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@article{Akerib:2020:10.1103/PhysRevD.101.012003,
author = {Akerib, DS and Alsum, S and Araujo, HM and Bai, X and Balajthy, J and Baxter, A and Bernard, EP and Bernstein, A and Biesiadzinski, TP and Boulton, EM and Boxer, B and Bras, P and Burdin, S and Byram, D and Carmona-Benitez, MC and Chan, C and Cutter, JE and de, Viveiros L and Druszkiewicz, E and Fan, A and Fiorucci, S and Gaitskell, RJ and Ghag, C and Gilchriese, MGD and Gwilliam, C and Hall, CR and Haselschwardt, SJ and Hertel, SA and Hogan, DP and Horn, M and Huang, DQ and Ignarra, CM and Jacobsen, RG and Jahangir, O and Ji, W and Kamdin, K and Kazkaz, K and Khaitan, D and Korolkova, EV and Kravitz, S and Kudryavtsev, VA and Leason, E and Lenardo, BG and Lesko, KT and Liao, J and Lin, J and Lindote, A and Lopes, MI and Manalaysay, A and Mannino, RL and Marangou, N and Marzioni, MF and McKinsey, DN and Mei, D-M and Moongweluwan, M and Morad, JA and Murphy, ASJ and Naylor, A and Nehrkorn, C and Nelson, HN and Neves, F and Nilima, A and Oliver-Mallory, KC and Palladino, KJ and Pease, EK},
doi = {10.1103/PhysRevD.101.012003},
journal = {Physical Review D: Particles, Fields, Gravitation and Cosmology},
pages = {012003  1--012003  8},
title = {First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data},
url = {http://dx.doi.org/10.1103/PhysRevD.101.012003},
volume = {101},
year = {2020}
}

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TY  - JOUR
AB  - We present the results of a direct detection search for mirror dark matter interactions, using data collected from the Large Underground Xenon experiment during 2013, with an exposure of 95 live−days×118  kg. Here, the calculations of the mirror electron scattering rate in liquid xenon take into account the shielding effects from mirror dark matter captured within the Earth. Annual and diurnal modulation of the dark matter flux and atomic shell effects in xenon are also accounted for. Having found no evidence for an electron recoil signal induced by mirror dark matter interactions we place an upper limit on the kinetic mixing parameter over a range of local mirror electron temperatures between 0.1 and 0.9 keV. This limit shows significant improvement over the previous experimental constraint from orthopositronium decays and significantly reduces the allowed parameter space for the model. We exclude mirror electron temperatures above 0.3 keV at a 90% confidence level, for this model, and constrain the kinetic mixing below this temperature.
AU  - Akerib,DS
AU  - Alsum,S
AU  - Araujo,HM
AU  - Bai,X
AU  - Balajthy,J
AU  - Baxter,A
AU  - Bernard,EP
AU  - Bernstein,A
AU  - Biesiadzinski,TP
AU  - Boulton,EM
AU  - Boxer,B
AU  - Bras,P
AU  - Burdin,S
AU  - Byram,D
AU  - Carmona-Benitez,MC
AU  - Chan,C
AU  - Cutter,JE
AU  - de,Viveiros L
AU  - Druszkiewicz,E
AU  - Fan,A
AU  - Fiorucci,S
AU  - Gaitskell,RJ
AU  - Ghag,C
AU  - Gilchriese,MGD
AU  - Gwilliam,C
AU  - Hall,CR
AU  - Haselschwardt,SJ
AU  - Hertel,SA
AU  - Hogan,DP
AU  - Horn,M
AU  - Huang,DQ
AU  - Ignarra,CM
AU  - Jacobsen,RG
AU  - Jahangir,O
AU  - Ji,W
AU  - Kamdin,K
AU  - Kazkaz,K
AU  - Khaitan,D
AU  - Korolkova,EV
AU  - Kravitz,S
AU  - Kudryavtsev,VA
AU  - Leason,E
AU  - Lenardo,BG
AU  - Lesko,KT
AU  - Liao,J
AU  - Lin,J
AU  - Lindote,A
AU  - Lopes,MI
AU  - Manalaysay,A
AU  - Mannino,RL
AU  - Marangou,N
AU  - Marzioni,MF
AU  - McKinsey,DN
AU  - Mei,D-M
AU  - Moongweluwan,M
AU  - Morad,JA
AU  - Murphy,ASJ
AU  - Naylor,A
AU  - Nehrkorn,C
AU  - Nelson,HN
AU  - Neves,F
AU  - Nilima,A
AU  - Oliver-Mallory,KC
AU  - Palladino,KJ
AU  - Pease,EK
AU  - Riffard,Q
AU  - Rischbieter,GRC
AU  - Rhyne,C
AU  - Rossiter,P
AU  - Shaw,S
AU  - Shutt,TA
AU  - Silva,C
AU  - Solmaz,M
AU  - Solovov,VN
AU  - Sorensen,P
AU  - Sumner,TJ
AU  - Szydagis,M
AU  - Taylor,DJ
AU  - Taylor,R
AU  - Taylor,WC
AU  - Tennyson,BP
AU  - Terman,PA
AU  - Tiedt,DR
AU  - To,WH
AU  - Tripathi,M
AU  - Tvrznikova,L
AU  - Utku,U
AU  - Uvarov,S
AU  - Vacheret,A
AU  - Velan,V
AU  - Webb,RC
AU  - White,JT
AU  - Whitis,TJ
AU  - Witherell,MS
AU  - Wolfs,FLH
AU  - Woodward,D
AU  - Xu,J
AU  - Zhang,C
DO  - 10.1103/PhysRevD.101.012003
EP  - 1
PY  - 2020///
SN  - 1550-2368
SP  - 012003
TI  - First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data
T2  - Physical Review D: Particles, Fields, Gravitation and Cosmology
UR  - http://dx.doi.org/10.1103/PhysRevD.101.012003
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000505485600002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.101.012003
UR  - http://hdl.handle.net/10044/1/80604
VL  - 101
ER  -

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