Low Energy Neutrino Physics at Reactors

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Presentation transcript:

Low Energy Neutrino Physics at Reactors Kuo-Sheng Neutrino Laboratory & Program Update of Neutrino Magnetic Moment results Sensitivities of Magnetic Moment Searches Neutrino-Nucleus Coherent Scatterings : Physics & Motivations Ultra-Low Energy High-Purity Germanium Detector Prototype Status & Plans Henry T. Wong Academia Sinica @ WIN-05, Delphi

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 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

Kuo Sheng Reactor Neutrino Laboratory Front View (cosmic vetos, shieldings, control room …..) Configuration: Modest yet Unique Flexible Design: Allows different detectors conf. for different physics Inner Target Volume

Reactor Neutrino Interaction Cross-Sections mass quality Detector requirements R&D : Coh. (nN) T < 1 keV Results & More Data: mn(ne) T ~ 1-100 keV On-Going Data Taking & Analysis SM s(ne) T > 2 MeV

Other (More Speculative / Fun) Studies : production and physics potentials of ne’s at reactors (hep-ex/0502001) looking for neutrino-induced nuclear transitions production of axions at reactor & their searches …… not discussed here

Improved Magnetic Moment Analysis simple compact all-solid design : HPGe (mass 1 kg) enclosed by active NaI/CsI anti-Compton, further by passive shieldings & cosmic veto selection: single-event after cosmic-veto, anti-Comp., PSD TEXONO data (4712/1250 hours ON/OFF) [PRL 90, 2003] background comparable to underground CDM experiment : ~ 1 day-1keV-1kg-1 (cpd) DAQ threshold 5 keV analysis threshold 12 keV

Combined Analysis with all Information : Denote Limit: mn(ne) < 1.0 X 10-10 mB (90% CL) X 3 data volume : expect sensitivity range mn(ne) 8 X 10-11 mB ON-OFF only 1s contour

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 ]

Sensitivity Improvement Statistically cales as: Nn : signal events B : background level m : target mass t : measurement time Nn  fn (neutrino flux) & related to T-threshold T-threshold : e.g. Nn increase X~3 from 10 keV to 10 eV in Ge (1/T  atomic energy level threshold) BIG statistical boost in mn comes from enhancement in fn by, e.g. artificial n-sources, b-beams etc. BUT: for systematics control, coupled with low threshold to keep mn >> SM rates maintain low background level

MAMONT Project : 3H-source (Russia, USA, Germany) e.g. As Illustrations…… MAMONT Project : 3H-source (Russia, USA, Germany) TRITIUM SOURCE of 40 MCi activity (4 kg 3H) with flux of 61014 cm-2s-1 (!) ULTRA-LOW-THRESHOLD DETECTORS Eth~10 eV (!): SILICON CRYODETECTOR 15100cc M=3kg, ionization-into-heat conversion effect (CWRU-Stanford-JINR) HIGH-PURITY-GERMANIUM DETECTOR 6150cc, M=4.8kg, internal amplification by avalanche multiplication (ITEP) SENSITIVITY (95% C.L.):  2.5 10-12B 50 cm Conceptual layout of the -e scattering experiment with 40 MCi tritium source Status : R&D

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 Stardard Model 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

Expected Interaction Rates at KS @ different Quenching Factors e.g. at QF=0.25 & 100 eV threshold Rate ~ 11 kg-1 day-1

“Ultra-Low-Energy” HPGe Prototype ULEGe – developed for soft X-rays detection ; easy & inexpensive & robust operation Prototype : mass 5 g ; can be constructed in multi-array form threshold <100 eV after modest PSD [lowest achieved for bulk radiation detectors] study feasibilities in nN coherent scattering and Dark Matter searches [ mn search a by-product ]

ULE-HPGe Prototype Results threshold <100 eV , calibration by linear extrapolation from 1-6 keV PSD Cut Threshold ~ 100 eV Threshold < 100 eV background measurement at KS Nov 03 – May 04 Signal Band

min. 700 m of rock overburden 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 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 ………

Background Measurements & Comparisons Similar background at KS & Y2L Apparent difference between 5 g & 1 kg due to scaling with surface area instead, reproduced in simulations i.e. background can be ~ O(1 cpd) at > 1 keV range for 1 kg ULEGe in compact array form

First-Ever Low Background Data down to 100 eV ……. ! (keV) ….. detailed analysis & background understand underway “ don’t know what to expect & what are expected .”

R&D Program towards Realistic O(1 kg) Size Experiments (both nN & CDM) : measure & study background at sub-keV range at KS & Y2L N=4 elements array produced & being studied devise calibration scheme at sub-keV range measure quenching factor of Ge with neutron beam develop advanced PSD techniques to further suppress noise-edge  reduce threshold studying new possibilities with Ge-detector larger modular mass segmented Ge dual readout channels by-product : T>500 eV gives mn(ne)  2 X 10-11 mB at ~1 cpd background

Summary & Outlook Kuo-Sheng Neutrino Lab.: Established & Operational  Modular & Flexible Design Physics Data Taking since June 01 ※ Unique HPGe Low Energy Data (@ 10 keV threshold) ※ Bkg Level ~ Underground CDM Expt. Results on mn (Gn)  Other analyses under way Future goals : get to 100 eV threshold  observe neutrino-nucleus coherent scattering  perform LE-CDM experiment R&D program pursued : prototype ULEGe with ~100 eV threshold first background measurement in the 100 eV – 1 keV region