<<<<<<<<<<<<<<<<<<< CRC News No.1389：2009年 11月 2日 >>>>>>>>>>>>>>>>>>>>> ＣＲＣ会員 各位 ＣＲＣ事務局 宇宙線研支部 *******＜ 「高エネルギー宇宙物理と加速器科学」に関する国際研究会 ＞******* 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理論センターで行われる「高エネルギー宇宙物理と加速器科学」に関する国際 研究会のsecond circularを送らせていただきます。 旅費補助にまだまだ余裕がありますので、明日１１月３日（火）まで参加登録を 会議ホームページ http://www-conf.kek.jp/heap09/ にて受け付けます。 FermiチームのIgor Moskalenko、PAMELAチームのMarco Casolino、OxfordのSubir Sarkarなど多くの招待講演が予定されています。 ぜひご参加ください。 研究会LOC =========================================================================== KEK-CPWS-HEAP2009 KEK Theory Center Cosmophysics Group Workshop on High Energy Astrophysics 2009 --- Cosmic Particles, Jets and Accelerator Science --- 10 (Tue) - 12 (Thu) Nov. 2009 KEK, Tsukuba, Japan Seminar Hall, 1F Building 4 (Yon-Go-Kan Bldg.) URL: http://www-conf.kek.jp/heap09/ Second Circular (1 Nov. 2009) =========================================================================== This is the second circular of the KEK Theory Center Cosmophysics Group Workshop "High Energy Astrophysics 2009 - Cosmic Particles, Jets and Accelerator Science -". The program has shortened from 10-13 Nov. to 10-12 Nov., and the registration fee has changed to 1,000 yen. Sorry for these alternations. Aim: High energy astrophysics is now a crossover discipline tying the diverse fields of particle physics, astrophysics and cosmology. The Large Hadron Collider (LHC) will soon begin its exploration of TeV scale physics, whose results can profoundly affect the future development of cosmology and particle astrophysics. The recently-launched Fermi Gamma-ray Space Telescope has already detected numerous objects at GeV energies, including new pulsars and cosmological jet sources such as gamma-ray bursts and active galactic nuclei. Possible excesses of cosmic-ray electrons and positrons, recently indicated by PAMELA and ATIC/PPB-BETS, also connect dark matter physics and astrophysics. In the TeV gamma-ray sky, ground-based telescopes (HESS/MAGIC/VERITAS/MILAGRO) have successfully made many new discoveries, leading to dedicated plans for next-generation facilities (CTA/AGIS/HAWC). We are also witnessing the dawn of a new era of multi-messenger astronomy, utilizing not only photons but also cosmic-rays (Auger/TA), neutrinos (IceCube/ANTARES) and gravitational waves (LIGO/Virgo/GEO/LCGT/AIGO/LISA/DECIGO). In these interdisciplinary fields, the role of accelerator laboratories are becoming ever more important, both technologically and scientifically, as exemplified by the Fermi experiment led by SLAC. In view of the difficulties in advancing the energy frontier in terrestrial experiments, this trend is expected to intensify along with future increases in energy scale and project size. Thus, the time is ripe to seriously consider how KEK can commit itself in this direction, including the iniation of large, experimental cosmophysics projects as its main activity on a 10-year time scale. The aim of this workshop is to exchange ideas on some of the most fundamental problems in cosmophysics, such as the origin of cosmic particles and jets and the nature of dark matter, as well as to address the future of accelerator laboratories including KEK, by discussing the latest observational and theoretical developments in these fields with invited researchers from around the world. Invited Speakers: Ballmer, Stefan W. (NAOJ/Caltech) [GW] Casolino, Marco (Roma2, INFN) [PAMELA] Fox, Patrick (FNAL) [Particle Physics] Kappes, Alexander (Erlangen) [Neutrino] Moskalenko, Igor (Stanford) [Anti-CR] (via EVO) Mueller, Berndt (Duke) [Hadron Physics] (via EVO) Sarkar, Subir (Oxford) [Astro-particle] Teshima, Masahiro (MPI) [Gamma, CTA] Uchiyama, Yasunobu (SLAC) [Gamma, Fermi] Asano, Katsuaki (Tokyo Inst Tech) [GRB] Hirano, Tetsufumi (Tokyo) [Hadron Physics] Inoue, Susumu (Kyoto) [Gamma] Itow, Yoshitaka (Nagoya) [LHCf] Nakamura, Takuji (NiPR) [Radar] Kohri, Kazunori (Tohoku) [Astro-particle] Shimizu, Hirohiko (KEK) [EUSO] Takahashi, Fuminobu (IPMU) [Particle Physics] Torii, Shoji (Waseda) [CALET] Totani, Tomonori (Kyoto) [Gamma] Tsuboi, Masato (JAXA) [ASTRO-G] Registration: The registration desk is open from 9:30 on 10 (Tue). The registration fee is 1,000 yen. Only cash is accepted and will be collected at the registration desk. You may get your name tag and receipt. Please return the name tag after the conference. Banquet: A banquet is held on the 2nd day (3,000 yen) at the KEK restaurant. The fee will be collected at the registration desk by cash. Receipts will be issued. Oral presentation: A liquid crystal display (LCD) projector is available. We will collect your talk files (ppt or pdf) after presentations to upload on our website. KEK dormitory: Key: The key can be received at the entrance of the KEK dormitory till 22:00 and at the information center after 22:00. Charge: The dormitory charge will be withheld from the travel support if you receive the support from KEK. If you do not have the support from KEK, the charge should be paid at the User's Office located behind the information center. The User's Ofiice is open from 9:00 to 17:00. For invited speakers, we have booked a hotel, URBAN HOTEL http://www.urbanhotel.co.jp/uhotel.html which is within walking distance of KEK (~20-25min) and ~10min from Tsukuba Center by car. Internet: To use the wireless LAN, you need to apply for it in advance according to the following procedure. http://www.kek.jp/uskek/eng/other/lan2.html Access: For general information: http://www.kek.jp/intra-e/access/index.html Bus from Narita airport to Tsukuba Center: We note that the seat reservation is required to go to the Narita airport from Tsukuba Center. Please let us know if you need the reservation. http://www.kek.jp/RSO/guide/transportation/narita_jikokuhyo.html Bus from Tsukuba Center (station) to KEK http://www.kek.jp/intra-e/access/timetable1.html For invited speakers, a shuttle bus from Urban Hotel to KEK is provided 10 Nov. 9:35 from Urban to KEK, 18:45 from KEK to Urban 11 Nov. 8:35 from Urban to KEK, 21:00 from KEK to Urban 12 Nov. 9:05 from Urban to KEK, 18:30 from KEK to Urban Climate: The weather information is available, for example, from http://www.weather-forecast.com/locations/Tsukuba/forecasts/latest Currency Exchange: We recommend you to exchange your money into Japanese Yens at a Currency Exchange counter at the Airport on your arrival. The information is available from http://www.narita-airport.jp/en/guide/service/list/svc_11.html Program: 10 (Tue) Nov. 9:30-10:15 Registration 10:15-10:30 Opening Address 10:30-11:30 Uchiyama, Yasunobu (SLAC) [50+10] First Year Results from the Fermi Gamma-ray Space Telescope 11:30-12:45 Lunch 12:45-13:30 Asano, Katsuaki (Tokyo Inst Tech) [40+5] High-Energy Gamma-Rays and Physical Implication for GRBs in Fermi Era 13:30-14:15 Totani, Tomonori (Kyoto) [40+5] The Cosmic Gamma-Ray Background Radiation 14:15-15:00 Inoue, Susumu (Kyoto) [40+5] Gamma-ray absorption by cosmic radiation fields [Gamma] 15:00-15:30 Murase, Kohta (YITP, Kyoto) [25+5] Ultrahigh-energy photons as a probe of the highest-energy cosmic-ray sources 15:30-16:00 Break 16:00-17:00 Teshima, Masahiro (MPI) [50+10] TBA [Gamma, CTA] 17:00-17:45 Tsuboi, Masato (JAXA) [40+5] VSOP2 Project: "Astronomical Microscope" 17:45-18:30 Nakamura, Takuji (NiPR) [40+5] TBA [Radar] 11 (Wed) Nov. 9:00-10:00 Mueller, Berndt (Duke) via EVO [50+10] Probing the equilibrium and pre-equilibrium structure of the quark-gluon plasma in relativistic heavy ion collisions 10:00-10:45 Hirano, Tetsufumi (Tokyo) [40+5] Perfect fluidity of the QGP in relativistic heavy ion collisions [Hadron Physics] 10:45-11:30 Itow, Yoshitaka (Nagoya) [40+5] TBA [LHCf] 11:30-12:45 Lunch 12:45-13:30 Shimizu, Hirohiko (KEK) [40+5] TBA [EUSO] 13:30-14:30 Kappes, Alexander (Erlangen) [50+10] TBA [Neutrino] 14:30-15:00 Takami, Hajime (IPMU) [25+5] Spatial correlation of highest energy cosmic rays with galaxies in local Universe 15:00-15:30 Break 15:30-16:30 Ballmer, Stefan W. (NAOJ/Caltech) [50+10] An upper limit on the stochastic gravitational-wave background of cosmological origin [GW] 16:30-17:00 Ando, Masaki (Kyoto) [25+5] DECIGO and pathfinder missions 17:00-17:30 Suwa, Yudai (U. Tokyo) [25+5] Probing the central engine of long gamma-ray bursts and hypernovae with gravitational waves 17:30-17:45 Short Break 17:45-18:45 Casolino, Marco (Roma2, INFN) [50+10] Pamela results and status 18:45-21:00 Banquet 12 (Thu) Nov. 9:30-10:30 Moskalenko, Igor (Stanford) via EVO [50+10] TBA [Cosmic-Ray] 10:30-11:30 Sarkar, Subir (Oxford) [50+10] Explaining the PAMELA/FERMI data with a nearby cosmic ray accelerator 11:30-12:45 Lunch 12:45-13:30 Torii, Shoji (Waseda) [40+5] TBA [CALET] 13:30-14:00 Osone, Satoko (N/A) [25+5] High energy resolution GeV gamma ray detector 14:00-14:30 Kawanaka, Norita (KEK) [25+5] Cosmic-Ray Electron Excess from Pulsars is Spiky or Smooth?: Continuous and Multiple Electron/Positron Injections 14:30-15:00 Yamada, Toshifumi (KEK) [25+5] Singlet Dark Matter, Type II Seesaw and Cosmic Ray Signals 15:00-15:30 Break 15:30-16:30 Fox, Patrick (FNAL) [50+10] TBA [Particle Physics] 16:30-17:15 Takahashi, Fuminobu (IPMU) [40+5] Decaying dark matter and cosmic rays 17:15-18:00 Kohri, Kazunori (Tohoku) [40+5] Positron excess? -- from viewpoint of both particle physics and astrophysics -- SOC: Asano, Katsuaki (Tokyo Inst Tech) Hazumi, Masashi (KEK) Inoue, Susumu (Kyoto) Itakura, Kazunori (KEK) Kamae, Tsuneyoshi (SLAC) Kawamura, Seiji (NAOJ) Nojiri, Mihoko (KEK) Shimizu, Hirohiko (KEK) Takahashi, Tadayuki (JAXA) Teshima, Masahiro (MPI) Torii, Shoji (Waseda) Yamamoto, Akira (KEK) Yamazaki, Ryo (Hiroshima) Yoshimura, Koji (KEK) LOC: Kodama, Hideo Ioka, Kunihito Kawanaka, Norita Suwa, Yudai Contact: Secretary: Shishido, Tamao Theory Center, Institute of Particle and Nuclear Studies KEK (High Energy Accelerator Research Organization) 1-1 Oho, Tsukuba 305-0801, Japan tamawo (at) post.kek.jp Supported by: 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, No.21684014. KEK Theory Center. ＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝＝