Imperial College London
Professor Timothy Sumner

ProfessorTimothySumner

Faculty of Natural Sciences, Department of Physics

Professor of Experimental Astrophysics
 
 
 
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Contact

 

+44 (0)20 7594 7552t.sumner

 
 
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Location

 

1108Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Akerib:2021:10.1103/physrevc.104.065501,
author = {Akerib, DS and Al, Musalhi AK and Alsum, SK and Amarasinghe, CS and Ames, A and Anderson, TJ and Angelides, N and Araújo, HM and Armstrong, JE and Arthurs, M and Bai, X and Balajthy, J and Balashov, S and Bang, J and Bargemann, JW and Bauer, D and Baxter, A and Beltrame, P and Bernard, EP and Bernstein, A and Bhatti, A and Biekert, A and Biesiadzinski, TP and Birch, HJ and Blockinger, GM and Bodnia, E and Boxer, B and Brew, CAJ and Brás, P and Burdin, S and Busenitz, JK and Buuck, M and Cabrita, R and Carmona-Benitez, MC and Cascella, M and Chan, C and Chott, NI and Cole, A and Converse, MV and Cottle, A and Cox, G and Creaner, O and Cutter, JE and Dahl, CE and de, Viveiros L and Dobson, JEY and Druszkiewicz, E and Eriksen, SR and Fan, A and Fayer, S and Fearon, NM and Fiorucci, S and Flaecher, H and Fraser, ED and Fruth, T and Gaitskell, RJ and Genovesi, J and Ghag, C and Gibson, E and Gokhale, S and van, der Grinten MGD and Gwilliam, CB and Hall, CR and Haselschwardt, SJ and Hertel, },
doi = {10.1103/physrevc.104.065501},
journal = {Physical Review C},
pages = {1--11},
title = {Projected sensitivity of the LUX-ZEPLIN experiment to the two-neutrino and neutrinoless double β decays of Xe134},
url = {http://dx.doi.org/10.1103/physrevc.104.065501},
volume = {104},
year = {2021}
}
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RIS format (EndNote, RefMan)

TY  - JOUR
AB  - The projected sensitivity of the LUX-ZEPLIN (LZ) experiment to two-neutrino and neutrinoless double β decay of 134Xe is presented. LZ is a 10-tonne xenon time-projection chamber optimized for the detection of dark matter particles and is expected to start operating in 2021 at Sanford Underground Research Facility, USA. Its large mass of natural xenon provides an exceptional opportunity to search for the double β decay of 134Xe, for which xenon detectors enriched in 136Xe are less effective. For the two-neutrino decay mode, LZ is predicted to exclude values of the half-life up to 1.7×1024 years at 90% confidence level (CL) and has a three-sigma observation potential of 8.7×1023 years, approaching the predictions of nuclear models. For the neutrinoless decay mode LZ, is projected to exclude values of the half-life up to 7.3×1024 years at 90% CL.
AU  - Akerib,DS
AU  - Al,Musalhi AK
AU  - Alsum,SK
AU  - Amarasinghe,CS
AU  - Ames,A
AU  - Anderson,TJ
AU  - Angelides,N
AU  - Araújo,HM
AU  - Armstrong,JE
AU  - Arthurs,M
AU  - Bai,X
AU  - Balajthy,J
AU  - Balashov,S
AU  - Bang,J
AU  - Bargemann,JW
AU  - Bauer,D
AU  - Baxter,A
AU  - Beltrame,P
AU  - Bernard,EP
AU  - Bernstein,A
AU  - Bhatti,A
AU  - Biekert,A
AU  - Biesiadzinski,TP
AU  - Birch,HJ
AU  - Blockinger,GM
AU  - Bodnia,E
AU  - Boxer,B
AU  - Brew,CAJ
AU  - Brás,P
AU  - Burdin,S
AU  - Busenitz,JK
AU  - Buuck,M
AU  - Cabrita,R
AU  - Carmona-Benitez,MC
AU  - Cascella,M
AU  - Chan,C
AU  - Chott,NI
AU  - Cole,A
AU  - Converse,MV
AU  - Cottle,A
AU  - Cox,G
AU  - Creaner,O
AU  - Cutter,JE
AU  - Dahl,CE
AU  - de,Viveiros L
AU  - Dobson,JEY
AU  - Druszkiewicz,E
AU  - Eriksen,SR
AU  - Fan,A
AU  - Fayer,S
AU  - Fearon,NM
AU  - Fiorucci,S
AU  - Flaecher,H
AU  - Fraser,ED
AU  - Fruth,T
AU  - Gaitskell,RJ
AU  - Genovesi,J
AU  - Ghag,C
AU  - Gibson,E
AU  - Gokhale,S
AU  - van,der Grinten MGD
AU  - Gwilliam,CB
AU  - Hall,CR
AU  - Haselschwardt,SJ
AU  - Hertel,SA
AU  - Horn,M
AU  - Huang,DQ
AU  - gnarra,MCI
AU  - Jahangir,O
AU  - James,RS
AU  - Ji,W
AU  - Johnson,J
AU  - Kaboth,AC
AU  - Kamaha,AC
AU  - Kamdin,K
AU  - Kazkaz,K
AU  - Khaitan,D
AU  - Khazov,A
AU  - Khurana,I
AU  - Kodroff,D
AU  - Korley,L
AU  - Korolkova,EV
AU  - Kraus,H
AU  - Kravitz,S
AU  - Kreczko,L
AU  - Krikler,B
AU  - Kudryavtsev,VA
AU  - Leason,EA
AU  - Lee,J
AU  - Leonard,DS
AU  - Lesko,KT
AU  - Levy,C
AU  - Liao,J
AU  - Lin,J
AU  - Lindote,A
AU  - Linehan,R
AU  - Lippincott,WH
AU  - Liu,X
AU  - Lopes,MI
AU  - López,Asamar E
AU  - López,Paredes B
AU  - Lorenzon,W
AU  - Luitz,S
AU  - Majewski,PA
AU  - Manalaysay,A
AU  - Manenti,L
AU  - Mannino,RL
AU  - Marangou,N
AU  - McCarthy,ME
AU  - McKinsey,DN
AU  - McLaughlin,J
AU  - Miller,EH
AU  - Mizrachi,E
AU  - Monte,A
AU  - Monzani,ME
AU  - Morad,JA
AU  - Morales,Mendoza JD
AU  - Morrison,E
AU  - Mount,BJ
AU  - Murphy,ASJ
AU  - Naim,D
AU  - Naylor,A
AU  - Nedlik,C
AU  - Nelson,HN
AU  - Neves,F
AU  - Nikoleyczik,JA
AU  - Nilima,A
AU  - Olcina,I
AU  - Oliver-Mallory,KC
AU  - Pal,S
AU  - Palladino,KJ
AU  - Palmer,J
AU  - Patton,S
AU  - Parveen,N
AU  - Pease,EK
AU  - Penning,B
AU  - Pereira,G
AU  - Piepke,A
AU  - Qie,Y
AU  - Reichenbacher,J
AU  - Rhyne,CA
AU  - Richards,A
AU  - Riffard,Q
AU  - Rischbieter,GRC
AU  - Rosero,R
AU  - Rossiter,P
AU  - Santone,D
AU  - Sazzad,ABMR
AU  - Schnee,RW
AU  - Scovell,PR
AU  - Shaw,S
AU  - Shutt,TA
AU  - Silk,JJ
AU  - Silva,C
AU  - Smith,R
AU  - Solmaz,M
AU  - Solovov,VN
AU  - Sorensen,P
AU  - Soria,J
AU  - Stancu,I
AU  - Stevens,A
AU  - Stifter,K
AU  - Suerfu,B
AU  - Sumner,TJ
AU  - Swanson,N
AU  - Szydagis,M
AU  - Taylor,WC
AU  - Taylor,R
AU  - Temples,DJ
AU  - Terman,PA
AU  - Tiedt,DR
AU  - Timalsina,M
AU  - To,WH
AU  - Tovey,DR
AU  - Tripathi,M
AU  - Tronstad,DR
AU  - Turner,W
AU  - Utku,U
AU  - Vaitk
DO  - 10.1103/physrevc.104.065501
EP  - 11
PY  - 2021///
SN  - 2469-9985
SP  - 1
TI  - Projected sensitivity of the LUX-ZEPLIN experiment to the two-neutrino and neutrinoless double β decays of Xe134
T2  - Physical Review C
UR  - http://dx.doi.org/10.1103/physrevc.104.065501
UR  - https://journals.aps.org/prc/abstract/10.1103/PhysRevC.104.065501
UR  - http://hdl.handle.net/10044/1/94096
VL  - 104
ER  -
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