184 citations · 815 across the 21 of their papers we have counts for
21 papers
The Eos detector: a demonstrator of hybrid optical detection technology
Eos Collaboration, S. Arora, M. Askins +64
Eos is an R&D testbed for hybrid detector technologies, featuring state-of-the-art sub-ns photosensors, the first implementation of dichroicons in a large-scale demonstrator, and t…
Performance of the Eos detector with water
Eos Collaboration, S. Arora, M. Askins +64
In this manuscript we present the first results from Eos, a four tonne optical detector located at the University of California, Berkeley. The primary goal of Eos is to demonstrate…
Search for solar neutrinos and the diffuse supernova neutrino background using all three phases of the Sudbury Neutrino Observatory
B. Aharmim, S. N. Ahmed, A. E. Anthony +129
A search has been performed for neutrinos from two sources, the reaction in the solar fusion chain and the component of the diffuse supernova neutrino background (…
Cosmogenic Neutron Production at the Sudbury Neutrino Observatory
B. Aharmim, S. N. Ahmed, A. E. Anthony +128
Neutrons produced in nuclear interactions initiated by cosmic-ray muons present an irreducible background to many rare-event searches, even in detectors located deep underground. M…
Measurement of neutron production in atmospheric neutrino interactions at the Sudbury Neutrino Observatory
SNO Collaboration, B. Aharmim, S. N. Ahmed +129
Neutron production in GeV-scale neutrino interactions is a poorly studied process. We have measured the neutron multiplicities in atmospheric neutrino interactions in the Sudbury N…
Constraints on Neutrino Lifetime from the Sudbury Neutrino Observatory
SNO Collaboration, B. Aharmim, S. N. Ahmed +128
The long baseline between the Earth and the Sun makes solar neutrinos an excellent test beam for exploring possible neutrino decay. The signature of such decay would be an energy-d…
Tests of Lorentz invariance at the Sudbury Neutrino Observatory
SNO Collaboration, B. Aharmim, S. N. Ahmed +131
Experimental tests of Lorentz symmetry in systems of all types are critical for ensuring that the basic assumptions of physics are well-founded. Data from all phases of the Sudbury…
Search for Zero-Neutrino Double Beta Decay in 76Ge with the Majorana Demonstrator
C. E. Aalseth, N. Abgrall, E. Aguayo +126
The \MJ\ Collaboration is operating an array of high purity Ge detectors to search for neutrinoless double-beta decay in Ge. The \MJ\ \DEM\ comprises 44.1~kg of Ge detectors…
The search for neutron-antineutron oscillations at the Sudbury Neutrino Observatory
SNO Collaboration, B. Aharmim, S. N. Ahmed +122
Tests on symmetry breaking models are important probes to search for new physics. One proposed model with involves the oscillations of a neutron to an antineutron.…
Single electron detection and spectroscopy via relativistic cyclotron radiation
D. M. Asner, R. F. Bradley, L. de Viveiros +24
It has been understood since 1897 that accelerating charges must emit electromagnetic radiation. Cyclotron radiation, the particular form of radiation emitted by an electron orbiti…
The MAJORANA DEMONSTRATOR: A Search for Neutrinoless Double-beta Decay of Germanium-76
MAJORANA Collaboration, S. R. Elliott, N. Abgrall +80
The {\sc Majorana} collaboration is searching for neutrinoless double beta decay using Ge, which has been shown to have a number of advantages in terms of sensitivities and…
The MAJORANA Experiment
The MAJORANA Collaboration
The MAJORANA collaboration is actively pursuing research and development aimed at a tonne-scale 76Ge neutrinoless double-beta decay) experiment. The current, primary focus is the c…
The MAJORANA DEMONSTRATOR: A Search for Neutrinoless Double-beta Decay of Germanium-76
MAJORANA Collaboration, A. G. Schubert, E. Aguayo +90
The observation of neutrinoless double-beta decay would determine whether the neutrino is a Majorana particle and provide information on the absolute scale of neutrino mass. The MA…
A Monte Carlo simulation of the Sudbury Neutrino Observatory proportional counters
B. Beltran, H. Bichsel, B. Cai +28
The third phase of the Sudbury Neutrino Observatory (SNO) experiment added an array of 3He proportional counters to the detector. The purpose of this Neutral Current Detection (NCD…
The Majorana Experiment
V. E. Guiseppe
The Majorana Collaboration is assembling an array of HPGe detectors to search for neutrinoless double-beta decay in Ge-76. Initially, Majorana aims to construct a prototype module…
Astroparticle Physics with a Customized Low-Background Broad Energy Germanium Detector
MAJORANA Collaboration, C. E. Aalseth, M. Amman +100
The MAJORANA Collaboration is building the MAJORANA DEMONSTRATOR, a 60 kg array of high purity germanium detectors housed in an ultra-low background shield at the Sanford Undergrou…
TThe {\sc Majorana} Project
The MAJORANA collaboration
The {\sc Majorana} Project, a neutrinoless double-beta decay experiment is described with an emphasis on the choice of Ge-detector configuration.
Searches for High Frequency Variations in the B Solar Neutrino Flux at the Sudbury Neutrino Observatory
SNO Collaboration
We have performed three searches for high-frequency signals in the solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO), motivated by the possibility that solar $…
The MAJORANA DEMONSTRATOR: An R&D project towards a tonne-scale germanium neutrinoless double-beta decay search
Reyco Henning
The MAJORANA collaboration is pursuing the development of the so-called MAJORANA DEMONSTRATOR. The DEMONSTRATOR is intended to perform research and development towards a tonne-scal…
Measurement of the Cosmic Ray and Neutrino-Induced Muon Flux at the Sudbury Neutrino Observatory
SNO Collaboration
Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbur…
Measurement of the and Total B Solar Neutrino Fluxes with the Sudbury Neutrino Observatory Phase I Data Set
SNO Collaboration
This article provides the complete description of results from the Phase I data set of the Sudbury Neutrino Observatory (SNO). The Phase I data set is based on a 0.65 kt-year expos…