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Constraining uncertainty in aerosol direct forcing
The uncertainty in present-day anthropogenic forcing is dominated by uncertainty in the strength of the contribution from aerosol. Much of the uncertainty in the direct aerosol forcing can be attributed to uncertainty in the anthropogenic fraction of aerosol in the present-day atmosphere, due to a lack of historical observations. Here we present a robust relationship between total present-day aerosol optical depth and the anthropogenic contribution across three multi-model ensembles and a large single-model perturbed parameter ensemble. Using observations of aerosol optical depth, we determine a reduced likely range of the anthropogenic component and hence a reduced uncertainty in the direct forcing of aerosol
Development Toward a Ground-Based Interferometric Phased Array for Radio Detection of High Energy Neutrinos
The in-ice radio interferometric phased array technique for detection of high
energy neutrinos looks for Askaryan emission from neutrinos interacting in
large volumes of glacial ice, and is being developed as a way to achieve a low
energy threshold and a large effective volume at high energies. The technique
is based on coherently summing the impulsive Askaryan signal from multiple
antennas, which increases the signal-to-noise ratio for weak signals. We report
here on measurements and a simulation of thermal noise correlations between
nearby antennas, beamforming of impulsive signals, and a measurement of the
expected improvement in trigger efficiency through the phased array technique.
We also discuss the noise environment observed with an analog phased array at
Summit Station, Greenland, a possible site for an interferometric phased array
for radio detection of high energy neutrinos.Comment: 13 Pages, 14 Figure
Measurements and Modeling of Near-Surface Radio Propagation in Glacial Ice and Implications for Neutrino Experiments
We present measurements of radio transmission in the 100 MHz range
through a m deep region below the surface of the ice at Summit
Station, Greenland, called the firn. In the firn, the index of refraction
changes due to the transition from snow at the surface to glacial ice below,
affecting the propagation of radio signals in that region. We compare our
observations to a finite-difference time-domain (FDTD) electromagnetic wave
simulation, which supports the existence of three classes of propagation: a
bulk propagation ray-bending mode that leads to so-called "shadowed" regions
for certain geometries of transmission, a surface-wave mode induced by the
ice/air interface, and an arbitrary-depth horizontal propagation mode that
requires perturbations from a smooth density gradient. In the non-shadowed
region, our measurements are consistent with the bulk propagation ray-bending
mode both in timing and in amplitude. We also observe signals in the shadowed
region, in conflict with a bulk-propagation-only ray-bending model, but
consistent with FDTD simulations using a variety of firn models for Summit
Station. The amplitude and timing of our measurements in all geometries are
consistent with the predictions from FDTD simulations. In the shadowed region,
the amplitude of the observed signals is consistent with a best-fit coupling
fraction value of % (0.06% in power) or less to a surface or horizontal
propagation mode from the bulk propagation mode. The relative amplitude of
observable signals in the two regions is important for experiments that aim to
detect radio emission from astrophysical high-energy neutrinos interacting in
glacial ice, which rely on a radio propagation model to inform simulations and
perform event reconstruction.Comment: 14 pages, 13 figures, version accepted to PR
Background Rejection in the DMTPC Dark Matter Search Using Charge Signals
The Dark Matter Time Projection Chamber (DMTPC) collaboration is developing
low-pressure gas TPC detectors for measuring WIMP-nucleon interactions. Optical
readout with CCD cameras allows for the detection for the daily modulation in
the direction of the dark matter wind, while several charge readout channels
allow for the measurement of additional recoil properties. In this article, we
show that the addition of the charge readout analysis to the CCD allows us too
obtain a statistics-limited 90% C.L. upper limit on the rejection factor
of for recoils with energies between 40 and 200
keV. In addition, requiring coincidence between charge signals
and light in the CCD reduces CCD-specific backgrounds by more than two orders
of magnitude.Comment: 8 pages, 6 figures. For proceedings of DPF 2011 conferenc
First Dark Matter Search Results from a Surface Run of the 10-L DMTPC Directional Dark Matter Detector
The Dark Matter Time Projection Chamber (DMTPC) is a low pressure (75 Torr
CF4) 10 liter detector capable of measuring the vector direction of nuclear
recoils with the goal of directional dark matter detection. In this paper we
present the first dark matter limit from DMTPC. In an analysis window of 80-200
keV recoil energy, based on a 35.7 g-day exposure, we set a 90% C.L. upper
limit on the spin-dependent WIMP-proton cross section of 2.0 x 10^{-33} cm^{2}
for 115 GeV/c^2 dark matter particle mass.Comment: accepted for publication in Physics Letters
Measurement of the directional sensitivity of Dark Matter Time Projection Chamber detectors
The Dark Matter Time Projection Chamber (DMTPC) is a direction-sensitive
detector designed to measure the direction of recoiling F and C
nuclei in low-pressure CF gas using optical and charge readout systems. In
this paper, we employ measurements from two DMTPC detectors, with operating
pressures of 30-60 torr, to develop and validate a model of the directional
response and performance of such detectors as a function of recoil energy.
Using our model as a benchmark, we formulate the necessary specifications for a
scalable directional detector with sensitivity comparable to that of
current-generation counting (non-directional) experiments, which measure only
recoil energy. Assuming the performance of existing DMTPC detectors, as well as
current limits on the spin-dependent WIMP-nucleus cross section, we find that a
10-20 kg scale direction-sensitive detector is capable of correlating the
measured direction of nuclear recoils with the predicted direction of incident
dark matter particles and providing decisive (3) confirmation that a
candidate signal from a non-directional experiment was indeed induced by
elastic scattering of dark matter particles off of target nuclei.Comment: 13 pages, 10 figures. Accepted for publication in Phys. Rev. D. Added
color figures, switched to more compact layout, and fixed some reference
KMS states and conformal measures
From a non-constant holomorphic map on a connected Riemann surface we
construct an 'etale second countable locally compact Hausdorff groupoid whose
associated groupoid C*-algebra admits a one-parameter group of automorphisms
with the property that its KMS states corresponds to conformal measures in the
sense of Sullivan. In this way certain quadratic polynomials give rise to
quantum statistical models with a phase transition arising from spontaneous
symmetry breaking.Comment: The last section revised. This version will appear in Comm. Math.
Phy
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