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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 / 中央研究院@ 9th CIPANP 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. mn0 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 Kuo-Sheng Nuclear Power Plant KS NPS-II : 2 cores 2.9 GW KS n Lab: 28 m from core#1 Kuo Sheng Reactor Neutrino Laboratory Front View (cosmic veto, shielding, control room …..) Inner Target Volume Fne (6.4 X 10 12 /s ) Configuration: n/fission Modest yet Unique 235U: Flexible Design: 3.4 238U: 0.5 239Pu: 1.8 241Pu: 0.4 U (n,g) 1.2 Allows different detectors conf. for different physics Reactor Neutrino Interaction Cross-Sections quality Detector requirements On-Going Data Taking & Analysis R&D : Coh. (nN) T < 1 keV mass Results & More Data: SM s(ne) mn(ne) T > 3 MeV T ~ 1-100 keV 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] 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 cosmicveto, anti-Comp., PSD Combined Analysis with all Information : Denote F i- ; F i for the reactor OFF/ON data ; After ACV CRV cuts, it turns into F f / F f n SM mn F f n F f F f n F f i i F n F TEXONO data -1st results @PRL 90, 131802 (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 10-11 mB (90% CL) @ hep- ex /0605006 ds (ne) 2 1 1 m 2 m dT me2 T En n 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 ~1.2 238U capture-n per fission ] Neutrino radiative decay nee scattering However, SM >>MM at few MeV ! The differential cross section can be represented 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) Z = 0 cm Z =40 cm 208Tl 137Cs 40K Region of Interest for SM s(ne) Preliminary Result 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) The best fit of based on 6500/ 3600 day*kg for Reactor of ON/OFF Global analysis of all spectra 0.37+- 0.13 at 3-8MeV 0.30+- 0.22 at 3.5-8MeV Goal 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 “Ultra-Low-Energy” HPGe Prototype ULEGe – developed for soft X-rays detection ; easy & inexpensive & robust operation 5 g 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 10-11 mB ] 4 X 5 g Threshold < 100 eV TEXONO KIMS @ 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 Sensitivity Plot for CDM-WIMP search with 1 kg ULEGe at 100 eV threshold .. Yangyang (襄陽) Lab (Y2L) min. 700 m of rock overburden Survey for other research program Evaluate ne flux at standard reactors \ Explore ne flux enhancement in loaded reactor (e.g. with Cr) @Phys. Rev. D 72, 012006 (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 10-16 g/g) 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