Imperial College London

ProfessorRobertoTrotta

Faculty of Natural SciencesDepartment of Physics

Visiting Professor
 
 
 
//

Contact

 

+44 (0)20 7594 7793r.trotta Website CV

 
 
//

Assistant

 

Mrs Sheila Ekudo +44 (0)20 7594 2086

 
//

Location

 

1009Blackett LaboratorySouth Kensington Campus

//

Summary

 

Publications

Citation

BibTex format

@article{Althueser:2022:07/P07018,
author = {Althueser, L and Antunovic, B and Aprile, E and Bajpai, D and Baudis, L and Baur, D and Baxter, AL and Bellagamba, L and Biondi, R and Biondi, Y and Bismark, A and Brown, A and Budnik, R and Chauvin, A and Colijn, AP and Cuenca-Garcia, JJ and D'Andrea, V and Di, Gangi P and Dierle, J and Diglio, S and Doerenkamp, M and Eitel, K and Farrell, S and Ferella, AD and Ferrari, C and Findley, C and Fischer, H and Galloway, M and Girard, F and Glade-Beucke, R and Grandi, L and Guida, M and Hansmann-Menzemer, S and Joerg, F and Jones, L and Kavrigin, P and Krauss, LM and von, Krosigk B and Kuger, F and Landsman, H and Lang, RF and Li, S and Liang, S and Lindner, M and Loizeau, J and Lombardi, F and Undagoitia, TM and Masbou, J and Masson, E and Matias-Lopes, J and Milutinovic, S and Monteiro, CMB and Murra, M and Ni, K and Oberlack, U and Ostrovskiy, I and Pandurovic, M and Peres, R and Qin, J and Silva, MR and Garcia, DR and Sanchez-Lucas, P and dos, Santos JMF and Schumann, M and Selvi, M and},
doi = {07/P07018},
journal = {Journal of Instrumentation},
title = {GPU-based optical simulation of the DARWIN detector},
url = {http://dx.doi.org/10.1088/1748-0221/17/07/P07018},
volume = {17},
year = {2022}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - Understanding propagation of scintillation light is critical for maximizing the discovery potential of next-generation liquid xenon detectors that use dual-phase time projection chamber technology. This work describes a detailed optical simulation of the DARWIN detector implemented using Chroma, a GPU-based photon tracking framework. To evaluate the framework and to explore ways of maximizing efficiency and minimizing the time of light collection, we simulate several variations of the conventional detector design. Results of these selected studies are presented. More generally, we conclude that the approach used in this work allows one to investigate alternative designs faster and in more detail than using conventional Geant4 optical simulations, making it an attractive tool to guide the development of the ultimate liquid xenon observatory.
AU - Althueser,L
AU - Antunovic,B
AU - Aprile,E
AU - Bajpai,D
AU - Baudis,L
AU - Baur,D
AU - Baxter,AL
AU - Bellagamba,L
AU - Biondi,R
AU - Biondi,Y
AU - Bismark,A
AU - Brown,A
AU - Budnik,R
AU - Chauvin,A
AU - Colijn,AP
AU - Cuenca-Garcia,JJ
AU - D'Andrea,V
AU - Di,Gangi P
AU - Dierle,J
AU - Diglio,S
AU - Doerenkamp,M
AU - Eitel,K
AU - Farrell,S
AU - Ferella,AD
AU - Ferrari,C
AU - Findley,C
AU - Fischer,H
AU - Galloway,M
AU - Girard,F
AU - Glade-Beucke,R
AU - Grandi,L
AU - Guida,M
AU - Hansmann-Menzemer,S
AU - Joerg,F
AU - Jones,L
AU - Kavrigin,P
AU - Krauss,LM
AU - von,Krosigk B
AU - Kuger,F
AU - Landsman,H
AU - Lang,RF
AU - Li,S
AU - Liang,S
AU - Lindner,M
AU - Loizeau,J
AU - Lombardi,F
AU - Undagoitia,TM
AU - Masbou,J
AU - Masson,E
AU - Matias-Lopes,J
AU - Milutinovic,S
AU - Monteiro,CMB
AU - Murra,M
AU - Ni,K
AU - Oberlack,U
AU - Ostrovskiy,I
AU - Pandurovic,M
AU - Peres,R
AU - Qin,J
AU - Silva,MR
AU - Garcia,DR
AU - Sanchez-Lucas,P
AU - dos,Santos JMF
AU - Schumann,M
AU - Selvi,M
AU - Semeria,F
AU - Simgen,H
AU - Steidl,M
AU - Tan,P-L
AU - Terliuk,A
AU - Thieme,K
AU - Trotta,R
AU - Tunnell,CD
AU - Toennies,F
AU - Valerius,K
AU - Vetter,S
AU - Volta,G
AU - Wang,W
AU - Wittweg,C
AU - Xing,Y
DO - 07/P07018
PY - 2022///
SN - 1748-0221
TI - GPU-based optical simulation of the DARWIN detector
T2 - Journal of Instrumentation
UR - http://dx.doi.org/10.1088/1748-0221/17/07/P07018
UR - https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000849218600003&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=a2bf6146997ec60c407a63945d4e92bb
UR - https://iopscience.iop.org/article/10.1088/1748-0221/17/07/P07018
UR - http://hdl.handle.net/10044/1/109399
VL - 17
ER -