413 research outputs found
The CosmicWatch Desktop Muon Detector: a self-contained, pocket sized particle detector
The CosmicWatch Desktop Muon Detector is a self-contained, hand-held cosmic
ray muon detector that is valuable for astro/particle physics research
applications and outreach. The material cost of each detector is under $100 and
it takes a novice student approximately four hours to build their first
detector. The detectors are powered via a USB connection and the data can
either be recorded directly to a computer or to a microSD card. Arduino- and
Python-based software is provided to operate the detector and an online
application to plot the data in real-time. In this paper, we describe the
various design features, evaluate the performance, and illustrate the detectors
capabilities by providing several example measurements.Comment: 11 pages, 8 figure
The LSND and MiniBooNE Oscillation Searches at High
This paper reviews the results of the LSND and MiniBooNE experiments. The
primary goal of each experiment was to effect sensitive searches for neutrino
oscillations in the mass region with eV. The two
experiments are complementary, and so the comparison of results can bring
additional information with respect to models with sterile neutrinos. Both
experiments obtained evidence for
oscillations, and MiniBooNE also observed a excess.
In this paper, we review the design, analysis, and results from these
experiments. We then consider the results within the global context of sterile
neutrino oscillation models. The final data sets require a more extended model
than the simple single sterile neutrino model imagined at the time that LSND
drew to a close and MiniBooNE began. We show that there are apparent
incompatibilities between data sets in models with two sterile neutrinos.
However, these incompatibilities may be explained with variations within the
systematic error. Overall, models with two (or three) sterile neutrinos seem to
succeed in fitting the global data, and they make interesting predictions for
future experiments.Comment: Posted with permission from the Annual Review of Nuclear and Particle
Science, Volume 63. \c{opyright} 2013 by Annual Reviews,
http://www.annualreviews.or
Sterile Neutrinos: An Introduction to Experiments
This paper is written as one chapter in a collection of essays on neutrino physics for beginning graduate students. The text presents important experimental methods and issues for those interested in searches for sterile neutrinos. Other essays in the collection, written by other authors, will cover introduction to neutrinos in the Standard Model, a description of the theory, and discussion of details of detectors, thus these aspects are not covered here. However, beyond these points, this represents a self-contained tutorial on experimental studies of sterile neutrino oscillations, covering such issues as signals vs. limits, designing experiments, and performing and interpreting global fits to the oscillation data.National Science Foundation (U.S.) (Grant 1505855)National Science Foundation (U.S.) (Grant 1505858)National Science Foundation (U.S.) (Grant 1404209
Exploring a Non-Minimal Sterile Neutrino Model Involving Decay at IceCube and Beyond
We study the phenomenology of neutrino decay together with neutrino
oscillations in the context of eV-scale sterile neutrinos. We review the
formalism of visible neutrino decay in which one of the decay products is a
neutrino that potentially can be observed. We apply the formalism developed for
decay to the recent sterile neutrino search performed by IceCube with TeV
neutrinos. We show that for lifetime , the interpretation of the high-energy IceCube analysis can be
significantly changed.Comment: 12 pages, 7 figures. Find code at:
https://github.com/arguelles/nuSQUIDSDeca
First Constraints on the Complete Neutrino Mixing Matrix with a Sterile Neutrino
Neutrino oscillation models involving one extra mass eigenstate beyond the standard three (3+1) are fit to global short baseline experimental data and the recent IceCube ν[subscript μ] + [bar over v][subscript μ] disappearance search result. We find a best fit of Δm[subscript 41][superscript 2]=1.75  eV[superscript 2] with Δx[subscript null-min][superscript 2]/d.o.f. of 50.61/4. We find that the combined IceCube and short baseline data constrain θ[subscript 34] to <80°(<6°) at 90% C.L. for Δm[subscript 41][superscript 2]≈2(6)  eV[superscript 2], which is improved over present limits. Incorporating the IceCube information provides the first constraints on all entries of the 3+1 mixing matrix.National Science Foundation (U.S.) (Grant 1505858)National Science Foundation (U.S.) (Grant 1505855
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