Neutrino directionality measurement with Double Chooz
-- Romain Roncin, on behalf of the Double Chooz Collaboration -- -- Applied Anti-neutrino Physics 2013 @ Seoul -- -- 02/11/2013 -- -- Outline --
-- Final aim of our work
-- Evaluate resolution on anti-νe point-like source reconstruction
-- Plan of this talk
-- Motivations of this work
-- Reminder on the Double Chooz experiment
-- Neutrino directionality with neutron capture on Gd
-- Only one reactor on (NEW!)
-- Neutrino directionality with neutron capture on H (NEW!)
Romain Roncin @ AAP 2013 2 -- Motivations of this work --
-- Improving neutrino directionality measurement can lead to a very powerful tool when looking at particular sources such as a core-collapse supernovae, when searching for geo-neutrinos or for nuclear reactor monitoring Core-collapse supernovae
Nuclear reactors Detector
Geo-neutrinos
Romain Roncin @ AAP 2013 3 -- Detecting anti-νe --
-- Anti-νe detection through the inverse beta decay interactions
Prompt signal (positron): + + ⌫¯e + p e + n - e scintillation + annihilation e E ≈ E – T – 0.8 MeV ! e+ prompt ν n
e+
νe p
n n Gd/H
Delayed signal (neutron):
n capture on Gd OR n capture on H E ≈ 8 MeV E ≈ 2.2 MeV delayed delayed Δt ≈ 30 μs Δt ≈ 200 μs
-- Use of liquid scintillator doped with Gd to accelerate the neutron capture but neutron capture on H is alsoRomain possible Roncin @ AAP 2013 4 -- Angular distribution --
-- From P. Vogel and J.F. Beacom (Phys. Rev. D 60, 053003 (1999))
( ) e- Prompt signal positron : + We assume the positron interaction vertex to e be the neutrino interaction vertex
e+
νe p initial n direction
n n θn Gd/H Delayed signal (neutron): ν direction « the neutron must always be emitted in the forward hemisphere »
2 2 2E⌫ ( me) cos(✓n)max = p E⌫ Romain Roncin @ AAP 2013 5 -- Motivations of this work --
-- Studies in literature focused on scintillators doped with high neutron capture cross-section elements (such as Gd), which should minimize neutron diffusion
HOWEVER
-- Directionality studies using neutron capture on H is possible and is potentially very interesting for future large-scale neutrino detectors, such as LENA, JUNO or RENO-50 which will use undoped scintillators
-- H analysis permits also to cross-check the method and the results from Gd analysis
VS
Romain Roncin @ AAP 2013 6 -- The Double Chooz Collaboration --
Brazil France Germany Japan Russia Spain USA
CBPF APC EKU Tübingen Tohoku U. INR RAS CIEMAT-Madrid U. Alabama UNICAMP CEA/DSM/ MPIK Tokyo Inst. Tech. IPC RAS ANL UFABC IRFU : Heidelberg Tokyo Metro. U. RRC Kurchatov U. Chicago SPP RWTH Aachen Niigata U. Columbia U. SPhN TU München Kobe U. UC Davis SEDI U. Hamburg Tohoku Gakuin U. Drexel U. SIS Hiroshima Inst. IIT SENAC Tech. KSU CNRS/ LLNL IN2P3: MIT Subatech U. Notre Dame IPHC U. Tennessee
Spokesperson : H. de Kerret (IN2P3)
Project Manager : Ch. Veyssière (CEA-Saclay)
Web Site : www.doublechooz.org/
Romain Roncin @ AAP 2013 7 -- The Double Chooz far detector --
-- Outer Veto -- 82 m2 of 400 mm thick plastic scintillator strips
-- Inner Veto -- 90 m3 liquid scintillator in a 8 mm steel vessel, seen by 78 10’’ PMTs
-- Buffer Volume -- 110 m3 mineral oil in a 3 mm stain- less steel vessel, seen by 390 10’’ PMTs
-- Gamma-Catcher -- 22.3 m3 liquid scintillator in a 12 mm thick acrylic vessel
-- Neutrino Target -- 10.3 m3 Gd-doped liquid scintillator in a 8 mm thick acrylic vessel Romain Roncin @ AAP 2013 8 -- The Double Chooz experimental site --
Vincent Durand @ Blois 2012
Romain Roncin @ AAP 2013 9 -- The Double Chooz layout --
Nuclear reactors
B1 B2
x -- The Double Chooz far detector y is 1 km away from the two nuclear reactors of the Chooz power plant ϕtrue ≈ 84° -- From the x-axis of the detector frame, the reactors are located at around 84° Double Chooz far detector
Romain Roncin @ AAP 2013 10 -- Direction reconstruction method --
-- Each neutrino candidate is then composed of two signals: -- a prompt signal (Xprompt) prompt -- a delayed signal (Xdelayed)
-- From these two vectors we can build the signal vector: XSignal = Xprompt – Xdelayed
-- We also need to build the unit signal vector: y XSignal = XSignal / |XSignal| delayed
-- The average neutrino wind p is then prompt defined as the average of vectors Xsignal: XSignal delayed x N 1 i p~ = Xˆ N Signal i=1 X
Romain Roncin @ AAP 2013 11 -- Direction reconstruction method --
-- From p we can finally deduce ϕ (azimuthal angle) and θ (zenithal angle):
py = Arctan p p ✓ x ◆ py p ϕ ✓ = Arctan z
0 p2 + p2 1 px x y @q A -- In this analysis, we used the way Chooz did to compute the uncertainty on the measured angles (Phys. Rev. D 61, 012001 (1999))
δ
p~ B1 B2
« An uncertainty on the measurement of the neutrino direction can be given as the cone around p which contains 68 % of the integral of the p distribution. »
Romain Roncin @ AAP 2013 12 -- The Double Chooz data analysis --
-- This analysis uses data collected from April 13, 2011 to March 15, 2012 for a total live time of 227.9 days for the Gd analysis and 240.1 days for the H analysis
-- We have selected:
-- 8246 anti-νe interactions followed by neutron capture on Gd -- 7498 anti-νe interactions followed by neutron capture on H
-- We present the directionality measurement with these samples in comparison with the corresponding Monte Carlo simulations (MC)
VS
Romain Roncin @ AAP 2013 13 -- Gd neutrino candidates selection --
-- Prompt signal: -- 0.7 < E < 12.2 MeV prompt 14 -- Light noise cuts 102
-- Delayed signal: 12 delayed E (MeV) -- 6.0 < Edelayed < 12.0 MeV
-- Light noise cuts 10 10 -- 2 < ΔT < 100 μs -- Muon cuts 8 -- Rejection of any signal detected in the OV 6 1 -- No additional triggers from 100 μs 4 preceding the prompt signal to 400 μs 2 4 6 8 10 12 14 after it prompt E (MeV)
Phys. Rev. D 86, 052008 (2012)
Romain Roncin @ AAP 2013 14 -- Directionality with Gd neutrino candidates --
-- Distributions of the XSignal components when taking N=8246 neutrino candidates 280 280 #Entries = 8246 #Entries = 8246 260 260
#Entries µ = 0.0055 ± 0.0064 #Entries µ = 0.0585 ± 0.0063 σ = 0.5828 σ = 0.5733 240 240
220 220 200 200 180 180
160 Double Chooz 160 Double Chooz Preliminary Preliminary 140 140 -1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1 -1 -0.8 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 0.8 1 p (normalised) p (normalised) Nx y 1 ˆ i -- By defining p~ = XSignal we can then calculate the average neutrino wind N i=1 -- p = (0.0055, 0.0585, X-0.0049)