<<<<<<<<<<<<<<<<<<< CRC News No.1768：2011年 9月20日 >>>>>>>>>>>>>>>>>>>>> ＣＲＣ会員 各位 ＣＲＣ事務局 宇宙線研支部 *******＜ KEK理論センター国際研究会 KEK-CPWS-HEAP2011: 2nd circ. ＞******* 皆様 （このメールを重複して受け取られた場合はご容赦ください。） KEK理論センターで２０１１年１１月１３日（日）〜１１月１５日（火）に行われる 国際研究会「High Energy Astroparticle Physics」のセカンドサーキュラーを お送ります。 参加登録，講演申し込み等は会議ホームページ http://kds.kek.jp/conferenceDisplay.py?confId=7625 から受付けています。今月末締切です。 皆様の参加をお待ちしております。 HEAP2011 SOC & LOC =========================================================================== KEK-CPWS-HEAP2011 KEK Theory Center Cosmophysics Group Workshop High Energy Astroparticle Physics 2011 --- Gamma-Ray Universe: Fermi to CTA --- 13 (Sun) - 15 (Tue) Nov. 2011 Kobayashi-Hall, Kenkyu-Honkan Bldg. KEK, Tsukuba, Japan URL: http://kds.kek.jp/conferenceDisplay.py?confId=7625 (A username and a password will also appear on the screen) Second Circular (20 Sep. 2011) =========================================================================== Aim: The high energy astrophysics and astroparticle physics is now a crossover discipline tying the diverse fields of Particle Physics, Cosmology and Astrophysics. The aim of the workshop is to exchange ideas on the intertwined fundamental problems, such as the origin of cosmic particles and jets, the nature of dark matter and Physics beyond the Standard Model by discussing the latest observational and theoretical developments in these fields with leading researchers from around the world. The workshop is held as part of annual activities in KEK to promote these attractive areas. This year we put some emphasis on the gamma-ray universe revealed by the current Fermi Gamma-ray Space Telescope and future Cerenkov Telescope Array (CTA), still widely covering the related topics. As evidenced by the Fermi satellite, the gamma-ray sky provides the prime mover not only scientifically but also technologically for the accelerator laboratories. CTA is the next generation instrument constructed internationally, with a factor of 5-10 improvement in sensitivity in the 100 GeV to 10 TeV range and the extension to energies well below 100 GeV and above 100 TeV. We discuss the scientific prospects on top of the recent developments led by the ongoing projects, such as Fermi, LHC, PAMELA, AKARI, IceCube, etc. Invited Speakers: Casolino, Marco (RIKEN) [Cosmic Ray, PAMELA] Ebisuzaki, Toshikazu [Cosmic Ray, EUSO] Gondolo, Paolo (Utah) [Dark Matter] Itow, Yoshitaka (Nagoya) [LHCf] Kohri, Kazunori (KEK) [Axion] Matsumoto, Toshio (Seoul) [Cosmic Infrared Background] Ohira, Yutaka (KEK) [Supernova Remnant] Ostapchenko, Sergey (NTNU) [Hadron] Paneque, David (MPI) [Fermi] [Axion] Reville, Brian (Oxford) [Particle Acceleration] Sarkar, Subir (Oxford) [Fundamental Physics, Cosmic Ray] Siegal-Gaskins, Jennifer (Ohio/Caltech) [Gamma-Ray Background] Stawarz, Lukasz (JAXA) [Active Galactic Nuclei] Teshima, Masahiro (MPI/ICRR) [CTA, Very-High-Energy Highlights] Toma, Kenji (Osaka) [Gamma-Ray Burst] Torii, Shoji (Waseda) [Cosmic Ray, CALET] Totani, Tomonori (Kyoto) [Extragalactic Background Light, Gamma] Wang, Xiang-Yu (Nanjing) [Hypernova, Cosmic Ray] Yoshida, Shigeru (Chiba) [Neutrino, IceCube] Yoshimura, Koji (KEK) [Cosmic Ray, BESS] Registration (Deadline: 30 Sep. 2011): All participants are required to make an on-line registration through KEK User Registration as instructed in the webpage: http://kds.kek.jp/internalPage.py?pageId=10&confId=7625 The registration fee will be collected at the registration desk by cash. Abstract submission (Deadline: 30 Sep. 2011): In addition to the invited talks, we have slots for oral talks. If you would like to have a talk, please give the title and abstract at the on-line registration. We will collect your talk files (ppt or pdf) after presentations to upload on our website. If we have too many applications, we will prepare poster boards. Social Events (Deadline: 30 Sep. 2011): A reception and a banquet will be held on the 1st and 2nd nights. We will also have a lunch box at the 1st day because the Cafeteria is closed on Sunday. Please apply for these at the on-line registration. Accommodation: - Daiwa Roynet Hotel (http://www.daiwaroynet.jp/tsukuba/): Near Tsukuba Center. 20 min to KEK by bus. - Okura Frontier Hotel (http://www.okura-tsukuba.co.jp/): Near Tsukuba Center. 20 min to KEK by bus. Get a discount by telling that you attend the KEK workshop. - Urban Hotel (http://www.urbanhotel.co.jp/uhotel.html): 20-25 min walk to KEK. Get a discount by telling that you attend the KEK workshop. - KEK dormitory (http://www.kek.jp/intra-e/map/annai/shukuhaku.html): Apply at the KEK User Registration. The number of rooms with bath and toilet is limited. For rooms without bath and toilet, we have a comfortable public bath/shower/toilet. We will book the hotel (Daiwa Roynet Hotel) for invited speakers. Internet: To use the wireless LAN, you need to apply for it in advance at the registration page: http://kds.kek.jp/internalPage.py?pageId=10&confId=7625 Access: - General information between Airport, Tsukuba Center and KEK: http://www.kek.jp/RSO/eng/Timetable_Map.html - Bus from Narita Airport to Tsukuba Center: Airport Bus is the most convenient way to get Tsukuba Center from Narita Airport. http://www.kek.jp/RSO/transportation/NaritaAirport.pdf - Bus from Tsukuba Center to KEK: We have two choices, Hokubu-Shuttle-Bus (convenient) and Kantetsu-Bus. http://www.kek.jp/RSO/eng/transportation/Center_KEK0401.pdf Currency Exchange: We recommend you to exchange your money into Japanese Yens at the Airport on your arrival. Program (tentative): 13 (Sun) Nov. -- 11:30 David Paneque (MPI) Astrophysics with the Fermi satellite 11:30 - 13:00 Lunch 13:00 -- Kenji Toma (Osaka) [Gamma-Ray Burst] Xiang-Yu Wang (Nanjing) Hypernova model for ultra-high energy cosmic rays Lukasz Stawarz (JAXA) [Active Galactic Nuclei] Brian Reville (Oxford) Particle acceleration and CTA: Beyond the diffusion approximation Yutaka Ohira (KEK) [Supernova Remnant] 14 (Mon) Nov. -- 11:30 Masahiro Teshima (MPI/ICRR) [CTA, Very-High-Energy Highlights] Shigeru Yoshida (Chiba) [Neutrino, IceCube] 11:30 - 13:00 Lunch 13:00 -- Paolo Gondolo (Utah) [Dark Matter] Subir Sarkar (Oxford) [Fundamental Physics, Cosmic Ray] David Paneque (MPI) Indirect detection of Axion-Like-Particles through gamma-ray astronomy Kazunori Kohri (KEK) [Axion] 15 (Tue) Nov. -- 11:30 Jennifer Siegal-Gaskins (Ohio/Caltech) The diffuse gamma-ray background Toshio Matsumoto (Seoul) [Cosmic Infrared Background] Tomonori Totani (Kyoto) [Extragalactic Background Light, Gamma] 11:30 - 13:00 Lunch 13:00 -- Yoshitaka Itow (Nagoya) [LHCf] Sergey Ostapchenko (NTNU) LHC and UHECR physics Marco Casolino (RIKEN) [Cosmic Ray, PAMELA] Koji Yoshimura (KEK) [Cosmic Ray, BESS] Shoji Torii (Waseda) [Cosmic Ray, CALET] Toshikazu Ebisuzaki [Cosmic Ray, EUSO] Subir Sarkar (Oxford) Summary SOC: Hagiwara, Kaoru (KEK) Ioka, Kunihito (KEK) Kodama, Hideo (KEK) Kohri, Kazunori (KEK) Nojiri, Mihoko (KEK/IPMU) Okada, Yasuhiro (KEK) Tajima, Hiro (SLAC/Nagoya) Teshima, Masahiro (MPI/ICRR) Totani, Tomonori (Kyoto) Yoshida, Tatsuo (Ibaraki) LOC: Ioka, Kunihito (KEK) Kawanaka, Norita (KEK) Kodama, Hideo (KEK) Kohri, Kazunori (KEK) Mizuta, Akira (KEK) Ohira, Yutaka (KEK) Contact: Inquiries to: Ioka, Kunihito Secretary: Shishido, Tamao Theory Center, Institute of Particle and Nuclear Studies KEK (High Energy Accelerator Research Organization) 1-1 Oho, Tsukuba 305-0801, Japan Supported by: - KEK Theory Center. - Hayama Center for Advanced Studies, the Graduate University for Advanced Studies (SOKENDAI). - Grant-in-Aid from the Ministry of Education, Culture, Sports, Science and Technology (MEXT) of Japan, 23540327, 21684014. ＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝