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Overview of TEXONO Collaboration Kuo-Sheng Reactor Neutrino Laboratory

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Presentation on theme: "Overview of TEXONO Collaboration Kuo-Sheng Reactor Neutrino Laboratory"— Presentation transcript:

1 Low Energy Neutrino Physics at the Kuo-Sheng Reactor Laboratory in Taiwan
Overview of TEXONO Collaboration Kuo-Sheng Reactor Neutrino Laboratory Results on Neutrino Magnetic Moments Preliminary Results on Neutrino-Electron Elastic Scattering R&D projects towards Neutrino-Nucleus Coherent Scattering Survey of Other Research Program Summary & Outlook Lin,, Sin-Ted/ 林興德 On Behalf of Taiwan Experiment On NeutrinO (TEXONO) Collaboration Insititute of Physics, Academia Sinica / 9th CIPANP

2 Program: Low Energy Neutrino & Astroparticle Physics
TEXONO Collaboration Collaboration : Taiwan (AS, INER, KSNPS, NTU) ; China (IHEP, CIAE, THU, NJU) ; Turkey (METU) ; USA (UMD) ; India (BHU) Program: Low Energy Neutrino & Astroparticle Physics Kuo-Sheng (KS) Reactor Neutrino Laboratory reactor : high flux of low energy electron anti-neutrinos oscillation expts.  mn0  anomalous n properties & interactions n physics full of surprises , need intense n-source study/constraint new regime wherever experimentally accessible explore possible new detection channels Diversified R&D Projects

3 Kuo-Sheng Nuclear Power Plant
KS NPS-II : 2 cores  2.9 GW KS n Lab: 28 m from core#1

4 Kuo Sheng Reactor Neutrino Laboratory
Front View (cosmic veto, shielding, control room …..) Inner Target Volume Fne (6.4 X 1012 /s ) n/fission 235U: 238U: 239Pu: 1.8 241Pu: 0.4 U (n,g) 1.2 Configuration: Modest yet Unique Flexible Design: Allows different detectors conf. for different physics

5 Reactor Neutrino Interaction Cross-Sections
mass quality Detector requirements R&D : Coh. (nN) T < 1 keV Results & More Data: mn(ne) T ~ keV On-Going Data Taking & Analysis SM s(ne) T > 3 MeV

6 KS Experiment: Period I, II, III Detectors
ULB-HPGe [1 kg] CsI(Tl) Array FADC Readout [16 ch., 20 MHz, 8 bit] Multi-Disks Array [1 Tb*5]

7 Magnetic Moment Searches @ KS
Neutrino Electromagnetic Properties simple compact all-solid design : HPGe (mass 1 kg) enclosed by active NaI/CsI anti-Compton, further by passive shielding & cosmic veto selection: single-event after cosmic-veto, anti-Comp., PSD

8 Combined Analysis with all Information :
Denote TEXONO data -1st 90, (2003) . background comparable to underground CDM experiment : ~ 1 day-1keV-1kg-1 (cpd) DAQ threshold 5 keV analysis threshold 12 keV The limit based on 570.7/127.8 days of Reactor ON/OFF: mn(ne) <7.2 X mB (90% hep- ex /

9 Search of mn at low energy
high signal rate & robustness: mn>>SM [ decouple irreducible bkg  unknown sources ] T<<En  ds/dT depends on total fn flux but NOT spectral shape [ flux well known : ~6 fission-n  ~ U capture-n per fission ] Neutrino radiative decay

10 nee scattering However, SM >>MM at few MeV ! The differential cross section can be represented

11 CsI(Tl) Array (~200 kg) : s(ne)
Data analysis under way .. (25000/8000 day-kg for ON/OFF in PI,II,III) Single Crystal QL Vs QR (Raw Data) Region of Interest for SM s(ne) Z = 0 cm 208Tl 40K 137Cs Z =40 cm

12 Preliminary Result Goal Further analysis =>reduce the background
PSD on e/g in few MeV region X 4 data Background understanding and suppression (Cosmic ray, g cascades of 208Th, Pair Production) Global analysis of all spectra Goal The best fit of based on 6500/ 3600 day*kg for Reactor of ON/OFF at 3-8MeV at 3.5-8MeV

13 Neutrino-Nucleus Coherent Scattering
Standard Model Cross-Sections: a fundamental neutrino interaction never been experimentally-observed s~N2 applicable at En<50 MeV where q2r2<1 a sensitive test to Standard Model (Say, with Q.F.=0.25; Bkg ~1 cpd; Threshold~100eV, the Signal-to-Background ratio~ 20) an important interaction/energy loss channel in astrophysics media a promising new detection channel for neutrinos, without strict lower bound on En & the channel for WIMP direct detection ! involves new energy range at low energy, many experimental challenges & much room to look for scientific surprises

14 “Ultra-Low-Energy” HPGe Prototype
ULEGe – developed for soft X-rays detection ; easy & inexpensive & robust operation Prototype : (I) 5 g ; (II) 4 X 5 g ; (III) 10 g ; (IV) segmented 20 g threshold <100 eV after modest PSD [lowest achieved for bulk radiation detectors] study feasibilities for 1-kg-ish detector for nN coherent scattering and Dark Matter searches [ mn search  mB ] 5 g 4 X 5 g Threshold < 100 eV

15 min. 700 m of rock overburden
TEXONO  Y2L Install 5 g ULB-ULEGe at Y2L on January 2005 Study background and feasibility for CDM searches may evolve into a full-scale (1 kg) CDM experiment Yangyang (襄陽) Lab (Y2L) min. 700 m of rock overburden Sensitivity Plot for CDM-WIMP search with 1 kg ULEGe at 100 eV threshold ..

16 Survey for other research program
Evaluate ne flux at standard reactors \ Explore ne flux enhancement in loaded reactor (e.g. with Rev. D 72, (2005) Looking for n-induced nuclear transition Search for reactor axions * Reactor core has intense M1 transitions : e.g. 7Li, 91Y, 97Nb etc. Trace Radio-purity measured with AMS * develop quick\small sample techniques ( e.g. 40K g/g)

17 Summary & Outlook TEXONO Collaboration:
 Built-Up from Scratch & Maturing Kuo-Sheng Neutrino Lab.:  Established & Operational  Modular & Flexible Design  Physics Data Taking since June 01 ※ Unique HPGe Low Energy Data ※ Bkg Level ~ Underground CDM Expt Results published on mn (Gn) & reactor ne Diversified Program in Parallel Main Thrust on  ~200 kg CsI(Tl) [s(ne) …]  ULEGe: for scoh(nN) + CDM ;


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