CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on...

6
Current Yufeng Xin sin 2 2θ 12 4% 0.7% 0.5% Δm 2 21 3% 0.6% 0.4% Δm 2 32 3% 0.4% 0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix, test models of neutrino masses and

Transcript of CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on...

Page 1: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

Current Yufeng Xin

sin22θ12 4% 0.7% 0.5%

Δm221 3% 0.6% 0.4%

Δm232 3% 0.4% 0.3%

Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix, test models of neutrino masses and mixing …

Page 2: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

20 kT liquid scintillator detector deep underground

Acrylic tank： F34.5mStainless Steel tank ： F37.5m

<3% energy resolution @ 1 MeV ~ 80% photon coverage, 700 m rock burden

Civil construction 2014-2017Detector component production 2016-2017PMT production 2016-2019Detector installation 2018-2019Filling and data taking 2020

Page 3: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

Yangjiang NPP

TaishanNPP

Daya Bay NPP

HuizhouNPP

LufengNPP

53 km53 km

Hong Kong

Macau

Guang Zhou

Shen Zhen

Zhu Hai700 munderground

2.5 h drive

NPP Daya Bay Huizhou Lufeng Yangjiang Taishan

Status Operational Planned Planned Under construction Under construction

Power 17.4 GW 17.4 GW 17.4 GW 17.4 GW 18.4 GW

Page 4: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

Additional Physics Topics• Supernova neutrinos– Mass of neutrinos through

time of flight– Sensitive to both anti-nu_e

(IBD) and NC channel– Relic Supernova neutrinos

• Proton decay (K^+ channel)• Geoneutrinos + Solar• …

Page 5: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

Calibration of JUNO detector• Important to reach 3% @ 1 MeV energy resolution• Important to reach sub-1% absolute energy scale• Calibrate the PMT timing pulse-shape

discrimination ability of JUNO• Synergies with DYB/PROSPECT: – Energy model is important to extract neutrino spectrum crucial for JUNO, as no near detector

• Ideas: positron sources, B12, diffused beta or positron sources, neutron sources, electron/positron pelletrons …

• Also high performance LS R&D …

Page 6: CurrentYufengXin sin 2 2θ 12 4%0.7%0.5% Δm 2 21 3%0.6%0.4% Δm 2 32 3%0.4%0.3% Impacts on neutrinoless beta decay, future unitarity tests of PMNS matrix,

Measuring Angleepx.phys.tohoku.ac.jp/~yhitoshi/Talks/tohoku.pdf · Measuring Angle `3=° Hitoshi Yamamoto University of Hawaii At Tohoku University, 2000/8 1. CP Violation and Unitarity

Measuring Angleepx.phys.tohoku.ac.jp/~yhitoshi/Talks/tohoku.pdf · Measuring Angle `3=° Hitoshi Yamamoto University of Hawaii At Tohoku University, 2000/8 1. CP Violation and Unitarity

PowerPoint at Reading · 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 10-2 rt st 10-1 ROAD & SKY 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 10-2 WALLS No Tree Real Cities 100 H/W (-) -0.1, À

PowerPoint at Reading · 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 10-2 rt st 10-1 ROAD & SKY 0.9 0.8 0.7 0.6 0.5 0.4 0.3 0.2 10-2 WALLS No Tree Real Cities 100 H/W (-) -0.1, À

Neutrino masses and unitarity of the leptonic mixing matrixactive.pd.infn.it/g4/seminars/2007/files/biggio.pdf · 2010. 2. 2. · Neutrino masses and unitarity of the leptonic mixing

Neutrino masses and unitarity of the leptonic mixing matrixactive.pd.infn.it/g4/seminars/2007/files/biggio.pdf · 2010. 2. 2. · Neutrino masses and unitarity of the leptonic mixing

From — Status and Prospects Tim Gershonbozzi/IFAE2003/CKM2003/gershon_4_06.pdf · 2003-04-12 · VudVub * VcdVcb * V ... Tim Gershon Workshop on the CKM Unitarity Triangle April

From — Status and Prospects Tim Gershonbozzi/IFAE2003/CKM2003/gershon_4_06.pdf · 2003-04-12 · VudVub * VcdVcb * V ... Tim Gershon Workshop on the CKM Unitarity Triangle April

Ukuran Pemusatan Data - … · Komponen Tugas Quiz UTS UAS Bobot 20% 10% 30% 40% Nilai 80 75 65 75 0.2 80 0.1 75 0.3 65 0.4 75 73 w 0.2 0.1 0.3 0.4 x u u u u ... Median terletak diantara

Ukuran Pemusatan Data - … · Komponen Tugas Quiz UTS UAS Bobot 20% 10% 30% 40% Nilai 80 75 65 75 0.2 80 0.1 75 0.3 65 0.4 75 73 w 0.2 0.1 0.3 0.4 x u u u u ... Median terletak diantara

A 0.4 GHz - 4 GHz Direct RF-to-Digital Σ∆ Multi-Mode Receiverbora/Conferences/2013/...A 0.4 GHz - 4 GHz Direct RF-to-Digital Σ∆ Multi-Mode Receiver Charles Wu and Borivoje Nikolic

A 0.4 GHz - 4 GHz Direct RF-to-Digital Σ∆ Multi-Mode Receiverbora/Conferences/2013/...A 0.4 GHz - 4 GHz Direct RF-to-Digital Σ∆ Multi-Mode Receiver Charles Wu and Borivoje Nikolic

Chart of Elementary Particles - SNOLAB · 2014-06-13 · If neutrinos have mass: ν l = ∑U li ν i) E Δm L P(ν µ ν e) θ ( . 2 → = sin2 2 sin2 127 For 3 Active neutrinos.

Chart of Elementary Particles - SNOLAB · 2014-06-13 · If neutrinos have mass: ν l = ∑U li ν i) E Δm L P(ν µ ν e) θ ( . 2 → = sin2 2 sin2 127 For 3 Active neutrinos.

Mass Analyzers - University of Minnesotamslab.chem.umn.edu/class/lecture/1115_MassAnalyzers.pdf · 2006. 11. 22. · Mass Analyzers • Resolution – R = m / Δm • Accuracy/Precision

Mass Analyzers - University of Minnesotamslab.chem.umn.edu/class/lecture/1115_MassAnalyzers.pdf · 2006. 11. 22. · Mass Analyzers • Resolution – R = m / Δm • Accuracy/Precision

The Higgs System M. Veltman MacArthur Emeritus Professor ... · Plan of the Lectures 1 Introduction Vacuum expectation value. Cosmological constant. 2 The original Higgs Model Unitarity

The Higgs System M. Veltman MacArthur Emeritus Professor ... · Plan of the Lectures 1 Introduction Vacuum expectation value. Cosmological constant. 2 The original Higgs Model Unitarity

Find the orbital periods of Mercury (~0.4 AU from the Sun ...humanic/p1200_lecture11.pdfExample: Find the orbital periods of Mercury (~0.4 AU from the Sun) and Neptune (~30 AU from

Find the orbital periods of Mercury (~0.4 AU from the Sun ...humanic/p1200_lecture11.pdfExample: Find the orbital periods of Mercury (~0.4 AU from the Sun) and Neptune (~30 AU from

Dan Barbasch - pi.math.cornell.edupi.math.cornell.edu/~barbasch/lusztig2006.pdfPrimitive Ideals and Unitarity These are interesting nilpotents in many ways. In particular the component

Dan Barbasch - pi.math.cornell.edupi.math.cornell.edu/~barbasch/lusztig2006.pdfPrimitive Ideals and Unitarity These are interesting nilpotents in many ways. In particular the component

18 - Structure of the Universe. Extragalactic Distance Scale Cepheids M V =-3.35logΠ-2.13+2.13(B-V) Π=period (days) Novae M V (max)=-9.96-2.31log(Δm/day)

18 - Structure of the Universe. Extragalactic Distance Scale Cepheids M V =-3.35logΠ-2.13+2.13(B-V) Π=period (days) Novae M V (max)=-9.96-2.31log(Δm/day)

Chemical Bonding and Aromaticity in Furan, Pyrrole, and ...szolcsanyi/education/files/Chemia... · ca. 0.4 ppm, respectively. Another interesting observation is that the MP2-GIAO

Chemical Bonding and Aromaticity in Furan, Pyrrole, and ...szolcsanyi/education/files/Chemia... · ca. 0.4 ppm, respectively. Another interesting observation is that the MP2-GIAO

Super Charm/Tau Factory @ Novosibirsk (project) · Super B Factory and Super Charm/Tau Factory synergy: •The model-independent Unitarity triangle Gamma angle measuring requires

Super Charm/Tau Factory @ Novosibirsk (project) · Super B Factory and Super Charm/Tau Factory synergy: •The model-independent Unitarity triangle Gamma angle measuring requires

Ecography ECOG-04117 · 5-5 0 5 10 0.0 0.2 0.4 0.6 0.8 1.0 Log 10 Area Dissimilarity Power Law Linear Logit-5 0 5 10 0.0 0.2 0.4 0.6 0.8 1.0 Log 10 Area Dissimilarity Power Law Linear

Ecography ECOG-04117 · 5-5 0 5 10 0.0 0.2 0.4 0.6 0.8 1.0 Log 10 Area Dissimilarity Power Law Linear Logit-5 0 5 10 0.0 0.2 0.4 0.6 0.8 1.0 Log 10 Area Dissimilarity Power Law Linear

Weyl Group Representations and Unitarity of …apantano/pdf_documents/windsor.pdfLet G be a Lie group and let g be its Lie algebra. For all x 2 G, there is an inner automorphism Int(x):

Weyl Group Representations and Unitarity of …apantano/pdf_documents/windsor.pdfLet G be a Lie group and let g be its Lie algebra. For all x 2 G, there is an inner automorphism Int(x):

11. THE CKM QUARK-MIXING MATRIX · 2006. 9. 6. · 2 11. CKM quark-mixing matrix Figure 11.1: Sketch of the unitarity triangle. The CKM matrix elements are fundamental parameters

11. THE CKM QUARK-MIXING MATRIX · 2006. 9. 6. · 2 11. CKM quark-mixing matrix Figure 11.1: Sketch of the unitarity triangle. The CKM matrix elements are fundamental parameters

CKM Unitarity and Neutron Beta Decay · Neutron Beta-Decay Two free parameters within SM (G F from muon decay) Ratio of coupling constants Quark mixing Axial-vector g A und vector

CKM Unitarity and Neutron Beta Decay · Neutron Beta-Decay Two free parameters within SM (G F from muon decay) Ratio of coupling constants Quark mixing Axial-vector g A und vector

SHIVAJI UNIVERSITY, KOLHAPUR Schedule/Exam Schedule 2016... · Measure the angles of minimum deviation (δm) for different colours in the spectrum of the mercury source produced by

SHIVAJI UNIVERSITY, KOLHAPUR Schedule/Exam Schedule 2016... · Measure the angles of minimum deviation (δm) for different colours in the spectrum of the mercury source produced by

VRF MV6 - Clivet · 2019. 8. 5. · VRF MV6 SPLIT VRF CONTROL SYSTEM AIR R-410A DC Inverter P h Δm m R NI4 3 Unique Innovations High efficiency heat pump outdoor units Thanks to

VRF MV6 - Clivet · 2019. 8. 5. · VRF MV6 SPLIT VRF CONTROL SYSTEM AIR R-410A DC Inverter P h Δm m R NI4 3 Unique Innovations High efficiency heat pump outdoor units Thanks to