Potential sites of Deep Sea Anti-Neutrino Detector around Taiwan M.A. Huang 1 & H.T. Wang 2 1 General Education Center, National United University, Miao-Li,

Slides:



Advertisements
Similar presentations
AGASA Results Max-Planck-Institut für Physik, München, Germany Masahiro Teshima for AGASA collaboration at 3 rd Int. Workshop on UHECR, Univ. Leeds.
Advertisements

Сессия ЯФ ОФН РАН, г., ИТЭФ Статус экспериментальных работ по измерению магнитного момента нейтрино Старостин А.С. ИТЕФ.
Searching for an underground national lab in China Yifang Wang July 23, 2008.
VHENTW, 4/25/206M.A. Huang SHENIE: Simulation of High Energy Neutrino Interacting with the Earth M.A. Huang a, Y.L. Hong b, C.H. Iong bc, G.L. Lin b (a)
20 January 2005Steve Dye, HPU1 Neutrino Geophysics in Hawaii Presentation by Steve Dye Associate Professor of Physics Hawaii Pacific University January.
George W.S. Hou & M.A. Huang Center for Cosmology and Particle Astrophysics Department of Physics, National Taiwan University, 1, Sec. 4, Roosevelt Rd.,Taipei,
Neutrino Physics - Lecture 6 Steve Elliott LANL Staff Member UNM Adjunct Professor ,
S. Dye /15/05 Neutrino Geophysics Workshop 1 Hawaii Anti-Neutrino Observatory For the Hanohano collaboration: Steve Dye University of Hawaii at Manoa.
INDIA-BASED NEUTRINO OBSERVATORY (INO) STATUS REPORT Naba K Mondal Tata Institute of Fundamental Research Mumbai, India NUFACT Scoping Study Meeting at.
12 December 2003APS Neutrino StudyE. Blucher APS Neutrino Study: Reactor Working Group What can we learn from reactor experiments? Future reactor experiments.
Ultra high energy cosmic rays: highlights of recent results J. Matthews Pierre Auger Observatory Louisiana State University 19 August August.
Antares/KM3NeT M. de Jong. neutrinos  p Scientific motivation: – origin cosmic rays – birth & composition relativistic jets – mechanism of cosmic particle.
Jun Cao Institute of High Energy Physics, Beijing Daya Bay Neutrino Experiment 3rd International Conference on Flavor Physics, Oct. 3-8, 2005 National.
Low Energy Neutrino Physics at the Kuo-Sheng Nuclear Power Plant  Overview of TEXONO Collaboration  Kuo-Sheng Reactor Neutrino Laboratory  Results on.
 Starting Points (Collaboration ; Laboratory )  1-kg HPGe : Magnetic Moment Results  Physics & Requirements of ULEGe Detectors  R&D on ULEGe Prototypes.
Neutrino Physics and Dark Matter Physics with Ultra-Low-Energy Germanium Detector  Overview of TEXONO Collaboration  Kuo-Sheng Reactor Neutrino Laboratory.
 Starting Points (Collaboration ; Laboratories ; Research Program)  Physics & Requirements for ULE-HPGe - focus on WIMP Searches  R&D on ULE-HPGe Prototypes.
Reactor Neutrino Experiments Jun Cao Institute of High Energy Physics Lepton-Photon 2007, Daegu, Aug , 2007.
1/8-10/2007M.A. Huang CRTNT Experiment Status  Introduction  Two prototype telescopes  Test run on ARGO-YBJ site, Tibet  Full scale experiment: 2008.
Theoretical Particle & Cosmology efforts in Taiwan – a small community Xiao-Gang He NCTS.
Eun-Ju Jeon Sejong Univ. Sept. 09, 2010 Status of RENO Experiment Neutrino Oscillation Workshop (NOW 2010) September 4-11, 2010, Otranto, Lecce, Italy.
Performance of CRTNT for Sub-EeV Cosmoc Ray Measurement Zhen Cao IHEP, Beijing & Univ. of Utah, SLC Aspen, CO, 04/2005.
Request to join MICE collaboration from MOMENT (IHEP and Sichuan Uni.) Jingyu Tang Institute of High Energy Physics, CAS MICE Collaboration Board Meeting.
 Kuo-Sheng Neutrino Laboratory & Program  Update of Neutrino Magnetic Moment results  Sensitivities of Magnetic Moment Searches  Neutrino-Nucleus Coherent.
Low Energy Neutrino Physics at the Kuo-Sheng Reactor Laboratory in Taiwan  Overview of TEXONO Collaboration  Kuo-Sheng Reactor Neutrino Laboratory 
Karsten M. Heeger US Reactor  13 Meeting, March 15, 2004 Comparison of Reactor Sites and  13 Experiments Karsten Heeger LBNL.
Highlights of the TEXONO Research Program : Status and Plans  Overview of TEXONO Collaboration  Research Program  Kuo-Sheng Reactor Neutrino Laboratory.
The Daya Bay Experiment to Measure  13 Herbert Steiner UC Berkeley & LBNL On behalf of the Daya Bay Collaboration Presented at the Erice School/Workshop.
March 02, Shahid Hussain for the ICECUBE collaboration University of Delaware, USA.
L. Oberauer, Paris, June 2004   Measurements at Reactors Neutrino 2004 CdF, Paris, June chasing the missing mixing angle.
Humberto Salazar (FCFM-BUAP) for the Pierre Auger Collaboration, CTEQ- Fermilab School Lima, Peru, August 2012 Ultrahigh Cosmic Rays: The highest energy.
Paul Sommers Fermilab PAC Nov 12, 2009 Auger Science South and North.
3/22/2002M.A. Huang George W.S. Hou & M.A. Huang Center for Cosmology and Particle Astrophysics Department of Physics, National Taiwan University.
,,,,, The Daya Bay Reactor Neutrino Experiment Liangjian Wen On behalf of the Daya Bay Collaboration Institute of High Energy Physics Daya Bay Detectors.
The Daya Bay Reactor Neutrino Experiment R. D. McKeown Caltech On Behalf of the Daya Bay Collaboration CIPANP 2009.
1 GEMMA: experimental searches for neutrino magnetic moment JINR: V. Brudanin, V. Egorov, D. Medvedev, M. Shirchenko, E. Shevchik, I. Zhitnikov, V. Belov.
High Energy Astrophysics in Taiwan Hsiang-Kuang Chang ( 張 祥光 ) Department of Physics and Institute of Astronomy National Tsing Hua University ( 國立清華大學.
 TEXONO Collaboration & Kuo-Sheng Laboratory & Program Overview  Results on Neutrino Magnetic Moments, Reactor Electron Neutrinos and Reactor Axion Search.
2 nd FCPPL Workshop Closing Remarks Hesheng CHen.
Daya Bay Reactor Neutrino Experiment On behalf of the DayaBay collaboration Virginia Polytechnic Institute and State University Joseph ykHor YuenKeung,
Daya Bay Neutrino Experiment Huang Xingtao Shandong University, Jinan, China On Behalf of the Daya Bay Collaboration.
Yangyang Underground Laboratory Sun Kee Kim Seoul National University.
  Measurement with Double Chooz IDM chasing the missing mixing angle e  x.
The CRTNT Project (Cosmic Ray & Tau Neutrino Telescope) --- sensitivity and prototype experiment Huihai He, IHEP, CAS On behalf of the CRTNT collaboration.
Limits on Low-Mass WIMP Dark Matter with an Ultra-Low-Energy Germanium Detector at 220 eV Threshold Overview (Collaboration; Program; Laboratory) Physics.
China Deep Underground Laboratory and Dark Matter Search Hesheng Chen Institute of High Energy Physics.
Results on  13 Neutrino Oscillations from Reactor Experiments Soo-Bong Kim (KNRC, Seoul National University) “INPC 2013, Firenze, June 2-7, 2013”
KM3NeT Neutrino conference 2-7 June 2014, Boston, U.S.A. Maarten de Jong on behalf of the KM3NeT collaboration The next generation neutrino telescope in.
Towards kg-scale Ultra-Low-Energy Ultra-Low-Background Ge Detector
Reactor anti-neutrinos and neutrinos
NEUTRINO OSCILLATION MEASUREMENTS WITH REACTORS
Dark Matter Search With an Ultra-low Threshold Germanium Detector proposed by Tsinghua University Seoul National University Academia Sinica Qian Yue.
5th Rencontres du Vietnam
Outline 1. Introduction & Overview 2. The experiment result 3. Future
Recent Result and Status of TEXONO Experiments
Low-Energy Neutrino and Dark Matter Physics with TEXONO Program
Building ICECUBE A Neutrino Telescope at the South Pole
Low Energy Neutrino Physics at Reactors
Low Energy Neutrino Physics at the Kuo-Sheng Reactor Laboratory
CRTNT Project & Cosmic RayτNeutrino (>1 PeV) Measurement
Highlights of the TEXONO Research Program :
Daya Bay Neutrino Experiment
Daya Bay Neutrino Experiment
Starting Points (Collaboration ; Laboratory ; Magnetic Moment Results)
Overview of TEXONO Collaboration Kuo-Sheng Reactor Neutrino Laboratory
Low Energy Neutrino Physics AT Nuclear Power Reactors
Kuo-Sheng(國聖) Reactor Neutrino Lab.
27th CMS User’s Group Meeting
Neutrino Magnetic Moment : Overview
Kuo-Sheng(國聖) Reactor Neutrino Lab.
Presentation transcript:

Potential sites of Deep Sea Anti-Neutrino Detector around Taiwan M.A. Huang 1 & H.T. Wang 2 1 General Education Center, National United University, Miao-Li, Taiwan, Institute of Physics, Academia Sinica, Taipei, Taiwan, 115 M.A. Huang 1 DOANOW workshop March 23-25, 2007

KAW4, 5/19/206M.A. Huang Nu physics and astrophysics in Taiwan Experimental – TEXONO: Academia Sinica – DYB: NTU, NCTU, NUU – CRTNT: NUU Theoretical – NCTU, NCTS – NUU TEXONO, Academia Sinica DYB, NTU NCTU, NCTS NUU CRTNT, NUU

KAW4, 5/19/206M.A. Huang TEXONO Collaboration Collaboration : Taiwan (AS, INER, KSNPS, NTU) ; China (IHEP, CIAE, THU, NJU) ; Turkey (METU) ; USA (UMD) Program: Low Energy Neutrino & Astroparticle Physics  Kuo-Sheng (KS) Reactor Neutrino Laboratory Taiwan EXperiment On NeutrinO KS NPS-II : 2 cores  2.9 GW KS Lab: 28 m from core#1 NPS-IV (under construction)

Neutrino magnetic moments, – PRL, 90, 2003; hep-ex/ Axion searches – Astro-ph/ , Nu-e cross sections – Undergoing analysis Ultra-Low-Energy HPGe Prototype – ~100 eV, 4x5g detector, working on1 kg detector. – Nu-N coherent scattering – Dark matter searches KAW4, 5/19/206M.A. Huang TEXONO Physics topics

1/8-10/2007M.A. Huang CRTNT CRTNT : Cosmic Ray Tau Neutrino Telescope – Detect shower from , which comes from Earth-skimming  Z. Cao et al., J. Phys. G, 31, , (2005) Highlight paper of the year 2005 by J. Phys. G

1/8-10/2007M.A. Huang Future plan of CRTNT 4 stations, each have telescopes, cover 16  64  field of view. Site: Balikun, Hsing-Jiang Energy range: E > 100TeV for neutrino, and E > 0.1EeV for UHECR. UHECR Mountain-passing  event C Earth-skimming  event

Daya Bay collaborators in Taiwan Nat’l Taiwan Univ. – PI: Yee Bob Hsiung – Acrylic vessel Nat’l Chiao Tung Univ. – PI: G.Y. Lin Nat’l United Univ. – PI: C.H. Wang – Y. Chang, S. Blyth 1/8-10/20077 Muon veto simulation, Aberdeen Tunnel prototype

Potential sites near Taiwan Selection requirements: – Near nuclear power plant ~ km. – Depth < -2.6 km (~ 1 km of std. rock) – Distance to nearest harbor Logistic support M.A. Huang 8

Nuclear Power Stations 3 existing NPS, all have two cores. NPS-1: 2  1775 MWt NPS-2: 2  2894 MWt NPS-3: 2  2785 MWt NPS-4 in construction. NPS-4: 2  4100 MWt ; Finish in 2009~ 2101 M.A. Huang 9

Northern Taiwan sites M.A. Huang 10 NP-1,2 are too far! only m

Northern Taiwan M.A. Huang 11 NP-4 is within 100 km! Site A: m only m

Southern Taiwan 2015/5/23 12 Site D: m Site C: m Site B: m Site E: m

Summary SiteABCDE Depth< -2.5< ~ < -3 Distance to harbor km, Su-Ao 20 km, Orchid Island; 70 km TaiDung 20 km, Orchid Island; 120 km, TaiDung 110 km, DongKang 160 km, TaiDong or DongKang Other issuesNPS-4 (2010) 2x4.1GW Combined signals of NPS- 1,2,4 Strong current River sediments Close to Philippine M.A. Huang 13 NPS-3: 2  2785 MWt

Future participation in HANOHANO If HANOHANO site is near Taiwan, we would be the host and provide local supports. – Site survey – Application/permission to government – Local control – Data transmission, storage, … etc. If not, … – HANOHANO is a good continuation of DYB, someone may still participate. Need consensus from colleague in Taiwan – HEP community, geo-physicists, funding agency, publics. M.A. Huang 14