REVIEW 3 cited by
The ANTARES detector: two decades of neutrino searches in the Mediterranean Sea
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
Interest for studying cosmic neutrinos using deep-sea detectors has increase after the discovery of a diffuse flux of cosmic neutrinos by the IceCube collaboration and the possibility of wider multi-messenger studies with the observations of gravitational waves. The ANTARES detector was the first neutrino telescope in seawater, operating successfully in the Mediterranean Sea for more than a decade and a half. All challenges related to the operation in the deep sea were accurately addressed by the collaboration. Deployment and connection operations became smoother over time; data taking and constant re-calibration of the detector due to the variable environmental conditions were fully automated. A wealth of results on the subject of astroparticle physics, particle physics and multi-messenger astronomy have been obtained, despite the relative modest size of the detector, paving the way to a new generation of larger undersea detectors. This review summarizes the efforts by the ANTARES collaboration that made the possibility to operate neutrino telescopes in seawater a reality and the results obtained in this endeavor.
Forward citations
Cited by 3 Pith papers
-
The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter
ANTARES Galactic Ridge upper limits yield competitive dark-matter annihilation/decay bounds, the first neutrino-based branon constraints, and a negative KM3NeT forecast for the thermal relic cross-section.
-
A Cost Effective Optimization of the hybrid-DOM Design for TRIDENT
Simulations show the 19-PMT, 4-inch hDOM for TRIDENT can match or exceed the 31-PMT, 3-inch design on neutrino efficiency and reconstruction, provided the 4-inch PMTs achieve comparable quantum efficiency and timing.
-
Probing Dark Matter and Phantom Field Effects on Neutrino Oscillations around Black Holes
For neutrinos deflected by a black hole embedded in phantom-field dark matter, the oscillation phase gains a logarithmic dark matter correction, while radially moving neutrinos see no net gravity effect.
Discussion (0). Continue with ORCID to comment.