STEREO experiment

The STEREO experiment (Search for Sterile Reactor Neutrino Oscillations) investigates the possible oscillation of neutrinos from a nuclear reactor into light so-called sterile neutrinos. It is located at the Institut Laue–Langevin (ILL) in Grenoble, France. The experiment started operating and taking data in November 2016.[1]

Detector
Measuring Principle
Figure 2: Comparison of the different spectra at 10 m and 12 m distance to the reactor. The black line shows the case without oscillation into sterile neutrinos while the blue and red show the case including the oscillation into a light sterile neutrino

The STEREO detector is placed at a distance of 10 m away from the research reactor at the ILL. The research reactor has a thermal power of 58 MW. STEREO is supposed to measure the neutrino flux and spectrum near the reactor.[1] To be able to detect the neutrinos radiated from the reactor, the detector is filled up with 1800 litres of organic liquid scintillator which is doped with gadolinium.[2] Inside the scintillator neutrinos are captured via the process of inverse beta decay

\( {\displaystyle {\overline {\nu }}_{e}+p\rightarrow n+e^{+}} \)

In this process a positron is produced. When the positron moves through the scintillator a light signal is produced, which is detected by the 48 photomultiplier tubes (PMTs) placed at the top of the detector cells.[3] The capturing of the neutron which is also produced during the inverse beta decay produces a second coincidence signal.

The expected distance between the oscillation maximum and minimum of light sterile neutrinos is about 2 m. To see the oscillation the detector is divided into 6 separate detector cells, which each measure the energy spectrum of the detected neutrinos. By comparing the measured spectra a possible oscillation could be discovered (see Figure 2).

The STEREO experiment detects \( {\displaystyle \sim 400} \) neutrinos per day.[4]
Detector Shielding

Neutrinos only interact weakly. Therefore, neutrino detectors such as STEREO need to be very sensitive and need a good shielding from additional background signals to be able to detect neutrinos precisely.[1]

To achieve this high sensitivity the 6 inner detector cells are surrounded by a liquid scintillator (without gadolinium) which acts as a "Gamma-Catcher" detecting in- and outgoing gamma radiation. This significantly increases the detection efficiency as well as the energy resolution of the detector. A cherenkov detector filled with water is placed on top of the detector to detect cosmic muons which are produced in the atmosphere and would otherwise act as a large background source. To shield the detector from radioactive sources coming from surrounding experiments it is surrounded and shielded by many layers (65 t) of mostly lead and polyethylene but also iron, steel and \( {\displaystyle {\ce {B_4C}}}. \)
Motivation
Figure 3: The reactor-antineutrino-anomaly (RAA)

Although neutrino oscillation is a phenomenon that is quite well understood today, there are still some experimental observations that question the completeness of our understanding. The most prominent of these observations is the so-called reactor-antineutrino-anomaly (RAA) (see Figure 3). A number of short baseline reactor-neutrino experiments have measured a significantly lower anti-electron-neutrino ( \( {\displaystyle {\overline {\nu }}_{e}}) \) flux compared to the theoretical predictions ( 2 , \( {\displaystyle 2{,}7\sigma } \) deviation).[5] Further experimental anomalies are the unexpected appearance of \( {\displaystyle {\overline {\nu }}_{e}}\) in a short-baseline \( {\displaystyle {\overline {\nu }}_{\mu }} \) -beam (LSND anomaly)[6] as well as the disappearance of \( \nu _{e} \) at short distances during the calibration phase of the GALLEX[7] and SAGE[8] experiments known as the gallium neutrino anomaly.

These anomalies could signify that our understanding of neutrino oscillations is not yet complete and that neutrinos oscillate into another 4th neutrino species. However measurements of the decay width of the Z-Boson at the Large Electron–Positron Collider (LEP) exclude the existence of a light 4th "active" (i.e. interacting via the weak force) neutrino.[9] Hence the oscillation into additional light "sterile" neutrinos is considered as a possible explanation of the observed anomalies. In addition sterile neutrinos appear in many prominent extensions of the Standard Model of particle physics like e.g. in the seesaw type 1 mechanism.
Results (December 2019)
Figure 4: Exclusion contour drawn by the latest STEREO data in the plane of the amplitude of the oscillation towards an hypothetical 4th neutrino (horizontal axis) and the frequency of this oscillation (vertical axis). The blue area shows the expected exclusion coverage at the available statistical precision which would be obtained if all STEREO observables correspond exactly to the expectations without a 4th neutrino. The red area is the actual exclusion contour based on the measured data resulting in statistical fluctuations around the blue limit. All points inside the red contour are excluded with at least 90% confidence level. This result rejects a large part of the domain of existence of the 4th neutrino predicted from the reactor neutrino anomaly (indicated by the black contours).

Initial results were released in 2018 exploiting a dataset of 66 days of reactor turned on.[10] Most of the parameter space that could account for the RAA was excluded at a 90% confidence level. Updated results in December 2019 are based on ∼ 65500 {\displaystyle \sim 65500} {\displaystyle \sim 65500} detected neutrinos (combined phase 1 and 2, 179 days of reactor-on data). Using the current data the region of exclusion is further extended (see figure 4).[11]
External links

Website of the STEREO experiment

References

Allemandou, N.; et al. (2018). "The STEREO experiment". Journal of Instrumentation. 13 (7): P07009.arXiv:1804.09052. Bibcode:2018JInst..13P7009A. doi:10.1088/1748-0221/13/07/P07009.
Buck, C.; Gramlich, B.; Lindner, M.; Roca, C.; Schoppmann, S. (2019). "Production and properties of the liquid scintillators used in the STEREO reactor neutrino experiment". Journal of Instrumentation. 14 (1): P01027.arXiv:1812.02998. Bibcode:2019JInst..14P1027B. doi:10.1088/1748-0221/14/01/P01027.
Bourrion, O.; et al. (2016). "Trigger and readout electronics for the STEREO experiment". Journal of Instrumentation. 11 (2): C02078.arXiv:1510.08238. doi:10.1088/1748-0221/11/02/c02078.
Bernard, Laura (2019). "Results from the STEREO Experiment with 119 days of Reactor-on Data".arXiv:1905.11896 [hep-ex].
Mention, G.; Fechner, M.; Lasserre, Th.; Mueller, Th. A.; Lhuillier, D.; Cribier, M.; Letourneau, A. (2011). "Reactor antineutrino anomaly". Physical Review D. 83 (7): 073006.arXiv:1101.2755. Bibcode:2011PhRvD..83g3006M. doi:10.1103/PhysRevD.83.073006.
Aguilar, A.; et al. (2001). "Evidence for neutrino oscillations from the observation of νe appearance in a νμ beam". Physical Review D. 64 (11): 112007.arXiv:hep-ex/0104049. doi:10.1103/PhysRevD.64.112007.
Giunti, Carlo; Laveder, Marco (2011). "Statistical significance of the gallium anomaly". Physical Review C. 83 (6): 065504.arXiv:1006.3244. Bibcode:2011PhRvC..83f5504G. doi:10.1103/PhysRevC.83.065504.
Abdurashitov, J. N.; et al. (2006). "Measurement of the response of a Ga solar neutrino experiment to neutrinos from a 37Ar source". Physical Review C. 73 (4): 045805.arXiv:nucl-ex/0512041. Bibcode:2006PhRvC..73d5805A. doi:10.1103/PhysRevC.73.045805.
Allemandou, N.; et al. (2006). "Precision electroweak measurements on the Z resonance". Physics Reports. 427 (5–6): 257–454.arXiv:hep-ex/0509008. Bibcode:2006PhR...427..257A. doi:10.1016/j.physrep.2005.12.006.
Almazán, Helena; et al. (2018). "Sterile neutrino constraints from the STEREO experiment with 66 days of reactor-on data".arXiv:1806.02096 [hep-ex].

Almazán, Helena; et al. (2018). "Improved sterile neutrino constraints from the STEREO experiment with 179 days of reactor-on data".arXiv:1912.06582 [hep-ex].

vte

Neutrino detectors, experiments, and facilities
Discoveries

Cowan–Reines ( ν e) Lederman–Schwartz–Steinberger ( ν μ) DONUT ( ν τ) Neutrino oscillation SN 1987 neutrino burst

Operating
(divided by
primary
neutrino
source)
Astronomical

ANITA ANTARES ASD BDUNT Borexino BUST HALO IceCube LVD NEVOD SAGE Super-Kamiokande SNEWS

Reactor

Daya Bay Double Chooz KamLAND RENO STEREO

Accelerator

ANNIE ICARUS (Fermilab) MicroBooNE MINERνA MiniBooNE NA61/SHINE NOνA NuMI T2K

0νββ

AMoRE COBRA CUORE EXO GERDA KamLAND-Zen MAJORANA NEXT PandaX SNO+ XMASS

Other

KATRIN WITCH

Construction

ARA ARIANNA Baikal-GVD BEST DUNE Hyper-Kamiokande JUNO KM3NeT SuperNEMO FASERν

Retired

AMANDA CDHS Chooz CNGS Cuoricino DONUT ERPM GALLEX Gargamelle GNO Heidelberg-Moscow Homestake ICARUS IGEX IMB K2K Kamiokande KARMEN KGF LSND MACRO MINOS MINOS+ NARC NEMO OPERA RICE SciBooNE SNO Soudan 2 Utah

Proposed

CUPID GRAND INO LAGUNA LEGEND LENA Neutrino Factory nEXO Nucifer SBND UNO JEM-EUSO WATCHMAN

Cancelled

DUMAND Project Long Baseline Neutrino Experiment NEMO Project NESTOR Project SOX BOREX