BibTex format
@article{Aalbers:2024:10.1103/physrevd.109.112010,
author = {Aalbers, J and Akerib, DS and Al, Musalhi AK and Alder, F and Amarasinghe, CS and Ames, A and Anderson, TJ and Angelides, N and Araújo, HM and Armstrong, JE and Arthurs, M and Baker, A and Balashov, S and Bang, J and Barillier, EE and Bargemann, JW and Baxter, A and Beattie, K and Benson, T and Bhatti, A and Biekert, A and Biesiadzinski, TP and Birch, HJ and Bishop, EJ and Blockinger, GM and Boxer, B and Brew, CAJ and Brás, P and Burdin, S and Buuck, M and Carmona-Benitez, MC and Carter, M and Chawla, A and Chen, H and Cherwinka, JJ and Chin, YT and Chott, NI and Converse, MV and Cottle, A and Cox, G and Curran, D and Dahl, CE and David, A and Delgaudio, J and Dey, S and de, Viveiros L and Di, Felice L and Ding, C and Dobson, JEY and Druszkiewicz, E and Eriksen, SR and Fan, A and Fearon, NM and Fiorucci, S and Flaecher, H and Fraser, ED and Fruth, TMA and Gaitskell, RJ and Geffre, A and Genovesi, J and Ghag, C and Gibbons, R and Gokhale, S and Green, J and van, der Grinten MGD and Hais},
doi = {10.1103/physrevd.109.112010},
journal = {Physical Review D: Particles, Fields, Gravitation and Cosmology},
title = {New constraints on ultraheavy dark matter from the LZ experiment},
url = {http://dx.doi.org/10.1103/physrevd.109.112010},
volume = {109},
year = {2024}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - Searches for dark matter with liquid xenon time projection chamber experiments have traditionally focused on the region of the parameter space that is characteristic of weakly interacting massive particles, ranging from a few GeV/2 to a few TeV/2. Models of dark matter with a mass much heavier than this are well motivated by early production mechanisms different from the standard thermal freeze-out, but they have generally been less explored experimentally. In this work, we present a reanalysis of the first science run of the LZ experiment, with an exposure of 0.9 tonne×yr, to search for ultraheavy particle dark matter. The signal topology consists of multiple energy deposits in the active region of the detector forming a straight line, from which the velocity of the incoming particle can be reconstructed on an event-by-event basis. Zero events with this topology were observed after applying the data selection calibrated on a simulated sample of signal-like events. New experimental constraints are derived, which rule out previously unexplored regions of the dark matter parameter space of spin-independent interactions beyond a mass of 1017 GeV/2.
AU - Aalbers,J
AU - Akerib,DS
AU - Al,Musalhi AK
AU - Alder,F
AU - Amarasinghe,CS
AU - Ames,A
AU - Anderson,TJ
AU - Angelides,N
AU - Araújo,HM
AU - Armstrong,JE
AU - Arthurs,M
AU - Baker,A
AU - Balashov,S
AU - Bang,J
AU - Barillier,EE
AU - Bargemann,JW
AU - Baxter,A
AU - Beattie,K
AU - Benson,T
AU - Bhatti,A
AU - Biekert,A
AU - Biesiadzinski,TP
AU - Birch,HJ
AU - Bishop,EJ
AU - Blockinger,GM
AU - Boxer,B
AU - Brew,CAJ
AU - Brás,P
AU - Burdin,S
AU - Buuck,M
AU - Carmona-Benitez,MC
AU - Carter,M
AU - Chawla,A
AU - Chen,H
AU - Cherwinka,JJ
AU - Chin,YT
AU - Chott,NI
AU - Converse,MV
AU - Cottle,A
AU - Cox,G
AU - Curran,D
AU - Dahl,CE
AU - David,A
AU - Delgaudio,J
AU - Dey,S
AU - de,Viveiros L
AU - Di,Felice L
AU - Ding,C
AU - Dobson,JEY
AU - Druszkiewicz,E
AU - Eriksen,SR
AU - Fan,A
AU - Fearon,NM
AU - Fiorucci,S
AU - Flaecher,H
AU - Fraser,ED
AU - Fruth,TMA
AU - Gaitskell,RJ
AU - Geffre,A
AU - Genovesi,J
AU - Ghag,C
AU - Gibbons,R
AU - Gokhale,S
AU - Green,J
AU - van,der Grinten MGD
AU - Haiston,JH
AU - Hall,CR
AU - Han,S
AU - Hartigan-OConnor,E
AU - Haselschwardt,SJ
AU - Hernandez,MA
AU - Hertel,SA
AU - Heuermann,G
AU - Homenides,GJ
AU - Horn,M
AU - Huang,DQ
AU - Hunt,D
AU - Ignarra,CM
AU - Jacquet,E
AU - James,RS
AU - Johnson,J
AU - Kaboth,AC
AU - Kamaha,AC
AU - Kannichankandy,M
AU - Khaitan,D
AU - Khazov,A
AU - Khurana,I
AU - Kim,J
AU - Kingston,J
AU - Kirk,R
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 - Lee,J
AU - Leonard,DS
AU - Lesko,KT
AU - Levy,C
AU - Lin,J
AU - Lindote,A
AU - Linehan,R
AU - Lippincott,WH
AU - Lopes,MI
AU - Lopez,Asamar E
AU - Lorenzon,W
AU - Lu,C
AU - Luitz,S
AU - Majewski,PA
AU - Manalaysay,A
AU - Mannino,RL
AU - Maupin,C
AU - McCarthy,ME
AU - McDowell,G
AU - McKinsey,DN
AU - McLaughlin,J
AU - McLaughlin,JB
AU - McMonigle,R
AU - Miller,EH
AU - Mizrachi,E
AU - Monte,A
AU - Monzani,ME
AU - Morales,Mendoza JD
AU - Morrison,E
AU - Mount,BJ
AU - Murdy,M
AU - Murphy,ASJ
AU - Naylor,A
AU - Nedlik,C
AU - Nelson,HN
AU - Neves,F
AU - Nguyen,A
AU - Nikoleyczik,JA
AU - Olcina,I
AU - Oliver-Mallory,KC
AU - Orpwood,J
AU - Palladino,KJ
AU - Palmer,J
AU - Pannifer,NJ
AU - Parveen,N
AU - Patton,SJ
AU - Penning,B
AU - Pereira,G
AU - Perry,E
AU - Pershing,T
AU - Piepke,A
AU - Qie,Y
AU - Reichenbacher,J
AU - Rhyne,CA
AU - Riffard,Q
AU - Rischbieter,GRC
AU - Riyat,HS
AU - Rosero,R
AU - Rushton,T
AU - Rynders,D
AU - Santone,D
AU - Sazzad,ABMR
AU - Schnee,RW
AU - Shaw,S
AU - Shutt,T
AU - Silk,JJ
AU - Silva,C
AU - Sinev,G
AU - Siniscalco,J
AU - Smith,R
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 - Szy
DO - 10.1103/physrevd.109.112010
PY - 2024///
SN - 1550-2368
TI - New constraints on ultraheavy dark matter from the LZ experiment
T2 - Physical Review D: Particles, Fields, Gravitation and Cosmology
UR - http://dx.doi.org/10.1103/physrevd.109.112010
UR - http://hdl.handle.net/10044/1/113167
VL - 109
ER -