Solar neutrino detection sensitivity in DARWIN via electron scattering

Publikationstyp:

Zeitschriftenaufsatz

Metadaten:

Autoren

J Aalbers
F Agostini
SEM Ahmed Maouloud
M Alfonsi
L Althueser
FD Amaro
J Angevaare
VC Antochi
B Antunovic
E Aprile
L Arazi
F Arneodo
M Balzer
L Baudis
D Baur
ML Benabderrahmane
Y Biondi
A Bismark
C Bourgeois
A Breskin
PA Breur
A Brown
E Brown
S Bruenner
G Bruno
R Budnik
C Capelli
J Cardoso
D Cichon
M Clark
AP Colijn
J Conrad
JJ Cuenca-Garcia
JP Cussonneau
MP Decowski
A Depoian
J Dierle
P Di Gangi
A Di Giovanni
S Diglio
D Douillet
G Drexlin
K Eitel
R Engel
E Erdal
AD Ferella
H Fischer
P Fischer
W Fulgione
P Gaemers
M Galloway
F Gao
D Giovagnoli
F Girard
R Glade-Beucke
F Glueck
L Grandi
S Grohmann
R Groessle
R Gumbsheimer
V Hannen
S Hansmann-Menzemer
C Hils
B Holzapfel
J Howlett
G Iaquaniello
F Joerg
M Keller
J Kellerer
G Khundzakishvili
B Kilminster
M Kleifges
TK Kleiner
G Koltmann
A Kopec
A Kopmann
LM Krauss
F Kuger
L LaCascio
H Landsman
RF Lang
S Lindemann
M Lindner
F Lombardi
JAM Lopes
A Loya Villalpando
Y Ma
C Macolino
J Mahlstedt
A Manfredini
T Marrodan Undagoitia
J Masbou
D Masson
E Masson
N McFadden
P Meinhardt
R Meyer
B Milosevic
S Milutinovic
A Molinario
CMB Monteiro
K Mora
E Morteau
Y Mosbacher
M Murra
JL Newstead
K Ni
UG Oberlack
M Obradovic
K Odgers
I Ostrovskiy
J Palacio
M Pandurovic
B Pelssers
R Peres
J Pienaar
M Pierre
V Pizzella
G Plante
J Qi
J Qin
D Ramirez Garcia
SE Reichard
N Rupp
P Sanchez-Lucas
JMF dos Santos
G Sartorelli
D Schulte
HC Schultz-Coulon
H Schulze Eissing
M Schumann
L Scotto Lavina
M Selvi
P Shagin
S Sharma
W Shen
M Silva
H Simgen
M Steidl
S Stern
D Subotic
P Szabo
A Terliuk
C Therreau
D Thers
K Thieme
F Toennies
R Trotta
CD Tunnell
K Valerius
G Volta
D Vorkapic
M Weber
Y Wei
C Weinheimer
M Weiss
D Wenz
C Wittweg
J Wolf
S Wuestling
M Wurm
Y Xing
T Zhu
Y Zhu
JP Zopounidis
K Zuber

Autoren-URL

https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=fis-test-1&SrcAuth=WosAPI&KeyUT=WOS:000598416900002&DestLinkType=FullRecord&DestApp=WOS_CPL

DOI

10.1140/epjc/s10052-020-08602-7

eISSN

1434-6052

Externe Identifier

Clarivate Analytics Document Solution ID: PE5PG

ISSN

1434-6044

Ausgabe der Veröffentlichung

Zeitschrift

EUROPEAN PHYSICAL JOURNAL C

Artikelnummer

ARTN 1133

Datum der Veröffentlichung

2020

Status

Published

Titel

Solar neutrino detection sensitivity in DARWIN via electron scattering

Sub types

Article

Ausgabe der Zeitschrift

Datenquelle: Web of Science (Lite)

Andere Metadatenquellen:

Abstract

AbstractWe detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, $$^7$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>7</mml:mn> </mml:msup> </mml:math>Be, $$^{13}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>13</mml:mn> </mml:msup> </mml:math>N, $$^{15}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>15</mml:mn> </mml:msup> </mml:math>O and pep. The precision of the $$^{13}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>13</mml:mn> </mml:msup> </mml:math>N, $$^{15}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>15</mml:mn> </mml:msup> </mml:math>O and pep components is hindered by the double-beta decay of $$^{136}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>136</mml:mn> </mml:msup> </mml:math>Xe and, thus, would benefit from a depleted target. A high-statistics observation of pp neutrinos would allow us to infer the values of the electroweak mixing angle, $$\sin ^2\theta _w$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:msup> <mml:mo>sin</mml:mo> <mml:mn>2</mml:mn> </mml:msup> <mml:msub> <mml:mi>θ</mml:mi> <mml:mi>w</mml:mi> </mml:msub> </mml:mrow> </mml:math>, and the electron-type neutrino survival probability, $$P_{ee}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>P</mml:mi> <mml:mrow> <mml:mi>ee</mml:mi> </mml:mrow> </mml:msub> </mml:math>, in the electron recoil energy region from a few keV up to 200 keV for the first time, with relative precision of 5% and 4%, respectively, with 10 live years of data and a 30 tonne fiducial volume. An observation of pp and $$^7$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>7</mml:mn> </mml:msup> </mml:math>Be neutrinos would constrain the neutrino-inferred solar luminosity down to 0.2%. A combination of all flux measurements would distinguish between the high- (GS98) and low-metallicity (AGS09) solar models with 2.1–2.5$$\sigma $$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>σ</mml:mi> </mml:math> significance, independent of external measurements from other experiments or a measurement of $$^8$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>8</mml:mn> </mml:msup> </mml:math>B neutrinos through coherent elastic neutrino-nucleus scattering in DARWIN. Finally, we demonstrate that with a depleted target DARWIN may be sensitive to the neutrino capture process of $$^{131}$$<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msup> <mml:mrow /> <mml:mn>131</mml:mn> </mml:msup> </mml:math>Xe.

Autoren

J Aalbers
F Agostini
SEM Ahmed Maouloud
M Alfonsi
L Althueser
FD Amaro
J Angevaare
VC Antochi
B Antunovic
E Aprile
L Arazi
F Arneodo
M Balzer
L Baudis
D Baur
ML Benabderrahmane
Y Biondi
A Bismark
C Bourgeois
A Breskin
PA Breur
A Brown
E Brown
S Brünner
G Bruno
R Budnik
C Capelli
J Cardoso
D Cichon
M Clark
AP Colijn
J Conrad
JJ Cuenca-García
JP Cussonneau
MP Decowski
A Depoian
J Dierle
P Di Gangi
A Di Giovanni
S Diglio
D Douillet
G Drexlin
K Eitel
R Engel
E Erdal
AD Ferella
H Fischer
P Fischer
W Fulgione
P Gaemers
M Galloway
F Gao
D Giovagnoli
F Girard
R Glade-Beucke
F Glück
L Grandi
S Grohmann
R Größle
R Gumbsheimer
V Hannen
S Hansmann-Menzemer
C Hils
B Holzapfel
J Howlett
G Iaquaniello
F Jörg
M Keller
J Kellerer
G Khundzakishvili
B Kilminster
M Kleifges
TK Kleiner
G Koltmann
A Kopec
A Kopmann
LM Krauss
F Kuger
L LaCascio
H Landsman
RF Lang
S Lindemann
M Lindner
F Lombardi
JAM Lopes
A Loya Villalpando
Y Ma
C Macolino
J Mahlstedt
A Manfredini
T Marrodán Undagoitia
J Masbou
D Masson
E Masson
N McFadden
P Meinhardt
R Meyer
B Milosevic
S Milutinovic
A Molinario
CMB Monteiro
K Morå
E Morteau
Y Mosbacher
M Murra
JL Newstead
K Ni
UG Oberlack
M Obradovic
K Odgers
I Ostrovskiy
J Palacio
M Pandurovic
B Pelssers
R Peres
J Pienaar
M Pierre
V Pizzella
G Plante
J Qi
J Qin
D Ramírez García
SE Reichard
N Rupp
P Sanchez-Lucas
JMF dos Santos
G Sartorelli
D Schulte
HC Schultz-Coulon
H Schulze Eißing
M Schumann
L Scotto Lavina
M Selvi
P Shagin
S Sharma
W Shen
M Silva
H Simgen
M Steidl
S Stern
D Subotic
P Szabo
A Terliuk
C Therreau
D Thers
K Thieme
F Toennies
R Trotta
CD Tunnell
K Valerius
G Volta
D Vorkapic
M Weber
Y Wei
C Weinheimer
M Weiss
D Wenz
C Wittweg
J Wolf
S Wuestling
M Wurm
Y Xing
T Zhu
Y Zhu
JP Zopounidis
K Zuber

DOI

10.1140/epjc/s10052-020-08602-7

eISSN

1434-6052

ISSN

1434-6044

Ausgabe der Veröffentlichung

Zeitschrift

The European Physical Journal C

Sprache

Artikelnummer

1133

Online publication date

2020

Datum der Veröffentlichung

2020

Status

Published

Herausgeber

Springer Science and Business Media LLC

Herausgeber URL

http://dx.doi.org/10.1140/epjc/s10052-020-08602-7

Datum der Datenerfassung

2021

Titel

Solar neutrino detection sensitivity in DARWIN via electron scattering

Ausgabe der Zeitschrift

Datenquelle: Crossref

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Solar neutrino detection sensitivity in DARWIN via electron scattering

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