{"id":1146,"date":"2025-10-10T10:17:16","date_gmt":"2025-10-10T01:17:16","guid":{"rendered":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/?page_id=1146"},"modified":"2026-08-20T15:13:53","modified_gmt":"2026-08-20T06:13:53","slug":"b03-results","status":"publish","type":"page","link":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/research-results\/b03-results\/","title":{"rendered":"B03\u73ed_\u7814\u7a76\u6210\u679c"},"content":{"rendered":"\n<p class=\"has-black-color has-text-color has-link-color has-medium-font-size wp-elements-1 wp-block-paragraph\" style=\"border-radius:13px;font-style:normal;font-weight:200;text-decoration:none\">\u2666\u6210\u679c\u2666\u3000<a href=\"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/planned-research\/pr-b3\/\" data-type=\"link\" data-id=\"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/planned-research\/pr-b3\/\">B03\u73ed \u91cd\u5143\u7d20\u5408\u6210\u904e\u7a0b\u306e\u89e3\u660e\u306b\u5411\u3051\u305f\u91cd\u3044\u4e2d\u6027\u5b50\u904e\u5270\u6838\u306e\u7814\u7a76<\/a><\/p>\n\n\n\n<p class=\"has-vk-color-custom-1-color has-text-color has-link-color wp-elements-2 wp-block-paragraph\">\ud83c\udf40<a href=\"https:\/\/www.riken.jp\/press\/2026\/20260819_2\/index.html\">B03\u73ed\u3010\u7814\u7a76\u4ee3\u8868\u8005\u3000\u897f\u6751\u4fca\u4e8c\u3011\u3067\u30d7\u30ec\u30b9\u30ea\u30ea\u30fc\u30b9\u304c\u767a\u8868\u3055\u308c\u307e\u3057\u305f(2026.08.19)\u3002<\/a><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40<a href=\"https:\/\/www.riken.jp\/press\/2026\/20260528_1\/index.html\">B03\u73ed\u3010\u7814\u7a76\u4ee3\u8868\u8005\u3000\u897f\u6751\u4fca\u4e8c\u3011\u3067\u30d7\u30ec\u30b9\u30ea\u30ea\u30fc\u30b9\u304c\u767a\u8868\u3055\u308c\u307e\u3057\u305f(2026.05.27)\u3002<\/a><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40<a href=\"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/b%ef%bc%90%ef%bc%93%e7%8f%ad%e3%80%90%e7%a0%94%e7%a9%b6%e4%bb%a3%e8%a1%a8%e8%80%85%e3%80%80%e8%a5%bf%e6%9d%91%e4%bf%8a%e4%ba%8c%e3%80%91%e3%81%a7%e3%83%97%e3%83%ac%e3%82%b9%e3%83%aa%e3%83%aa%e3%83%bc\/\">B03\u73ed\u3010\u7814\u7a76\u4ee3\u8868\u8005\u3000\u897f\u6751\u4fca\u4e8c\u3011\u3067\u30d7\u30ec\u30b9\u30ea\u30ea\u30fc\u30b9\u304c\u767a\u8868\u3055\u308c\u307e\u3057\u305f(2025.10.9)\u3002<\/a><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40\u8ad6\u6587\u767a\u8868(\u67fb\u8aad\u3042\u308a)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\u25ef 2026\u5e74\u5ea6<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>C.Y. Fu, W.D.Xian, T.Niwase, M. Rosenbusch, M. Wada, A. Scalesi, V. Som\u00e0, J. Lee, H. Ishiyama, S. Nishimura, S. Yoshida, A. Takamine, P. Schury, D.S. Hou, S. Kimura, Y. Hirayama, Y. Ito, S. Iimura, J.M. Yap, Y.X. Watanabe, Q.B. Zeng, V.H. Phong, T.T. Yeung, H. Ueno, H. Haba, T. Duguet, M. Frosini, Z.H. Li, H.Y. Wu, A. Estrade, M. Khandelwal, Y. Jang, J. Lee, A.I. Morales, R. Kanungo M. Tanaka, D.Suzuki, H.J. Ong, H. Sakurai, S. Michimasa, N. Fukuda, H. Takeda, H. Suzuki, Y.Shimizu, M. Ohtake, K. Kusaka, Y. Yanagisawa, Y. Togano, M. Yoshimoto, B. Hong, Y.H. Kim, X. Ma, B. Moon, J. Park, F.F. Zeng, and J.Z. Zhang, &#8220;<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/krq1-t8pr\">Mass Measurements of Exotic 48-50Ar Isotopes: Probing Proton-Neutron Interaction of the Doubly Magic 52Ca and the Robustness of N = 32 Subshell<\/a>&#8220;, Phys. Rev. Lett. <strong>137<\/strong>, 062502 (2026)<\/li>\n\n\n\n<li>Zu-Xing Yang, Xiao-Hua Fan, Peng-Hui Chen, and Shunji Nishimura, &#8220;<a href=\"https:\/\/journals.aps.org\/prc\/abstract\/10.1103\/6dtk-1tw2\">Determining the orientation dependence of observables in heavy-ion collisions via deep natural networks<\/a>&#8220;, Phys. Rev. C <strong>113<\/strong>, 064604 (2026)<\/li>\n\n\n\n<li>Ryuichiro Akaho, Hiroki Nagakura, Wakana Iwakami, Shun Furusawa, Akira Harada, Hirotada Okawa, Hideo Matsufuru, Kohsuke Sumiyoshi, and Shoichi Yamada, &#8220;<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/fksy-1jtw\">Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-Collapse Supernovae Informed by Multiangle Neutrino Radiation Hydrodynamics<\/a>&#8220;, Phys. Rev. Lett. <strong>136<\/strong>, 191002 (2026).<\/li>\n\n\n\n<li>Y. Anuar, R. Yokoyama, S. Kurosawa, A. Yamaji, S. Nishimura, V.H. Phong, N. Imai, &#8220;<a href=\"https:\/\/www.sciencedirect.com\/science\/article\/abs\/pii\/S0168900226004262\">Segmented 139La-GPS scintillator as an active stopper for \u03b2-decay studies at fragmentation facilities<\/a>&#8220;, Nucl. Instrum. Meth. A <strong>1091<\/strong>, 171700 (2026)<\/li>\n\n\n\n<li>Ian Cox, Robert Grzywacz, T.T. King, K.P. Rykazewski, S. Nishimura, R. Yokoyama, N. Fukuda, N. Kitamura, S. Go, C. Mazzocchi, J.M.Almond, A. Augustyn, N. Braukman, P. Brionnet, A. Esmaylzadeh, J. Fischer, G. Garcia de Lorenzo, S. Hanai, D. Hoskins, N. Imai, K. Kolos, A. Korgul, B. Kreider, S. Michimasa, K. Nishio, V. Phong, T.J Ruland, H. Sakurai, Y. Shimizu, A. Skruch, H. Suzuki, H. Takeda, Y. Togano, Z.Y. Xu &amp; M. Yoshimotoi, &#8220;<a href=\"https:\/\/www.nature.com\/articles\/s41586-026-10581-w\">Direct observation of the superallowed \u03b1-decay of <sup>140<\/sup>Te<\/a>&#8220;, Nature <strong>654<\/strong>, 52 (2026)<\/li>\n<\/ul>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\u25ef 2025\u5e74\u5ea6<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>Y. Shimizu, K.P. Rykaczewski, N. Fukuda, N.T. Brewer, I. Dillmann, R.K. Grzywacz, S. Nishimura, B.C. Rasco, J.L. Tain, H. Suzuki, H. Takeda, D.S. Ahn, T. Sumikama, N. Inabe, K. Yoshida, H. Ueno, S. Michimasa, A. Algora, J.M. Allmond, J. Agramunt, H. Baba, S. Bae, C.G. Bruno, R. Caballero-Folch, F. Calvino, P.J. Coleman-Smith, G. Corts, T. Davinson, C. Domingo-Pardo, A. Estrade, S. Go, C.J. Griffin, J. Ha, O. Hall, L.J. Harkness-Brennan, . Heideman, T Isobe, D, Kahl, M. Karny, L.H. Khiem, T.T. King, G.G. Kiss, A. Korgul, S. Kubono, M. Labiche, I. Lazarus, J. Liang, J. Liu, G. Lorusso, M. Madurga, K. Matsui, K. Miernik, F. Montes, A.I. Morales, P. Morrall, N. Nepal, R.D. Page, V.H. Phong, M. Piersa-Silkowska, M. Prydderch, V.F.E. Puckness, M.M. Rajabali, B. Rubio, Y. Saito, H. Sakurai, J. Simpson, M. Singh, D.W. Stracener, A. Tarifeno-Saldivia, S.L. Thomas, A. Tolosa-Delgado, M. Wolinska-Cichocka, P.J. Woods, X.X. Xu, and R. Yokoyama, &#8220;<a href=\"https:\/\/academic.oup.com\/ptep\/article\/2026\/3\/033D06\/8492949?login=false\">Exploration of Neutron-Rich Isotopes around N = 50 via the In-Flight Fission of a 345 MeV\/Nucleon 238U Beam<\/a>&#8220;, Prog. Theor. Exp. Phys. <strong>2026,<\/strong> 033D06 (2026)<\/li>\n\n\n\n<li>H.Y. Wu, Z.H. Li, M. Venaruzzo, L. Colombini, D.W. Luo, H. Hua, S. Nishimura, A. Abba, Y. Venturini, C. Tintori, M. Bianchini, &#8220;<a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0168900226000410?via%3Dihub\">The upgrade of the general-purpose digital data aquisition system (GDDAQ)<\/a>&#8220;, Nucl. Instrum. Meth. A <strong>1085,<\/strong> 171315 (2026)<\/li>\n\n\n\n<li>B. Moon, J. Lee, Y. Jang, H. Watanabe, S. Nishimura, V. Phong, Q. Zeng, H. Baba, S. Bae, A.M. Bruce, H. Chen, S. Choi, A. Esmaylzadeh, J. Fischer, L.M. Fraile, N. Fukuda, G. Garcia De Lorenzo, S. Go, A. Gorgen, M. Gorska, S. Guo, K.I. Hahn, J.S. Heines, B. Hong, Y.H. Kim, R. Lozeva, S. Michimasa, M. Mikolajczuk, A.I. Morales, J. Park, S. Pascu, Zs. Podolyak, P.H. Regan, E. Sahin, H. Sakurai, Y. Shimizu, H. uzuki, H. Takeda, Y. Togano, T.T. Yeung, M. Yoshimoto, &#8220;<a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0168900225010411?via%3Dihub\">Commissioning and performance of IDATEN: A large fast-timing \u03b3-ray detector array at RIBF<\/a>&#8220;, Nucl. Instrum. Meth. A <strong>1084,<\/strong> 171239 (2025)<\/li>\n\n\n\n<li>Nobuya Nishimura, Crla Frohlich and Thomas Rauscher, &#8220;<a href=\"https:\/\/academic.oup.com\/mnras\/article\/546\/3\/stag152\/8437925\">Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates<\/a>&#8220;, Month. Not. Roy. Astron. Soc. <strong>546,<\/strong> 1 (2025)<\/li>\n\n\n\n<li>Kenichi Nakazato, Hajime Togashi, Kohsuke Sumiyoshi, Hideyuki Suzuki,<a href=\"https:\/\/doi.org\/10.1093\/ptep\/ptaf156\"> &#8220;Role of Symmetry Energy at Subnuclear Densities in Protoneutron Star Crusts&#8221;<\/a>, Progress of Theoretical and Experimental Physics 2025 (2025) 123E01&nbsp;<\/li>\n\n\n\n<li>Q.B. Zeng, S. Nishimura, V.H. Phong, S. Yoshida, Z.H Li, Z. Liu, H.Y. Wu, C.Y. Fu, D.S. Hou, H. Ishiyama, Y. Jang, M. Khandelwal, J. Lee, A.I. Morales, T. Niwase, M. Rosenbusch, P. Schury, A. Takamine, M. Wada, W.D. Xian, T.T. Yeung, A. Estrade, N. Fukuda, L. Guo, Y. Hirayama, B. Hong, S. Iimura, Y. Ito, Y.H. Kim, S. Kimura, J. Lee, X. Ma, S. Michimasa, B. Moon, Y.F. Niu, J. Park, H. Sakurai, Y. Shimizu, H. Suzuki, H. Takeda, M. Tanaka, Y. Togano, Y.X. Watanabe, J.M. Yap, M. Yoshimoto, C.X Yuan, F.F. Zeng, J.Z. Zhang, and X.L. Zhi, &#8220;<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/227j-q7zf\">\u03b2-Decay Half-Lives of Neutron-Rich Sulfur to Potassium: Evolution of the N = 32 and 34 Subshell Closures below Calcium<\/a>&#8220;, Phys. Rev. Lett. <strong>135,<\/strong> 232501 (2025)<\/li>\n\n\n\n<li>Fumi Nakanishi, Ken&#8217;ichiro Nakazato, Masayuki Harada, Yusuke Koshio, Ryuichiro Akaho, Yosuke Ashida, Akira Harada, Masamitsu Mori, Kohsuke Sumiyoshi, Yudai Suwa, Roger A. Wendell, and Masamichi Zairen, &#8220;<a href=\"https:\/\/doi.org\/10.3847\/1538-4357\/adfcca\">Observing Supernova Neutrino Light Curves with Super-Kamiokande. VI. A Practical Data Analysis Texhnique Considering Realistic Experimental Backgrounds<\/a>&#8220;, Astrophys. Jour <strong>992<\/strong>, 27 (2025)\u3000\u3000<\/li>\n\n\n\n<li>W. Xian, M. Rosenbusch, V.H. Phong, M. Wada, P. Schury, D. Hou, S. Chen, T. Niwase, Y. Hirayama, H. Ishiyama, S. Iimura, Y. Ito, M. Kojima, S. Kimura, J. Liu, J. Lee, S. Michimasa, H. Miyatake, J.Y. Moon, M. Mukai, S. Nishimura, S. Naimi, T. Sonoda, Y.X. Watanabe, H. Wollnik, and S. Yan, &#8220;<a href=\"https:\/\/www.frontiersin.org\/journals\/physics\/articles\/10.3389\/fphy.2025.1644477\/full\">Atomic mass measurements of neutron-rich nuclides on the path to 78Ni with a \u03b2-TOF-equipped MRTOF device<\/a>&#8220;, Front. in Phys. <strong>13<\/strong>, 1644477, (2025)<\/li>\n\n\n\n<li>S. Kimura, M. Wada, C.Y. Fu, N. Fukuda, Y. Hirayama, D.S. Hou, S. Iimura, H. Ishiyama, Y. Ito, S. Kubono, K. Kusaka, S. Michimasa, H. Miyatake, S. Nishimura, T. Niwase, V. Phong, M. Rosenbusch, H. Schatz, P. Schury, Y. Shimizu, H. Suzuki, A. Takamine, H. Takeda, Y. Togano, Y.X. Watanabe, W.D. Xian, Y. Yanagisawa, T.T. Yeung, M. Yoshimoto, and S. Zha, &#8220;<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/2dyn-q7wp\">Precision Mass Measurements around 84Mo Rule Out ZrNb Cycle Formation in the Rapid Proton-Capture Process at Type I X-Ray Bursts<\/a>&#8220;, Phys. Rev. Lett. <strong>134<\/strong>, 152701 (2025)<\/li>\n\n\n\n<li>Hiroki Nagakura, Kohsuke Sumiyoshi, Sho Fujibayashi, Yuichiro Sekiguchi, and Masaru Shibata, &#8220;<a href=\"https:\/\/doi.org\/10.1103\/kf8q-d67t\">Neutrino flavor instabilities in a binary neutron star merger remnant: Roles of a long-lived hypermassive neutron star<\/a>&#8220;, Phys. Rev. D <strong>112<\/strong>, 043029 (2025)<\/li>\n\n\n\n<li>&nbsp;Y. Suwa, R. Akaho, Y. Ashida, A. Harada, M. Harada, Y. Koshio, M. Mori, F. Nakanishi, K. Nakazato,&nbsp; K. Sumiyoshi, R. A. Wendell and M. Zaizen,<a href=\"https:\/\/doi.org\/10.33232\/001c.147127\">&#8220;Neutrino Constraints on Black Hole Formation in M31&#8221;,<\/a>&nbsp;The Open Journal of Astrophysics, 8 (2025)&nbsp;<\/li>\n\n\n\n<li>A. Tolosa-Delgado,&nbsp;J. L. Tain,&nbsp;M. Reichert,&nbsp;A. Arcones,&nbsp;M. Eichler,&nbsp;B. C. Rasco,&nbsp;N. T. Brewer,&nbsp;K. P. Rykaczewski,&nbsp;R. Yokoyama,&nbsp;R. Grzywacz,&nbsp;I. Dillmann,&nbsp;J. Agramunt,&nbsp;D. S. Ahn,&nbsp;A. Algora,&nbsp;H. Baba,&nbsp;S. Bae,&nbsp;C. G. Bruno,&nbsp;R. Caballero Folch,&nbsp;F. Calvino,&nbsp;P. J. Coleman-Smith,&nbsp;G. Cortes,&nbsp;T. Davinson,&nbsp;C. Domingo-Pardo,&nbsp;A. Estrade,&nbsp;N. Fukuda,&nbsp;S. Go,&nbsp;C. J. Griffin,&nbsp;J. Ha,&nbsp;O. Hall,&nbsp;L. Harkness-Brennan,&nbsp;T. Isobe,&nbsp;D. Kahl,&nbsp;M. Karny,&nbsp;L. H. Khiem,&nbsp;G. G. Kiss,&nbsp;M. Kogimtzis,&nbsp;A. Korgul,&nbsp;S. Kubono,&nbsp;M. Labiche,&nbsp;I. Lazarus,&nbsp;J. Liang,&nbsp;J. Lee,&nbsp;J. Liu,&nbsp;G. Lorusso,&nbsp;K. Matsui,&nbsp;K. Miernik,&nbsp;F. Montes,&nbsp;B. Moon,&nbsp;A. I. Morales,&nbsp;N. Nepal,&nbsp;S. Nishimura,&nbsp;R. D. Page,&nbsp;M. Piersa-Silkowska,&nbsp;V. H. Phong,&nbsp;Zs. Podolyak,&nbsp;V. F. E. Pucknell,&nbsp;P. H. Regan,&nbsp;B. Rubio,&nbsp;Y. Saito,&nbsp;H. Sakurai,&nbsp;Y. Shimizu,&nbsp;J. Simpson,&nbsp;P.-A. Soderstrom,&nbsp;D. W. Stracener,&nbsp;T. Sumikama,&nbsp;R. Surman,&nbsp;H. Suzuki,&nbsp;M. Takechi,&nbsp;H. Takeda,&nbsp;A. Tarifeno-Saldivia,&nbsp;S. L. Thomas,&nbsp;M. Wolinska-Cichocka,&nbsp;P. J. Woods,&nbsp;X. X. Xu,<a href=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.134.172701\" data-type=\"link\" data-id=\"https:\/\/journals.aps.org\/prl\/abstract\/10.1103\/PhysRevLett.134.172701\">&#8220;Impact of newly measured&nbsp;\ud835\udefd-Delayed Neutron Emitters around <sup>7<\/sup>8Ni&nbsp;on Light Element Nucleosynthesis in the Neutrino Wind Following a Neutron Star Merger&#8221;<\/a>, Phys. Rev. Lett.&nbsp;<strong>134<\/strong>, 172701 (2025)<\/li>\n\n\n\n<li>A. Aoyama, T. Enoto, T. Takahashi, S. Watanabe, T. Takeda, W. Iwakiri, K. Yamasaki, S. Iwata, N. Ota, A. Jujo, T. Tamagawa, T. Mihara, C.-P. Hu, A. Dohi, N. Nishimura, M. Serino, M. Nakajima, T. Kitaguchi, Y. Kato, N. Kawai,<a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/addd00\"> &#8220;Thermonuclear Superburst of MAXI J1752-457 Observed with NinjaSat and MAXI&#8221;,<\/a> Astrophys. J. Lett. 986 L29 (2025)<\/li>\n\n\n\n<li>T. Takeda, T. Tamagawa, T. Enoto, W. Iwakiri, A. Dohi, T. Mihara, H. Takahashi, C.-P. Hu, A. Aoyama, N. Ota, S. Iwata, T. Takahashi, K. Yamasaki, T. Kita, S. Tsuchiya, Y. Nakano, M. Ichibakase, N. Nishimura, <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ae0e75\">&#8220;Return of the Clocked Burster: Exceptionally Short Recurrence Time in GS 1826-2381&#8221;<\/a>, Astrophys. J. Lett. 993 129 (2025)<\/li>\n\n\n\n<li>N. Nishimura, C. Fr\u00f6hlich, T. Rauscher, <a href=\"https:\/\/doi.org\/10.1093\/mnras\/stag152\">&#8220;Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates&#8221;, <\/a>Month. Not. Roy. Astron. Soc. 546, 1 (2026)<\/li>\n<\/ul>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40\u53e3\u982d\u767a\u8868(\u56fd\u969b\u7684\u306a\u7814\u7a76\u96c6\u4f1a\u3067\u306e\u62db\u5f85\u8b1b\u6f14)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\u25ef 2025\u5e74\u5ea6<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li>S. Nishimura, &#8220;Projects related to Nuclear Astrophysics at RIBF and Future Perspectives&#8221;,&#8221;<a href=\"https:\/\/agenda.infn.it\/event\/44038\">Italy-Japan Symposium on Joint Activities in Fundamental Physics<\/a>&#8220;, Mar. 9&#8211;12, 2026<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Current Status and Future Plans&#8221;,&#8221;<a href=\"https:\/\/indico.ibs.re.kr\/event\/1007\/\">Top-tier Nuclear Astrophysics Working Group Workshop<\/a>&#8220;, (Zoom), Dec. 22&#8211;23, 2025<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Experimental Challenges in Identifying the Sites of r-Process Nucleosynthesis&#8221;, &#8220;YN and YY interactions and neutron stars&#8221;, RIKEN, Japan, Nov. 20, 2025<\/li>\n\n\n\n<li>N. Nishimura, &#8220;Toward astro-physics-driven nuclear-reaction experiments for supernova nucleosynthesis&#8221;, <a href=\"http:\/\/N. Nishimura, &quot;Toward astro-physics-driven nuclear-reaction experiments for supernova nucleosynthesis&quot;, &quot;Origin of Elements and Cosmic Evolution&quot;, Beihang University (China), Nov. 10-14 2025.\">&#8220;Origin of Elements and Cosmic Evolution&#8221;<\/a>, Beihang University (China), Nov. 10-14 2025.<\/li>\n\n\n\n<li>&nbsp;N. Nishimura, <a href=\"https:\/\/indico.ectstar.eu\/event\/246\/\">&#8220;Neutron-capture reactions in nucleosynthesis of p-nuclei&#8221;, &#8220;Neutron-capture reactions for astrophysical processes&#8221;,<\/a> ECT* (Itary), Nov. 3-7 2025<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Exploring r-Process Signatures in Neutron-Rich Nuclei&#8221;, &#8220;<a href=\"https:\/\/appc16.scimeeting.cn\/\">The 16th Asia Pacific Physics Conference&#8221;<\/a>, Haikou, China, Oct. 19&#8211;24, 2025<\/li>\n\n\n\n<li>S. Nishimura, &#8220;A possible study of collective flows in low-energy collisions of deformed nuclei&#8221;, &#8220;<a href=\"https:\/\/indico.ihep.ac.cn\/event\/25334\/\">The 2nd International Workshop on Physics at High Baryon Density<\/a>&#8220;, Oct. 16&#8211;18, 2025, Wuhan, China<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Investigation of Nuclear Properties relevant to Nuclear Astrophysics&#8221;, &#8220;<a href=\"https:\/\/indico.impcas.ac.cn\/event\/172\/\">Nuclear Astrophysics Experiments with HIAF<\/a>&#8220;, Sep. 03&#8211;05, 2025, Huizhou, China<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Overview of Project #4&#8221;, &#8220;The 2nd Japan-Korea Symposium on TOPTIER Platform in Extreme Rare Isotope Science&#8221;, Aug. 19&#8211;21, 2025, RIKEN, Japan<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Role of Exotic Nuclei Away from Stability&#8221;, &#8220;<a href=\"https:\/\/indico.icc.ub.edu\/event\/341\/\">International Symposium on Nuclei in the Cosmos (NIC XVIII)<\/a>&#8220;, June 15&#8211;20, 2025, Girona, Spain<\/li>\n\n\n\n<li>S. Nishimura, &#8220;Projects related to Nuclear Astrophysics and TOPTIER&#8221;, &#8220;<a href=\"https:\/\/www.kps.or.kr\/conference\/event\/index.php?cfrid=24\">The Korean Physical Society Meeting<\/a>&#8220;, April 23&#8211;25, 2025, Daejeon, Korea<\/li>\n\n\n\n<li>&nbsp; K. Sumiyoshi, &#8220;Role of dense matter and neutrinos in core-collapse supernovae and hot neutron stars&#8221;, XIIIth International Symposium on Nuclear Symmetry Energy (NuSym25) , 2025.9.8-13 (9.11),  Integrated Innovation Building (IIB), RIKEN Kobe Campus, Japan (Invited talk)<\/li>\n<\/ul>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40\u53e3\u982d\u767a\u8868(\u56fd\u5185\u8b1b\u6f14)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\u25ef 2025\u5e74\u5ea6<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">1. <a href=\"https:\/\/sites.google.com\/g.ecc.u-tokyo.ac.jp\/sumi2026\/top?pli=1\">&nbsp;\u897f\u6751\u4fe1\u54c9, &#8220;\u8d85\u65b0\u661f\u7206\u767a\u3068\u300cr\u30d7\u30ed\u30bb\u30b9\u300d\u5143\u7d20\u5408\u6210&#8221;, \u300c\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u8f38\u9001\u3068\u539f\u5b50\u6838\u304b\u3089\u8aad\u307f\u89e3\u304f\u8d85\u65b0\u661f\u7206\u767a\u300d, \u95a2\u6771\u5b66\u9662\u5927\u5b66, 2026\u5e743\u670812-13\u65e5<\/a><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">2. Nobuya Nishimura, &#8220;Perspectives on RIBF Experiments on Explosive Nucleosynthesis: A view from Astrophysical Theory&#8221;, <a href=\"https:\/\/indico2.riken.jp\/event\/5428\/\">Advancing physics at next RIBF (ADRIB26)<\/a>, RIKEN,  2026\u5e743\u67085-6\u65e5<\/p>\n\n\n\n<p class=\"has-small-font-size wp-block-paragraph\">3.&nbsp;&nbsp;&nbsp;&nbsp; S. Li, J. Pang, H. Shen, J. Hu,&nbsp;\u4f4f\u5409\u5149\u4ecb, &#8220;\u8d85\u65b0\u661f\u30fb\u4e2d\u6027\u5b50\u661f\u306e\u72b6\u614b\u65b9\u7a0b\u5f0f\u306b\u304a\u3051\u308b\u6838\u5b50\u6709\u52b9\u8cea\u91cf\u306e\u5f71\u97ff&#8221;, \u65e5\u672c\u7269\u7406\u5b66\u4f1a \u7b2c80\u56de\u5e74\u6b21\u5927\u4f1a<\/p>\n\n\n\n<p class=\"has-small-font-size wp-block-paragraph\">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;\u5e83\u5cf6\u5927\u5b66(\u6771\u5e83\u5cf6\u30ad\u30e3\u30f3\u30d1\u30b9), 2025\u5e749\u670816\u65e5\u301c19\u65e5(\u8b1b\u6f14\u65e59.17)<\/p>\n\n\n\n<p class=\"has-small-font-size wp-block-paragraph\">4.&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;\u4f4f\u5409\u5149\u4ecb, &#8220;\u8d85\u65b0\u661f\u7206\u767a\u306b\u304a\u3051\u308b\u30cb\u30e5\u30fc\u30c8\u30ea\u30ce\u30fb\u539f\u5b50\u6838\u7269\u7406&#8221;, \u5b66\u8853\u5909\u9769(A)\u300c\u7cbe\u5bc6\u6570\u5024\u8a08\u7b97\u304c\u5207\u308a\u958b\u304f\u5b87\u5b99\u306e\u91cf\u5b50\u7269\u8cea\u79d1\u5b66\u300d\u9818\u57df\u7814\u7a76\u4f1a<\/p>\n\n\n\n<p class=\"has-small-font-size wp-block-paragraph\">&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;\u78d0\u68af\u71b1\u6d77,&nbsp;\u798f\u5cf6\u770c, 2026\u5e743\u67082\u65e5\u301c4\u65e5(\u8b1b\u6f14\u65e53.4)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">\ud83c\udf40\u30bb\u30df\u30ca\u30fc\u767a\u8868(\u62db\u5f85)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">(\u6d77\u5916)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">1. N. Nishimura, &#8220;Multi-messenger Signature of Explosive Nucleosynthesis from Neutron-Star Binaries&#8221;, SWIFAR Colloquium, Yunnan University (China), Jun. 10, 2025<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">2. N. Nishimura, &#8220;Multi-messenger signature of explosive nucleosynthesis from neutron-star binaries&#8221;, School of Physical Science and Technology Seminar, Xinjang University (China), Aug. 13 2025<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">(\u56fd\u5185)<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">1. N. Nishimura, &#8220;The Diversity of Matter and the Universe: UKAKUREN Workshop 2025 and Beyond&#8221;, IPNS Physics and Detector Seminars, KEK, Apr. 16, 2025<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><a href=\"https:\/\/kds.kek.jp\/event\/54795\">https:\/\/kds.kek.jp\/event\/54795<\/a><\/p>\n\n\n\n<p class=\"wp-block-paragraph\">2. \u897f\u6751\u4fe1\u54c9, &#8220;\u5b87\u5b99\u306b\u304a\u3051\u308b\u5143\u7d20\u306e\u5909\u63db\u3068\u5faa\u74b0 -\u7206\u767a\u5929\u4f53\u306b\u304a\u3051\u308br\u30d7\u30ed\u30bb\u30b9\u5143\u7d20\u5408\u6210-&#8220;, \u7dcf\u5408\u7406\u5de5\u7814\u7a76\u79d1\u300c\u5b66\u969b\u7814\u7a76\u300d\u30fb\u300c\u8ab2\u5916\u30bb\u30df\u30ca\u30fc\u300d, \u8fd1\u757f\u5927\u5b66, 2025\u5e745\u67082\u65e5<\/p>\n\n\n\n<p class=\"has-small-font-size wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>\u2666\u6210\u679c\u2666\u3000B03\u73ed \u91cd\u5143\u7d20\u5408\u6210\u904e\u7a0b\u306e\u89e3\u660e\u306b\u5411\u3051\u305f\u91cd\u3044\u4e2d\u6027\u5b50\u904e\u5270\u6838\u306e\u7814\u7a76 \ud83c\udf40B03\u73ed\u3010\u7814\u7a76\u4ee3\u8868\u8005\u3000\u897f\u6751\u4fca\u4e8c\u3011\u3067\u30d7\u30ec\u30b9\u30ea\u30ea\u30fc\u30b9\u304c\u767a\u8868\u3055\u308c\u307e\u3057\u305f(2026.08.19)\u3002 \ud83c\udf40B03\u73ed\u3010\u7814\u7a76\u4ee3\u8868\u8005\u3000\u897f\u6751\u4fca\u4e8c\u3011\u3067\u30d7\u30ec\u30b9\u30ea\u30ea\u30fc\u30b9\u304c\u767a [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":0,"parent":47,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_locale":"ja","_original_post":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/?page_id=1146","footnotes":""},"class_list":["post-1146","page","type-page","status-publish","hentry","ja"],"_links":{"self":[{"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/pages\/1146","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/comments?post=1146"}],"version-history":[{"count":71,"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/pages\/1146\/revisions"}],"predecessor-version":[{"id":1627,"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/pages\/1146\/revisions\/1627"}],"up":[{"embeddable":true,"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/pages\/47"}],"wp:attachment":[{"href":"https:\/\/lambda.phys.tohoku.ac.jp\/qm-science\/wp-json\/wp\/v2\/media?parent=1146"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}