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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
by A. Bismark , J. P. Cussonneau , J. Dierle , J. M. F. dos Santos , F. Girard , C. Macolino , D. Thers , C. Capelli , S. Milutinovic , V. Pizzella , U. G. Oberlack , A. Depoian , J. Wolf , C. D. Tunnell , A. P. Colijn , H. Landsman , S. Diglio , L. M. Krauss , J. Pienaar , G. Volta , B. Antunovic , A. Manfredini , F. Agostini , M. Schumann , G. Bruno , P. Meinhardt , C. M. B. Monteiro , H. Simgen , M. Steidl , K. Zuber , A. Loya Villalpando , N. Rupp , L. Scotto Lavina , D. Ramírez García , P. A. Breur , A. Terliuk , Y. Biondi , D. Cichon , H. Fischer , J. Cardoso , F. Gao , J. A. M. Lopes , J. P. Zopounidis , M. Pandurovic , D. Baur , L. Althueser , A. Brown , R. Gumbsheimer , S. Lindemann , F. Jörg , D. Vorkapic , M. Clark , M. Lindner , C. Therreau , F. Amaro , S. Hansmann-Menzemer , R. Budnik , E. Masson , E. Aprile , A. Kopec , J. J. Cuenca-García , K. Thieme , R. Trotta , L. Grandi , J. Masbou , M. Murra , R. F. Lang , K. Eitel , C. Weinheimer , R. Peres , T. Marrodán Undagoitia , DARWIN Collaboration , J. Qin , K. Valerius , P. Sanchez-Lucas , A. Di Giovanni , S. E. M. Ahmed Maouloud , L. Baudis , F. Glück , G. Drexlin , A. D. Ferella , G. Khundzakishvili , F. Kuger , A. Molinario , S. Reichard , M. Galloway , D. Schulte , M. Pierre , M. S
2020
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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
by A. Bismark , J. P. Cussonneau , J. Dierle , J. M. F. dos Santos , F. Girard , C. Macolino , D. Thers , C. Capelli , S. Milutinovic , V. Pizzella , U. G. Oberlack , A. Depoian , J. Wolf , C. D. Tunnell , A. P. Colijn , H. Landsman , S. Diglio , L. M. Krauss , J. Pienaar , G. Volta , B. Antunovic , A. Manfredini , F. Agostini , M. Schumann , G. Bruno , P. Meinhardt , C. M. B. Monteiro , H. Simgen , M. Steidl , K. Zuber , A. Loya Villalpando , N. Rupp , L. Scotto Lavina , D. Ramírez García , P. A. Breur , A. Terliuk , Y. Biondi , D. Cichon , H. Fischer , J. Cardoso , F. Gao , J. A. M. Lopes , J. P. Zopounidis , M. Pandurovic , D. Baur , L. Althueser , A. Brown , R. Gumbsheimer , S. Lindemann , F. Jörg , D. Vorkapic , M. Clark , M. Lindner , C. Therreau , F. Amaro , S. Hansmann-Menzemer , R. Budnik , E. Masson , E. Aprile , A. Kopec , J. J. Cuenca-García , K. Thieme , R. Trotta , L. Grandi , J. Masbou , M. Murra , R. F. Lang , K. Eitel , C. Weinheimer , R. Peres , T. Marrodán Undagoitia , DARWIN Collaboration , J. Qin , K. Valerius , P. Sanchez-Lucas , A. Di Giovanni , S. E. M. Ahmed Maouloud , L. Baudis , F. Glück , G. Drexlin , A. D. Ferella , G. Khundzakishvili , F. Kuger , A. Molinario , S. Reichard , M. Galloway , D. Schulte , M. Pierre , M. S
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2020
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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
by A. Bismark , J. P. Cussonneau , J. Dierle , J. M. F. dos Santos , F. Girard , C. Macolino , D. Thers , C. Capelli , S. Milutinovic , V. Pizzella , U. G. Oberlack , A. Depoian , J. Wolf , C. D. Tunnell , A. P. Colijn , H. Landsman , S. Diglio , L. M. Krauss , J. Pienaar , G. Volta , B. Antunovic , A. Manfredini , F. Agostini , M. Schumann , G. Bruno , P. Meinhardt , C. M. B. Monteiro , H. Simgen , M. Steidl , K. Zuber , A. Loya Villalpando , N. Rupp , L. Scotto Lavina , D. Ramírez García , P. A. Breur , A. Terliuk , Y. Biondi , D. Cichon , H. Fischer , J. Cardoso , F. Gao , J. A. M. Lopes , J. P. Zopounidis , M. Pandurovic , D. Baur , L. Althueser , A. Brown , R. Gumbsheimer , S. Lindemann , F. Jörg , D. Vorkapic , M. Clark , M. Lindner , C. Therreau , F. Amaro , S. Hansmann-Menzemer , R. Budnik , E. Masson , E. Aprile , A. Kopec , J. J. Cuenca-García , K. Thieme , R. Trotta , L. Grandi , J. Masbou , M. Murra , R. F. Lang , K. Eitel , C. Weinheimer , R. Peres , T. Marrodán Undagoitia , DARWIN Collaboration , J. Qin , K. Valerius , P. Sanchez-Lucas , A. Di Giovanni , S. E. M. Ahmed Maouloud , L. Baudis , F. Glück , G. Drexlin , A. D. Ferella , G. Khundzakishvili , F. Kuger , A. Molinario , S. Reichard , M. Galloway , D. Schulte , M. Pierre , M. S
2020

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Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe
Journal Article

Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of¹³⁶136 Xe

A. Bismark,
J. P. Cussonneau,
J. Dierle,
J. M. F. dos Santos,
F. Girard,
C. Macolino,
D. Thers,
C. Capelli,
S. Milutinovic,
V. Pizzella,
U. G. Oberlack,
A. Depoian,
J. Wolf,
C. D. Tunnell,
A. P. Colijn,
H. Landsman,
S. Diglio,
L. M. Krauss,
J. Pienaar,
G. Volta,
B. Antunovic,
A. Manfredini,
F. Agostini,
M. Schumann,
G. Bruno,
P. Meinhardt,
C. M. B. Monteiro,
H. Simgen,
M. Steidl,
K. Zuber,
A. Loya Villalpando,
N. Rupp,
L. Scotto Lavina,
D. Ramírez García,
P. A. Breur,
A. Terliuk,
Y. Biondi,
D. Cichon,
H. Fischer,
J. Cardoso,
F. Gao,
J. A. M. Lopes,
J. P. Zopounidis,
M. Pandurovic,
D. Baur,
L. Althueser,
A. Brown,
R. Gumbsheimer,
S. Lindemann,
F. Jörg,
D. Vorkapic,
M. Clark,
M. Lindner,
C. Therreau,
F. Amaro,
S. Hansmann-Menzemer,
R. Budnik,
E. Masson,
E. Aprile,
A. Kopec,
J. J. Cuenca-García,
K. Thieme,
R. Trotta,
L. Grandi,
J. Masbou,
M. Murra,
R. F. Lang,
K. Eitel,
C. Weinheimer,
R. Peres,
T. Marrodán Undagoitia,
DARWIN Collaboration,
J. Qin,
K. Valerius,
P. Sanchez-Lucas,
A. Di Giovanni,
S. E. M. Ahmed Maouloud,
L. Baudis,
F. Glück,
G. Drexlin,
A. D. Ferella,
G. Khundzakishvili,
F. Kuger,
A. Molinario,
S. Reichard,
M. Galloway,
D. Schulte,
M. Pierre,
M. S
2020
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Overview
Abstract The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of¹³⁶136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of¹³⁶136 Xe. Here, we show that its projected half-life sensitivity is2.4× 10²⁷ \\hbox year2.4×1027year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t  ⋅ ·  year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in¹³⁶136 Xe.
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