4,231 research outputs found
A way to measure the water quality of the LHAASO-WCDA with cosmic muon signals
The Large High Altitude Air Shower Observatory (LHAASO) is to be built at
Daocheng, Sichuan Province, China. As one of the major components of the LHAASO
project, a Water Cherenkov Detector Array (WCDA), with an area of 78,000~, contains 350,000~tons of purified water. The water transparency and its
stability are critical for successful long-term operation of this project. To
gain full knowledge of the water Cherenkov technique and investigate the
engineering issues, a 9-cell detector array has been built at the Yangbajing
site, Tibet, China. With the help of the distribution of single cosmic muon
signals, the monitoring and measurement of water transparency are studied. The
results show that a precision of several percent can be obtained for the
attenuation length measurement, which satisfies the requirements of the
experiment. In the near future, this method could be applied to the LHAASO-WCDA
project
Limits on light WIMPs from the CDEX-1 experiment with a p-type point-contact germanium detector at the China Jingping Underground Laboratory
We report results of a search for light Dark Matter WIMPs with CDEX-1
experiment at the China Jinping Underground Laboratory, based on 53.9 kg-days
of data from a p-type point-contact germanium detector enclosed by a NaI(Tl)
crystal scintillator as anti-Compton detector. The event rate and spectrum
above the analysis threshold of 475 eVee are consistent with the understood
background model. Part of the allowed regions for WIMP-nucleus coherent elastic
scattering at WIMP mass of 6-20 GeV are probed and excluded. Independent of
interaction channels, this result contradicts the interpretation that the
anomalous excesses of the CoGeNT experiment are induced by Dark Matter, since
identical detector techniques are used in both experiments.Comment: 5 pages, 5 figure
Limits on Light Weakly Interacting Massive Particles from the First 102.8 kg day Data of the CDEX-10 Experiment
We report the first results of a light weakly interacting massive particles
(WIMPs) search from the CDEX-10 experiment with a 10 kg germanium detector
array immersed in liquid nitrogen at the China Jinping Underground Laboratory
with a physics data size of 102.8 kg day. At an analysis threshold of 160 eVee,
improved limits of 8 and 3 cm at a
90\% confidence level on spin-independent and spin-dependent WIMP-nucleon cross
sections, respectively, at a WIMP mass () of 5 GeV/ are
achieved. The lower reach of is extended to 2 GeV/.Comment: 5 pages, 4 figure
A Unified Approach to the Classical Statistical Analysis of Small Signals
We give a classical confidence belt construction which unifies the treatment
of upper confidence limits for null results and two-sided confidence intervals
for non-null results. The unified treatment solves a problem (apparently not
previously recognized) that the choice of upper limit or two-sided intervals
leads to intervals which are not confidence intervals if the choice is based on
the data. We apply the construction to two related problems which have recently
been a battle-ground between classical and Bayesian statistics: Poisson
processes with background, and Gaussian errors with a bounded physical region.
In contrast with the usual classical construction for upper limits, our
construction avoids unphysical confidence intervals. In contrast with some
popular Bayesian intervals, our intervals eliminate conservatism (frequentist
coverage greater than the stated confidence) in the Gaussian case and reduce it
to a level dictated by discreteness in the Poisson case. We generalize the
method in order to apply it to analysis of experiments searching for neutrino
oscillations. We show that this technique both gives correct coverage and is
powerful, while other classical techniques that have been used by neutrino
oscillation search experiments fail one or both of these criteria.Comment: 40 pages, 15 figures. Changes 15-Dec-99 to agree more closely with
published version. A few small changes, plus the two substantive changes we
made in proof back in 1998: 1) The definition of "sensitivity" in Sec. V(C).
It was inconsistent with our actual definition in Sec. VI. 2) "Note added in
proof" at end of the Conclusio
Observation of decays into vector meson pairs , , and
Decays of to vector meson pairs , and
are observed for the first time using
\psip events accumulated at the BESIII detector at the BEPCII
collider. The branching fractions are measured to be , , and , for , , and ,
respectively. The observation of decays into a pair of vector
mesons , and indicates that the hadron
helicity selection rule is significantly violated in decays. In
addition, the measurement of gives the rate of doubly
OZI-suppressed decay. Branching fractions for and
decays into other vector meson pairs are also measured with improved precision.Comment: 4 pages, 2 figure
Evidence for at center-of-mass energies from 4.009 to 4.360 GeV
Using data samples collected at center-of-mass energies of =
4.009, 4.230, 4.260, and 4.360 GeV with the BESIII detector operating at the
BEPCII collider, we perform a search for the process
and find evidence for and
with statistical significances of 3.0 and
3.4, respectively. The Born cross sections
, as well as their upper limits at the
90% confidence level are determined at each center-of-mass energy.Comment: 8 pages, 7 figures, 3 table
production at low transverse momentum in p+p and d+Au collisions at = 200 GeV
We report on the measurement of production in the dielectron
channel at mid-rapidity (|y|<1) in p+p and d+Au collisions at =
200 GeV from the STAR experiment at the Relativistic Heavy Ion Collider. The
transverse momentum spectra in p+p for < 4 GeV/c and d+Au
collisions for < 3 GeV/c are presented. These measurements extend the
STAR coverage for production in p+p collisions to low .
The from the measured invariant cross section in
p+p and d+Au collisions are evaluated and compared to similar measurements at
other collision energies. The nuclear modification factor for is
extracted as a function of and collision centrality in d+Au and
compared to model calculations using the modified nuclear Parton Distribution
Function and a final-state nuclear absorption cross section
High non-photonic electron production in + collisions at = 200 GeV
We present the measurement of non-photonic electron production at high
transverse momentum ( 2.5 GeV/) in + collisions at
= 200 GeV using data recorded during 2005 and 2008 by the STAR
experiment at the Relativistic Heavy Ion Collider (RHIC). The measured
cross-sections from the two runs are consistent with each other despite a large
difference in photonic background levels due to different detector
configurations. We compare the measured non-photonic electron cross-sections
with previously published RHIC data and pQCD calculations. Using the relative
contributions of B and D mesons to non-photonic electrons, we determine the
integrated cross sections of electrons () at 3 GeV/10 GeV/ from bottom and charm meson decays to be = 4.0({\rm
stat.})({\rm syst.}) nb and =
6.2({\rm stat.})({\rm syst.}) nb, respectively.Comment: 17 pages, 17 figure
Search for dark matter in events with heavy quarks and missing transverse momentum in pp collisions with the ATLAS detector
This article reports on a search for dark matterpair production in association with bottom or top quarks in20.3fb−1ofppcollisions collected at√s=8TeVbytheATLAS detector at the LHC. Events with large missing trans-verse momentum are selected when produced in associationwith high-momentum jets of which one or more are identifiedas jets containingb-quarks. Final states with top quarks areselected by requiring a high jet multiplicity and in some casesa single lepton. The data are found to be consistent with theStandard Model expectations and limits are set on the massscale of effective field theories that describe scalar and tensorinteractions between dark matter and Standard Model par-ticles. Limits on the dark-matter–nucleon cross-section forspin-independent and spin-dependent interactions are alsoprovided. These limits are particularly strong for low-massdark matter. Using a simplified model, constraints are set onthe mass of dark matter and of a coloured mediator suitableto explain a possible signal of annihilating dark matter
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