From: "Mihoko M. Nojiri"
To: sg-l__AT__yukawa.kyoto-u.ac.jp
Date: Tue, 6 Oct 2009 22:11:46 +0900
Subject: [sg-l 5301] KEK-CPWS-HEAP2009 

KEK理論センターの workshop のお知らせです。
野尻
＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃＃


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理論センターでは２００９年１１月１０日（火）〜１１月１３日 
（金）に
「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を行います。
FermiやPAMELAなどに関する多くの招待講演が予定されています。
参加登録，講演申し込み等は会議ホームページ
http://www-conf.kek.jp/heap09/
から受付けています。
締切が間近ですが、多数の参加をお待ちしております。

井岡　邦仁

= 
= 
= 
========================================================================

                          KEK-CPWS-HEAP2009

              KEK Theory Center Cosmophysics Group Workshop
                    on High Energy Astrophysics 2009
         --- Cosmic Particles, Jets and Accelerator Science ---

                     10 (Tue) - 13 (Fri) Nov. 2009
                          KEK, Tsukuba, Japan
              Seminar Hall, 1F Building 4 (Yon-Go-Kan Bldg.)

                  URL: http://www-conf.kek.jp/heap09/

                     First Circular (5 Oct. 2009)

= 
= 
= 
========================================================================

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]
Beloborodov, Andrei (Columbia)* [GRB]
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]
Kawai, Nobuyuki (Tokyo Inst Tech)* [Fermi, MAXI]
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]
(* to be confirmed)

Registration (Deadline: 31 Oct. 2009):
The online registration is available through the webpage
http://www-conf.kek.jp/heap09/. Through the same page,
you can make your abstract submission and KEK User Registration.
All visitors to KEK are supposed to make the KEK User Registration,
independently of the workshop registration. Instructions can be
found on the webpage.

Abstract submission (Deadline: 21 Oct. 2009):
In addition to the invited talks, we have some slots for oral talks.
We will have no poster session. If you would like to give a talk,
please give the title and abstract when you make the online  
registration.

Registration Fee:
The registration fee is 500 yen. The fee will be collected at the
registration desk by cash. This covers beverage and food during
coffee break.

Banquet:
We are planning to have a banquet on the 2nd day (~3000 yen).
The fees will be collected at the registration desk by cash.

Accommodation:
KEK has a big dormitory for visitors. If you would like to book a
single bedroom without bath and restroom, you can make a reservation
when you make the online registration. This dormitory is equipped with
laundry rooms, shower rooms and shared kitchens. The room charge is
1,500 yen per night. Although you can reserve a room with bath and
restroom, it is limited in number and you have to make a reservation
by yourself through the webpage of the KEK Users Office. You also need
to make the User Registration in advance. There are a couple of hotels
outside the KEK campus as well. If you would like to use them, please
make booking by yourself. For invited speakers, we will make
arrangements for 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.

Financial support (Deadline: 21 Oct. 2009):
We will support the expenses of the domestic travel and accommodation in
the KEK dormitory for participants, in priority to oral speakers. Note
that we can only provide the dormitory-rate-equivalent even if you stay
at a hotel. You can apply for the financial support when you make the
online registration.

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

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

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.
%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
From: "Mihoko M. Nojiri"
To: sg-l__AT__yukawa.kyoto-u.ac.jp
Date: Mon, 2 Nov 2009 16:53:16 +0900
Subject: [sg-l 5356] KEK理論センター国際研究会 High Energy Astrophysics 2009 (KEK-CPWS-HEAP2009): Second circular

依頼により転送します。
>
>
> 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.