100 research outputs found
Two novel human NUMB isoforms provide a potential link between development and cancer
We previously identified four functionally distinct human NUMB isoforms. Here, we report the identification of two additional isoforms and propose a link between the expression of these isoforms and cancer. These novel isoforms, NUMB5 and NUMB6, lack exon 10 and are expressed in cells known for polarity and migratory behavior, such as human amniotic fluid cells, glioblastoma and metastatic tumor cells. RT-PCR and luciferase assays demonstrate that NUMB5 and NUMB6 are less antagonistic to NOTCH signaling than other NUMB isoforms. Immunocytochemistry analyses show that NUMB5 and NUMB6 interact and complex with CDC42, vimentin and the CDC42 regulator IQGAP1 (IQ (motif) GTPase activating protein 1). Furthermore, the ectopic expression of NUMB5 and NUMB6 induces the formation of lamellipodia (NUMB5) and filopodia (NUMB6) in a CDC42- and RAC1-dependent manner. These results are complemented by in vitro and in vivo studies, demonstrating that NUMB5 and NUMB6 alter the migratory behavior of cells. Together, these novel isoforms may play a role in further understanding the NUMB function in development and cancer
Consensus on guidelines for stereotactic neurosurgery for psychiatric disorders
For patients with psychiatric illnesses remaining refractory to 'standard' therapies, neurosurgical procedures may be considered. Guidelines for safe and ethical conduct of such procedures have previously and independently been proposed by various local and regional expert groups
Measurement of the νe -Nucleus Charged-Current Double-Differential Cross Section at «eν »=2.4 GeV Using NOvA
The inclusive electron neutrino charged-current cross section is measured in the NOvA near detector using 8.02×1020 protons-on-target in the NuMI beam. The sample of GeV electron neutrino interactions is the largest analyzed to date and is limited by ≃17% systematic rather than the ≃7.4% statistical uncertainties. The double-differential cross section in final-state electron energy and angle is presented for the first time, together with the single-differential dependence on Q2 (squared four-momentum transfer) and energy, in the range 1 GeV≤Eν<6 GeV. Detailed comparisons are made to the predictions of the GENIE, GiBUU, NEUT, and NuWro neutrino event generators. The data do not strongly favor a model over the others consistently across all three cross sections measured, though some models have especially good or poor agreement in the single differential cross section vs Q2
Measurement of the double-differential muon-neutrino charged-current inclusive cross section in the NOvA near detector
We report cross-section measurements of the final-state muon kinematics for νμ charged-current interactions in the NOvA near detector using an accumulated 8.09×1020 protons on target in the NuMI beam. We present the results as a double-differential cross section in the observed outgoing muon energy and angle, as well as single-differential cross sections in the derived neutrino energy, Eν, and square of the four-momentum transfer, Q2. We compare the results to inclusive cross-section predictions from various neutrino event generators via χ2 calculations using a covariance matrix that accounts for bin-to-bin correlations of systematic uncertainties. These comparisons show a clear discrepancy between the data and each of the tested predictions at forward muon angle and low Q2, indicating a missing suppression of the cross section in current neutrino-nucleus scattering models
Search for slow magnetic monopoles with the NOvA detector on the surface
We report a search for a magnetic monopole component of the cosmic-ray flux in a 95-day exposure
of the NOvA experiment’s Far Detector, a 14 kt segmented liquid scintillator detector designed primarily to
observe GeV-scale electron neutrinos. No events consistent with monopoles were observed, setting an
upper limit on the flux of 2 × 10−14 cm−2 s−1 sr−1 at 90% C.L. for monopole speed 6 × 10−4 < β <
5 × 10−3 and mass greater than 5 × 108 GeV. Because of NOvA’s small overburden of 3 meters-water
equivalent, this constraint covers a previously unexplored low-mass region
Seasonal Variation of Multiple-Muon Cosmic Ray Air Showers Observed in the NOvA Detector on the Surface
We report the rate of cosmic ray air showers with multiplicities exceeding 15
muon tracks recorded in the NOvA Far Detector between May 2016 and May 2018.
The detector is located on the surface under an overburden of 3.6 meters water
equivalent. We observe a seasonal dependence in the rate of multiple-muon
showers, which varies in magnitude with multiplicity and zenith angle. During
this period, the effective atmospheric temperature and surface pressure ranged
between 210 K to 230 K and 940mbar to 990mbar, respectively; the shower rates
are anti-correlated with the variation in the effective temperature. The
variations are about 30% larger for the highest multiplicities than the lowest
multiplicities and 20% larger for showers near the horizon than vertical
showers
Measurement of the Double-Differential Muon-neutrino Charged-Current Inclusive Cross Section in the NOvA Near Detector
We report cross-section measurements of the final-state muon kinematics for
\numu charged-current interactions in the NOvA near detector using an
accumulated 8.09 protons-on-target (POT) in the NuMI beam. We
present the results as a double-differential cross section in the observed
outgoing muon energy and angle, as well as single-differential cross sections
in the derived neutrino energy, , and square of the four-momentum
transfer, . We compare the results to inclusive cross-section predictions
from various neutrino event generators via calculations using a
covariance matrix that accounts for bin-to-bin correlations of systematic
uncertainties. These comparisons show a clear discrepancy between the data and
each of the tested predictions at forward muon angle and low , indicating
a missing suppression of the cross section in current neutrino-nucleus
scattering models
An Improved Measurement of Neutrino Oscillation Parameters by the NOvA Experiment
We present new , ,
, and
oscillation measurements by
the NOvA experiment, with a 50% increase in neutrino-mode beam exposure over
the previously reported results. The additional data, combined with previously
published neutrino and antineutrino data, are all analyzed using improved
techniques and simulations. A joint fit to the , ,
, and candidate samples within the
3-flavor neutrino oscillation framework continues to yield a best-fit point in
the normal mass ordering and the upper octant of the mixing
angle, with eV and
. The data disfavor combinations of
oscillation parameters that give rise to a large asymmetry in the rates of
and appearance. This includes values of the
CP-violating phase in the vicinity of which are
excluded by for the inverted mass ordering, and values around
in the normal ordering which are disfavored at
2 confidence.Comment: 11 pages, 6 figures. Supplementary material attached (7 figures
Measurement of the Nucleus Charged-Current Double-Differential Cross Section at 2.4 GeV using NOvA
The inclusive electron neutrino charged-current cross section is measured in
the NOvA near detector using protons-on-target (POT) in the
NuMI beam. The sample of GeV electron neutrino interactions is the largest
analyzed to date and is limited by 17\% systematic rather than the
7.4\% statistical uncertainties. The double-differential cross section
in final-state electron energy and angle is presented for the first time,
together with the single-differential dependence on (squared
four-momentum transfer) and energy, in the range 1 GeV 6 GeV.
Detailed comparisons are made to the predictions of the GENIE, GiBUU, NEUT, and
NuWro neutrino event generators. The data do not strongly favor a model over
the others consistently across all three cross sections measured, though some
models have especially good or poor agreement in the single differential cross
section vs.
Extended search for supernova-like neutrinos in NOvA coincident with LIGO/Virgo detections
A search is performed for supernova-like neutrino interactions coincident
with 76 gravitational wave events detected by the LIGO/Virgo Collaboration. For
40 of these events, full readout of the time around the gravitational wave is
available from the NOvA Far Detector. For these events, we set limits on the
fluence of the sum of all neutrino flavors of at 90% C.L. assuming energy and time distributions
corresponding to the Garching supernova models with masses
9.6(27). Under the hypothesis that any given gravitational
wave event was caused by a supernova, this corresponds to a distance of kpc at 90% C.L. Weaker limits are set for other gravitational wave
events with partial Far Detector data and/or Near Detector data.Comment: 10 pages, 2 figure
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