Appendix 1. CRC 13 Appendix Appendix LCGT 18 DECIGO 18 XMASS 19 GADZOOKS! 20 NEWAGE(

Similar documents
Telescope Array FD SD SD

CMB and DM (Cosmic Microwave Background and Dark Matter) ~ ~

PowerPoint プレゼンテーション

スーパーカミオカンデにおける 高エネルギーニュートリノ研究

E 1 GeV E 10 GeV 1 2, X X , GeV 10 GeV 1 GeV GeV π

untitled

(e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ,µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) [ ] [ ] [ ] ν e ν µ ν τ e µ τ, e R,µ R,τ R (2.1a

_spring_school.key

1/2 ( ) 1 * 1 2/3 *2 up charm top -1/3 down strange bottom 6 (ν e, ν µ, ν τ ) -1 (e) (µ) (τ) 6 ( 2 ) 6 6 I II III u d ν e e c s ν µ µ t b ν τ τ (2a) (

7-1yamazaki.pptx

<4D F736F F F696E74202D205A FC82C982E682E B18E CC95A8979D2E >

cm λ λ = h/p p ( ) λ = cm E pc [ev] 2.2 quark lepton u d c s t b e 1 3e electric charge e color charge red blue green qq

W 1983 W ± Z cm 10 cm 50 MeV TAC - ADC ADC [ (µs)] = [] (2.08 ± 0.36) 10 6 s 3 χ µ + µ 8 = (1.20 ± 0.1) 10 5 (Ge

Microsoft PowerPoint - okamura.ppt[読み取り専用]

空気シャワーコア観測によるKnee起源の解明

TAMA --> CLIO ---> LCGT TAMA 300m基線長 三鷹(NAOJ) CLIO 100m 神岡 低温鏡 年5月17日火曜日

1 223 KamLAND 2014 ( 26 ) KamLAND 144 Ce CeLAND 8 Li IsoDAR CeLAND IsoDAR ν e ν µ ν τ ν 1 ν 2 ν MNS m 2 21

LHC ALICE (QGP) QGP QGP QGP QGP ω ϕ J/ψ ALICE s = ev + J/ψ

306 [7] GeV TeV PAMELA 100 GeV PAMELA AMS GeV [8] TeV [9] PAMELA[10] AMS BESS-Polar 95 [11]AMS 1.3 AMS AMS rigidity TOFTime Of Flight TRDE

Bethe-Bloch Bethe-Bloch (stopping range) Bethe-Bloch FNAL (Fermi National Accelerator Laboratory) - (SciBooNE ) SciBooNE Bethe-Bloch FNAL - (SciBooNE

LHCfZ (RHICf, LHC 軽原子核衝突 ) さこ隆志名大 STE/KMI 2014/03/14 CRC タウンミーティング 1

Fermi ( )

21 Daya Bay θ 13 Lawrence Berkeley National Laboratory Brookhaven National Laboratory 2012 ( 24 ) Daya Bay 2011

Mathews Grant J. (University of Notre Dame) Boyd Richard N. (Lawrence Livermore National Laboratory) 2009/5/21

Microsoft Word - 最終報告_ 期_v6.9.doc

( ) Note Ω m = 1 Ω m : ( ) r-process α 1: 2 32T h(t 1/2 = y) 2 38U(t 1/2 = y) 2 35U(t 1/2 = 7.038

スライド 1

スライド 1

共同利用2017-ALPACA-Ver.0.2.key

PowerPoint Presentation

JPS-Niigata pptx

6 2 T γ T B (6.4) (6.1) [( d nm + 3 ] 2 nt B )a 3 + nt B da 3 = 0 (6.9) na 3 = T B V 3/2 = T B V γ 1 = const. or T B a 2 = const. (6.10) H 2 = 8π kc2

加速器の基本概念 V : 高周波加速の基礎

( ) 09:00 17:40 08: :00 09: :05 10:15 1 ( ) -01 ( 5 ) (10:15 10:25 ) 10:25 11:50 2 ( ) -02 ( 6 ) (11:50 13:00 ) 13:00 1

Μ粒子電子転換事象探索実験による世界最高感度での 荷電LFV探索 第3回機構シンポジューム 2009年5月11日 素粒子原子核研究所 三原 智

2 X-ray 6 gamma-ray :38m 0:77m nm 17.2 Hz Hz 1 E p E E = h = ch= (17.2) p = E=c = h=c = h= (17.3) continuum continuous spectrum line spectru

B

スライド 1

Δ Δ Δ 250


(Cherenkov Telescope Array : CTA) (Large-Sized Telescope : LST) 2f CTA CTA CTA CTA-Japan LST CTA CTA 3 20 GeV 100 TeV 20 GeV 1000 GeV LST 23 m 23 m 1.

NEWAGE

1 2 2 (Dielecrics) Maxwell ( ) D H

: 8.2: A group (i.e. a very small cluster) of galaxies superimposed on a x-ray image from the ROSAT satellite

LEPS

07.報文_及川ら-二校目.indd

Microsoft PowerPoint - Ppt ppt[読み取り専用]


レジャー産業と顧客満足の課題

豪雨・地震による土砂災害の危険度予測と 被害軽減技術の開発に向けて

X線分析の進歩36 別刷

( ) Note (e ) (µ ) (τ ) ( (ν e,e ) e- (ν µ, µ ) µ- (ν τ,τ ) τ- ) ( ) ( ) (SU(2) ) (W +,Z 0,W ) * 1) 3 * 2) [ ] [ ] [ ] ν e ν µ ν τ e

Solar Flare neutrino for Super Novae Conference


jigp60-★WEB用★/ky494773452500058730

プログラム



Supersymmetry after Higgs discovery

研究歴

放射線化学, 92, 39 (2011)

Thick-GEM 06S2026A 22 3

cm H.11.3 P

subaruUM2010_murayama

宇宙ガンマ線観測で解き明かす暗黒物

nakajima_

NEWAGE

1.7 D D 2 100m 10 9 ev f(x) xf(x) = c(s)x (s 1) (x + 1) (s 4.5) (1) s age parameter x f(x) ev 10 9 ev 2

J-PARC October 14-15, 2005 KEK

スライド 1

150518_shin_gakujutsu

Report10.dvi

スライド 1

03J_sources.key


-1-

Undulator.dvi

Title ブラックホールと重力波天文学 Author(s) 長峯, 健太郎 Citation 高大連携物理教育セミナー報告書. 28 Issue Date Text Version publisher URL DO

Proposal of a next-generation GW detector using huge mirrors abstract April 10, introduction 1 2 design parameters and sensitivity 2 3 mirror c


Operation_test_of_SOFIST

PowerPoint プレゼンテーション

スライド 1

LHC ATLAS Large Hadron Collider 27km TeV ~48pb -1 ATLAS LHC Higgs Muon spectrometer MDT RPC,TGC


研究成果報告書

IEEE HDD RAID MPI MPU/CPU GPGPU GPU cm I m cm /g I I n/ cm 2 s X n/ cm s cm g/cm

untitled

VUV MPPC study

訪問看護ステーションにおける安全性及び安定的なサービス提供の確保に関する調査研究事業報告書

Transcription:

CRC 22

1 3 2 4 2-1 2-2 2-3 2-4 3 9 3-1 3-2 3-3 3-4 3-5 4 12 Appendix 1. CRC 13 Appendix 2. 14 Appendix 3. 17 LCGT 18 DECIGO 18 XMASS 19 GADZOOKS! 20 NEWAGE( ) 21 22 24 CTA (Cherenkov Telescope Array) 25 CALET 26 Tibet AS+MD+YAC Project 27 TALE TA-phase2 28 JEM-EUSO 29 IceCube/ARA 30 31 Gamma-ray burst for UNravelling Dark Ages Mission : GUNDAM 33 2

SciCR 35 LHCf 36 37 3

1 CRC 1 2010 9 16 17 84 Appendix 1 CRC 2 1950 1980 AGASA 3 CANGAROO 4 5 6 7 2000 1 http://www.icrr.u-tokyo.ac.jp/crc/ 2 50 50 51 7 1996 3 http://www-akeno.icrr.u-tokyo.ac.jp/agasa/ 4 http://vesper.icrr.u-tokyo.ac.jp/ 5 http://www.icrr.u-tokyo.ac.jp/em/index-j.html 6 http://www-sk.icrr.u-tokyo.ac.jp/sk/index.html 7 http://taws100.icrr.u-tokyo.ac.jp/ 4

CRC 2010 LCGT CRC 5

2 ( 1) 1 2 3 4 2-1 1912 V. Hess 100 20 X Fermi 8 10 14 ev 10 15 ev LHC 10 20 ev GZK 9 8 http://fermi.gsfc.nasa.gov/ 9 K. Greisen, Phys. Rev. Lett. 16, 748 (1966); G.T. Zatsepin, V.A. Kuz min, JETP Lett. 4, 78 (1966) 6

AGASA GZK 10 20 ev Pierre Auger 10 Telescope ArrayGZK 10 19 ev 1989 Whipple 1990 100 TeV CANGAROO H.E.S.S. 11 MAGIC 12 VERITAS 13 TeV 1960 1990 Compton 14 BATSE 1997 BeppoSAX 15 X HETE-2 Swift Fermi 10 http://www.auger.org/ 11 http://www.mpi-hd.mpg.de/hfm/hess/hess.html 12 http://wwwmagic.mppmu.mpg.de/ 13 http://veritas.sao.arizona.edu/ 14 http://heasarc.gsfc.nasa.gov/docs/cgro/index.html 15 http://www.asdc.asi.it/bepposax/ 7

8 図1 宇宙線研究の各分野と本シンポで取り上げられた現行 将来アクティビティ

2-2 Kamiokande 1987 2 1987A 1996 Super-Kamiokande Kamiokande KamLAND Maki-Nakagawa-Sakata 13 1 3 CP IceCube 16 1 km 3 17 WMAP 18 4 23 73 WIMP (Weakly Interacting Massive Particle) CERN LHC (Large Hadron Collider) 19 XMASS 16 http://icecube.wisc.edu/ 17 IceCube 18 http://map.gsfc.nasa.gov/ 19 http://lhc.web.cern.ch/lhc/ 9

2-3 20 TAMA300 2010 LCGT LIGO (Laser Interferometer Gravitational-wave Observatory) 21 VIRGO 22 2 4 km LCGT Short GRB 20 J. H. Taylor Jr. and R. A. Hulse, Astrophys. J. (Lett.) 196, L1 (1975) 21 http://www.ligo.caltech.edu/ 22 http://www.virgo.infn.it/ 10

s 2-4 X KamLAND LHC 11

3 23 Appendix 2 1 Appendix 3 3-1 CALET (CALorimetric Electron Telescope) 2 2010 4 2013 TeV 1 kpc CTA (Cherenkov Telescope Array) H.E.S.S. 24 MAGIC 25 Tibet AS+MD+YAC MD (Muon Detector array) YAC (Yangbajing Air shower Core detector) Telescope Array TALE (Telescope Array Low energy Extension) 10 17 ev 2 TA-phase2 JEM-EUSO (Extreme Universe Space Observatory onboard Japanese Experiment Module) LHC 23 24 http://www.mpi-hd.mpg.de/hfm/hess/hess.shtml 25 http://wwwmagic.mppmu.mpg.de/ 12

3-2 GADZOOKS! Super-Kamiokande 0.1 HyperKamiokande SuperKamiokande J-PARC (MNS CP KamLAND-Zen KamLAND 2011 KamLAND2-Zen KamLANDi-Zen Super-Kamiokande Super-KamLAND-Zen IceCube 2012 IceCube/ARA (Askaryan Radio Array) GZK 3-3 XMASS (Xenon detector for weakly interacting MASSive particle ) XMASS-I 800kg 10 XMASS-II 10ton pp NEWAGE (New generation WIMP search with an advanced gaseous tracker experiment) 30 13

3-4 LCGT (Large-scale Cryogenic Gravitational wave Telescope) 2010 3 km 7 2017 DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) LCGT (0.1 10 Hz) 1,000 km 3 2027 3-5 GUNDAM (Gamma-ray burst for UNravelling Dark Ages Mission) 0.1 20 Pathfinder JAXA ETCC) MeV SciCR(SciBar detector for Cosmic Ray) 1 6 SciBar LHCf(LHC forward experiment) LHC 0 11 14

4 LCGT 15

Appendix 1. CRC 2010 9 16 ( ) 10:30 17 ( ) 15 00 633-635 + ( ) 9 16 LCGT 30 DECIGO 20 XMASS 30 GADZOOKS! 20 NEWAGE 20 40 20 Cherenkov Telescope Array 40 CALET 30 Tibet AS+MD+YAC Project 30 STE CR activity STE 40 9 17 TALE TA-phase2 40 JEM-EUSO 30 The IceCube/ARA experiment 30 30 Gamma-ray burst for UNravelling Dark Ages Mission : GUNDAM 20 Discussion 120 16

Appendix 2. 17

18

時系列で示した一覧表 19

Appendix 3. LCGT 22 6 LCGT 22 7 3 LCGT LCGT 7 LCGT R&D 3 2017 LCGT LCGT LCGT LCGT R&D LCGT 20

DECIGO 22 10 7 DECIGO DECIGO Deci-hertz Interferometer Gravitational-Wave Observatory 0.1 Hz 10 Hz DECIGO LCGT DECIGO 1,000 km 3 DECIGO 0.1 Hz 10 Hz 10-23 Hz -1/2 4 2 10,000 21

XMASS XMASS SI=10-47 cm 2 10 pp- 2 30 mev 1keV 42 Z 54 3 850 kg 100 kg 10 1 50 SUSY 100 GeV WIMPs 10-45 cm 2 2010 II 1 5 pp- I 24 3 15 1 III 2 2 10 10 136 Xe 870 kg 30 mev Inverted mass hierarchy 29 3 96 6 22

GADZOOKS! SK 32000 40 SK 0.1 SK 100 10 (SRN) SRN 10-30 MeV SK 0.1% 10 5-33 SRN 10 MeV 3000 3 MeV m 2 12 1 6 10 kpc 8000 inverse-beta 300 6 3 95 2 Si 1000 200 240 SK 2010 2011 23

2012 3 SK SK 1 10 NEWAGE( ) mm 800 kg XMASS 2010 9 XMASS TPC (0.1 ) 2015 10 24

2007 30 cm TPC R&D 2015 60 cm DAMA 2020 1 m 1-2 1-3 Super-KamLAND 4 25% 80 km 1-3 4 25% Super-KamLAND 8 B 7 Be pep/cno KamLAND2 2 KamLANDi 3 136Xe -Zen: Zero Neutrino Double Beta CdWO4 CaF2 (CANDLES) DAMA/LIBRA NaI KamLAND-Zen 1 KamLAND2-Zen KamLANDi-Zen Super-KamLAND-Zen 25

1 KamLAND-Zen 400 kg 136 Xe KKDC 2011 2 KamLAND2(-Zen) 1000 kg 136 Xe 2015 3 KamLANDi(-Zen) ~1% 4 Super-KamLAND(-Zen) Zen 136 Xe 15wt 26

1998 0.05eV/c 2 6 6 100 20 1035 JPARC CP 2015 2025 723 10 27

CTA (Cherenkov Telescope Array) GeV TeV HESS MAGIC TeV GeV TeV CTA (Cherenkov Telescope Array) TeV TeV 1000 TeV 2009 2010 preparatory phase study 2014-15 CTAJapan Collaboration TeV 50 CTA CTA 10-20% CTA 150 MEuro 20-40 28

CALET JAXA ISS CALET: CALorimetric Electron Telescope CALET JAXA 2013 ISS 2 CALET ISS TeV PeV 29

1. Tibet AS+MD+YAC Project 2. takita@icrr.u-tokyo.ac.jp tel:04-7136-5128 3. ASγ 80 10,000 m 2 MD AS 4300 m 100 TeV Knee Knee Knee MD YAC 3-4 MD 1/3 30

TALE TA-phase2 700km 2 Surface Detector SD 38 Fluorescence Detectors FDsTA-phase1 2003 2008 FD Telescope Array Low energy Extension (TALE) TA-phase1 FD15 SD 100 10 17 ev TA-phase1 10 TA-phase20.5 TA-phase1 SD Stereoscopic FD 1747 FD 55 FD 40 km 61000 km 2 FD PMT 10 19 ev 100% duty factor 10% 6100 km 2 AGASA 61 TA-SD 9 Auger-South 2 TA-phase2 260 R&D TA-phase1 2015 31

JEM-EUSO (ISS) 10 13 ev 10 20 ev JEM-EUSO JEM-EUSO 10 19 ev < E < 10 21 ev 10 10 60 60 JEM-EUSO 3 5.5 10 19 ev 500 Greisen-Zatsepin-Kuz min GZK 10 11 GZK JEM-EUSO 2009 7 2010 8 2016 JAXA 2010 5 12 32

European Space Agency (ESA) Fundamental Physics Roadmap Team Astronomy Working Group European Science Foundation ESA ELIPSE 2010 11 1 SALMON IceCube/ARA IceCube 1 Km GeV 2005 2010 9 2011 IceCube 250 Collaboration IceCube TeV PeV EeV 10 20 ev GZK IceCube 2008-2009 GZK 0.5-1 10 17 ev 10 19 ev 2011 IceCube 2012 5 1 GZK IceCube GZK 5 33

GZK EeV IceCube IceCube ARA (Askaryan Radio Array) IceCube 80 km 2 200m Askaryan ARA 300 PeV IceCube GZK IceCube ANITA RICE 2010 3 Collaboration $2M R&D phase-i 2010-2012 3 ARA $10M IceCube GZK IceCube GPS slow control WiFi 30% 3 MeV ETCC)2006 100keV-1MeV SMILE-I 30cm ETCC 3 5 SMILE-II EU EISCAT Relativistic electron precipitation; REP EISCAT STE 2012 ERG JAXA REP 34

ETCC 100 kev- MeV REP 10 2012 ERG 2 REP 50 cm ETCC 30 cm ETCC 10 X 5 ETCC MeV GRB (z>10) 0.1-50MeV 10 100 MeV (S)(H21 25 ) 2, 3 5 10-20 8 EISCAT STE JAXA GRB WG( ) 35

Gamma-ray burst for UNravelling Dark Ages Mission : GUNDAM ( ) (GRB) GRB 2009 4 23 GRB 090423 z=8.2 (130 ) GRB z=20 GRB GRB z >10 GRB CRC TeV Epeak Luinosity z >2 z >2 ( m, ) Ia Ia WFIRST z <2 GRB z=0.1 20 GRB GUNDAM PATHFINDER GRB GRB (1) (2) (1) X X 100 kev 100 MeV 100 1 str 1. GUNDAM PATHFINDER GRB X 36

Swift GRB (2) 45 cm Ly- (z >7 ) TMT (30 m ) SPICA() ALMA z=13 2. GRB z=7 8 45cm 15 21 GRB 200 K 1.7 m z=13 45 cm 2 1 1 15 21 2 GRB z=7 8 GRB GRB GRB090423 (z=8.2) 2011 12 GUNDAM CRC CRC (GUNDAM PATHFINDER: 10 20 ) z >10 GRB GRB GUNDAM GRB 37

SciCR STE STE in-situ 90 µ 3m 3m 1.7m 38

SciCR SciBooNe Fermilab SciBar 4700 SciBar 2.6 cm 1.3 cm 3m 15000 64 X-Y64 2011 2014 LHCf STE 10 20 ev AUGER TA Arm 1 Front Counter Front Counter Arm 2 140 m 140 m 8 cm 6 cm n 0 f (Arm1) IP1 (ATLAS) f (Arm2) 39

QGSJET, DPMJET, SYBILL, EPOS 2009 Large Hadron Collider (LHC)10 17 ev LHCf LHC 0 π 0 LHC2010 0.9 TeV 7 TeV 10 TeV~14 TeV LHC STE STE JAMSTEC 1997 Svensmark 3.2 km 40

41