Physics - High Energy Physics - Experiment Physics - High Energy Physics - Phenomenology Physics - Nuclear Theory
Electron-neutrino charged-current interactions with xenon nuclei were modeled
in the nEXO neutrinoless double-beta decay detector (~5-tonne, 90%
^{136}$Xe, 10% ^{134}$Xe) to evaluate its sensitivity to supernova
neutrinos. Predictions for event rates and detectable signatures were modeled
using the MARLEY event generator. We find good agreement between MARLEY's
predictions and existing theoretical calculations of the inclusive cross
sections at supernova neutrino energies. The interactions modeled by MARLEY
were simulated within the nEXO simulation framework and were run through an
example reconstruction algorithm to determine the detector's efficiency for
reconstructing these events. The simulated data, incorporating the detector
response, were used to study the ability of nEXO to reconstruct the incident
electron-neutrino spectrum and these results were extended to a larger xenon
detector of the same isotope enrichment. We estimate that nEXO will be able to
observe electron-neutrino interactions with xenon from supernovae as far as 5
to 8 kpc from earth, while the ability to reconstruct incident
electron-neutrino spectrum parameters from observed interactions in nEXO is
limited to closer supernovae.
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Details
Title
Supernova Electron-Neutrino Interactions with Xenon in the nEXO Detector
Creators
S Hedges
S. Al Kharusi
E Angelico
J. P Brodsky
G Richardson
S Wilde
A Amy
A Anker
I. J Arnquist
P Arsenault
A Atencio
I Badhrees
J Bane
V Belov
E. P Bernard
T Bhatta
A Bolotnikov
J Breslin
P. A Breur
E Brown
T Brunner
E Caden
G. F Cao
L. Q Cao
D Cesmecioglu
E Chambers
B Chana
S. A Charlebois
D Chernyak
M Chiu
R Collister
M Cvitan
J Dalmasson
T Daniels
L Darroch
R DeVoe
M. L di Vacri
Y. Y Ding
M. J Dolinski
B Eckert
M Elbeltagi
R Elmansali
L Fabris
W Fairbank
J Farine
N Fatemighomi
B Foust
Y. S Fu
D Gallacher
N Gallice
W Gillis
D Goeldi
A Gorham
R Gornea
G Gratta
Y. D Guan
C. A Hardy
M Heffner
E Hein
J. D Holt
E. W Hoppe
A House
W Hunt
A Iverson
P Kachru
A Karelin
D Keblbeck
A Kuchenkov
K. S Kumar
A Larson
M. B Latif
K. G Leach
B. G Lenardo
D. S Leonard
H Lewis
G Li
Z Li
C Licciardi
R Lindsay
R MacLellan
S Majidi
C Malbrunot
P Martel-Dion
J Masbou
K McMichael
M Medina-Peregrina
B Mong
D. C Moore
J Nattress
C. R Natzke
X. E Ngwadla
K Ni
A Nolan
S. C Nowicki
J. C. Nzobadila Ondze
J. L Orrell
G. S Ortega
C. T Overman
L Pagani
H. Peltz Smalley
A Perna
A Piepke
T. Pinto Franco
A Pocar
J. -F Pratte
H Rasiwala
D Ray
K Raymond
S Rescia
V Riot
R Ross
R Saldanha
S Sangiorgio
S Schwartz
S Sekula
J Soderstrom
A. K Soma
F Spadoni
X. L Sun
S Thibado
A Tidball
T Totev
S Triambak
R. H. M Tsang
O. A Tyuka
E van Bruggen
M Vidal
S Viel
M Walent
Q. D Wang
W Wang
Y. G Wang
M Watts
M Wehrfritz
W Wei
L. J Wen
U Wichoski
X. M Wu
H Xu
H. B Yang
L Yang
M Yu
M Yvaine
O Zeldovich
J Zhao
Publication Details
ArXiv.org
Resource Type
Preprint
Language
English
Academic Unit
Physics
Other Identifier
991021881386304721
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