{"id":626,"date":"2016-03-22T20:55:40","date_gmt":"2016-03-22T11:55:40","guid":{"rendered":"http:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/?page_id=626"},"modified":"2024-12-04T14:07:43","modified_gmt":"2024-12-04T05:07:43","slug":"%e5%9b%bd%e5%86%85%e5%a4%96%e3%81%ae%e4%bc%9a%e8%ad%b0%e3%80%81%e7%a0%94%e7%a9%b6%e4%bc%9a%e3%80%81%e3%82%bb%e3%83%9f%e3%83%8a%e3%83%bc%e7%ad%89%e3%81%a7%e3%81%ae%e8%ac%9b%e6%bc%94","status":"publish","type":"page","link":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/talks_ws.html","title":{"rendered":"\u56fd\u5185\u5916\u306e\u4f1a\u8b70\u3001\u7814\u7a76\u4f1a\u3001\u30bb\u30df\u30ca\u30fc\u7b49\u3067\u306e\u8b1b\u6f14"},"content":{"rendered":"<h4>2024\u5e74<\/h4>\n<ol>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u30d5\u30ec\u30fc\u30d0\u30fc\u7269\u7406\u306e\u57fa\u790e<br \/>\nFlavor Physics Workshop 2024, Dec\/2-5, \u30db\u30c6\u30eb\u660e\u5c71\u8358<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\nDark Matter Considering Temperature Evolution of Mass Due to the Electroweak Phase Transition<br \/>\nMeeting of New Higgs Working Group, Oct. 12, Osaka University<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\nRelic Abundance of Dark Matter with Temperature-Dependent Mass during Phase Transitions<br \/>\nThe 4th DMNet symposium : Revealing Dark matter in the Universe with Multidisciplinary Approaches in Particle Physics and Astrophysics, 5th\u20137th Sep. 2024, IBS Science and Culture Center(Poster Session)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectroweak baryogenesis in a complex singlet extension of the Standard Model<br \/>\nFourth Mini-workshop on the Early Universe, 3rd-6th Sep. 2024, Yatsugatake Commons, Yamanashi prefecture<\/li>\n<li>\u5c0f\u6797\u304a\u304d<br \/>\nSearching for signatures of 2HDM with Z4 symmetry at a muon collider<br \/>\n\u57fa\u7814\u7814\u7a76\u4f1a\u3000\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552024\u30012024\/8\/19-23\u3001\u4eac\u90fd\u5927\u5b66 \u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240(\u30dd\u30b9\u30bf\u30fc\u767a\u8868)<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\n\u6e29\u5ea6\u4f9d\u5b58\u6027\u3092\u8003\u616e\u3057\u305f\u6697\u9ed2\u7269\u8cea\u306e\u8cea\u91cf\u3067\u306e\u521d\u671f\u5b87\u5b99\u306e\u76f8\u8ee2\u79fb\u306b\u3088\u308b\u6b8b\u5b58\u91cf<br \/>\n\u57fa\u7814\u7814\u7a76\u4f1a\u3000\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552024\u30012024\/8\/19-23\u3001\u4eac\u90fd\u5927\u5b66 \u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240(\u30dd\u30b9\u30bf\u30fc\u767a\u8868)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nA complex singlet extension of the Standard Model with a singlet fermion dark matter<br \/>\nSeminar at Kanazawa University, 5th Jul. 2024<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectron electric dipole moment and electroweak baryogenesis in a complex singlet extension of the Standard Model<br \/>\n37th Regular Meeting of New Higgs Working Group, Jan. 20, Osaka University<\/li>\n<\/ol>\n<h4>2023\u5e74<\/h4>\n<ol>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u8907\u7d20\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u5f31\u30d0\u30ea\u30aa\u30b8\u30a7\u30cd\u30b7\u30b9\u3001\u5948\u826f\u5973\u5b50\u5927\u5b66\u7d20\u7c92\u5b50\u8ad6\u7814\u7a76\u5ba4\u30bb\u30df\u30ca\u30fc\u30012023\/Dec\/22\u3001\u5948\u826f\u5973\u5b50\u5927\u5b66<\/li>\n<li>\u5c0f\u6797\u304a\u304d<br \/>\nSearching for signatures of 2HDM with Z4 symmetry at a muon collider<br \/>\nKEK-NAOJ Student Workshop 2023, 2023\/12\/16-17, Online<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\nTwo-component dark matter model with degenerate scalars<br \/>\nKEK-NAOJ Student Workshop 2023, 2023\/12\/16-17, Online<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\nTwo-component dark matter model with degenerate scalars<br \/>\n\u7b2c12\u56de \u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2023\/12\/11-13, \u4f50\u8cc0\u5927\u5b66<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u8907\u7d20\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306eCP\u4f4d\u76f8\u306b\u3088\u308b\u91cd\u529b\u6ce2\u304a\u3088\u3073\u96fb\u6c17\u53cc\u6975\u5b50\u30e2\u30fc\u30e1\u30f3\u30c8\u3078\u306e\u5bc4\u4e0e<br \/>\n\u7b2c12\u56de \u89b3\u6e2c\u7684\u5b87\u5b99\u8ad6\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7, 2023\/12\/11-13, \u4f50\u8cc0\u5927\u5b66<\/li>\n<li>\u72ac\u5bae\u7406\u6075<br \/>\nTwo-component dark matter model with degenerate scalars<br \/>\nFlavor Physics workshop 2023, 2023\/11\/22\u301c25,\u00a0 \u71b1\u6d77\u30fb\u4f0a\u8c46\u5c71\u6e29\u6cc9\u30cf\u30fc\u30c8\u30d4\u30a2\u71b1\u6d77 (\u9759\u5ca1\u770c\u71b1\u6d77\u5e02\u4f0a\u8c46\u5c71)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectric dipole moment and electroweak baryogenesis in a complex scalar extension of the Standard Model<br \/>\nSeminar at Tianqin Senter in SUN YAT-SEN University (\u4e2d\u5c71\u5927\u5b66,\u5929\u7434\u4e2d\u5fc3) , 24th Nov, 2023, SUN YAT-SEN University, Guangdong, China<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectron electric dipole moment and electroweak baryogenesis in a complex scalar extension of the Standard Model<br \/>\nKEK Theory Meeting on Particle Physics Phenomenology (KEK-PH2023), Nov\/7-10, KEK<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectric dipole moment and electroweak baryogenesis in a complex scalar extension of the Standard Model<br \/>\nSeminar at Science and technology advanced institute (STAI), Van Lang University , 8th Sep, 2023, Van Lang University (Ho Chi Minh city, Vietnam)<\/li>\n<li>\u9f4a\u85e4\u7dbe\u4e43<br \/>\nSearching for signatures of 2HDM with Z4 symmetry at a muon collider<br \/>\n\u300c\u57fa\u7814\u7814\u7a76\u4f1a\u3000\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552023\u300d\u30012023\/8\/28-9\/1\u3001\u4eac\u90fd\u5927\u5b66 \u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240(\u30dd\u30b9\u30bf\u30fc\u767a\u8868)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u9ad8\u6b21\u5143\u6f14\u7b97\u5b50\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u6c17\u53cc\u6975\u5b50\u30e2\u30fc\u30e1\u30f3\u30c8\u3068\u96fb\u5f31\u30d0\u30ea\u30aa\u30f3\u6570\u751f\u6210\u3001\u300c\u57fa\u7814\u7814\u7a76\u4f1a\u3000\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552023\u300d\u30012023\/8\/28-9\/1\u3001\u4eac\u90fd\u5927\u5b66 \u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240(\u30dd\u30b9\u30bf\u30fc\u767a\u8868)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u6697\u9ed2\u7269\u8cea-\u6838\u5b50\u6563\u4e71\u6291\u5236\u30e1\u30ab\u30cb\u30ba\u30e0\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306e\u5206\u6790\u304a\u3088\u3073\u96fb\u5f31\u76f8\u8ee2\u79fb\u3068\u306e\u95a2\u9023<br \/>\n\u6771\u4eac\u7406\u79d1\u5927\u5b66\u963f\u90e8\u7814\u7a76\u5ba4\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012023\/Jun\/12, \u6771\u4eac\u7406\u79d1\u5927\u5b66<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectric dipole moment and electroweak baryogenesis in a complex singlet extension of the Standard Model with degenerate scalars<br \/>\nThe 6th International Workshop on Higgs as a Probe of New Physics 2023 (HPNP2023), Jun\/5-9, Osaka University<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u65b0\u7269\u7406\u6291\u5236\u30e1\u30ab\u30cb\u30ba\u30e0\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u5f31\u76f8\u8ee2\u79fb\u304a\u3088\u3073\u305d\u306e\u73fe\u8c61\u8ad6\u7684\u5e30\u7d50<br \/>\n\u6a2a\u6d5c\u56fd\u7acb\u5927\u5b66\u7d20\u7c92\u5b50\u7406\u8ad6\u7814\u7a76\u5ba4\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012023\/Apr\/7, \u6a2a\u6d5c\u56fd\u7acb\u5927\u5b66<\/li>\n<li>Gi-Chol Cho<br \/>\nDegenerate scalar scenario in a singlet scalar extension of the Standard Model(\u62db\u5f85\u8b1b\u6f14)<br \/>\nNITEP\u7d20\u7c92\u5b50\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a2022, Mar\/16-18, \u5927\u962a\u516c\u7acb\u5927\u5b66<\/li>\n<li>Chikako Idegawa<br \/>\n\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b \u591a\u91cd\u81e8\u754c\u70b9\u539f\u7406\u306e\u9069\u7528\u304a\u3088\u3073\u96fb\u5f31\u76f8\u8ee2\u79fb\u3068\u306e\u95a2\u9023<br \/>\nNITEP\u7d20\u7c92\u5b50\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a2022, Mar\/16-18, \u5927\u962a\u516c\u7acb\u5927\u5b66<\/li>\n<\/ol>\n<h4>2022\u5e74<\/h4>\n<ol>\n<li>Momoka Sasanuki<br \/>\nCKM anomaly and Minimal supersymmetric standard model with R-parity violation<br \/>\n13th Ewha-JWU-Ochanomizu Joint Symposium 2022, Dec. 5-7,\u00a0 Ewha Womans University, Seoul, Korea<\/li>\n<li>Chikako Idegawa<br \/>\nElectroweak phase transition and Gravitational waves in a complex singlet extension of the Standard Model with degenerate scalars<br \/>\n13th Ewha-JWU-Ochanomizu Joint Symposium 2022, Dec. 5-7,\u00a0 Ewha Womans University, Seoul, Korea<\/li>\n<li>Chikako Idegawa<br \/>\nCP-violating effects on gravitational waves in a complex singlet extension of the Standard Model with degenerate scalars<br \/>\nKEK Theory Meeting on Particle Physics Phenomenology (KEK-PH2022) and International Joint Workshop on the Standard Model and beyond,<br \/>\nNov. 30- Dec. 2, KEK<\/li>\n<li>Chikako Idegawa<br \/>\nCPV effects on GW in a singlet extension with mass degenerated scalars<br \/>\n35th Regular Meeting of New Higgs Working Group, Nov. 18, Osaka University<\/li>\n<li>\u6749\u539f\u68a8\u592e<br \/>\n\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u30b9\u30ab\u30e9\u30fc\u30dd\u30c6\u30f3\u30b7\u30e3\u30eb\u306e\u5206\u6790 (\u30dd\u30b9\u30bf\u30fc\u767a\u8868)<br \/>\nFlavor Physics workshop 2022, 2022\/11\/7\u301c10, \u30cb\u30e5\u30fc\u516b\u666f\u5712(\u9759\u5ca1\u770c\u4f0a\u8c46\u306e\u56fd\u5e02)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u7e2e\u9000\u30b9\u30ab\u30e9\u30fc\u3092\u6301\u3064\u8907\u7d20\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308bCP\u5bfe\u79f0\u6027\u3092\u7834\u308b\u4f4d\u76f8\u306e\u96fb\u5f31\u76f8\u8ee2\u79fb\u3078\u306e\u52b9\u679c<br \/>\nFlavor Physics workshop 2022, 2022\/11\/7\u301c10, \u30cb\u30e5\u30fc\u516b\u666f\u5712(\u9759\u5ca1\u770c\u4f0a\u8c46\u306e\u56fd\u5e02)<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u65b0\u7269\u7406\u6291\u5236\u30e1\u30ab\u30cb\u30ba\u30e0\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u5f31\u76f8\u8ee2\u79fb<br \/>\n2022\/10\/20, \u6771\u4eac\u5973\u5b50\u5927\u5b66\u7406\u8ad6\u7269\u7406\u7814\u7a76\u5ba4\u30bb\u30df\u30ca\u30fc, \u6771\u4eac\u5973\u5b50\u5927\u5b66<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u7e2e\u9000\u30b9\u30ab\u30e9\u30fc\u3092\u6301\u3064\u8907\u7d20\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308bCP\u5bfe\u79f0\u6027\u3092\u7834\u308b\u4f4d\u76f8\u306e\u91cd\u529b\u6ce2\u3078\u306e\u5bc4\u4e0e<br \/>\n\u57fa\u7814\u7814\u7a76\u4f1a \u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552022\u30012022\/8\/29-9\/2\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u7e2e\u9000\u30b9\u30ab\u30e9\u30fc\u30b7\u30ca\u30ea\u30aa\u306b\u304a\u3051\u308b\u6697\u9ed2\u7269\u8cea\u3068\u96fb\u5f31\u76f8\u8ee2\u79fb<br \/>\n\u5ca9\u624b\u5927\u5b66\u6559\u80b2\u5b66\u90e8\u7406\u79d1\u6559\u80b2\u79d1\u7269\u7406\u5b66\u6559\u5ba4\u7b2c12\u56de\u7d20\u7c92\u5b50\u30fb\u5b87\u5b99\u30bb\u30df\u30ca\u30fc\u30012022\/5\/30 (<a href=\"https:\/\/physics.edu.iwate-u.ac.jp\/seminar\">https:\/\/physics.edu.iwate-u.ac.jp\/seminar<\/a>)<\/li>\n<\/ol>\n<h4>2021\u5e74<\/h4>\n<ol>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nEW phase transition with degenerate scalars<br \/>\n\u65b0\u30d2\u30c3\u30b0\u30b9\u52c9\u5f37\u4f1a\u7b2c31\u56de\u5b9a\u4f8b\u4f1a\u30012021\/11\/27\u3001\u5927\u962a\u5927\u5b66<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\nElectroweak phase transition\u00a0 in a complex singlet extension of the Standard Model with degenerate scalars<br \/>\n\u4e5d\u5dde\u5927\u5b66\u7d20\u7c92\u5b50\u8ad6\u7814\u7a76\u5ba4\u30bb\u30df\u30ca\u30fc\u30012021\/11\/16, online<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u8db3\u7acb\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012021\u5e7411\u670813\u65e5\u300114\u65e5<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u7e2e\u9000\u30b9\u30ab\u30e9\u30fc\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u5f31\u76f8\u8ee2\u79fb<br \/>\n\u7d20\u7c92\u5b50\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a2021, 2021\/11\/6-8, \u5927\u962a\u5e02\u7acb\u5927\u5b66<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u93e1\u306e\u5411\u3053\u3046\u306e\u7269\u7406\u5b66\u301c\u529b\u3068\u5bfe\u79f0\u6027<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012021\u5e7410\u670830\u65e5\u300131\u65e5<\/li>\n<li>Chikako Idegawa<br \/>\n1st order phase transition in CxSM with degenerate scalars<br \/>\nSummer camp on ILC accelerator physics and detectors 2021 Sep\/21-24, Online<\/li>\n<li>Gi-Chol Cho<br \/>\nProbing a degenerate-scalar scenario in a pseudoscalar dark-matter model<br \/>\nSummer camp on ILC accelerator physics and detectors 2021 Sep\/21-24, Online<\/li>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u7e2e\u9000\u30b9\u30ab\u30e9\u30fc\u3092\u6301\u3064\u8907\u7d20\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u30b9\u30ab\u30e9\u30fc\u62e1\u5f35\u6a21\u578b\u306b\u304a\u3051\u308b\u96fb\u5f31\u76f8\u8ee2\u79fb<br \/>\n\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c55\u300d2021,2021\/9\/6~9\/10 , Online<\/li>\n<li>Chikako Idegawa<br \/>\n1st order phase transition in Complex singlet extension of the Standard Model<br \/>\nAsia-Pacific Workshop on Particle Physics and\u00a0Cosmology 2021, Oct\/2-6, Online<\/li>\n<li>\u66fa \u57fa\u54f2<br \/>\n\u7269\u7406\u5b66\u306f\u3058\u3081\u306e\u4e00\u6b69<br \/>\n\u653e\u9001\u5927\u5b66\u8db3\u7acb\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012021\u5e745\u670815\u65e5\u300116\u65e5<\/li>\n<li>\u66fa \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012021\u5e745\u67081\u65e5\u30012\u65e5<\/li>\n<li>Chikako Idegawa<br \/>\n1st order phase transition in Complex singlet extension of the Standard Model<br \/>\nThe 5th International Workshop on \u201dHiggs as a Probe of New Physics\u201d Special Edition 2021 (HPNP2021), Mar\/25-27, Online<\/li>\n<\/ol>\n<h4>2020\u5e74<\/h4>\n<ol>\n<li>\u66fa \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u8db3\u7acb\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012020\u5e7411\u670814\u65e5\u300115\u65e5<\/li>\n<\/ol>\n<ol>\n<li>\u66fa \u57fa\u54f2<br \/>\n\u93e1\u306e\u5411\u3053\u3046\u306e\u7269\u7406\u5b66\u301c\u529b\u3068\u5bfe\u79f0\u6027\u301c<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012020\u5e7410\u670817\u65e5\u300118\u65e5<\/li>\n<\/ol>\n<ol>\n<li>\u51fa\u5ddd\u667a\u9999\u5b50<br \/>\n\u30b7\u30f3\u30b0\u30ec\u30c3\u30c8\u8907\u7d20\u30b9\u30ab\u30e9\u30fc\u6a21\u578b\u306b\u304a\u3051\u308b\u4e00\u6b21\u76f8\u8ee2\u79fb\u306e\u6761\u4ef6<br \/>\n\u7d20\u7c92\u5b50\u82e5\u624b\u30aa\u30f3\u30e9\u30a4\u30f3\u7814\u7a76\u4f1a2020\u30012020\u5e748\u670826-28\u65e5<\/li>\n<li>Kana Hayami<br \/>\nGrand Unification of a simple extension of the Standard Model with Minimal Dark Matter and Color Octet Scalars<br \/>\n\u57fc\u7389\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012020\u5e746\u670819\u65e5<\/li>\n<li>Mio Kubota<br \/>\nHiggs Infration in metric and Palatini formalisms: Required suppression of higher dimensional operators<br \/>\nThe 23rd New Physics Forum, Feb\/10, 2020, Ochanomizu University<\/li>\n<\/ol>\n<h4>2019\u5e74<\/h4>\n<ol>\n<li>Gi-Chol Cho<br \/>\nSuppression of DM-nucleon scattering and degenerate scalars in an extension of the SM<br \/>\nThe 27th regular meeting of the New Higgs Working Group (NHWG27), Dec\/13-14, 2019<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u93e1\u306e\u5411\u3053\u3046\u306e\u7269\u7406\u5b66\u301c\u529b\u3068\u5bfe\u79f0\u6027\u301c<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012019\u5e7410\u670826\u65e5\u300127\u65e5<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nLepton-flavor violation via four-Fermi contact interactions at e+ e- linear collider (\u5927\u962a\u5e02\u7acb\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012019\u5e747\u670816\u65e5)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u8db3\u7acb\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012019\u5e745\u670811\u65e5\u300112\u65e5<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012019\u5e744\u670820\u65e5\u300121\u65e5<\/li>\n<li>Sachiho Abe<br \/>\nSuppression of dark matter-nucleon scattering in singlet Higgs extension of the SM and its signature at collider experiments<br \/>\n(The 4th International Workshop on &#8220;Higgs as a Probe of New Physics 2019&#8221;, Feb\/18-22, Osaka University)<\/li>\n<li>Mio Kubota<br \/>\nOn the fine-tuning of Higgs inflation in metric and Palatini formulations<br \/>\n(The 4th International Workshop on &#8220;Higgs as a Probe of New Physics 2019&#8221;, Feb\/18-22, Osaka University)<\/li>\n<li>Kana Hayami<br \/>\nCoupling unification in an extension of the minimal dark matter model and collider signatures<br \/>\n(The 4th International Workshop on &#8220;Higgs as a Probe of New Physics 2019&#8221;, Feb\/18-22, Osaka University)<\/li>\n<li>Miki Yonemura<br \/>\nConstraints on a light scalar in a singlet Higgs extension of the SM at Belle-II<br \/>\n(The 4th International Workshop on &#8220;Higgs as a Probe of New Physics 2019&#8221;, Feb\/18-22, Osaka University)<\/li>\n<\/ol>\n<h4>2018\u5e74<\/h4>\n<ol>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u93e1\u306e\u5411\u3053\u3046\u306e\u7269\u7406\u5b66\u301c\u529b\u3068\u5bfe\u79f0\u6027\u301c<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012018\u5e7410\u670826\u65e5\u300127\u65e5<\/li>\n<li>\u901f\u6c34 \u9999\u5948<br \/>\n\u62e1\u5f35\u3055\u308c\u305f minimal dark matter model \u306b\u304a\u3051\u308b gauge \u7d50\u5408\u5b9a\u6570\u306e\u7d71\u4e00<br \/>\n(\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c55 2018\u300d\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012018\u5e748\u67086\u65e5\u301c10\u65e5\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240)<\/li>\n<li>\u963f\u90e8 \u7965\u6b69<br \/>\n\u30b9\u30ab\u30e9\u30fc\u30c0\u30fc\u30af\u30de\u30bf\u30fc\u6a21\u578b\u306e\u6838\u5b50\u6563\u4e71\u6291\u5236\u6761\u4ef6\u3068\u73fe\u8c61\u8ad6\u7684\u5236\u9650<br \/>\n(\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c55 2018\u300d\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012018\u5e748\u67086\u65e5\u301c10\u65e5\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240)<\/li>\n<li>\u7c73\u6751 \u7f8e\u7d00<br \/>\n\u5149\u5b50-\u967d\u5b50\u885d\u7a81\u306b\u304a\u3051\u308b\u30b9\u30d4\u30f3 1 \u7c92\u5b50\u3092\u5a92\u4ecb\u3068\u3057\u305f\u6697\u9ed2\u7269\u8cea\u306e\u63a2\u7d22\u306b\u3064\u3044\u3066<br \/>\n(\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c55 2018\u300d\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012018\u5e748\u67086\u65e5\u301c10\u65e5\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nLepton-flavor violation via four-Fermi contact interactions at e+e- linear collider<br \/>\nAsian Linear Collider Workshop 2018 (ALCW 2018)<br \/>\nMay\/28-June\/01, 2018, Fukuoka, Japan<a href=\"https:\/\/agenda.linearcollider.org\/event\/7826\/\"> (URL)<\/a><\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nA suppression mechanism of dark matter-nucleon scattering in singlet extension of the SM (\u5de5\u5b66\u9662\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012018\u5e744\u670818\u65e5)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u5c0f\u3055\u306a\u7d20\u7c92\u5b50\u3001\u5927\u304d\u306a\u5b87\u5b99<br \/>\n\u653e\u9001\u5927\u5b66\u6587\u4eac\u5b66\u7fd2\u30bb\u30f3\u30bf\u30fc\u3067\u306e\u9762\u63a5\u6388\u696d\u30012018\u5e744\u670814\u65e5\u300115\u65e5<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nSearch for Dark Neutrino via Vacuum Magnetic Birefringence Experiment<br \/>\n(KEK Theory Meeting on Particle Physics Phenomenology (KEK-PH2018)\u30012018\u5e742\u670813\u65e5\u301c16\u65e5)<\/li>\n<\/ol>\n<h4>2017\u5e74<\/h4>\n<ol>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(\u56fd\u7acb\u6e05\u83ef\u5927\u5b66\/NCTS \u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e7412\u670821\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(\u56fd\u7acb\u53f0\u6e7e\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e7412\u670818\u65e5)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nDimension, Scale and Particle Physics<br \/>\n(8th Ewha-JWU-Ochanomizu Joint Symposium 2017, 2017\/Dec\/12-14, Ewha University, Seoul, Korea)<\/li>\n<li>\u7c73\u6751\u7f8e\u7d00<br \/>\nSearching for signatures of the Dark Sector in Collider Experiments<br \/>\n(8th Ewha-JWU-Ochanomizu Joint Symposium 2017, 2017\/Dec\/12-14, Ewha University, Seoul, Korea)<\/li>\n<li>\u901f\u6c34\u9999\u83dc<br \/>\nSearch for the Possibility of Grand Unification and Higgs Inflation<br \/>\n(8th Ewha-JWU-Ochanomizu Joint Symposium 2017, 2017\/Dec\/12-14, Ewha University, Seoul, Korea)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\n\u96a0\u308c\u305fU(1)\u30b2\u30fc\u30b8\u5834\u3092\u5a92\u4ecb\u3068\u3057\u3066\u5149\u3068\u30d1\u30ea\u30c6\u30a3\u3092\u7834\u3063\u305f\u76f8\u4e92\u4f5c\u7528\u3092\u3059\u308b\u30d5\u30a7\u30eb\u30df\u30aa\u30f3\u306e4\u5149\u5b50\u6709\u52b9\u30e9\u30b0\u30e9\u30f3\u30b8\u30a2\u30f3\u3068\u771f\u7a7a\u8907\u5c48\u6298\u5b9f\u9a13\u3067\u306e\u63a2\u7d22\u306b\u3064\u3044\u3066<br \/>\n(\u4eac\u90fd\u7523\u696d\u5927\u5b66\u76ca\u5ddd\u587e\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e7411\u670820\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\n\u30b9\u30d4\u30f32\u306e\u7c92\u5b50\u3092\u5a92\u4ecb\u3068\u3057\u305f\u6697\u9ed2\u7269\u8cea\u6a21\u578b\u3078\u306eLHC\u304b\u3089\u306e\u5236\u9650<br \/>\n(\u5927\u962a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7 2017\u300c\u5730\u4e0a\u5b9f\u9a13\u3067\u691c\u8a3c\u53ef\u80fd\u306a\u65b0\u7269\u7406\u300d\u30012017\u5e7411\u670811\u65e5\u301c13\u65e5\u3001\u5927\u962a\u5927\u5b66)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nLepton flavor violation via four-Fermi contact interactions at future lepton colliders<br \/>\n(\u5927\u962a\u30ef\u30fc\u30af\u30b7\u30e7\u30c3\u30d7 2017\u300c\u5730\u4e0a\u5b9f\u9a13\u3067\u691c\u8a3c\u53ef\u80fd\u306a\u65b0\u7269\u7406\u300d\u30012017\u5e7411\u670811\u65e5\u301c13\u65e5\u3001\u5927\u962a\u5927\u5b66)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nLepton flavor violation via four-Fermi contact interactions at future lepton colliders<br \/>\n(The 7th KIAS workshop on particle physics and cosomology, The 2nd KEK-NCTS-KIAS joint workshop on particle physics phenomenology\u3067\u306e\u8b1b\u6f14\u30012017\u5e7411\u67086\u65e5\u301c10\u65e5\u3001\u30bd\u30a6\u30eb(\u97d3\u56fd))<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\n\u6a19\u6e96\u7406\u8ad6\u5165\u9580(\u524d\u7de8\u30fb\u5f8c\u7de8)<br \/>\n(Flavor Physics Workshop 2017\u3067\u306e\u8b1b\u6f14\u30012017\u5e7410\u670830\u65e5\u301c11\u67082\u65e5\u3001\u4e09\u6d66\u6d77\u5cb8)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(IBS-CTPU(\u97d3\u56fd)\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e749\u670828\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(KIAS(\u97d3\u56fd)\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e749\u670825\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(APCTP(\u97d3\u56fd)\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e749\u670822\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from<br \/>\nthe Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552017\u300d\u3001\u4eac\u90fd\u5927\u5b66\u57fa\u790e\u7269\u7406\u5b66\u7814\u7a76\u6240\u30012017\u5e747\u670831\u65e5\u301c8\u67084\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;DSU 2017 (The 13th International Workshop on the Dark Side of the Universe\u3001KIAS\u3001\u97d3\u56fd\u30012017\u5e747\u670810\u65e5\u301c7\u670814\u65e5)&#8221;<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nImplications for the Vacuum Magnetic Birefringence Experiment from the Parity Violating Interactions between Fermionic Dark Matter and Extra U(1) Mediator<br \/>\n(\u57fc\u7389\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012017\u5e747\u67087\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nSimplified dark matter models with a spin-2 mediator at the LHC<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;LHCTheory ERC meeting&#8221;\u3001\u30eb\u30fc\u30f4\u30a1\u30f3\u30fb\u30ab\u30c8\u30ea\u30c3\u30af\u5927\u5b66\u3001\u30d9\u30eb\u30ae\u30fc\u3001\u00a02017\u5e743\u670822\u65e5\u301c3\u670824\u65e5)<\/li>\n<\/ol>\n<h4>2016\u5e74<\/h4>\n<ol>\n<li>\u4e0b\u83ef\u5948\u5b50<br \/>\nSearch for charged lepton flavor violation at the ILC<br \/>\n(\u53e3\u982d\u767a\u8868\u30fb\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u201dEwha-JWU-Ocha Joint Symposium 2016\u201d\u3001\u68a8\u82b1\u5973\u5b50\u5927\u30012016\u5e7412\u67086\u65e5\u301c8\u65e5)<\/li>\n<li>\u66fa\u00a0 \u57fa\u54f2<br \/>\nPerturbative unification of gauge couplings in supersymmetric E6 models<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u201dEwha-JWU-Ocha Joint Symposium 2016\u201d\u3001\u68a8\u82b1\u5973\u5b50\u5927\u5b66\u3001\u97d3\u56fd\u30012016\u5e7412\u67086\u65e5\u301c8\u65e5)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nDark matter constraints on simplified models with s-channel spin-2 mediators (AEPSHEP2016\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012016\u5e7410\u670812\u65e5\u301c25\u65e5\u3001\u5317\u4eac)<\/li>\n<li>\u5c71\u4e0b\u516c\u5b50<br \/>\nRatchet Baryogenesis with an Analogy to the Forced Pendulum(AEPSHEP2016\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012016\u5e7410\u670812\u65e5\u301c25\u65e5\u3001\u5317\u4eac)<\/li>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nConstruction of a Model of Monopolium and its Search via Multi-Photon Channels at LHC(\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552016\u300d\u3067\u306e\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u30012016\u5e749\u67085\u65e5\u301c9\u65e5)<\/li>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nSearch for Kaluza-Klein gravitons in extra dimension models via forward detectors at the LHC (Laboratory of Subatomic Physics &amp; Cosmology Grenoble\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012016\u5e743\u670811\u65e5)<\/li>\n<\/ol>\n<h4>2015\u5e74<\/h4>\n<ol>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nRatchet Baryogenesis during reheating<br \/>\n(\u30d0\u30fc\u30b8\u30cb\u30a2\u5de5\u79d1\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012015\u5e7410\u670821\u65e5)<\/li>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nRatchet Baryogenesis during reheating<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;SUSY 2015&#8243;, 2015\u5e748\u670823-29\u65e5)<\/li>\n<li>\u66f9\u3000\u57fa\u54f2<br \/>\nGauge coupling unification in supersymmetric E6 models<br \/>\n(\u5c71\u5f62\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012015\u5e748\u670827\u65e5)<\/li>\n<li>\u77e2\u8429\u3000\u91cf\u5b50<br \/>\nEnergy-momentum current of gravity in Finsler-Kawaguchi Lagrangian formulation<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;Gravity and Beyond (GRaB100)&#8221;, National Taiwan University, July\/6-10, 2015)<\/li>\n<li>\u77e2\u8429\u3000\u91cf\u5b50<br \/>\nFinite-temperature behavior of an impurity in the spin-1\/2 XXZ chain<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;Integrable Systems and Quantum symmetries (ISQS-23)&#8221;<br \/>\n\u30c1\u30a7\u30b3, 6\u670823\u65e5\u301c27\u65e5)<\/li>\n<li>\u9f4b\u85e4\u3000\u9ebb\u7531\u7f8e<br \/>\nHydrodynamics on non-commutative space<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;Gravity and Beyond (GRaB100)&#8221;, National Taiwan University, July\/6-10, 2015)<\/li>\n<li>\u5927\u91ce\u3000\u6176\u5b50<br \/>\nRadion in Randall-Sundrum model at the LHC and photon collider<br \/>\n(\u5927\u962a\u5e02\u7acb\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012015\u5e747\u67087\u65e5)<\/li>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nSearch for Kaluza-Klein gravitons in extra dimension models via forward detectors at the LHC<br \/>\n(\u5bcc\u5c71\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012015\u5e745\u670829\u65e5)<\/li>\n<li>\u66f9 \u57fa\u54f2<br \/>\nGauge coupling unification in supersymmetric E6 models<br \/>\n(KIAS(\u97d3\u56fd\u9ad8\u7b49\u79d1\u5b66\u9662)\u3067\u306e\u30bb\u30df\u30ca\u30fc\u3001\u30bd\u30a6\u30eb\u3001\u97d3\u56fd\u30012015\u5e74 4\u670827\u65e5)<\/li>\n<li>\u66f9 \u57fa\u54f2<br \/>\nSearching for signatures of extra dimensions at the LHC<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;JPS-KPS Joint Symposium: Present and Future of Collider Physics&#8221;, Daejeon Convention Center, Korea, Apr\/24\/2015)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nDescriptions of inflation in scalar field theories, perfect fluid, and F(R) gravity<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001&#8221;Sakata Memorial KMI Workshop on &#8220;Origin of Mass and Strong Coupling Gauge Theories&#8221; (SCGT15), Sakata-Hirata Hall, Nagoya University, Nagoya, Japan&#8221;\u30012015\u5e743\u67083-6\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nLarge-scale magnetic fields, non-Gaussianity, and gravitational waves from inflation<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;Sakata Memorial KMI Workshop on &#8220;Origin of Mass and Strong Coupling Gauge Theories&#8221; (SCGT15), Sakata-Hirata Hall, Nagoya University, Nagoya, Japan&#8221;\u30012015\u5e743\u67083-6\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nCosmological Issues in F(T) Gravity Theory<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;The International Conference on Relativistic Astrophysics, Department of Mathematics, University of the Punjab, Lahore, Pakistan&#8221;\u3001 2015\u5e742\u670810-14\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nLarge-scale magnetic fields, non-Gaussianity, and primordial gravitational waves from inflation<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;KEK-CPWS The 4th UTQuest Workshop, KEK Theory<br \/>\nCenter Cosmophysics Group Workshop, B-mode Cosmology, -Intermediate Scale Inflation and Hidden Sector -, KEK, Tsukuba, Japan&#8221;\u30012015\u5e742\u670819-21\u65e5)<\/li>\n<\/ol>\n<h4>2014\u5e74<\/h4>\n<ol>\n<li>\u5927\u91ce\u3000\u6176\u5b50<br \/>\nRadion in Randall-Sundrum model at the LHC and photon collider<br \/>\n(\u5cf6\u6839\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012014\u5e7412\u670822\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nInflationary cosmology in $R^2$ gravity with quantum corrections<br \/>\n(\u53e3\u982d\u767a\u8868\u3001&#8221;The 24th Workshop on General Relativity and Gravitation<br \/>\n(JGRG24),<br \/>\nKavli IPMU, the University of Tokyo&#8221;\u30012014\u5e7411\u670810-14\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nInflationary models and the recent observations<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;2nd International Workshop on Particle Physics and Cosmology after Higgs and Planck, National Center for Theoretical Sciences, Hsinchu and<br \/>\nFo-Guang-Shan, Kaohsiung, Taiwan&#8221;\u30012014\u5e7410\u67088-11\u65e5)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nInflationary models and recent cosmological observations<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;Workshop on COSMOLOGY AND THE QUANTUM VACUUM<br \/>\nCentro de Ciencias de Benasque Pedro Pascual, Av. Francia 17, Benasque 22440, Spain&#8221;\u30012014\u5e749\u67087-13\u65e5)<\/li>\n<li>\u5c71\u4e0b\u3000\u516c\u5b50<br \/>\nSearch for extra dimensions via forward detectors at the LHC<br \/>\n(SUSY2014, Manchester, England, July 21-26)<\/li>\n<li>\u99ac\u5872\u3000\u4e00\u6674<br \/>\nLarge-scale magnetic fields, non-Gaussianity, and primordial gravitational waves in inflationary cosmology<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;\u30b8\u30e7\u30a4\u30f3\u30c8\u30bb\u30df\u30ca\u30fc(\u65e9\u7a32\u7530\u5927\u5b66)&#8221;\u30012014\u5e747\u670814\u65e5)<\/li>\n<li>\u66f9\u3000\u57fa\u54f2<br \/>\nCollider phenomenology in warped extra dimension models<br \/>\n(\u62db\u5f85\u8b1b\u6f14\u3001&#8221;\u677e\u6c5f\u73fe\u8c61\u8ad6\u7814\u7a76\u4f1a2014&#8243;\u30012014\u5e742\u67088-9\u65e5)<\/li>\n<\/ol>\n<h4>2013\u5e74<\/h4>\n<ol>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\nRadion in Randall-Sundrum model at the LHC and photon collider<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u56fd\u969b\u4f1a\u8b70&#8221;KMI International Symposium 2013 &#8211; on Quest for the origin of particles and the Universe&#8221;\u30012013\u5e7412\u670811-13\u65e5)<\/li>\n<li>\u66f9\u3000\u57fa\u54f2<br \/>\n\u7d20\u7c92\u5b50\u6a19\u6e96\u6a21\u578b\u306e\u7cbe\u5bc6\u691c\u8a3c\u3068\u30c6\u30e9\u30b9\u30b1\u30fc\u30eb\u7269\u7406<br \/>\n(\u96c6\u4e2d\u8b1b\u7fa9\u3001\u9996\u90fd\u5927\u5b66\u6771\u4eac\u30012013\u5e7412\u67089, 10\u65e5)<\/li>\n<li>\u5742\u4e0b\u3042\u3044<br \/>\nCompartmentalization by confinement in multi-lamellar vesicles<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u56fd\u969b\u4f1a\u8b70&#8221;International Soft Matter Conference 2013&#8243;\u30012013\u5e749\u670815-19\u65e5\u3001\u30ed\u30fc\u30de)<\/li>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\n\u30e9\u30c7\u30a3\u30aa\u30f3\u8cea\u91cf\u306b\u5bfe\u3059\u308b\u30d2\u30c3\u30b0\u30b9\u63a2\u7d22\u5b9f\u9a13\u304b\u3089\u306e\u5236\u9650<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u57fa\u7814\u7814\u7a76\u4f1a\u300c\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u306e\u9032\u5c552013\u300d2013\u5e748\u67085\u65e5-9\u65e5\u3001\u4eac\u90fd\u5927\u5b66)<\/li>\n<li>\u77e2\u8429\u91cf\u5b50<br \/>\nA Solvable XXZ Model with an Impurity<br \/>\n(\u30dd\u30b9\u30bf\u30fc\u767a\u8868\u3001\u56fd\u969b\u4f1a\u8b70&#8221;Mathematical Statistical Physics&#8221;\u30012013\u5e747\u670829\u65e5-8\u67083\u65e5\u3001\u4eac\u5927\u57fa\u7814)<\/li>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\nConstraints on radion in a warped extra dimension model from Higgs boson searches at the LHC<br \/>\n(\u300c\u52a0\u901f\u5668\u30fb\u7269\u7406\u5408\u540c ILC \u590f\u306e\u5408\u5bbf2013\u300d\u30012013\u5e747\u670820\u65e5-23\u65e5\u3001\u5bcc\u5c71)<\/li>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\nConstraints on radion in a warped extra dimension model from Higgs boson searches at the LHC<br \/>\n(\u795e\u6238\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012013\u5e746\u670819\u65e5)<\/li>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\nConstraints on radion mass from search for Higgs boson at the LHC<br \/>\n(\u5317\u91cc\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012013\u5e745\u670831\u65e5)<\/li>\n<li>\u66f9\u3000\u57fa\u54f2<br \/>\n\u7cbe\u5bc6\u6e2c\u5b9a\u304b\u3089\u30c6\u30e9\u30b9\u30b1\u30fc\u30eb\u3078<br \/>\n(\u65b0\u5b66\u8853\u9818\u57df\u300c\u5148\u7aef\u52a0\u901f\u5668LHC\u304c\u5207\u308a\u62d3\u304f\u30c6\u30e9\u30b9\u30b1\u30fc\u30eb\u306e\u7d20\u7c92\u5b50\u7269\u7406\u5b66\u300d\u7814\u7a76\u4f1a\u3001\u540d\u53e4\u5c4b\u5927\u5b66\u30012013\u5e745\u670823\u65e5\u301c25\u65e5)<\/li>\n<li>\u77e2\u8429\u91cf\u5b50<br \/>\n\u4e0d\u7d14\u7269\u306e\u3042\u308b\u53ef\u89e3 XXZ \u9396\u306b\u3064\u3044\u3066<br \/>\n(\u7acb\u6559\u5927\u5b66\u3067\u306e\u30bb\u30df\u30ca\u30fc\u30012013\u5e745\u670814\u65e5)<\/li>\n<li>\u66f9\u3000\u57fa\u54f2<br \/>\n\u96fb\u5f31\u7cbe\u5bc6\u6e2c\u5b9a\u306e\u7269\u7406<br \/>\n(\u672d\u5e4c\u30a6\u30a3\u30f3\u30bf\u30fc\u30b9\u30af\u30fc\u30eb2013\u3067\u306e\u8b1b\u7fa9\u3001\u5317\u6d77\u9053\u5927\u5b66\u30012013\u5e742\u670813-15\u65e5)<\/li>\n<\/ol>\n<h4>2012\u5e74<\/h4>\n<ol>\n<li>\u9577\u5ca1\u53cb\u7f8e<br \/>\nSequential melting of quarkonia in quark-gluon fluid at RHIC and LHC<br \/>\n(The 4th Asian Triangle Heavy Ion Conference, Pusan, Korea, Nov.14-17)<\/li>\n<li>\u5927\u91ce\u6176\u5b50<br \/>\nProduction and decay of a heavy radion in Rundall-Sundrum model at the LHC<br \/>\n(Hadron Collider Physics Symposium 2012, Kyoto, Nov. 12-16)<\/li>\n<li>\u677e\u5c3e\u5149<br \/>\nConstraints on R-parity violating couplings from B \u2192 D^(*)tau nu decays<br \/>\n(B workshop 2012, \u5ca9\u624b\u770c\u82b1\u5dfb\u5e02\u30012012\u5e7411\u67085-8\u65e5)<\/li>\n<li>\u5c0f\u4fe3\u5df4\u82b3<br \/>\nB\u2192K\u03c0 decay in R-parity violating supersymmetric standard model<br \/>\n(B workshop 2012, \u5ca9\u624b\u770c\u82b1\u5dfb\u5e02\u30012012\u5e7411\u67085-8\u65e5)<\/li>\n<li>\u7c73\u5c71\u4eac\u5b50<br \/>\nProgress in Gauge-Higgs Unification on the Lattice<br \/>\n(The STRONGnet 2012, Madrid, Spain, Oct.15-19)<\/li>\n<li>\u677e\u5c3e\u5149<br \/>\nConstraints on R-parity violating interactions in MSSM from leptonic decays of pseudoscalar mesons<br \/>\n(\u7b2c18\u56de \u6771\u4eac\u5927\u5b66\u7d20\u7c92\u5b50\u7269\u7406\u56fd\u969b\u7814\u7a76\u30bb\u30f3\u30bf\u30fc\u30b7\u30f3\u30dd\u30b8\u30a6\u30e0,\u9577\u91ce,2012\u5e742\u6708)<\/li>\n<li>Gi-Chol Cho<br \/>\nThe MSSM confronts the precision electroweak data and the muon g-2<br \/>\nseminar at Czech Technical University at Prague, Feb.21.2012<\/li>\n<\/ol>\n","protected":false},"excerpt":{"rendered":"<p>2024\u5e74 \u66fa\u00a0 \u57fa\u54f2 \u30d5\u30ec\u30fc\u30d0\u30fc\u7269\u7406\u306e\u57fa\u790e Flavor Physics Workshop 2024, Dec\/2-5, \u30db\u30c6\u30eb\u660e\u5c71\u8358 \u72ac\u5bae\u7406\u6075 Dark Matter Considering Temperature  &hellip; <a href=\"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/talks_ws.html\">\u7d9a\u304d\u3092\u8aad\u3080 <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":26,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-626","page","type-page","status-publish","hentry"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/pages\/626","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/users\/26"}],"replies":[{"embeddable":true,"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/comments?post=626"}],"version-history":[{"count":73,"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/pages\/626\/revisions"}],"predecessor-version":[{"id":2571,"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/pages\/626\/revisions\/2571"}],"wp:attachment":[{"href":"https:\/\/www-p.sci.ocha.ac.jp\/phys-hep\/wp-json\/wp\/v2\/media?parent=626"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}