25 research outputs found
The LUX-ZEPLIN (LZ) Experiment
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alquahtani A
- Alsum SK
- Anderson TJ
- Angelides N
- AraĂșjo HM
- Arbuckle A
- Armstrong JE
- Arthurs M
- Auyeung H
- Bai X
- Bailey AJ
- Balajthy J
- Balashov S
- Bang J
- Barry MJ
- Barthel J
- Bauer D
- Bauer P
- Baxter A
- Belle J
- Beltrame P
- Bensinger J
- Benson T
- Bernard EP
- Bernstein A
- Bhatti A
- Biekert A
- Biesiadzinski TP
- Birrittella B
- Boast KE
- Bolozdynya AI
- Boulton EM
- Boxer B
- Bramante R
- Branson S
- Breidenbach M
- BrĂĄs P
- Buckley JH
- Bugaev VV
- Bunker R
- Burdin S
- Busenitz JK
- Campbell JS
- Carels C
- Carlsmith DL
- Carlson B
- Carmona-Benitez MC
- Cascella M
- Chan C
- Cherwinka JJ
- Chiller AA
- Chiller C
- Chott NI
- Cole A
- Coleman J
- Collaboration TLZ
- Colling D
- Conley RA
- Cottle A
- Coughlen R
- Craddock WW
- Cunha JPD
- Curran D
- Currie A
- Cutter JE
- Dahl CE
- Dardin S
- Dasu S
- Davis J
- Davison TJR
- Decheine N
- Dobi A
- Dobson JEY
- Druszkiewicz E
- Dushkin A
- Edberg TK
- Edwards BN
- Edwards J
- Edwards WR
- Elnimr MM
- Emmet WT
- Eriksen SR
- Faham CH
- Fan A
- Fayer S
- Fiorucci S
- Flaecher H
- Florang IMF
- Ford P
- Francis VB
- Froborg F
- Fruth T
- Gaitskell RJ
- Gantos NJ
- Garcia D
- Geffre A
- Gehman VM
- Gelfand R
- Genovesi J
- Gerhard RM
- Ghag C
- Gibson E
- Gilchriese MGD
- Gokhale S
- Gomber B
- Gonda TG
- Greenall A
- Greenwood S
- Gregerson G
- Grinten MGDVD
- Gwilliam CB
- Hall CR
- Hamilton D
- Hans S
- Hanzel K
- Harrington T
- Harrison A
- Haselschwardt SJ
- Hasselkus C
- Heise J
- Hemer D
- Hertel SA
- Hillbrand S
- Hitchcock O
- Hjemfelt C
- Hoff MD
- Holbrook B
- Holtom E
- Hor JY-K
- Horn M
- Huang DQ
- Hurteau TW
- Ignarra CM
- Irving MN
- Jacobsen RG
- Jahangir O
- Jeffery SN
- Ji W
- Johnson J
- Johnson M
- Johnson P
- Jones WG
- Kaboth AC
- Kamaha A
- Kamdin K
- Kasey V
- Kazkaz K
- Keefner J
- Khaitan D
- Khaleeq M
- Khazov A
- Khromov AV
- Khurana I
- Kim WT
- Kim YD
- Kocher CD
- Konovalov AM
- Korley L
- Korolkova EV
- Koyuncu M
- Kras J
- Kraus H
- Kravitz SW
- Krebs HJ
- Kreczko L
- Krikler B
- Kudryavtsev VA
- Kumpan AV
- Kyre S
- Lambert AR
- Landerud B
- Larsen NA
- Laundrie A
- Leason EA
- Lee C
- Lee HS
- Lee J
- Lenardo BG
- Leonard DS
- Leonard R
- Lesko KT
- Levy C
- Li J
- Liao F-T
- Liao J
- Lin J
- Lindote A
- Linehan R
- Lippincott WH
- Liu R
- Liu X
- Liu Y
- Loniewski C
- Lopes MI
- Lorenzon W
- Lucero D
- Luitz S
- Lyle JM
- Lynch C
- Majewski PA
- Makkinje J
- Malling DC
- Manalaysay A
- Manenti L
- Mannino RL
- Marangou N
- Markley DJ
- MarrLaundrie P
- Martin TJ
- Marzioni MF
- Maupin C
- McConnell CT
- McKinsey DN
- McLaughlin J
- Mei D-M
- Meng Y
- Migneault J
- Miller EH
- Minaker ZJ
- Mizrachi E
- Mock J
- Molash D
- Monte A
- Monzani ME
- Morad JA
- Morrison E
- Mount BJ
- Murphy ASJ
- Naim D
- Naylor A
- Nedlik C
- Nehrkorn C
- Nelson HN
- Nesbit J
- Neves F
- Nikkel JA
- Nikoleyczik JA
- Nilima A
- O'Dell J
- O'Neill FG
- O'Sullivan K
- Oh H
- Olcina I
- Olevitch MA
- Oliver-Mallory KC
- Oxborough L
- Pagac A
- Pagenkopf D
- Pal S
- Palladino KJ
- Palmaccio VM
- Palmer J
- Pangilinan M
- Paredes BL
- Patton SJ
- Pease EK
- Penning BP
- Pereira C
- Pereira G
- Peterson IB
- Piepke A
- Pierson S
- Powell S
- Preece RM
- Pushkin K
- Qie Y
- Racine M
- Ratcliff BN
- Reichenbacher J
- Reichhart L
- Rhyne CA
- Richards A
- Riffard Q
- Rischbieter GRC
- Rodrigues JP
- Rose HJ
- Rosero R
- Rossiter P
- Rucinski R
- Rutherford G
- Rynders D
- Saba JS
- Sabarots L
- Santone D
- Sarychev M
- Sazzad ABMR
- Schnee RW
- Schubnell M
- Scovell PR
- Severson M
- Seymour D
- Shaw S
- Shutt GW
- Shutt TA
- Silk JJ
- Silva C
- Skarpaas K
- Skulski W
- Smith AR
- Smith RE
- Smith RJ
- So J
- Solmaz M
- Solovov VN
- Sorensen P
- Sosnovtsev VV
- Stancu I
- Stark MR
- Stephenson S
- Stern N
- Stevens A
- Stiegler TM
- Stifter K
- Studley R
- Sumner TJ
- Sundarnath K
- Sutcliffe P
- Swanson N
- Szydagis M
- Tan M
- Taylor DJ
- Taylor R
- Taylor WC
- Temples D
- Tennyson BP
- Terman PA
- Thomas KJ
- Thomson JA
- Tiedt DR
- Timalsina M
- To WH
- TomĂĄs A
- Tope TE
- Tripathi M
- Tronstad DR
- Tull CE
- Turner W
- Tvrznikova L
- Utes M
- Utku U
- Uvarov S
- Va'vra J
- Vacheret A
- Vaitkus A
- Verbus JR
- Vietanen T
- Viveiros LD
- Voirin E
- Vuosalo CO
- Walcott S
- Waldron WL
- Walker K
- Wang JJ
- Wang L
- Wang R
- Wang Y
- Watson JR
- Weatherly S
- Webb RC
- Wei W-Z
- While M
- White DT
- White JT
- White RG
- Whitis TJ
- Wilson K
- Wisniewski WJ
- Witherell MS
- Wolfs FLH
- Wolfs JD
- Woodward D
- Worm SD
- Xiang X
- Xiao Q
- Xu J
- Yeh M
- Yin J
- Young I
- Zhang C
- Publication venue
- Publication date
- 11/02/2020
- Field of study
We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850' level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements
Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alsum SK
- AraĂșjo HM
- Arnquist IJ
- Arthurs M
- Bai X
- Bailey AJ
- Balajthy J
- Balashov S
- Barry MJ
- Belle J
- Beltrame P
- Benson T
- Bernard EP
- Bernstein A
- Biesiadzinski TP
- Boast KE
- Bolozdynya A
- Boxer B
- Bramante R
- BrĂĄs P
- Buckley JH
- Bugaev VV
- Bunker R
- Burdin S
- Busenitz JK
- Carels C
- Carlsmith DL
- Carlson B
- Carmona-Benitez MC
- Chan C
- Cherwinka JJ
- Chiller AA
- Chiller C
- Cottle A
- Coughlen R
- Craddock WW
- Currie A
- Dahl CE
- Davison TJR
- Dobi A
- Dobson JEY
- Druszkiewicz E
- Edberg TK
- Edwards WR
- Emmet WT
- Faham CH
- Fiorucci S
- Fruth T
- Gaitskell RJ
- Gantos NJ
- Gehman VM
- Gerhard RM
- Ghag C
- Gilchriese MGD
- Gomber B
- Grinten MGDVD
- Hall CR
- Hans S
- Hanzel K
- Haselschwardt SJ
- Hertel SA
- Hillbrand S
- Hjemfelt C
- Hoff MD
- Holbrook B
- Holtom E
- Hoppe EW
- Hor JY-K
- Horn M
- Huang DQ
- Hurteau TW
- Ignarra CM
- Jacobsen RG
- Ji W
- Kaboth A
- Kamdin K
- Kazkaz K
- Khaitan D
- Khazov A
- Khromov AV
- Konovalov AM
- Korolkova EV
- Koyuncu M
- Kraus H
- Krebs HJ
- Kudryavtsev VA
- Kumpan AV
- Kyre S
- Lee C
- Lee HS
- Lee J
- Leonard DS
- Leonard R
- Lesko KT
- Levy C
- Liao F-T
- Lin J
- Lindote A
- Linehan RE
- Lippincott WH
- Liu X
- Lopes MI
- Lorenzon W
- Luitz S
- Majewski P
- Manalaysay A
- Manenti L
- Mannino RL
- Markley DJ
- Martin TJ
- Marzioni MF
- McConnell CT
- McKinsey DN
- Mei D-M
- Meng Y
- Miller EH
- Mizrachi E
- Mock J
- Monzani ME
- Morad JA
- Mount BJ
- Murphy ASJ
- Nehrkorn C
- Nelson HN
- Neves F
- Nikkel JA
- O'Dell J
- O'Sullivan K
- Olcina I
- Olevitch MA
- Oliver-Mallory KC
- Palladino KJ
- Paredes BL
- Pease EK
- Piepke A
- Powell S
- Preece RM
- Pushkin K
- Ratcliff BN
- Reichenbacher J
- Reichhart L
- Rhyne CA
- Richards A
- Rodrigues JP
- Rose HJ
- Rosero R
- Rossiter P
- Saba JS
- Sarychev M
- Schnee RW
- Schubnell M
- Scovell PR
- Shaw S
- Shutt TA
- Silva C
- Skarpaas K
- Skulski W
- Solmaz M
- Solovov VN
- Sorensen P
- Sosnovtsev VV
- Stancu I
- Stark MR
- Stephenson S
- Stiegler TM
- Stifter K
- Sumner TJ
- Szydagis M
- Taylor DJ
- Taylor WC
- Temples D
- Terman PA
- Thomas KJ
- Thomson JA
- Tiedt DR
- Timalsina M
- To WH
- TomĂĄs A
- Tope TE
- Tripathi M
- Tvrznikova L
- Va'vra J
- Vacheret A
- Verbus JR
- Vuosalo CO
- Waldron WL
- Wang R
- Watson R
- Webb RC
- Wei W-Z
- While M
- White DT
- Whitis TJ
- Wisniewski WJ
- Witherell MS
- Wolfs FLH
- Woodward D
- Worm S
- Xu J
- Yeh M
- Yin J
- Zhang C
- Publication venue
- 'Elsevier BV'
- Publication date
- Field of study
The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active detector volume demand the use of material with extremely low intrinsic radioactivity. We report on the radioassay campaign conducted to identify suitable metals, the determination of factors limiting radiopure production, and the selection of titanium for construction of the LZ cryostat and other detector components. This titanium has been measured with activities of 238Ueâ~<1.6~mBq/kg, 238Ulâ~<0.09~mBq/kg, 232Theâ~=0.28±0.03~mBq/kg, 232Thlâ~=0.25±0.02~mBq/kg, 40K~<0.54~mBq/kg, and 60Co~<0.02~mBq/kg (68\% CL). Such low intrinsic activities, which are some of the lowest ever reported for titanium, enable its use for future dark matter and other rare event searches. Monte Carlo simulations have been performed to assess the expected background contribution from the LZ cryostat with this radioactivity. In 1,000 days of WIMP search exposure of a 5.6-tonne fiducial mass, the cryostat will contribute only a mean background of 0.160±0.001(stat)±0.030(sys) counts
LUX-ZEPLIN (LZ) Technical Design Report
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alsum SK
- AraĂșjo HM
- Arthurs M
- Auyeung H
- Bai X
- Bailey AJ
- Balajthy J
- Balashov S
- Barry MJ
- Bauer D
- Bauer P
- Belle J
- Beltrame P
- Benson T
- Bernard EP
- Bernstein A
- Biesiadzinski TP
- Boast KE
- Bolozdynya AI
- Boulton EM
- Boxer B
- Bramante R
- Breidenbach M
- BrĂĄs P
- Buckley JH
- Bugaev VV
- Bunker R
- Burdin S
- Busenitz JK
- Carels C
- Carlsmith DL
- Carlson B
- Carmona-Benitez MC
- Cascella M
- Chan C
- Cherwinka JJ
- Chiller AA
- Chiller C
- Cole A
- Colling D
- Conley R
- Cottle A
- Coughlen R
- Craddock WW
- Currie A
- Cutter JE
- Dahl CE
- Dasu S
- Davison TJR
- Dobi A
- Dobson JEY
- Druszkiewicz E
- Edberg TK
- Edwards WR
- El-Jurf S
- Elnimr M
- Emmet WT
- Faham CH
- Fan A
- Fayer S
- Fiorucci S
- Ford P
- Francis V
- Froborg F
- Fruth T
- Gaitskell RJ
- Gantos NJ
- Gehman VM
- Gerhard RM
- Ghag C
- Gilchriese MGD
- Gomber B
- Greenall A
- Greenwood S
- Gregerson G
- Grinten MGDVD
- Hall CR
- Hans S
- Hanzel K
- Haselschwardt SJ
- Hau A
- Hemer D
- Hertel S
- Hillbrand S
- Hjemfelt C
- Hoff MD
- Holbrook B
- Holtom E
- Hor JY-K
- Horn M
- Huang DQ
- Hurteau TW
- Ignarra CM
- Jacobsen RG
- Ji W
- Johnson M
- Jones WG
- Kaboth A
- Kamdin K
- Kasey V
- Kazkaz K
- Keefner J
- Khaitan D
- Khaleeq M
- Khazov A
- Khromov AV
- Kim YD
- Konovalov AM
- Korolkova EV
- Koyuncu M
- Kraus H
- Krebs HJ
- Kreczko L
- Krikler B
- Kudryavtsev VA
- Kumpan AV
- Kyre S
- Larsen NA
- Lee C
- Lee HS
- Lee J
- Lenardo BG
- Leonard DS
- Leonard R
- Lesko KT
- Levy C
- Li J
- Liao F-T
- Lin J
- Lindote A
- Linehan R
- Lippincott WH
- Liu X
- Lopes MI
- Lorenzon W
- Luitz S
- Majewski P
- Makkinje J
- Malling DC
- Manalaysay AG
- Manenti L
- Mannino RL
- Markley DJ
- Martin TJ
- Marzioni MF
- Maupin C
- McConnell CT
- McKinsey DN
- Mei D-M
- Meng Y
- Miller EH
- Mizrachi E
- Mock J
- Monzani ME
- Morad JA
- Morrison E
- Mount BJ
- Murphy ASJ
- Nehrkorn C
- Nelson HN
- Neves F
- Nikkel JA
- Nilima A
- O'Dell J
- O'Neill FG
- O'Sullivan K
- Olcina I
- Olevitch MA
- Oliver-Mallory KC
- Pagac A
- Palladino KJ
- Pangilinan M
- Paredes BL
- Patton SJ
- Pease EK
- Penning B
- Piepke A
- Pierson S
- Powell S
- Preece RM
- Pushkin K
- Racine M
- Ratcliff BN
- Reichenbacher J
- Reichhart L
- Rhyne CA
- Richards A
- Rodrigues JP
- Rose HJ
- Rosero R
- Rossiter P
- Saba JS
- Sarychev M
- Schnee RW
- Schubnell M
- Scovell PR
- Shaw S
- Shutt GW
- Shutt TA
- Silk JS
- Silva C
- Skarpaas K
- Skulski W
- Solmaz M
- Solovov VN
- Sorensen P
- Sosnovtsev VV
- Stancu I
- Stark MR
- Stephenson S
- Stiegler TM
- Stifter K
- Sumner TJ
- Sundarnath K
- Sutcliffe P
- Szydagis M
- Taylor DJ
- Taylor WC
- Temples D
- Tennyson BP
- Terman PA
- Thomas KJ
- Thomson JA
- Tiedt DR
- Timalsina M
- To WH
- TomĂĄs A
- Tope TE
- Tripathi M
- Tull CE
- Tvrznikova L
- Utes M
- Utku U
- Uvarov S
- Va'vra J
- Vacheret A
- Verbus JR
- Viveiros LD
- Vuosalo CO
- Waldron WL
- Wang L
- Wang R
- Watson R
- Webb RC
- Wei W-Z
- While M
- White DT
- Whitis TJ
- Wisniewski WJ
- Witherell MS
- Wolfs FLH
- Woodward D
- Worm SD
- Xiao Q
- Xu J
- Yeh M
- Yin J
- Young I
- Zhang C
- Publication venue
- Publication date
- Field of study
In this Technical Design Report (TDR) we describe the LZ detector to be built at the Sanford Underground Research Facility (SURF). The LZ dark matter experiment is designed to achieve sensitivity to a WIMP-nucleon spin-independent cross section of three times ten to the negative forty-eighth square centimeters
Scintillation light detection in the 6-m drift-length ProtoDUNE Dual Phase liquid argon TPC
- Author
- Abi B
- Abud A Abed
- Acciarri R
- Acero MA
- Adames MR
- Adamov G
- Adamowski M
- Adams D
- Adinolfi M
- Aduszkiewicz A
- Aguilar J
- Ahmad Z
- Ahmed J
- Aimard B
- Ali-Mohammadzadeh B
- Alion T
- Allison K
- Alonso MJ Rodriguez
- AlRashed M
- Alt C
- Alton A
- Alvarez R
- Alzas P Barham
- Amedo P
- Anderson J
- Andreopoulos C
- Andreotti M
- Andrews M
- Andrianala F
- Andringa S
- Anfimov N
- Ankowski A
- Antoniassi M
- Antonova M
- Antoshkin A
- Antusch S
- Aranda-Fernandez A
- Arellano L
- Arnold LO
- Arroyave MA
- Asaadi J
- Asquith L
- Aurisano A
- Aushev V
- Autiero D
- Ayala Lara V
- Ayala-Torres M
- Azfar F
- Back A
- Back H
- Back JJ
- Backhouse C
- Bagaturia I
- Bagby L
- Balashov N
- Balasubramanian S
- Baldi P
- Baller B
- Bambah B
- Barao F
- Barenboim G
- Barker G
- Barkhouse W
- Barnes C
- Barr G
- Barranco Monarca J
- Barros A
- Barros N
- Barrow JL
- Basharina-Freshville A
- Bashyal A
- Basque V
- Batchelor C
- Battat JBR
- Battisti F
- Bay F
- Bazetto MCQ
- Bazo Alba JLL
- Beacom JF
- Bechetoille E
- Behera B
- Beigbeder C
- Bellantoni L
- Bellettini G
- Bellini V
- Beltramello O
- Benekos N
- Berger J
- Berkman S
- Bernardini P
- Berner RM
- Bersani A
- Bertolucci S
- Betancourt M
- Betancur Rodriguez A
- Bevan A
- Bezawada Y
- Bezerra TJC
- Bhardwaj A
- Bhatnagar V
- Bhattacharjee M
- Bhattarai D
- Bhuller S
- Bhuyan B
- Biagi S
- Bian J
- Biassoni M
- Biery K
- Bilki B
- Bishai M
- Bitadze A
- Blake A
- Blaszczyk F
- Blazey GC
- Blucher E
- Boissevain J
- Bolognesi S
- Bolton T
- Bomben L
- Bonesini M
- Bongrand M
- Bonilla-Diaz C
- Bonini F
- Booth A
- Boran F
- Bordoni S
- Borkum A
- Bostan N
- Bour P
- Bourgeois C
- Boyden D
- Bracinik J
- Braga D
- Brailsford D
- Branca A
- Brandt A
- Bremer J
- Breton D
- Brew C
- Brice SJ
- Brizzolari C
- Bromberg C
- Brooke J
- Bross A
- Brunetti G
- Brunetti M
- Buchanan N
- Budd H
- Butorov I
- Cagnoli I
- Cai T
- Caicedo DA Martinez
- Caiulo D
- Calabrese R
- Calafiura P
- Calcutt J
- Calin M
- Calvez S
- Calvo E
- Caminata A
- Campanelli M
- Caratelli D
- Carber D
- Carceller JC
- Carini G
- Carlus B
- Carneiro MF
- Carniti P
- Carranza H
- Carroll T
- Castano Forero JF
- Castillo A
- Castromonte C
- Catano-Mur E
- Cattadori C
- Cavalier F
- Cavallaro G
- Cavanna F
- Centro S
- Cerati G
- Cervelli A
- Cervera Villanueva A
- Chalifour M
- Chappell A
- Chardonnet E
- Charitonidis N
- Chatterjee A
- Chattopadhyay S
- Chavarry Neyra MSS
- Chen H
- Chen M
- Chen Y
- Chen Z
- Chen-Wishart Z
- Cheon Y
- Cherdack D
- Chi C
- Childress S
- Chirco R
- Chiriacescu A
- Chisnall G
- Cho K
- Choate S
- Chokheli D
- Chong PS
- Christensen A
- Christian D
- Christodoulou G
- Chukanov A
- Chung M
- Church E
- Cicero V
- Clarke P
- Cline G
- Coan TE
- Cocco AG
- Coelho JAB
- Colton N
- Conley E
- Conley R
- Conrad J
- Convery M
- Copello S
- Cova P
- Cremaldi L
- Cremonesi L
- Crespo-Anadon J
- Crisler M
- Cristaldo E
- Crnkovic J
- Cross R
- Cudd A
- Cuesta C
- Cui Y
- Cussans D
- Dalager O
- DaMotta H
- das Chagas E Batista
- David C
- David Q
- Davies GS
- Davini S
- Dawson J
- De Bonis I
- De Gouvea A
- De Holanda PC
- De Icaza Astiz IL
- De Jong P
- De Lurgio P
- De Mello Neto JRT
- De Roeck A
- De Romeri V
- De Souza G
- de Souza H Vieira
- De K
- De S
- Debbins P
- Decowski MP
- Deisting A
- Delbart A
- Delepine D
- Delgado M
- Delgado MA Ramirez
- Dell'Acqua A
- Delmonte N
- DeMuth DM
- Dennis S
- Densham C
- Deptuch GW
- Devi R
- Dharmapalan R
- Di Domizio S
- Di Giulio L
- Di Noto L
- Dias M
- Diaz F
- Diaz JS
- Ding P
- Dirkx G
- Distefano C
- Diurba R
- Diwan M
- Djurcic Z
- Doering D
- Dolan S
- Dolinski M
- Domine L
- Donon Y
- Douglas D
- Douillet D
- Dragone A
- Drake G
- Drielsma F
- Duarte L
- Duchesneau D
- Duffy K
- Dunne P
- Dutta B
- Duyang H
- Dvornikov O
- Dwyer D
- Dyshkant A
- Eads M
- Earle A
- Edmunds D
- Eisch J
- Emberger L
- Emery S
- Englezos P
- Ereditato A
- Erjavec T
- Escobar C
- Eurin G
- Evans JJ
- Ewart E
- Ezeribe AC
- Fahey K
- Falcone A
- Fani' M
- Farnese C
- Farzan Y
- Fedoseev D
- Felix J
- Feng Y
- Fernandez Menendez P
- Fernandez Morales M
- Fernandez-Martinez E
- Ferraro F
- Fields L
- Filip P
- Filthaut F
- Fiorini M
- Fischer V
- Fitzpatrick RS
- Flanagan W
- Fleming B
- Flight R
- Fogarty S
- Foreman W
- Fowler J
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- Freeman J
- Freestone J
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- Furic IK
- Furman K
- Furmanski AP
- Gabrielli A
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- Gallagher H
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- Gastler D
- Gauvreau J
- Ge G
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- Giammaria P
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- Macias CT
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- Maddalena A
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- Miotto G Lehmann
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- Molina J
- Monsalve S Alonso
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- Nelson JK
- Nesbit J
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- Neves F Bento
- Newbold D
- Newcomer M
- Newton H
- Nichol R
- Nicolas-Arnaldos F
- Nikolica A
- Niner E
- Nishimura K
- Norman A
- Norrick A
- Northrop R
- Novella P
- Nowak JA
- Nunes M Soares
- Oberling M
- Ochoa-Ricoux J
- Olivier A
- Olshevskiy A
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- Onishchuk Y
- Oregui B Tapia
- Ott J
- Pagani L
- Palacio G
- Palamara O
- Palestini S
- Paley JM
- Pallavicini M
- Palomares C
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- Paolone V
- Papadimitriou V
- Papaleo R
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- Patton SJ
- Patzak T
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- Pavlovic Z
- Pawloski G
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- Peeters SJM
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- Peres OLG
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- Pershey D
- Pessina G
- Petrillo G
- Petta C
- Petti R
- Pia V
- Piastra F
- Pickering L
- Pietropaolo F
- Pimentel VL
- Pinaroli G
- Plata M Manrique
- Plows K
- Plunkett R
- Poling R
- Pompa F
- Pons X
- Poonthottathil N
- Poppi F
- Pordes S
- Porter J
- Potekhin M
- Potenza R
- Potukuchi BVKS
- Pozimski J
- Pozzato M
- Prakash S
- Prakash T
- Prest M
- Prince S
- Psihas F
- Pugnere D
- Qian X
- Raaf JL
- Radeka V
- Rademacker J
- Radics B
- Rafique A
- Raguzin E
- Rai M
- Rajaoalisoa M
- Rakhno I
- Rakotonandrasana A
- Rakotondravohitra L
- Rameika R
- Ramson B
- Rappoldi A
- Raselli G
- Ratoff P
- Raut S
- Razakamiandra RF
- Rea EM
- Real JS
- Rebel B
- Rechenmacher R
- Reggiani-Guzzo M
- Reichenbacher J
- Reitzner SD
- Renshaw A
- Rescia S
- Resnati F
- Ribas M
- Riboldi S
- Riccio C
- Riccobene G
- Rice LCJ
- Ricol JS
- Rigamonti A
- Rigaut Y
- Rincon E
- Ritchie-Yates H
- Rivera D
- Robayo F Fuentes
- Robert A
- Rochester L
- Roda M
- Rodrigues P
- Rodriguez Bonilla E
- Rondon J Rodriguez
- Rosauro-Alcaraz S
- Rosenberg M
- Rosier P
- Roskovec B
- Rossella M
- Rossi M
- Rout J
- Rubbia A
- Rubbia C
- Russell B
- Ruterbories D
- Rybnikov A
- Saa-Hernandez A
- Saakyan R
- Sacerdoti S
- Safford T
- Sahu N
- Sakashita K
- Sala P
- Samios N
- Samoylov O
- Sanchez MC
- Sandberg V
- Sanders DA
- Sankey D
- Santana S
- Santos-Maldonado M
- Saoulidou N
- Sapienza P
- Sarasty C
- Sarcevic I
- Savage G
- Savinov V
- Scaramelli A
- Scarff A
- Scarpelli A
- Schefke T
- Schellman H
- Schifano S
- Schlabach P
- Schmitz D
- Schneider AW
- Scholberg K
- Schukraft A
- Segreto E
- Selyunin A
- Senise CR
- Sensenig J
- Sergi A
- Sfar H Rejeb
- Sgalaberna D
- Shaevitz MH
- Shafaq S
- Shaker F
- Shamma M
- Sharankova R
- Sharma HR
- Sharma R
- Sharma RK
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- Shepherd-Themistocleous C
- Sheshukov A
- Shin S
- Shoemaker I
- Shooltz D
- Shrock R
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- Sinev G
- Singh J
- Singh J
- Singh L
- Singh P
- Singh V
- Sipos R
- Sippach FW
- Sirri G
- Sitraka A
- Siyeon K
- Skarpaas K
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- Smith E
- Smith P
- Smolik J
- Smy M
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- Snowden-Ifft D
- Sobel H
- Soderberg M
- Sokolov S
- Solano Salinas CJ
- Soldner-Rembold S
- Soleti SR
- Solomey N
- Solovov V
- Sondheim WE
- Sorel M
- Sotnikov A
- Soto Ugaldi FA
- Soto-Oton J
- Sousa A
- Soustruznik K
- Spagliardi F
- Spanu M
- Spitz J
- Spooner NJC
- Spurgeon K
- Stancari M
- Stanco L
- Stanford C
- Stein R
- Steiner HM
- Steklain Lisboa AF
- Stewart J
- Stillwell B
- Stock J
- Stocker F
- Stokes T
- Strait M
- Strauss T
- Strigari L
- Stuart A
- Suarez Suncion JM
- Suarez JG
- Sullivan H
- Summers D
- Surdo A
- Susic V
- Suter L
- Sutera CM
- Svoboda R
- Szczerbinska B
- Szelc AM
- Tanaka H
- Tang S
- Tapia A
- Tapper A
- Tariq S
- Tarpara E
- Tata N
- Tatar E
- Tayloe R
- Teklu AM
- Tennessen P
- Tenti M
- Terao K
- Ternes CA
- Terranova F
- Terrazas I Caro
- Testera G
- Thakore T
- Thea A
- Thompson JL
- Thorn C
- Timm SC
- Tishchenko V
- Tomassetti L
- Tonazzo A
- Torbunov D
- Torti M
- Tortola M
- Tortorici F
- Tosi N
- Totani D
- Toups M
- Touramanis C
- Travaglini R
- Trevor J
- Trilov S
- Trzaska WH
- Tsai Y
- Tsai Y-T
- Tsamalaidze Z
- Tsang K
- Tsverava N
- Tufanli S
- Tull C
- Tyley E
- Tzanov M
- Uboldi L
- Uchida MA
- Urheim J
- Usher T
- Uzunyan S
- Vagins MR
- Vahle P
- Valder S
- Valdiviesso GDA
- Valencia E
- Valentim R
- Vallari Z
- Vallazza E
- Valle JWF
- Vallecorsa S
- Van Berg R
- Van de Water RG
- Vanegas Forero D
- Vannerom D
- Varanini F
- Vargas Oliva D
- Varner G
- Vasel J
- Vasina S
- Vasseur G
- Vaughan N
- Vaziri K
- Vazquez W Panduro
- Ventura S
- Verdugo A
- Vergani S
- Vermeulen MA
- Verzocchi M
- Vicenzi M
- Vignoli C
- Vilela C
- Viren B
- Vrba T
- Wachala T
- Waldron A
- Wallbank M
- Wallis C
- Wang H
- Wang J
- Wang L
- Wang MHLS
- Wang X
- Wang Y
- Wang Y
- Warburton K
- Warner D
- Wascko MO
- Waters D
- Watson A
- Wawrowska K
- Weatherly P
- Weber A
- Weber M
- Wei H
- Weinstein A
- Wenman D
- Wetstein M
- White A
- Whitehead LH
- Whittington D
- Wilking MJ
- Wilkinson A
- Wilkinson C
- Williams Z
- Wilson F
- Wilson RJ
- Wisniewski W
- Wolcott J
- Wongjirad T
- Wood A
- Wood K
- Worcester E
- Worcester M
- Wresilo K
- Wret C
- Wu W
- Wu W
- Xiao Y
- Xie F
- Yaeggy B
- Yandel E
- Yang G
- Yang K
- Yang T
- Yankelevich A
- Yershov N
- Yonehara K
- Yoon YS
- Young T
- Yu B
- Yu H
- Yu H
- Yu J
- Yu Y
- Yuan W
- Zaki R
- Zalesak J
- Zambelli L
- Zamorano B
- Zani A
- Zazueta L
- Zeller GP
- Zennamo J
- Zeug K
- Zhang C
- Zhang S
- Zhang Y
- Zhao M
- Zhivun E
- Zhu G
- Zimmerman ED
- Zucchelli S
- Zuklin J
- Zutshi V
- Zwaska R
- Publication venue
- 'Springer Fachmedien Wiesbaden GmbH'
- Publication date
- 16/07/2022
- Field of study
DUNE is a dual-site experiment for long-baseline neutrino oscillation studies, neutrino astrophysics and nucleon decay searches. ProtoDUNE Dual Phase (DP) is a 6Â Ă Â 6Â Ă Â 6Â m 3 liquid argon time-projection-chamber (LArTPC) that recorded cosmic-muon data at the CERN Neutrino Platform in 2019-2020 as a prototype of the DUNE Far Detector. Charged particles propagating through the LArTPC produce ionization and scintillation light. The scintillation light signal in these detectors can provide the trigger for non-beam events. In addition, it adds precise timing capabilities and improves the calorimetry measurements. In ProtoDUNE-DP, scintillation and electroluminescence light produced by cosmic muons in the LArTPC is collected by photomultiplier tubes placed up to 7Â m away from the ionizing track. In this paper, the ProtoDUNE-DP photon detection system performance is evaluated with a particular focus on the different wavelength shifters, such as PEN and TPB, and the use of Xe-doped LAr, considering its future use in giant LArTPCs. The scintillation light production and propagation processes are analyzed and a comparison of simulation to data is performed, improving understanding of the liquid argon properties
LUX-ZEPLIN (LZ) Conceptual Design Report
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alsum SK
- AraĂșjo HM
- Bai X
- Bailey AJ
- Balajthy J
- Balashov S
- Barry MJ
- Bauer P
- Beltrame P
- Bernard EP
- Bernstein A
- Biesiadzinski TP
- Boast KE
- Bolozdynya AI
- Boulton EM
- Bramante R
- Buckley JH
- Bugaev VV
- Bunker R
- Burdin S
- Busenitz JK
- Carels C
- Carlsmith DL
- Carlson B
- Carmona-Benitez MC
- Cascella M
- Chan C
- Cherwinka JJ
- Chiller AA
- Chiller C
- Collaboration TLZ
- Craddock WW
- Cunha JPD
- Currie A
- Cutter JE
- Dahl CE
- Dasu S
- Davison TJR
- Dobi A
- Dobson JEY
- Druszkiewicz E
- Edberg TK
- Edwards BN
- Edwards WR
- Elnimr MM
- Emmet WT
- Faham CH
- Fiorucci S
- Ford P
- Francis VB
- Fu C
- Gaitskell RJ
- Gantos NJ
- Gehman VM
- Gerhard RM
- Ghag C
- Gilchriese MGD
- Gomber B
- Grinten MGDVD
- Hall CR
- Harris A
- Haselschwardt SJ
- Hertel SA
- Hoff MD
- Holbrook B
- Holtom E
- Huang DQ
- Hurteau TW
- Ignarra CM
- Jacobsen RG
- Ji W
- Ji X
- Johnson M
- Ju Y
- Kamdin K
- Kazkaz K
- Khaitan D
- Khazov A
- Khromov AV
- Konovalov AM
- Korolkova EV
- Kraus H
- Krebs HJ
- Kudryavtsev VA
- Kumpan AV
- Kyre S
- Larsen NA
- Lee C
- Lenardo BG
- Lesko KT
- Liao F-T
- Lin J
- Lindote A
- Lippincott WH
- Liu J
- Liu X
- Lopes MI
- Lorenzon W
- Luitz S
- Majewski P
- Malling DC
- Manalaysay AG
- Manenti L
- Mannino RL
- Markley DJ
- Martin TJ
- Marzioni MF
- McKinsey DN
- Mei D-M
- Meng Y
- Miller EH
- Mock J
- Monzani ME
- Morad JA
- Murphy ASJ
- Nelson HN
- Neves F
- Nikkel JA
- O'Dell J
- O'Neill FG
- O'Sullivan K
- Olevitch MA
- Oliver-Mallory KC
- Palladino KJ
- Pangilinan M
- Patton SJ
- Pease EK
- Piepke A
- Powell S
- Preece RM
- Pushkin K
- Ratcliff BN
- Reichenbacher J
- Reichhart L
- Rhyne C
- Rodrigues JP
- Rose HJ
- Rosero R
- Saba JS
- Sarychev M
- Schnee RW
- Schubnell MSG
- Scovell PR
- Shaw S
- Shutt TA
- Silva C
- Skarpaas K
- Skulski W
- Solovov VN
- Sorensen P
- Sosnovtsev VV
- Stancu I
- Stark MR
- Stephenson S
- Stiegler TM
- Sumner TJ
- Sundarnath K
- Szydagis M
- Taylor DJ
- Taylor W
- Tennyson BP
- Terman PA
- Thomas KJ
- Thomson JA
- Tiedt DR
- To WH
- TomĂĄs A
- Tripathi M
- Tull CE
- Tvrznikova L
- Uvarov S
- Va'vra J
- Verbus JR
- Viveiros LD
- Vuosalo CO
- Waldron WL
- Wang L
- Webb RC
- Wei W-Z
- While M
- White DT
- Whitis TJ
- Wisniewski WJ
- Witherell MS
- Wolfs FLH
- Woods E
- Woodward D
- Worm SD
- Yeh M
- Yin J
- Young SK
- Zhang C
- Publication venue
- U.S. Department of Energy
- Publication date
- 01/01/2015
- Field of study
The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report. LZ is a second-generation dark-matter detector with the potential for unprecedented sensitivity to weakly interacting massive particles (WIMPs) of masses from a few GeV/c2 to hundreds of TeV/c2. With total liquid xenon mass of about 10 tonnes, LZ will be the most sensitive experiment for WIMPs in this mass region by the end of the decade. This report describes in detail the design of the LZ technical systems. Expected backgrounds are quantified and the performance of the experiment is presented. The LZ detector will be located at the Sanford Underground Research Facility in South Dakota. The organization of the LZ Project and a summary of the expected cost and current schedule are given
The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alquahtani A
- Alsum SK
- Anderson TJ
- Angelides N
- AraĂșjo HM
- Arbuckle A
- Armstrong JE
- Arthurs M
- Auyeung H
- Aviles S
- Bai X
- Bailey AJ
- Balajthy J
- Balashov S
- Bang J
- Barry MJ
- Bauer D
- Bauer P
- Baxter A
- Belle J
- Beltrame P
- Bensinger J
- Benson T
- Bernard EP
- Bernstein A
- Bhatti A
- Biekert A
- Biesiadzinski TP
- Birch HJ
- Birrittella B
- Boast KE
- Bolozdynya AI
- Boulton EM
- Boxer B
- Bramante R
- Branson S
- Breidenbach M
- Brew CAJ
- BrĂĄs P
- Buckley JH
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- Tiedt DR
- Timalsina M
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- TomĂĄs A
- Tope TE
- Tripathi M
- Tronstad DR
- Tull CE
- Turner W
- Tvrznikova L
- Utes M
- Utku U
- Uvarov S
- Vacheret A
- Vaitkus A
- van der Grinten MGD
- Vaâvra J
- Verbus JR
- Vietanen T
- Voirin E
- Vuosalo CO
- Walcott S
- Waldron WL
- Walker K
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- Webb RC
- Wei W-Z
- While M
- White DT
- White JT
- White RG
- Whitis TJ
- Wilson K
- Wisniewski WJ
- Witherell MS
- Wolfs FLH
- Wolfs JD
- Woodward D
- Worm SD
- Xiang X
- Xiao Q
- Xu J
- Yeh M
- Yin J
- Young I
- Zarzhitsky P
- Zhang C
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 29/08/2020
- Field of study
LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with spin-independent WIMP-nucleon scattering sensitivity above 1.4Ă10â48cm2 for a WIMP mass of 40GeV/c2 and a 1000days exposure. LZ achieves this sensitivity through a combination of a large 5.6t fiducial volume, active inner and outer veto systems, and radio-pure construction using materials with inherently low radioactivity content. The LZ collaboration performed an extensive radioassay campaign over a period of six years to inform material selection for construction and provide an input to the experimental background model against which any possible signal excess may be evaluated. The campaign and its results are described in this paper. We present assays of dust and radon daughters depositing on the surface of components as well as cleanliness controls necessary to maintain background expectations through detector construction and assembly. Finally, examples from the campaign to highlight fixed contaminant radioassays for the LZ photomultiplier tubes, quality control and quality assurance procedures through fabrication, radon emanation measurements of major sub-systems, and bespoke detector systems to assay scintillator are presented
Separation of track- and shower-like energy deposits in ProtoDUNE-SP using a convolutional neural network
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- Publication venue
- Publication date
- 01/01/2022
- Field of study
Liquid argon time projection chamber detector technology provides high spatial and calorimetric resolutions on the charged particles traversing liquid argon. As a result, the technology has been used in a number of recent neutrino experiments, and is the technology of choice for the Deep Underground Neutrino Experiment (DUNE). In order to perform high precision measurements of neutrinos in the detector, final state particles need to be effectively identified, and their energy accurately reconstructed. This article proposes an algorithm based on a convolutional neural network to perform the classification of energy deposits and reconstructed particles as track-like or arising from electromagnetic cascades. Results from testing the algorithm on data from ProtoDUNE-SP, a prototype of the DUNE far detector, are presented. The network identifies track- and shower-like particles, as well as Michel electrons, with high efficiency. The performance of the algorithm is consistent between data and simulation
Separation of track- and shower-like energy deposits in ProtoDUNE-SP using a convolutional neural network
- Author
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- Zimmerman ED
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- Zuklin J
- Zutshi V
- Zwaska R
- Publication venue
- 'Springer Science and Business Media LLC'
- Publication date
- 01/01/2022
- Field of study
Liquid argon time projection chamber detector technology provides high spatial and calorimetric resolutions on the charged particles traversing liquid argon. As a result, the technology has been used in a number of recent neutrino experiments, and is the technology of choice for the Deep Underground Neutrino Experiment (DUNE). In order to perform high precision measurements of neutrinos in the detector, final state particles need to be effectively identified, and their energy accurately reconstructed. This article proposes an algorithm based on a convolutional neural network to perform the classification of energy deposits and reconstructed particles as track-like or arising from electromagnetic cascades. Results from testing the algorithm on experimental data from ProtoDUNE-SP, a prototype of the DUNE far detector, are presented. The network identifies track- and shower-like particles, as well as Michel electrons, with high efficiency. The performance of the algorithm is consistent between experimental data and simulation
Design, construction and operation of the ProtoDUNE-SP Liquid Argon TPC
- Author
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- Publication venue
- 'IOP Publishing'
- Publication date
- 04/08/2021
- Field of study
The ProtoDUNE-SP detector is a single-phase liquid argon time projection chamber (LArTPC) that was constructed and operated in the CERN North Area at the end of the H4 beamline. This detector is a prototype for the first far detector module of the Deep Underground Neutrino Experiment (DUNE), which will be constructed at the Sandford Underground Research Facility (SURF) in Lead, South Dakota, U.S.A. The ProtoDUNE-SP detector incorporates full-size components as designed for DUNE and has an active volume of 7 Ă 6 Ă 7.2 m3. The H4 beam delivers incident particles with well-measured momenta and high-purity particle identification. ProtoDUNE-SP's successful operation between 2018 and 2020 demonstrates the effectiveness of the single-phase far detector design. This paper describes the design, construction, assembly and operation of the detector components
The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs
- Author
- Akerib DS
- Akerlof CW
- Akimov DY
- Alquahtani A
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- Anderson TJ
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- Stark MR
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- Sumner TJ
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- Sutcliffe P
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- Xu J
- Yeh M
- Yin J
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- Zarzhitsky P
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