{"id":848,"date":"2015-10-02T14:42:02","date_gmt":"2015-10-02T05:42:02","guid":{"rendered":"http:\/\/core-u.hiroshima-u.ac.jp\/?p=848"},"modified":"2015-10-02T14:42:02","modified_gmt":"2015-10-02T05:42:02","slug":"%e9%80%9a%e7%ae%97%e7%ac%ac-12-%e5%9b%9e-2015-%e5%b9%b4%e5%ba%a6%e7%ac%ac-7-%e5%9b%9e-%e5%ba%83%e5%b3%b6%e5%a4%a7%e5%ad%a6%e6%a5%b5%e9%99%90%e5%ae%87%e5%ae%99%e7%a0%94%e7%a9%b6%e6%8b%a0%e7%82%b9-co-2","status":"publish","type":"post","link":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/blog\/2015\/10\/02\/%e9%80%9a%e7%ae%97%e7%ac%ac-12-%e5%9b%9e-2015-%e5%b9%b4%e5%ba%a6%e7%ac%ac-7-%e5%9b%9e-%e5%ba%83%e5%b3%b6%e5%a4%a7%e5%ad%a6%e6%a5%b5%e9%99%90%e5%ae%87%e5%ae%99%e7%a0%94%e7%a9%b6%e6%8b%a0%e7%82%b9-co-2\/","title":{"rendered":"\u901a\u7b97\u7b2c 12 \u56de (2015 \u5e74\u5ea6\u7b2c 7 \u56de) \u5e83\u5cf6\u5927\u5b66\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9 (CORE-U) \u30bb\u30df\u30ca\u30fc\u306e\u304a\u77e5\u3089\u305b"},"content":{"rendered":"

10\/7(\u6c34) 15:00\u3088\u308aE305\u3067\u304a\u3053\u306a\u3044\u307e\u3059\u3001\u300c\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\uff08CORE-U\uff09\u30bb\u30df\u30ca\u30fc\u300d\u3092\u304a\u77e5\u3089\u305b\u3044\u305f\u3057\u307e\u3059\u3002\u4e8b\u524d\u306e\u53c2\u52a0\u767b\u9332\u306f\u5fc5\u8981\u3042\u308a\u307e\u305b\u3093\u306e\u3067\u3001\u591a\u304f\u306e\u65b9\u306e\u3054\u53c2\u52a0\u3092\u304a\u5f85\u3061\u3057\u3066\u304a\u308a\u307e\u3059\u3002
\u3088\u308d\u3057\u304f\u304a\u9858\u3044\u3057\u307e\u3059\u3002<\/p>\n

\n

2015\u5e74\u5ea6\u7b2c7\u56de(\u901a\u7b97\u7b2c12\u56de) Core-U\u30bb\u30df\u30ca\u30fc<\/p>\n

\u65e5\u6642\uff1a2015\u5e7410\u67087\u65e5(\u6c34) 15:00-
\u5834\u6240\uff1aE305\u6559\u5ba4
\u8b1b\u5e2b\uff1a\u4e95\u4e0a\u82b3\u5e78\u6c0f(ISAS\/JAXA International Top Young Fellow)
\u30bf\u30a4\u30c8\u30eb\uff1aCosmic Gamma-ray Background Radiation<\/p>\n

\u30a2\u30d6\u30b9\u30c8\u30e9\u30af\u30c8\uff1a
The cosmic gamma-ray background radiation is one of the most
fundamental observables in the gamma-ray band. Although the origin of
the cosmic gamma-ray background radiation has been a mystery for a
long time, the Fermi gamma-ray space telescope has recently measured
it at 0.1-820 GeV and revealed that the cosmic GeV gamma-ray
background is composed of blazars, radio galaxies, and star-forming
galaxies. However, Fermi still leaves the following questions. Those
are dark matter contribution, origins of the cosmic MeV gamma-ray
background, and the connection to the IceCube TeV-PeV neutrino events.
In this talk, I will review our current understandings of the cosmic
gamma-ray background and discuss future prospects of cosmic gamma-ray
background radiation studies.<\/p>\n

\n

 <\/p>\n

\u6975\u9650\u5b87\u5b99\u62e0\u70b9(Core-U)\u30bb\u30df\u30ca\u30fc\u4fc2\u3000\u5fd7\u57a3\u3001\u4e21\u89d2\u3001\u6c34\u91ce(\u6587\u8cac)<\/p>\n","protected":false},"excerpt":{"rendered":"

10\/7(\u6c34) 15:00\u3088\u308aE305\u3067\u304a\u3053\u306a\u3044\u307e\u3059\u3001\u300c\u6975\u9650\u5b87\u5b99\u7814\u7a76\u62e0\u70b9\uff08CORE-U\uff09\u30bb\u30df\u30ca\u30fc\u300d\u3092\u304a\u77e5\u3089\u305b\u3044\u305f\u3057\u307e\u3059\u3002\u4e8b\u524d\u306e\u53c2\u52a0\u767b\u9332\u306f\u5fc5\u8981\u3042\u308a\u307e\u305b\u3093\u306e\u3067\u3001\u591a\u304f\u306e\u65b9\u306e\u3054\u53c2\u52a0\u3092\u304a\u5f85\u3061\u3057\u3066\u304a\u308a\u307e\u3059\u3002\u3088\u308d\u3057\u304f\u304a\u9858\u3044\u3057\u307e\u3059\u3002 2015\u5e74\u5ea6\u7b2c7\u56de(\u901a\u7b97\u7b2c12\u56de) Core-U\u30bb\u30df\u30ca\u30fc \u65e5\u6642\uff1a2015\u5e7410\u67087\u65e5(\u6c34) 15:00-\u5834\u6240\uff1aE305\u6559\u5ba4\u8b1b\u5e2b\uff1a\u4e95\u4e0a\u82b3\u5e78\u6c0f(ISAS\/JAXA International Top Young Fellow)\u30bf\u30a4\u30c8\u30eb\uff1aCosmic Gamma-ray Background Radiation \u30a2\u30d6\u30b9\u30c8\u30e9\u30af\u30c8\uff1aThe cosmic gamma-ray background radiation is one of the mostfundamental observables in the gamma-ray band. Although the origin ofthe cosmic gamma-ray background radiation has been a mystery for along time, the Fermi gamma-ray space telescope has recently measuredit at 0.1-820 GeV and revealed that the cosmic GeV gamma-raybackground is composed of blazars, radio galaxies, and star-forminggalaxies. However, Fermi still leaves the following questions. Thoseare dark matter contribution, origins of the cosmic MeV gamma-raybackground, and the connection to the IceCube TeV-PeV neutrino events.In this talk, I will review our current understandings of the cosmicgamma-ray background and discuss future […]<\/p>\n","protected":false},"author":2,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_exactmetrics_skip_tracking":false,"footnotes":""},"categories":[8],"tags":[],"class_list":["post-848","post","type-post","status-publish","format-standard","hentry","category-news-list-en"],"_links":{"self":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/posts\/848","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/comments?post=848"}],"version-history":[{"count":1,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/posts\/848\/revisions"}],"predecessor-version":[{"id":849,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/posts\/848\/revisions\/849"}],"wp:attachment":[{"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=848"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/categories?post=848"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/core-u.hiroshima-u.ac.jp\/en\/wp-json\/wp\/v2\/tags?post=848"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}