{"id":14855,"date":"2026-04-15T09:25:27","date_gmt":"2026-04-15T00:25:27","guid":{"rendered":"http:\/\/www-wp22.ile.osaka-u.ac.jp\/?p=14855"},"modified":"2026-04-16T09:28:05","modified_gmt":"2026-04-16T00:28:05","slug":"post-14855","status":"publish","type":"post","link":"http:\/\/www-wp22.ile.osaka-u.ac.jp\/2026\/04\/15\/post-14855\/","title":{"rendered":"\u7b2c663\u56de\u30ec\u30fc\u30b6\u30fc\u79d1\u5b66\u7814\u7a76\u6240\u30b3\u30ed\u30ad\u30a6\u30e0"},"content":{"rendered":"

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\u25cf\u65e5\u6642(Date):
\n2026\u5e744\u670827\u65e5(\u6708) 10\u664230\u5206\uff5e12\u664200\u5206<\/p>\n

\u25cb\u5834\u6240(Place):
\n\u30ec\u30fc\u30b6\u30fc\u79d1\u5b66\u7814\u7a76\u6240 \u7814\u7a76\u68df3\u968e \u5927\u4f1a\u8b70\u5ba4 (R302)<\/p>\n

\u25cf\u8b1b\u6f14\u8005(Speaker):
\nBruce Remington (Lawrence Livermore National Laboratory)<\/p>\n

\u25cb\u984c\u76ee(Title):
\nNew regimes of high energy density science on the National Ignition Facility<\/p>\n

\u25cf\u6982\u8981(Abstract):
\nResults from NIF Discovery Science will be presented. Examples include nuclear reactions relevant to stellar nucleosynthesis. [1] Equations of state at extreme pressures relevant to planetary and exoplanet interiors are being measured. [2] Studies of Rayleigh-Taylor instabilities at high Reynolds number, relevant to supernova explosions, are being studied. [3, 4] Experiments to study magnetic reconnection at HED conditions have been done. [5] High velocity, low density interpenetrating plasmas that generate collisionless astrophysical shocks, magnetic fields, and that accelerate particles relevant to cosmic ray sources are also being studied. [6] NIF experiments have demonstrated strong suppression of heat conduction in a replica of galaxy-cluster turbulent plasmas. [7]. Experiments relevant to turbulent star formation dynamics are underway on NIF. [8, 9] And relativistically hot plasmas are being generated and studied on the NIF ARC laser. [10]<\/p>\n

[1] D.T. Casey, Frontiers in Physics (2023).
\n[2] T. D\u00f6ppner, Nature (2023).
\n[3] J.P. Sauppe, PRL (2020).
\n[4] S.R. Nagel, PoP 2017, PoP 2022.
\n[5] V.V. Valenzuela, PoP (2024).
\n[6] F. Fiuza, Nat. Phys. (2020).
\n[7] J. Meinecke, Sci. Advances (2022).
\n[8] S. Davidovits, PRE (2022).
\n[9] S. Dhawalikar, MNRAS (2022).
\n[10] G.J. Williams, PRE (2021).<\/p>\n

\u25cb\u9023\u7d61\u5148(Contact Person):
\n\u4f50\u91ce \u5b5d\u597d sano.takayoshi.ile@osaka-u.ac.jp<\/p>\n","protected":false},"excerpt":{"rendered":"

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