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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$Xe
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Abstract
We correct an overestimation of the production rate of
$$^{137}$$
137
Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic background source is now at a level similar to the irreducible background from solar
$$^8$$
8
B neutrinos, thus unproblematic at the LNGS depth. The projected half-life sensitivity for the neutrinoless double beta decay (
$$0\nu \beta \beta $$
0
ν
β
β
) of
$$^{136}$$
136
Xe improves by
$$22\%$$
22
%
compared to the previously reported number and is now
$$T^{0\nu }_{1/2}= {3.0\times 10^{27}} \hbox { yr}$$
T
1
/
2
0
ν
=
3.0
×
10
27
yr
(90% C.L.) after 10 years of DARWIN operation.
Springer Science and Business Media LLC
F. Agostini
S. E. M. Ahmed Maouloud
L. Althueser
F. Amaro
B. Antunovic
E. Aprile
L. Baudis
D. Baur
Y. Biondi
A. Bismark
P. A. Breur
A. Brown
G. Bruno
R. Budnik
C. Capelli
J. Cardoso
D. Cichon
M. Clark
A. P. Colijn
J. J. Cuenca-García
J. P. Cussonneau
M. P. Decowski
A. Depoian
J. Dierle
P. Di Gangi
A. Di Giovanni
S. Diglio
J. M. F. dos Santos
G. Drexlin
K. Eitel
R. Engel
A. D. Ferella
H. Fischer
M. Galloway
F. Gao
F. Girard
F. Glück
L. Grandi
R. Größle
R. Gumbsheimer
S. Hansmann-Menzemer
F. Jörg
G. Khundzakishvili
A. Kopec
F. Kuger
L. M. Krauss
H. Landsman
R. F. Lang
S. Lindemann
M. Lindner
J. A. M. Lopes
A. Loya Villalpando
C. Macolino
A. Manfredini
T. Marrodán Undagoitia
J. Masbou
E. Masson
P. Meinhardt
S. Milutinovic
A. Molinario
C. M. B. Monteiro
M. Murra
U. G. Oberlack
M. Pandurovic
R. Peres
J. Pienaar
M. Pierre
V. Pizzella
J. Qin
D. Ramírez García
S. Reichard
N. Rupp
P. Sanchez-Lucas
G. Sartorelli
D. Schulte
M. Schumann
L. Scotto Lavina
M. Selvi
M. Silva
H. Simgen
M. Steidl
A. Terliuk
C. Therreau
D. Thers
K. Thieme
R. Trotta
C. D. Tunnell
K. Valerius
G. Volta
D. Vorkapic
C. Weinheimer
C. Wittweg
J. Wolf
J. P. Zopounidis
K. Zuber
Title: Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$Xe
Description:
Abstract
We correct an overestimation of the production rate of
$$^{137}$$
137
Xe in the DARWIN detector operated at LNGS.
This formerly dominant intrinsic background source is now at a level similar to the irreducible background from solar
$$^8$$
8
B neutrinos, thus unproblematic at the LNGS depth.
The projected half-life sensitivity for the neutrinoless double beta decay (
$$0\nu \beta \beta $$
0
ν
β
β
) of
$$^{136}$$
136
Xe improves by
$$22\%$$
22
%
compared to the previously reported number and is now
$$T^{0\nu }_{1/2}= {3.
0\times 10^{27}} \hbox { yr}$$
T
1
/
2
0
ν
=
3.
0
×
10
27
yr
(90% C.
L.
) after 10 years of DARWIN operation.
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