., Paolucci, F., Garbuglia, A., Gutierrez, D., Masiello, A., Mico, G., Labate, C., Readman, P., Bragulat, E., Bailly-Maitre, L., Gomez, G., Kouzmenko, G., Albajar, F., Kashiwagi, M., Tobari, H., Kojima, A., Murayama, M., Hatakeyama, S., Oshita, E., Maejima, T., Shibata, N., Yamashita, Y., Watanabe, K., Singh, N. P., Singh, M. J., Dhola, H., Fantz, U., Heinemann, B., Wimmer, C., Wünderlich, D., Tsumori, K., Croci, G., Gorini, G., Muraro, A., Rebai, M., Tardocchi, M., Giacomelli, L., Rigamonti, D., Taccogna, F., Bruno, D., Rutigliano, M., Longo, S., Deambrosis, S., Miorin, E., Montagner, F., Tonti, A., and Panin, F.

Subjects
Physics - Plasma Physics, Physics - Accelerator Physics
Abstract

ITER envisages the use of two heating neutral beam injectors plus an optional one as part of the auxiliary heating and current drive system. The 16.5 MW expected neutral beam power per injector is several notches higher than worldwide existing facilities. A Neutral Beam Test Facility (NBTF) was established at Consorzio RFX, exploiting the synergy of two test beds, SPIDER and MITICA. SPIDER is dedicated to developing and characterizing large efficient negative ion sources at relevant parameters in ITER-like conditions: source and accelerator located in the same vacuum where the beam propagates, immunity to electromagnetic interferences of multiple radio-frequency (RF) antennas, avoidance of RF-induced discharges on the outside of the source. Three years of experiments on SPIDER have addressed to the necessary design modifications to enable full performances. The source is presently under a long shut-down phase to incorporate learnings from the experimental campaign. Parallelly, developments on MITICA, the full-scale prototype of the ITER NBI featuring a 1 MV accelerator and ion neutralization, are underway including manufacturing of in-vessel components, while power supplies and auxiliary plants are already under final testing and commissioning. Integration, commissioning and tests of the 1MV power supplies are essential for this first-of-kind system, unparalleled both in research and industry field. The integrated test to confirm 1MV output by combining invertor systems, DC generators and transmission lines extracted errors/accidents in some components. To realize a concrete system for ITER, solutions for the repair and the improvement of the system were developed. Hence, NBTF is emerging as a necessary facility, due to the large gap with existing injectors, effectively dedicated to identify issues and find solutions to enable successful ITER NBI operations in a time bound fashion.

Published
2023
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5. Synthesizing $2h/e^2$ resistance plateau at the first Landau level confined in a quantum point contact

Author

Fauzi, M. H., Nakagawara, K., Hashimoto, K., Shibata, N., and Hirayama, Y.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

A comprehensive understanding of quantum Hall edge transmission, especially the hole-conjugate of a Laughlin state such as a $2/3$ state, is critical for advancing fundamental quantum Hall physics and enhancing the design of quantum Hall edge interferometry. In this study, we report a robust intermediate $2h/e^2$ resistance quantization in a quantum point contact (QPC) when the bulk is set at the fractional filling $2/3$ quantum Hall state. Our results suggest the occurrence of two equilibration processes. First, the co-propagating $1/3$ edges moving along a soft QPC arm confining potential fully equilibrate and act as a single $2/3$ edge mode. Second, the $2/3$ edge mode is further equilibrated with an integer $1$ edge mode formed in the QPC. The complete mixing between them results in a diagonal resistance value quantized at $2h/e^2$. Similar processes occur for a bulk filling $5/3$, leading to an intermediate $(2/3)h/e^2$ resistance quantization., Comment: typo in the formula has been fixed, 10 pages including supplementary material

Published
2023

6. Safety comparison of additives in antiglaucoma prostaglandin (PG) analog ophthalmic formulations

Author

Fukuda M, Shibata S, Shibata N, Hagihara K, Yaguchi H, Osada H, Takahashi N, Kubo E, and Sasaki H

Subjects
Ophthalmology, RE1-994
Abstract

Masamichi Fukuda, Shinsuke Shibata, Naoko Shibata, Kenta Hagihara, Hiromoto Yaguchi, Hiromi Osada, Nobuo Takahashi, Eri Kubo, Hiroshi SasakiDepartment of Ophthalmology, Kanazawa Medical University, Uchinada, JapanPurpose: To investigate the safety of five types of antiglaucoma prostaglandin analog ophthalmic formulations, and to clarify their differences in accordance with contained additives (preservatives and surface-active agents).Methods: The following five types of ophthalmic solutions and three types of additives were investigated: latanoprost (Xalatan®; latanoprost), tafluprost (Tapros®; tafluprost), bimatoprost (Lumigan®; bimatoprost), travoprost (Travatan®; travoprost), travoprost (Travatan Z®; travoprost-Z), benzalkonium chloride (BAK), polyoxyethylene hardening castor oil 40 (HCO-40), and polysorbate 80 (P-80). These experimental solutions were exposed to the cultured cells of a rabbit-derived corneal cell line for a certain time, and the exposure time causing 50% cell damage (CD50), indicated by the ratio of viable cells to total cells was calculated (in vitro). In addition, corneal resistance (CR) was measured and CR ratio (post-treatment CR/pretreatment CR × 100) was calculated (in vivo).Results: CD50 of each ophthalmic solution was the longest with tafluprost, followed by travoprost-Z, bimatoprost, travoprost, and latanoprost. CD50 of 0.005%, 0.01%, and 0.02% BAK was 14.5 minutes, 8.1 minutes, and 4.0 minutes, respectively. The number of viable cells decreased to 60%, 8 minutes after exposure with HCO-40, and 30 minutes after being exposed to P-80. The CR ratio was 81.0% with travoprost and 82.0% with latanoprost, indicating a significant posttreatment reduction of CR (P < 0.05). The CR ratio did not decrease after treatment with tafluprost, travoprost-Z, or bimatoprost. The CR ratio of 0.005%, 0.01%, and 0.02% BAK was 105.0%, 90.5%, and 68.7%, respectively, and that of HCO-40 and P-80 was 108.7% and 114.2%, respectively.Conclusion: BAK, HCO-40, and P-80 were thought to be involved in corneal injuries caused by each ophthalmic solution. Corneal injuries due to surface action were observed when using HCO-40 and P-80. When HCO-40 was combined with BAK, it induced micellar BAK and reduced corneal injuries by BAK.Keywords: corneal resistance measuring device, additives, prostaglandin analogs, surface-active agents, corneal epithelial injury

Published
2013

7. First High-speed Video Camera Observations of a Lightning Flash Associated with a Downward Terrestrial Gamma-ray Flash

Author

Abbasi, R. U., Saba, M. M. F., Belz, J. W., Krehbiel, P. R., Rison, W., Kieu, N., da Silva, D. R., Rodeheffer, Dan, Stanley, M. A., Remington, J., Mazich, J., LeVon, R., Smout, K., Petrizze, A., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Bergman, D. R., Blake, S. A., Buckland, I., Cheon, B. G., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashida, N., He, H., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwakura, H., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawakami, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, S. W., Kimura, Y., Komae, I., Kubota, Y., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Myers, I., Nagataki, S., Nakai, K., Nakamura, R., Nakamura, T., Nakamura, Y., Nakazawa, A., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Ohnishi, M., Ohoka, H., Oku, Y., Okuda, T., Omura, Y., Ono, M., Oshima, A., Ozawa, S., Park, I. H., Potts, M., Pshirkov, M. S., Rodriguez, D. C., Rott, C., Rubtsov, G. I., Ryu, D., Sagawa, H., Sakaki, N., Sako, T., Sakurai, N., Sato, K., Seki, T., Sekino, K., Shah, P. D., Shibasaki, Y., Shibata, N., Shibata, T., Shikita, J., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Stokes, B. T., Stroman, T. A., Takahashi, K., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Udo, S., Uehama, T., Urban, F., Warren, D., Wong, T., Yamamoto, M., Yamazaki, K., Yashiro, K., Yoshida, F., Zhezher, Y., and Zundel, Z.

Subjects
Physics - Atmospheric and Oceanic Physics, Astrophysics - Instrumentation and Methods for Astrophysics, High Energy Physics - Experiment
Abstract

In this paper, we present the first high-speed video observation of a cloud-to-ground lightning flash and its associated downward-directed Terrestrial Gamma-ray Flash (TGF). The optical emission of the event was observed by a high-speed video camera running at 40,000 frames per second in conjunction with the Telescope Array Surface Detector, Lightning Mapping Array, interferometer, electric-field fast antenna, and the National Lightning Detection Network. The cloud-to-ground flash associated with the observed TGF was formed by a fast downward leader followed by a very intense return stroke peak current of -154 kA. The TGF occurred while the downward leader was below cloud base, and even when it was halfway in its propagation to ground. The suite of gamma-ray and lightning instruments, timing resolution, and source proximity offer us detailed information and therefore a unique look at the TGF phenomena.

Published
2022
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8. Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic Rays

Author

The ANTARES collaboration, Albert, A., Alves, S., André, M., Anghinolfi, M., Ardid, M., Ardid, S., Aubert, J. -J., Aublin, J., Baret, B., Basa, S., Belhorma, B., Bendahman, M., Bertin, V., Biagi, S., Bissinger, M., Boumaaza, J., Bouta, M., Bouwhuis, M. C., Brânzaş, H., Bruijn, R., Brunner, J., Busto, J., Caiffi, B., Calvo, D., Capone, A., Caramete, L., Carr, J., Carretero, V., Celli, S., Chabab, M., Chau, T. N., Moursli, R. Cherkaoui El, Chiarusi, T., Circella, M., Coleiro, A., Coniglione, R., Coyle, P., Creusot, A., Díaz, A. F., Distefano, C., Di Palma, I., Domi, A., Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., van Eeden, T., van Eijk, D., Khayati, N. El, Enzenhöfer, A., Fermani, P., Ferrara, G., Filippini, F., Fusco, L., Gatelet, Y., Gay, P., Glotin, H., Gozzini, R., Ruiz, R. Gracia, Graf, K., Guidi, C., Hallmann, S., van Haren, H., Heijboer, A. J., Hello, Y., Hernández-Rey, J. J., Hößl, J., Hofestädt, J., Huang, F., Illuminati, G., James, C. W., Jisse-Jung, B., de Jong, M., de Jong, P., Kadler, M., Kalekin, O., Katz, U., Khan-Chowdhury, N. R., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Breton, R. Le, LeStum, S., Lefèvre, D., Leonora, E., Levi, G., Lopez-Coto, D., Loucatos, S., Maderer, L., Manczak, J., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J. A., Martino, B., Melis, K., Migliozzi, P., Moussa, A., Muller, R., Nauta, L., Navas, S., Nezri, E., Fearraigh, B. Ó, Păun, A., Păvălaş, G. E., Pellegrino, C., Perrin-Terrin, M., Pestel, V., Piattelli, P., Pieterse, C., Poirè, C., Popa, V., Pradier, T., Randazzo, N., Real, D., Reck, S., Riccobene, G., Romanov, A., Sánchez-Losa, A., Greus, F. Salesa, Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabel, J., Schumann, J., Schüssler, F., Seneca, J., Spurio, M., Stolarczyk, Th., Taiuti, M., Tayalati, Y., Tingay, S. J., Vallage, B., Van Elewyck, V., Versari, F., Viola, S., Vivolo, D., Wilms, J., Zavatarelli, S., Zegarelli, A., Zornoza, J. D., Zúñiga, J., collaboration, The IceCube, Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Alameddine, J. M., Alispach, C., Alves Jr., A. A., Amin, N. M., Andeen, K., Anderson, T., Anton, G., Argüelles, C., Ashida, Y., Axani, S., Bai, X., V., A. Balagopal, Barbano, A., Barwick, S. W., Bastian, B., Basu, V., Baur, S., Bay, R., Beatty, J. J., Becker, K. -H., Tjus, J. Becker, Bellenghi, C., BenZvi, S., Berley, D., Bernardini, E., Besson, D. Z., Binder, G., Bindig, D., Blaufuss, E., Blot, S., Boddenberg, M., Bontempo, F., Borowka, J., Böser, S., Botner, O., Böttcher, J., Bourbeau, E., Bradascio, F., Braun, J., Brinson, B., Bron, S., Brostean-Kaiser, J., Browne, S., Burgman, A., Burley, R. T., Busse, R. S., Campana, M. A., Carnie-Bronca, E. G., Chen, C., Chen, Z., Chirkin, D., Choi, K., Clark, B. A., Clark, K., Classen, L., Collin, G. H., Conrad, J. M., Coppin, P., Correa, P., Cowen, D. F., Cross, R., Dappen, C., Dave, P., De Clercq, C., DeLaunay, J. J., López, D. Delgado, Dembinski, H., Deoskar, K., Desai, A., Desiati, P., de Vries, K. D., de Wasseige, G., de With, M., DeYoung, T., Diaz, A., Díaz-Vélez, J. C., Dittmer, M., Dujmovic, H., Dunkman, M., DuVernois, M. A., Dvorak, E., Ehrhardt, T., Eller, P., Erpenbeck, H., Evans, J., Evenson, P. A., Fan, K. L., Fazely, A. R., Fedynitch, A., Feigl, N., Fiedlschuster, S., Fienberg, A. T., Filimonov, K., Finley, C., Fischer, L., Fox, D., Franckowiak, A., Friedman, E., Fritz, A., Fürst, P., Gaisser, T. K., Gallagher, J., Ganster, E., Garcia, A., Garrappa, S., Gerhardt, L., Ghadimi, A., Glaser, C., Glauch, T., Glüsenkamp, T., Gonzalez, J. G., Goswami, S., Grant, D., Grégoire, T., Griswold, S., Günther, C., Gutjahr, P., Haack, C., Hallgren, A., Halliday, R., Halve, L., Halzen, F., Minh, M. Ha, Hanson, K., Hardin, J., Harnisch, A. A., Haungs, A., Hebecker, D., Helbing, K., Henningsen, F., Hettinger, E. C., Hickford, S., Hignight, J., Hill, C., Hill, G. C., Hoffman, K. 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A., Takagi, Y., Takahashi, Y., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Uchihori, Y., Udo, S., Uehama, T., Urban, F., Warren, D., Wong, T., Yamamoto, M., Yamazaki, K., Yashiro, K., Yoshida, F., Yoshioka, Y., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

For several decades, the origin of ultra-high-energy cosmic rays (UHECRs) has been an unsolved question of high-energy astrophysics. One approach for solving this puzzle is to correlate UHECRs with high-energy neutrinos, since neutrinos are a direct probe of hadronic interactions of cosmic rays and are not deflected by magnetic fields. In this paper, we present three different approaches for correlating the arrival directions of neutrinos with the arrival directions of UHECRs. The neutrino data is provided by the IceCube Neutrino Observatory and ANTARES, while the UHECR data with energies above $\sim$50 EeV is provided by the Pierre Auger Observatory and the Telescope Array. All experiments provide increased statistics and improved reconstructions with respect to our previous results reported in 2015. The first analysis uses a high-statistics neutrino sample optimized for point-source searches to search for excesses of neutrinos clustering in the vicinity of UHECR directions. The second analysis searches for an excess of UHECRs in the direction of the highest-energy neutrinos. The third analysis searches for an excess of pairs of UHECRs and highest-energy neutrinos on different angular scales. None of the analyses has found a significant excess, and previously reported over-fluctuations are reduced in significance. Based on these results, we further constrain the neutrino flux spatially correlated with UHECRs., Comment: 39 pages, 7 figures, 4 tables; updated source files including xml authorlist

Published
2022
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9. Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for Large-Scale Electric Field Changes

Author

Abbasi, R. U., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Fukushima, R., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashi, M., Hayashida, N., Hibino, K., Higuchi, R., Honda, K., Husseini, N., Ikeda, D., Inadomi, T., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwakura, H., Iwasaki, A., Jeong, H. M., Jeong, S., Johnson, H., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawai, H., Kawakami, S., Kawana, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, M. H., Kim, S. W., Kimura, Y., Kishigami, S., Kubota, Y., Kurisu, S., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., LeVon, R., Lubsandorzhiev, B., Lundquist, J. P., Machida, K., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Mazich, J., Minamino, M., Mukai, K., Myers, I., Myers, P., Nagataki, S., Nakai, K., Nakamura, R., Nakamura, T., Nakamura, Y., Nakazawa, A., Nishio, E., Nonaka, T., OBrien, K., Oda, H., Ogio, S., Ohnishi, M., Ohoka, H., Oku, Y., Okuda, T., Omura, Y., Ono, M., Onogi, R., Oshima, A., Ozawa, S., Park, I. H., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rubtsov, G. I., Ryu, D., Sagawa, H., Sahara, R., Saito, Y., Sakaki, N., Sako, T., Sakurai, N., Sano, K., Sato, K., Seki, T., Sekino, K., Shah, P. D., Shibasaki, Y., Shibata, F., Shibata, N., Shibata, T., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Sone, N., Stokes, B. T., Stroman, T. A., Takagi, Y., Takahashi, Y., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Uchihori, Y., Udo, S., Uehama, T., Urban, F., Wong, T., Yamamoto, M., Yamazaki, K., Yang, J., Yashiro, K., Yoshida, F., Yoshioka, Y., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment, Physics - Atmospheric and Oceanic Physics
Abstract

We present the first observation by the Telescope Array Surface Detector (TASD) of the effect of thunderstorms on the development of cosmic ray single count rate intensity over a 700 km$^{2}$ area. Observations of variations in the secondary low-energy cosmic ray counting rate, using the TASD, allow us to study the electric field inside thunderstorms, on a large scale, as it progresses on top of the 700 km$^{2}$ detector, without dealing with the limitation of narrow exposure in time and space using balloons and aircraft detectors. In this work, variations in the cosmic ray intensity (single count rate) using the TASD, were studied and found to be on average at the $\sim(0.5-1)\%$ and up to 2\% level. These observations were found to be both in excess and in deficit. They were also found to be correlated with lightning in addition to thunderstorms. These variations lasted for tens of minutes; their footprint on the ground ranged from 6 to 24 km in diameter and moved in the same direction as the thunderstorm. With the use of simple electric field models inside the cloud and between cloud to ground, the observed variations in the cosmic ray single count rate were recreated using CORSIKA simulations. Depending on the electric field model used and the direction of the electric field in that model, the electric field magnitude that reproduces the observed low-energy cosmic ray single count rate variations was found to be approximately between 0.2-0.4 GV. This in turn allows us to get a reasonable insight on the electric field and its effect on cosmic ray air showers inside thunderstorms.

Published
2021
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10. Indications of a Cosmic Ray Source in the Perseus-Pisces Supercluster

Author

Telescope Array Collaboration, Abbasi, R. U., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Fukushima, R., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashi, M., Hayashida, N., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inadomi, T., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwakura, H., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawai, H., Kawakami, S., Kawana, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, M. H., Kim, S. W., Kimura, Y., Kishigami, S., Kubota, Y., Kurisu, S., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Machida, K., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Minamino, M., Mukai, K., Myers, I., Nagataki, S., Nakai, K., Nakamura, R., Nakamura, T., Nakamura, Y., Nakazawa, A., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Ohnishi, M., Ohoka, H., Oku, Y., Okuda, T., Omura, Y., Ono, M., Onogi, R., Oshima, A., Ozawa, S., Park, I. H., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rubtsov, G. I., Ryu, D., Sagawa, H., Sahara, R., Saito, Y., Sakaki, N., Sako, T., Sakurai, N., Sano, K., Sato, K., Seki, T., Sekino, K., Shah, P. D., Shibasaki, Y., Shibata, F., Shibata, N., Shibata, T., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Sone, N., Stokes, B. T., Stroman, T. A., Takagi, Y., Takahashi, Y., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Uchihori, Y., Udo, S., Uehama, T., Urban, F., Wong, T., Yamamoto, M., Yamazaki, K., Yang, J., Yashiro, K., Yoshida, F., Yoshioka, Y., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The Telescope Array Collaboration has observed an excess of events with $E \ge 10^{19.4} ~{\rm eV}$ in the data which is centered at (RA, dec) = ($19^\circ$, $35^\circ$). This is near the center of the Perseus-Pisces supercluster (PPSC). The PPSC is about $70 ~{\rm Mpc}$ distant and is the closest supercluster in the Northern Hemisphere (other than the Virgo supercluster of which we are a part). A Li-Ma oversampling analysis with $20^\circ$-radius circles indicates an excess in the arrival direction of events with a local significance of about 4 standard deviations. The probability of having such excess close to the PPSC by chance is estimated to be 3.5 standard deviations. This result indicates that a cosmic ray source likely exists in that supercluster., Comment: 8 pages, 4 figures, 1 table

Published
2021

12. Factors limiting quantitative phase retrieval in atomic-resolution differential phase contrast scanning transmission electron microscopy using a segmented detector

Author

Mawson, T., Taplin, D. J., Brown, H. G., Clark, L., Ishikawa, R., Seki, T., Ikuhara, Y., Shibata, N., Paganin, D. M., Morgan, M. J., Weyland, M., Petersen, T. C., and Findlay, S. D.

Subjects
Condensed Matter - Materials Science
Abstract

Quantitative differential phase contrast imaging of materials in atomic-resolution scanning transmission electron microscopy using segmented detectors is limited by various factors, including coherent and incoherent aberrations, detector positioning and uniformity, and scan-distortion. By comparing experimental case studies of monolayer and few-layer graphene with image simulations, we explore which parameters require the most precise characterisation for reliable and quantitative interpretation of the reconstructed phases. Coherent and incoherent lens aberrations are found to have the most significant impact. For images over a large field of view, the impact of noise and non-periodic boundary conditions are appreciable, but in this case study have less of an impact than artefacts introduced by beam deflections coupling to beam scanning (imperfect tilt-shift purity)., Comment: 16 pages, 9 figures

Published
2021
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14. Surface detectors of the TAx4 experiment

Author

Telescope Array Collaboration, Abbasi, R. U., Abe, M., Abu-Zayyad, T., Allen, M., Arai, Y., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Fukushima, R., Furlich, G., Hanlon, W., Hayashi, M., Hayashida, N., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inadomi, T., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwakura, H., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawai, H., Kawakami, S., Kawana, S., Kawata, K., Kido, E., Kim, H. B., Kim, J. H., Kim, M. H., Kim, S. W., Kimura, Y., Kishigami, S., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Machida, K., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Minamino, M., Mukai, K., Myers, I., Nagataki, S., Nakai, K., Nakamura, R., Nakamura, T., Nakamura, Y., Nonaka, T., Oda, H., Ogio, S., Ohnishi, M., Ohoka, H., Oku, Y., Okuda, T., Omura, Y., Ono, M., Onogi, R., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rubtsov, G. I., Ryu, D., Sagawa, H., Sahara, R., Saito, Y., Sakaki, N., Sako, T., Sakurai, N., Sano, K., Sato, K., Seki, T., Sekino, K., Shah, P. D., Shibata, F., Shibata, N., Shibata, T., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Sone, N., Stokes, B. T., Stroman, T. A., Suzawa, T., Takagi, Y., Takahashi, Y., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Uchihori, Y., Udo, S., Uehama, T., Urban, F., Wong, T., Yada, K., Yamamoto, M., Yamazaki, K., Yang, J., Yashiro, K., Yoshida, F., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Instrumentation and Detectors
Abstract

Telescope Array (TA) is the largest ultrahigh energy cosmic-ray (UHECR) observatory in the Northern Hemisphere. It explores the origin of UHECRs by measuring their energy spectrum, arrival-direction distribution, and mass composition using a surface detector (SD) array covering approximately 700 km$^2$ and fluorescence detector (FD) stations. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV. In order to confirm this evidence with more data, it is necessary to increase the data collection rate.We have begun building an expansion of TA that we call TAx4. In this paper, we explain the motivation, design, technical features, and expected performance of the TAx4 SD. We also present TAx4's current status and examples of the data that have already been collected., Comment: 26 pages, 17 figures, submitted to Nuclear Inst. and Methods in Physics Research, A

Published
2021
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15. Suppressing dynamical diffraction artefacts in differential phase contrast scanning transmission electron microscopy of long-range electromagnetic fields via precession

Author

Mawson, T., Nakamura, A., Petersen, T. C., Shibata, N., Sasaki, H., Paganin, D. M., Morgan, M. J., and Findlay, S. D.

Subjects
Condensed Matter - Materials Science
Abstract

In differential phase contrast scanning transmission electron microscopy (DPC-STEM), variability in dynamical diffraction resulting from changes in sample thickness and local crystal orientation (due to sample bending) can produce contrast comparable to that arising from the long-range electromagnetic fields probed by this technique. Through simulation we explore the scale of these dynamical diffraction artefacts and introduce a metric for the magnitude of their confounding contribution to the contrast. We show that precession over an angular range of a few milliradian can suppress this confounding contrast by one-to-two orders of magnitude. Our exploration centres around a case study of GaAs near the [011] zone-axis orientation using a probe-forming aperture semiangle on the order of 0.1 mrad at 300 keV, but the trends found and methodology used are expected to apply more generally., Comment: 12 pages, 9 figures, submitted to Ultramicroscopy

Published
2020

16. The energy spectrum of cosmic rays measured by the Telescope Array using 10 years of fluorescence detector data

Author

Abbasi, R.U., Abe, Y., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J.W., Bergman, D.R., Blake, S.A., Buckland, I., Cheon, B.G., Chikawa, M., Fedynitch, A., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Furlich, G., Gerber, Z., Globus, N., Hanlon, W., Hayashida, N., He, H., Hibi, R., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwasaki, A., Jeong, H.M., Jeong, S., Jui, C.C.H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawakami, S., Kawata, K., Kharuk, I., Kido, E., Kim, H.B., Kim, J.H., Kim, S.W., Kimura, Y., Komae, I., Komori, K., Kusumori, Y., Kuznetsov, M., Kwon, Y.J., Lee, K.H., Lee, M.J., Lubsandorzhiev, B., Lundquist, J.P., Matsuyama, T., Matthews, J.A., Matthews, J.N., Mayta, R., Miyashita, K., Mizuno, K., Mori, M., Murakami, M., Myers, I., Nagataki, S., Nakai, K., Nakamura, T., Nishio, E., Nonaka, T., Ogio, S., Ohoka, H., Okazaki, N., Oku, Y., Okuda, T., Omura, Y., Onishi, M., Ono, M., Oshima, A., Oshima, H., Ozawa, S., Park, I.H., Park, K.Y., Potts, M., Pshirkov, M.S., Remington, J., Rodriguez, D.C., Rott, C., Rubtsov, G.I., Ryu, D., Sagawa, H., Saito, R., Sakaki, N., Sako, T., Sakurai, N., Sato, D., Sato, K., Sato, S., Sekino, K., Shah, P.D., Shibata, N., Shibata, T., Shikita, J., Shimodaira, H., Shin, B.K., Shin, H.S., Shinto, D., Smith, J.D., Sokolsky, P., Stokes, B.T., Stroman, T.A., Takagi, Y., Takahashi, K., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, K., Tanaka, M., Thomas, S.B., Thomson, G.B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Udo, S., Urban, F., Vaiman, I.A., Warren, D., Wong, T., Yamazaki, K., Yashiro, K., Yoshida, F., Zhezher, Y., and Zundel, Z.

Published
2023
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18. Evidence for Declination Dependence of the Ultrahigh Energy Cosmic Ray Spectrum in the Northern Hemisphere

Author

Abbasi, R. U., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Fukushima, R., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashi, M., Hayashida, N., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inadomi, T., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwakura, H., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawai, H., Kawakami, S., Kawana, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, M. H., Kim, S. W., Kimura, Y., Kishigami, S., Kubota, Y., Kurisu, S., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Machida, K., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Minamino, M., Mukai, K., Myers, I., Nagataki, S., Nakai, K., Nakamura, R., Nakamura, T., Nakamura, Y., Nakazawa, A., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Ohnishi, M., Ohoka, H., Oku, Y., Okuda, T., Omura, Y., Ono, M., Onogi, R., Oshima, A., Ozawa, S., Park, I. H., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rubtsov, G. I., Ryu, D., Sagawa, H., Sahara, R., Saito, Y., Sakaki, N., Sako, T., Sakurai, N., Sano, K., Sato, K., Seki, T., Sekino, K., Shah, P. D., Shibasaki, Y., Shibata, F., Shibata, N., Shibata, T., Shimodaira, H., Shin, B. K., Shin, H. S., Shinto, D., Smith, J. D., Sokolsky, P., Sone, N., Stokes, B. T., Stroman, T. A., Takagi, Y., Takahashi, Y., Takamura, M., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Tanoue, Y., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsuda, R., Tsunesada, Y., Uchihori, Y., Udo, S., Uehama, T., Urban, F., Wong, T., Yamamoto, M., Yamazaki, K., Yang, J., Yashiro, K., Yoshida, F., Yoshioka, Y., Zhezher, Y., and Zundel, Z.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Telescope Array (TA) is the largest experiment in the Northern Hemisphere studying ultrahigh energy cosmic rays. TA measurements of the cosmic ray spectrum using the surface detector have the best statistical power in the experiment, and observe the ankle of the spectrum and the high energy cutoff. When the data are divided into two declination bands, above and below 24.8 degrees, the cutoff appears at $10^{19.64 \pm 0.04}$ ($10^{19.84 \pm 0.02}$) eV in the lower (higher) band, an energy difference of 58\%. The global significance of the difference is 4.3 standard deviations. The lack of an instrumental cause of this difference implies it is astrophysical in nature.

Published
2018

19. Probing the limits of the rigid-intensity-shift model in differential phase contrast scanning transmission electron microscopy

Author

Clark, L., Brown, H. G., Paganin, D. M., Morgan, M. J., Matsumoto, T., Shibata, N., Petersen, T. C., and Findlay, S. D.

Subjects
Physics - Instrumentation and Detectors
Abstract

The rigid-intensity-shift model of differential phase contrast scanning transmission electron microscopy (DPC-STEM) imaging assumes that the phase gradient imposed on the probe by the sample causes the diffraction pattern intensity to shift rigidly by an amount proportional to that phase gradient. This behaviour is seldom realised exactly in practice. Through a combination of experimental results, analytical modelling and numerical calculations, we explore the breakdown of the rigid-intensity-shift behaviour and how this depends on the magnitude of the phase gradient and the relative scale of features in the phase profile and the probe size. We present guidelines as to when the rigid-intensity-shift model can be applied for quantitative phase reconstruction using segmented detectors, and propose probe-shaping strategies to further improve the accuracy., Comment: 13 pages

Published
2018
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23. DHCAL with Minimal Absorber: Measurements with Positrons

Author

The CALICE Collaboration, Freund, B., Neubüser, C., Repond, J., Schlereth, J., Xia, L., Dotti, A., Grefe, C., Ivantchenko, V., Antequera, J. Berenguer, Alamillo, E. Calvo, Fouz, M. -C., Marin, J., Puerta-Pelayo, J., Verdugo, A., Brianne, E., Ebrahimi, A., Gadow, K., Göttlicher, P., Günter, C., Hartbrich, O., Hermberg, B., Irles, A., Krivan, F., Krüger, K., Kvasnicka, J., Lu, S., Lutz, B., Morgunov, V., Provenza, A., Reinecke, M., Sefkow, F., Schuwalow, S., Tran, H. L., Garutti, E., Laurien, S., Matysek, M., Ramilli, M., Schroeder, S., Bilki, B., Norbeck, E., Northacker, D., Onel, Y., Cvach, J., Gallus, P., Havranek, M., Janata, M., Kovalcuk, M., Lednicky, D., Marcisovsky, M., Polak, I., Popule, J., Tomasek, L., Tomasek, M., Sicho, P., Smolik, J., Vrba, V., Zalesak, J., van Doren, B., Wilson, G. W., Kawagoe, K., Miyazaki, Y., Sudo, Y., Suehara, T., Tomita, T., Ueno, H., Yoshioka, T., Bilokin, S., Bonis, J., Cornebise, P., Pöschl, R., Richard, F., Thiebault, A., Zerwas, D., Hostachy, J. -Y., Morin, L., Besson, D., Chadeeva, M., Danilov, M., Markin, O., Popova, E., Gabriel, M., Goecke, P., Kiesling, C., van der Kolk, N., Simon, F., Szalay, M., Corriveau, F., Blazey, G. C., Dyshkant, A., Francis, K., Zutshi, V., Kotera, K., Ono, H., Takeshita, T., Ieki, S., Kamiya, Y., Ootani, W., Shibata, N., Jeans, D., Komamiya, S., and Nakanishi, H.

Subjects
Physics - Instrumentation and Detectors
Abstract

In special tests, the active layers of the CALICE Digital Hadron Calorimeter prototype, the DHCAL, were exposed to low energy particle beams, without being interleaved by absorber plates. The thickness of each layer corresponded approximately to 0.29 radiation lengths or 0.034 nuclear interaction lengths, defined mostly by the copper and steel skins of the detector cassettes. This paper reports on measurements performed with this device in the Fermilab test beam with positrons in the energy range of 1 to 10 GeV. The measurements are compared to simulations based on GEANT4 and a standalone program to emulate the detailed response of the active elements.

Published
2016
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24. Hadron shower decomposition in the highly granular CALICE analogue hadron calorimeter

Author

The CALICE Collaboration, Eigen, G., Price, T., Watson, N. K., Marshall, J. S., Thomson, M. A., Ward, D. R., Benchekroun, D., Hoummada, A., Khoulaki, Y., Apostolakis, J., Dotti, A., Folger, G., Ivantchenko, V., Ribon, A., Uzhinskiy, V., Hostachy, J. -Y., Morin, L., Brianne, E., Ebrahimi, A., Gadow, K., Göttlicher, P., Günter, C., Hartbrich, O., Hermberg, B., Irles, A., Krivan, F., Krüger, K., Kvasnicka, J., Lu, S., Lutz, B., Morgunov, V., Neubüser, C., Provenza, A., Reinecke, M., Sefkow, F., Schuwalow, S., Tran, H. L., Garutti, E., Laurien, S., Matysek, M., Ramilli, M., Schroeder, S., Briggl, K., Eckert, P., Munwes, Y., Schultz-Coulon, H. -Ch., Shen, W., Stamen, R., Bilki, B., Norbeck, E., Northacker, D., Onel, Y., van Doren, B., Wilson, G. W., Kawagoe, K., Hirai, H., Sudo, Y., Suehara, T., Sumida, H., Takada, S., Tomita, T., Yoshioka, T., Wing, M., Bonnevaux, A., Combaret, C., Caponetto, L., Grenier, G., Han, R., Ianigro, J. C., Kieffer, R., Laktineh, I., Lumb, N., Mathez, H., Mirabito, L., Steen, A., Antequera, J. Berenguer, Alamillo, E. Calvo, Fouz, M. -C., Marin, J., Puerta-Pelayo, J., Verdugo, A., Bobchenko, B., Markin, O., Novikov, E., Rusinov, V., Tarkovsky, E., Kirikova, N., Kozlov, V., Smirnov, P., Soloviev, Y., Besson, D., Buzhan, P., Chadeeva, M., Danilov, M., Drutskoy, A., Ilyin, A., Mironov, D., Mizuk, R., Popova, E., Gabriel, M., Goecke, P., Kiesling, C., van der Kolk, N., Simon, F., Szalay, M., Bilokin, S., Bonis, J., Cornebise, P., Pöschl, R., Richard, F., Thiebault, A., Zerwas, D., Anduze, M., Balagura, V., Becheva, E., Boudry, V., Brient, J-C., Cizel, J-B., Clerc, C., Cornat, R., Frotin, M., Gastaldi, F., Magniette, F., de Freitas, P. Mora, Musat, G., Pavy, S., Rubio-Roy, M., Ruan, M., Videau, H., Callier, S., Dulucq, F., Martin-Chassard, G., Raux, L., Seguin-Moreau, N., de la Taille, Ch., Cvach, J., Gallus, P., Havranek, M., Janata, M., Lednicky, D., Marcisovsky, M., Polak, I., Popule, J., Tomasek, L., Tomasek, M., Sicho, P., Smolik, J., Vrba, V., Zalesak, J., Kotera, K., Ono, H., Takeshita, T., Ieki, S., Kamiya, Y., Ootani, W., Shibata, N., Jeans, D., Komamiya, S., and Nakanishi, H.

Subjects
Physics - Instrumentation and Detectors
Abstract

The spatial development of hadronic showers in the CALICE scintillator-steel analogue hadron calorimeter is studied using test beam data collected at CERN and FNAL for single positive pions and protons with initial momenta in the range from 10 to 80 GeV/c. Both longitudinal and radial development of hadron showers are parametrised with two-component functions. The parametrisation is fit to test beam data and simulations using the QGSP_BERT and FTFP_BERT physics lists from Geant4 version 9.6. The parameters extracted from data and simulated samples are compared for the two types of hadrons. The response to pions and the ratio of the non-electromagnetic to the electromagnetic calorimeter response, h/e, are estimated using the extrapolation and decomposition of the longitudinal profiles., Comment: 38 pages, 19 figures, 5 tables; author list changed; submitted to JINST

Published
2016
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25. Exact non-magnetic ground state and residual entropy of S = 1/2 Heisenberg diamond spin lattices

Author

Morita, K. and Shibata, N.

Subjects
Condensed Matter - Strongly Correlated Electrons, Condensed Matter - Materials Science
Abstract

Exactly solvable frustrated quantum spin models consisting of a diamond unit structure are presented. The ground states are characterized by tetramer-dimer states with a macroscopic degeneracy in a certain range of isotropic exchange interaction. The lower bound of the excitation gap is exactly calculated to be finite and the bulk entropy in the limit of zero temperature remains finite depending on the shape of the boundary of system. Residual entropy is in a range of 0~6.1% of the entropy at high temperature for hexagonal diamond lattice and 0~8.4% for square diamond lattice. These diamond lattices are generalized to any dimensions and it is likely to be synthesized experimentally., Comment: 4 pages, 5 figures

Published
2015
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26. Shower development of particles with momenta from 15 GeV to 150 GeV in the CALICE scintillator-tungsten hadronic calorimeter

Author

The CALICE collaboration, Chefdeville, M., Karyotakis, Y., Repond, J., Schlereth, J., Xia, L., Eigen, G., Marshall, J. S., Thomson, M. A., Ward, D. R., Tehrani, N. Alipour, Apostolakis, J., Dannheim, D., Elsener, K., Folger, G., Grefe, C., Ivantchenko, V., Killenberg, M., Klempt, W., van der Kraaij, E., Linssen, L., Lucaci-Timoce, A. -I., Münnich, A., Poss, S., Ribon, A., Roloff, P., Sailer, A., Schlatter, D., Sicking, E., Strube, J., Uzhinskiy, V., Chang, S., Khan, A., Kim, D. H., Kong, D. J., Oh, Y. D., Blazey, G. C., Dyshkant, A., Francis, K., Zutshi, V., Giraud, J., Grondin, D., Hostachy, J. -Y., Brianne, E., Cornett, U., David, D., Falley, G., Gadow, K., Göttlicher, P., Günter, C., Hartbrich, O., Hermberg, B., Irles, A., Karstensen, S., Krivan, F., Krüger, K., Kvasnicka, J., Lu, S., Lutz, B., Morozov, S., Morgunov, V., Neubüser, C., Provenza, A., Reinecke, M., Sefkow, F., Smirnov, P., Terwort, M., Tran, H. L., Vargas-Trevino, A., Garutti, E., Laurien, S., Matysek, M., Ramilli, M., Schröder, S., Briggl, K., Eckert, P., Harion, T., Munwes, Y., Schultz-Coulon, H. -Ch., Shen, W., Stamen, R., Bilki, B., Onel, Y., Kawagoe, K., Hirai, H., Sudo, Y., Suehara, T., Sumida, H., Takada, S., Tomita, T., Yoshioka, T., Wing, M., Alamillo, E. Calvo, Fouz, M. -C., Marin, J., Puerta-Pelayo, J., Verdugo, A., Bobchenko, B., Chadeeva, M., Danilov, M., Markin, O., Mizuk, R., Novikov, E., Rusinov, V., Tarkovsky, E., Kirikova, N., Kozlov, V., Soloviev, Y., Besson, D., Buzhan, P., Popova, E., Gabriel, M., Kiesling, C., van der Kolk, N., Seidel, K., Simon, F., Soldner, C., Szalay, M., Tesar, M., Weuste, L., Amjad, M. S., Bonis, J., Cornebise, P., Richard, F., Pöschl, R., Rouëné, J., Thiebault, A., Anduze, M., Balagura, V., Boudry, V., Brient, J-C., Cizel, J-B., Cornat, R., Frotin, M., Gastaldi, F., Haddad, Y., Magniette, F., Nanni, J., Pavy, S., Rubio-Roy, M., Shpak, K., Tran, T. H., Videau, H., Yu, D., Callier, S., di Lorenzo, S. Conforti, Dulucq, F., Fleury, J., Martin-Chassard, G., de la Taille, Ch., Raux, L., Seguin-Moreau, N., Cvach, J., Gallus, P., Havranek, M., Janata, M., Kovalcuk, M., Lednicky, D., Marcisovsky, M., Polak, I., Popule, J., Tomasek, L., Tomasek, M., Ruzicka, P., Sicho, P., Smolik, J., Vrba, V., Zalesak, J., Ieki, S., Kamiya, Y., Ootani, W., Shibata, N., Chen, S., Jeans, D., Komamiya, S., Kozakai, C., Nakanishi, H., Götze, M., Sauer, J., Weber, S., and Zeitnitz, C.

Subjects
Physics - Instrumentation and Detectors, High Energy Physics - Experiment
Abstract

We present a study of showers initiated by electrons, pions, kaons, and protons with momenta from 15 GeV to 150 GeV in the highly granular CALICE scintillator-tungsten analogue hadronic calorimeter. The data were recorded at the CERN Super Proton Synchrotron in 2011. The analysis includes measurements of the calorimeter response to each particle type as well as measurements of the energy resolution and studies of the longitudinal and radial shower development for selected particles. The results are compared to Geant4 simulations (version 9.6.p02). In the study of the energy resolution we include previously published data with beam momenta from 1 GeV to 10 GeV recorded at the CERN Proton Synchrotron in 2010., Comment: 35 pages, 21 figures, 8 tables

Published
2015
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27. NMR profiling of quantum electron solids in high magnetic fields

Author

Tiemann, L., Rhone, T. D., Shibata, N., and Muraki, K.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics, Condensed Matter - Strongly Correlated Electrons
Abstract

When the motion of electrons is restricted to a plane under a perpendicular magnetic field B, a variety of quantum phases emerge at low temperatures whose properties are dictated by the Coulomb interaction and its interplay with disorder. At very strong B, the sequence of fractional quantum Hall (FQH) liquid phases terminates in an insulating phase, which is widely believed to be due to the solidification of electrons into domains possessing Wigner crystal (WC) order. The existence of such WC domains is signaled by the emergence of microwave pinning-mode resonances, which reflect the mechanical properties characteristic of a solid. However, the most direct manifestation of the broken translational symmetry accompanying the solidification - the spatial modulation of particles' probability amplitude - has not been observed yet. Here, we demonstrate that nuclear magnetic resonance (NMR) provides a direct probe of the density topography of electron solids in the integer and fractional quantum Hall regimes. The data uncover quantum and thermal fluctuation of lattice electrons resolved on the nanometre scale. Our results pave the way to studies of other exotic phases with non-trivial spatial spin/charge order., Comment: A revised version with additional data has been published in Nature Physics 10, 648 (2014)

Published
2014
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28. Impact of the size-dependent difference of excimer laser coronary angioplasty in ST-elevation acute myocardial infarction; nuclear scintigraphy findings

Author

Shibata, N, primary, Ohi, T, additional, Morita, Y, additional, Kanzaki, Y, additional, Watanabe, N, additional, Yoshioka, N, additional, Arao, Y, additional, Miyazawa, H, additional, Shimojo, K, additional, Goto, H, additional, Karasawa, H, additional, Nakagawa, Y, additional, and Morishima, I, additional

Published
2023
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30. Corrigendum to ‘A phase II trial of paclitaxel plus biweekly cetuximab for patients with recurrent or metastatic head and neck cancer previously treated with both platinum-based chemotherapy and anti-PD-1 antibody’: [ESMO Open volume 9 issue 6 (2024) 103476]

Author

Koyama, T., Kiyota, N., Boku, S., Imamura, Y., Shibata, N., Satake, H., Tanaka, K., Hayashi, H., Onoe, T., Asada, Y., Yamazaki, T., Nose, T., Ohata, S., Nagatani, Y., Kimbara, S., Funakoshi, Y., Teshima, M., Shinomiya, H., and Minami, H.

Published
2024
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33. Spin-Orbit Interaction Enhanced Fractional Quantum Hall States in the Second Landau Level

Author

Ito, T., Nomura, K., and Shibata, N.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

We study the fractional quantum Hall effect at filling fractions 7/3 and 5/2 in the presence of the spin-orbit interaction, using the exact diagonalization method and the density matrix renormalization group (DMRG) method in a spherical geometry. Trial wave functions at these fillings are the Laughlin state and the Moore-Reed-Pfaffian state. The ground state excitation energy gaps and pair-correlation functions at fractional filling factor 7/3 and 5/2 in the second Landau level are calculated. We find that the spin-orbit interaction stabilizes the fractional quantum Hall states., Comment: 4pages, 4figures

Published
2010
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34. Collapse of the fractional quantum Hall state by a unidirectional periodic potential modulation

Author

Endo, A., Shibata, N., and Iye, Y.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

We have investigated the effect of unidirectional periodic potential modulation on the fractional quantum Hall (FQH) states located within the filling factor range $1<\nu<2$. We find that odd-numerator FQH states are strongly suppressed, while the even-numerator ones are less affected or even enhanced, by the introduction of the modulation. In the picture of the composite fermions (CFs), the behaviors are equivalent to the suppression of the spin splitting of the CFs by the modulation. We discuss the origin of the suppression and the possible modulation-induced phase transition from the FQH state to the stripe state., Comment: 4 pages, 4 figures, EP2DS-18

Published
2009
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35. First High‐Speed Video Camera Observations of a Lightning Flash Associated With a Downward Terrestrial Gamma‐Ray Flash

Author

Abbasi, R. U., primary, Saba, M. M. F., additional, Belz, J. W., additional, Krehbiel, P. R., additional, Rison, W., additional, Kieu, N., additional, da Silva, D. R., additional, Stanley, M. A., additional, Rodeheffer, Dan, additional, Remington, J., additional, Mazich, J., additional, LeVon, R., additional, Smout, K., additional, Petrizze, A., additional, Abu‐Zayyad, T., additional, Allen, M., additional, Arimura, R., additional, Barcikowski, E., additional, Bergman, D. R., additional, Blake, S. A., additional, Buckland, I., additional, Cheon, B. G., additional, Chikawa, M., additional, Fujii, T., additional, Fujisue, K., additional, Fujita, K., additional, Fujiwara, R., additional, Fukushima, M., additional, Furlich, G., additional, Globus, N., additional, Gonzalez, R., additional, Hanlon, W., additional, Hayashida, N., additional, He, H., additional, Hibino, K., additional, Higuchi, R., additional, Honda, K., additional, Ikeda, D., additional, Inoue, N., additional, Ishii, T., additional, Ito, H., additional, Ivanov, D., additional, Iwakura, H., additional, Iwasaki, A., additional, Jeong, H. M., additional, Jeong, S., additional, Jui, C. C. H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kasahara, K., additional, Kasami, S., additional, Kawakami, S., additional, Kawata, K., additional, Kharuk, I., additional, Kido, E., additional, Kim, H. B., additional, Kim, J. H., additional, Kim, S. W., additional, Kimura, Y., additional, Komae, I., additional, Kubota, Y., additional, Kuznetsov, M., additional, Kwon, Y. J., additional, Lee, K. H., additional, Lubsandorzhiev, B., additional, Lundquist, J. P., additional, Matsuyama, T., additional, Matthews, J. N., additional, Mayta, R., additional, Myers, I., additional, Nagataki, S., additional, Nakai, K., additional, Nakamura, R., additional, Nakamura, T., additional, Nakazawa, A., additional, Nishio, E., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oku, Y., additional, Okuda, T., additional, Omura, Y., additional, Ono, M., additional, Oshima, A., additional, Ozawa, S., additional, Park, I. H., additional, Potts, M., additional, Pshirkov, M. S., additional, Rodriguez, D. C., additional, Rott, C., additional, Rubtsov, G. I., additional, Ryu, D., additional, Sagawa, H., additional, Sakaki, N., additional, Sako, T., additional, Sakurai, N., additional, Sato, K., additional, Seki, T., additional, Sekino, K., additional, Shah, P. D., additional, Shibasaki, Y., additional, Shibata, N., additional, Shibata, T., additional, Shikita, J., additional, Shimodaira, H., additional, Shin, B. K., additional, Shin, H. S., additional, Shinto, D., additional, Smith, J. D., additional, Sokolsky, P., additional, Stokes, B. T., additional, Stroman, T. A., additional, Takahashi, K., additional, Takamura, M., additional, Takeda, M., additional, Takeishi, R., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S. B., additional, Thomson, G. B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsuda, R., additional, Tsunesada, Y., additional, Udo, S., additional, Uehama, T., additional, Urban, F., additional, Warren, D., additional, Wong, T., additional, Yamamoto, M., additional, Yamazaki, K., additional, Yashiro, K., additional, Yoshida, F., additional, Zhezher, Y., additional, and Zundel, Z., additional

Published
2023
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37. Theory of Fano-Kondo effect in quantum dot systems: temperature dependence of the Fano line shapes

Author

Maruyama, I., Shibata, N., and Ueda, K.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics
Abstract

The Fano-Kondo effect in zero-bias conductance is studied based on a theoretical model for the T-shaped quantum dot by the finite temperature density matrix renormalization group method. The modification of the two Fano line shapes at much higher temperatures than the Kondo temperature is also investigated by the effective Fano parameter estimated as a fitting parameter., Comment: 2 pages, 2 figures, the proceeding of SCES'05

Published
2006
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38. Ground State Phase Diagram of 2D Electrons in High Magnetic Field

Author

Shibata, N. and Yoshioka, D.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics, Condensed Matter - Strongly Correlated Electrons
Abstract

The ground state of 2D electrons in high magnetic field is studied by the density matrix renormalization group method. The ground state energy, excitation gap, and pair correlation functions are systematically calculated at various fillings in the lowest and the second lowest Landau levels. The ground state phase diagram, which consists of incompressible liquid state, compressible liquid state, stripe state, pairing state, and Wigner crystal is determined., Comment: 10 pages, 21 figures, to appear in J. Phys. Soc. Jpn. Vol.72 No.3

Published
2002
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39. Thermodynamic Properties of the S=1/2 Heisenberg Chain with Staggered Dzyaloshinsky-Moriya Interaction

Author

Shibata, N. and Ueda, K.

Subjects
Condensed Matter - Strongly Correlated Electrons, Condensed Matter - Statistical Mechanics
Abstract

Thermodynamic properties of the S=1/2 Heisenberg chain in transverse staggered magnetic field H^y_s and uniform magnetic field H^x perpendicular to the staggered field is studied by the finite-temperature density-matrix renormalization-group method. The uniform and staggered magnetization and specific heat are calculated from zero temperature to high temperatures up to T/J=4 under various strength of magnetic fields from H^y_s/J, H^x/J=0 to 2.4. The specific heat and magnetization of the effective Hamiltonian of the Yb_4As_3 are also presented, and field induced gap formation and diverging magnetic susceptibility at low temperature are shown., Comment: 5 pages, 9 figures

Published
2001
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40. Ground state phase diagram of 2D electrons in a high Landau level: - DMRG study

Author

Shibata, N. and Yoshioka, D.

Subjects
Condensed Matter - Mesoscale and Nanoscale Physics, Condensed Matter - Strongly Correlated Electrons
Abstract

The ground state phase diagram of 2D electrons in a high Landau level (index N=2) is studied by the density matrix renormalization group method. Pair correlation functions are systematically calculated for various filling factors from v=1/8 to 1/2. It is shown that the ground state phase diagram consists of three different CDW states called stripe-phase, bubble-phase, and Wigner crystal. The boundary between the stripe and the bubble phases is determined to be v_c = 0.38, and that for the bubble phase and Wigner crystal is v_c = 0.24. Each transition is of first order., Comment: 4 pages, 6 figures

Published
2001
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42. Dynamic correlations in doped 1D Kondo insulator: Finite-T DMRG study

Author

Shibata, N. and Tsunetsugu, H.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

The finite-T DMRG method is applied to the one-dimensional Kondo lattice model to calculate dynamic correlation functions. Dynamic spin and charge correlations, S_f(omega), S_c(omega), and N_c(omega), and quasiparticle density of states rho(omega) are calculated in the paramagnetic metallic phase for various temperatures and hole densities. Near half filling, it is shown that a pseudogap grows in these dynamic correlation functions below the crossover temperature characterized by the spin gap at half filling. A sharp peak at omega=0 evolves at low temperatures in S_f(omega) and N_c(omega). This may be an evidence of the formation of the collective excitations, and this confirms that the metallic phase is a Tomonaga-Luttinger liquid in the low temperature limit., Comment: 5 pages, 6 Postscript figures, REVTeX

Published
1999
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43. Efficiency of symmetric targeting for finite-T DMRG

Author

Nishino, T. and Shibata, N.

Subjects
Condensed Matter - Statistical Mechanics, Condensed Matter - Strongly Correlated Electrons
Abstract

Two targeting schemes have been known for the density matrix renormalization group (DMRG) applied to non-Hermitian problems; one uses an asymmetric density matrix and the other uses symmetric density matrix. We compare the numerical efficiency of these two targeting schemes when they are used for the finite temperature DMRG., Comment: 4 pages, 3 Postscript figures, REVTeX

Published
1999
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44. Thermodynamics of doped Kondo insulator in one dimension: Finite Temperature DMRG Study

Author

Shibata, N. and Tsunetsugu, H.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

The finite-temperature density-matrix renormalization-group method is applied to the one-dimensional Kondo lattice model near half filling to study its thermodynamics. The spin and charge susceptibilities and entropy are calculated down to T=0.03t. We find two crossover temperatures near half filling. The higher crossover temperature continuously connects to the spin gap at half filling, and the susceptibilities are suppressed around this temperature. At low temperatures, the susceptibilities increase again with decreasing temperature when doping is finite. We confirm that they finally approach to the values obtained in the Tomonaga-Luttinger (TL) liquid ground state for several parameters. The crossover temperature to the TL liquid is a new energy scale determined by gapless excitations of the TL liquid. The transition from the metallic phase to the insulating phase is accompanied by the vanishing of the lower crossover temperature., Comment: 4 pages, 7 Postscript figures, REVTeX

Published
1998
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45. Thermodynamics of the t-J Ladder: A Stable Finite Temperature Density Matrix Renormalization Group Calculation

Author

Ammon, Beat, Troyer, Matthias, Rice, T. M., and Shibata, N.

Subjects
Condensed Matter
Abstract

Accurate numerical simulations of a doped t-J model on a two-leg ladder are presented for the particle number, chemical potential, magnetic susceptibility and entropy in the limit of large exchange coupling on the rung using a finite temperature density matrix renormalization group (TDMRG) method. This required an improved algorithm to achieve numerical stability down to low temperatures. The thermal dissociation of hole pairs and of the rung singlets are separately observed and the evolution of the hole pair binding energy and magnon spin gap with hole doping is determined., Comment: 4 pages, RevTex V3.0, includes 4 eps figures

Published
1998
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46. Spin, Charge and Quasiparticle Gaps in the One-Dimensional Kondo Lattice with f^2 Configuration

Author

Watanabe, S., Kuramoto, Y., Nishino, T., and Shibata, N.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

The ground state properties of the one-dimensional Kondo lattice with an f^2 configuration at each site are studied by the density matrix renormalization group method. At half-filling, competition between the Kondo exchange J and the antiferromagnetic intra f-shell exchange I leads to reduction of energy gaps for spin, quasi-particle and charge excitations. The attractive force among conduction electrons is induced by the competition and the bound state is formed. As J/I increases the f^2 singlet gives way to the Kondo singlet as the dominant local correlation. The remarkable change of the quasi-particle gap is driven by the change of the spin-1/2 excitation character from the itinerant one to the localized one. Possible metal-insulator transition is discussed which may occur as the ratio J/I is varied by reference to mean-field results in the f^2 lattice system and the two impurity Kondo system., Comment: 7 pages, 7 figures, submitted to J. Phys. Soc. Jpn

Published
1998
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47. Lessons learned after three years of SPIDER operation and the first MITICA integrated tests

Author

Marcuzzi, D., primary, Toigo, V., additional, Boldrin, M., additional, Chitarin, G., additional, Dal Bello, S., additional, Grando, L., additional, Luchetta, A., additional, Pasqualotto, R., additional, Pavei, M., additional, Serianni, G., additional, Zanotto, L., additional, Agnello, R., additional, Agostinetti, P., additional, Agostini, M., additional, Aprile, D., additional, Barbisan, M., additional, Battistella, M., additional, Berton, G., additional, Bigi, M., additional, Brombin, M., additional, Candela, V., additional, Candeloro, V., additional, Canton, A., additional, Casagrande, R., additional, Cavallini, C., additional, Cavazzana, R., additional, Cordaro, L., additional, Cruz, N., additional, Dalla Palma, M., additional, Dan, M., additional, De Lorenzi, A., additional, Delogu, R., additional, De Muri, M., additional, De Nardi, M., additional, Denizeau, S., additional, Fadone, M., additional, Fellin, F., additional, Ferro, A., additional, Gaio, E., additional, Gasparrini, C., additional, Gnesotto, F., additional, Jain, P., additional, La Rosa, A., additional, Lopez-Bruna, D., additional, Lorenzini, R., additional, Maistrello, A., additional, Manduchi, G., additional, Manfrin, S., additional, Marconato, N., additional, Mario, I., additional, Martini, G., additional, Milazzo, R., additional, Patton, T., additional, Peruzzo, S., additional, Pilan, N., additional, Pimazzoni, A., additional, Poggi, C., additional, Pomaro, N., additional, Pouradier-Duteil, B., additional, Recchia, M., additional, Rigoni-Garola, A., additional, Rizzetto, D., additional, Rizzolo, A., additional, Santoro, F., additional, Sartori, E., additional, Segalini, B., additional, Shepherd, A., additional, Siragusa, M., additional, Sonato, P., additional, Sottocornola, A., additional, Spada, E., additional, Spagnolo, S., additional, Spolaore, M., additional, Taliercio, C., additional, Tinti, P., additional, Tomsič, P., additional, Trevisan, L., additional, Ugoletti, M., additional, Valente, M., additional, Valisa, M., additional, Veronese, F., additional, Vignando, M., additional, Zaccaria, P., additional, Zagorski, R., additional, Zaniol, B., additional, Zaupa, M., additional, Zuin, M., additional, Cavenago, M., additional, Boilson, D., additional, Rotti, C., additional, Decamps, H., additional, Geli, F., additional, Sharma, A., additional, Veltri, P., additional, Zacks, J., additional, Simon, M., additional, Paolucci, F., additional, Garbuglia, A., additional, Gutierrez, D., additional, Masiello, A., additional, Mico, G., additional, Labate, C., additional, Readman, P., additional, Bragulat, E., additional, Bailly-Maitre, L., additional, Gomez, G., additional, Kouzmenko, G., additional, Albajar, F., additional, Kashiwagi, M., additional, Tobari, H., additional, Kojima, A., additional, Murayama, M., additional, Hatakeyama, S., additional, Oshita, E., additional, Maejima, T., additional, Shibata, N., additional, Yamashita, Y., additional, Watanabe, K., additional, Singh, N.P., additional, Singh, M.J., additional, Dhola, H., additional, Fantz, U., additional, Heinemann, B., additional, Wimmer, C., additional, Wünderlich, D., additional, Tsumori, K., additional, Croci, G., additional, Gorini, G., additional, Muraro, A., additional, Rebai, M., additional, Tardocchi, M., additional, Giacomelli, L., additional, Rigamonti, D., additional, Taccogna, F., additional, Bruno, D., additional, Rutigliano, M., additional, Longo, S., additional, Deambrosis, S., additional, Miorin, E., additional, Montagner, F., additional, Tonti, A., additional, and Panin, F., additional

Published
2023
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49. One Dimensional Kondo Lattice Model Studied by the Density Matrix Renormalization Group Method

Author

Shibata, N. and Ueda, K.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

Recent developments of the theoretical investigations on the one-dimensional Kondo lattice model by using the density matrix renormalization group (DMRG) method are discussed in this review. Short summaries are given for the zero-temperature DMRG, the finite-temperature DMRG, and also its application to dynamic quantities. Away from half-filling, the paramagnetic metallic state is shown to be a Tomonaga-Luttinger liquid with the large Fermi surface. For the large Fermi surface its size is determined by the sum of the densities of the conduction electrons and the localized spins. The correlation exponent K_rho of this metallic phase is smaller than 1/2. At half-filling the ground state is insulating. Excitation gaps are different depending on channels, the spin gap, the charge gap and the quasiparticle gap. Temperature dependence of the spin and charge susceptibilities and specific heat are discussed. Particularly interesting is the temperature dependence of various excitation spectra, which show unusual properties of the Kondo insulators., Comment: 18 pages, 23 Postscript figures, REVTeX

Published
1998
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50. Thermodynamic properties of the one-dimensional Kondo insulators studied by the density matrix renormalization group method

Author

Shibata, N., Ammon, B., Troyer, M., Sigrist, M., and Ueda, K.

Subjects
Condensed Matter - Strongly Correlated Electrons
Abstract

Thermodynamic properties of the one-dimensional Kondo lattice model at half-filling are studied by the density matrix renormalization group method applied to the quantum transfer matrix. Spin susceptibility, charge susceptibility, and specific heat are calculated down to T=0.1t for various exchange constants. The obtained results clearly show crossover behavior from the high temperature regime of nearly independent localized spins and conduction electrons to the low temperature regime where the two degrees of freedom couple strongly. The low temperature energy scales of the charge and spin susceptibilities are determined and shown to be equal to the quasiparticle gap and the spin gap, respectively, for weak exchange couplings., Comment: 4 pages, 3 Postscript figures, REVTeX, submitted to J. Phys. Soc. Jpn

Published
1997
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