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Li, Y.

Publications and source records attributed to Li, Y..

At least 271 records · Page 15

Dryland climate change: Recent progress and challenges: Dryland Climate Change

Drylands are home to more than 38% of the world's population and are one of the most sensitive areas to climate change and human activities. This review describes recent progress in dryland climate change research. Recent findings indicate that the long-term trend of the aridity index (AI) is mainly attributable to increased greenhouse gas emissions, while anthropogenic aerosols exert small effects but alter its attributions. Atmosphere-land interactions determine the intensity of regional response. The largest warming during the last 100 years was observed over drylands and accounted for more than half of the continental warming. The global pattern and interdecadal variability of aridity changes are modulated by oceanic oscillations. The different phases of those oceanic oscillations induce significant changes in land-sea and north-south thermal contrasts, which affect the intensity of the westerlies and planetary waves and the blocking frequency, thereby altering global changes in temperature and precipitation. During 1948–2008, the drylands in the Americas became wetter due to enhanced westerlies, whereas the drylands in the Eastern Hemisphere became drier because of the weakened East Asian summer monsoon. Drylands as defined by the AI have expanded over the last 60 years and are projected to expand in the 21st century. The largest expansion of drylands has occurred in semiarid regions since the early 1960s. Dryland expansion will lead to reduced carbon sequestration and enhanced regional warming. The increasing aridity, enhanced warming, and rapidly growing population will exacerbate the risk of land degradation and desertification in the near future in developing countries.

54 ENVIRONMENTAL SCIENCES↗

Measurement of the τ Lepton Polarization and R ( D * ) in the Decay B ¯ → D * τ - ν ¯ τ

Here, we discuss the first measurement of the τ lepton polarization P τ ( D * ) in the decay B ¯ → D * τ - ν ¯ τ as well as a new measurement of the ratio of the branching fractions R ( D * ) = B ( B ¯ → D * τ - ν ¯ τ ) / B ( B ¯ → D * ℓ - ν ¯ ℓ ) , where ℓ - denotes an electron or a muon, and the τ is reconstructed in the modes τ - → π - ν τ and τ - → ρ - ν τ . We use the full data sample of 772 × 1 0 6 B B ¯ pairs recorded with the Belle detector at the KEKB electron-positron collider. Our findings, P τ ( D * ) = - 0.38 ± 0.51 ( stat ) - 0.16 + 0.21 ( syst ) and R ( D * ) = 0.270 ± 0.035 ( stat ) - 0.025 + 0.028 ( syst ) , are consistent with the theoretical predictions of the standard model.

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

Precision studies of observables in $p p \rightarrow W \rightarrow l\nu _l$ and $ pp \rightarrow \gamma ,Z \rightarrow l^+ l^-$ processes at the LHC

This report was prepared in the context of the LPCC "Electroweak Precision Measurements at the LHC WG" and summarizes the activity of a subgroup dedicated to the systematic comparison of public Monte Carlo codes, which describe the Drell-Yan processes at hadron colliders, in particular at the CERN Large Hadron Collider (LHC). This work represents an important step towards the definition of an accurate simulation framework necessary for very high-precision measurements of electroweak (EW) observables such as the $W$ boson mass and the weak mixing angle. All the codes considered in this report share at least next-to-leading-order (NLO) accuracy in the prediction of the total cross sections in an expansion either in the strong or in the EW coupling constant. The NLO fixed-order predictions have been scrutinized at the technical level, using exactly the same inputs, setup and perturbative accuracy, in order to quantify the level of agreement of different implementations of the same calculation. A dedicated comparison, again at the technical level, of three codes that reach next-to-next-to-leading-order (NNLO) accuracy in quantum chromodynamics (QCD) for the total cross section has also been performed. These fixed-order results are a well-defined reference that allows a classification of the impact of higher-order sets of radiative corrections. Several examples of higher-order effects due to the strong or the EW interaction are discussed in this common framework. Also the combination of QCD and EW corrections is discussed, together with the ambiguities that affect the final result, due to the choice of a specific combination recipe.

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

First measurement of unpolarized semi-inclusive deep-inelastic scattering cross sections from a He 3 target [First measurement of unpolarized SIDIS cross section from a 3 He target]

Here, the unpolarized semi-inclusive deep-inelastic scattering (SIDIS) differential cross sections in 3 He(e,e'π ± )X have been measured for the first time in Jefferson Lab experiment E06-010 with a 5.9 GeV e – beam on a 3 He gas target. The experiment focuses on the valence quark region, covering a kinematic range 0.12 < x bj < 0.45,1 < Q 2 < 4(GeV/c) 2 ,0.45 < z h < 0.65, and 0.05 < P t < 0.55GeV/c. The extracted SIDIS differential cross sections of π± production are compared with existing phenomenological models while the 3 He nucleus approximated as two protons and one neutron in a plane-wave picture, in multidimensional bins. Within the experimental uncertainties, the azimuthal modulations of the cross sections are found to be consistent with zero.

73 NUCLEAR PHYSICS AND RADIATION PHYSICS↗

Plasma Brightenings in a Failed Solar Filament Eruption

Failed filament eruptions are solar eruptions that are not associated with coronal mass ejections. In a failed filament eruption, the filament materials usually show some ascending and falling motions as well as generating bright EUV emissions. Here we report a failed filament eruption (SOL2016-07-22) that occurred in a quiet-Sun region observed by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory . In this event, the filament spreads out but gets confined by the surrounding magnetic field. When interacting with the ambient magnetic field, the filament material brightens up and flows along the magnetic field lines through the corona to the chromosphere. We find that some materials slide down along the lifting magnetic structure containing the filament and impact the chromosphere, and through kinetic energy dissipation, cause two ribbon-like brightenings in a wide temperature range. There is evidence suggesting that magnetic reconnection occurs between the filament magnetic structure and the surrounding magnetic fields where filament plasma is heated to coronal temperatures. In addition, thread-like brightenings show up on top of the erupting magnetic fields at low temperatures, which might be produced by an energy imbalance from a fast drop of radiative cooling due to plasma rarefaction. Thus, this single event of a failed filament eruption shows the existence of a variety of plasma brightenings that may be caused by completely different heating mechanisms.

79 ASTRONOMY AND ASTROPHYSICS↗

Convolutional Neural Networks Applied to Neutrino Events in a Liquid Argon Time Projection Chamber

We present several studies of convolutional neural networks applied to data coming from the MicroBooNE detector, a liquid argon time projection chamber (LArTPC). The algorithms studied include the classification of single particle images, the localization of single particle and neutrino interactions in an image, and the detection of a simulated neutrino event overlaid with cosmic ray backgrounds taken from real detector data. These studies demonstrate the potential of convolutional neural networks for particle identifi-cation or event detection on simulated neutrino interactions. We also address technical issues that arise when applying this technique to data from a large LArTPC at or near ground level.

Acciarri, R↗

Development of shashlik electromagnetic calorimeter prototype for SoLID

A shashlik electromagnetic calorimeter will be produced in Hall A of Jefferson Laboratory for Solenoidal large Intensity Device (SoLID) to measure the energy deposition of electrons and hadrons, and to provide particle identification after the energy of the accelerator was upgraded to 12 GeV. Tsinghua University is the member of Hall A collaboration in charge of development and production of the large shashlik electromagnetic calorimeter of SoLID. One module of that calorimeter is composed by 194 layers. Each layer consists of a 1.5 mm thick plastic scintillator put on top of a 0.5 mm thick lead plate. Scintillation light is read out by wave-length shifter fibers penetrating through the calorimeter modules longitudinally along the direction of flight of the impact particle. This paper describes the design and construction of that module, as well as a few optimization studies meant to improve its performance. A detailed Geant4 simulation also shows that an energy resolution of 5%/√ E (GeV) and a good containment for electromagnetic showers can be achieved, as well as some basic electron identification. In conclusion, a prototype of that module will be tested soon with an electron beam at JLab.

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND ↗

Imaging Observations of Magnetic Reconnection in a Solar Eruptive Flare

Solar flares are among the most energetic events in the solar atmosphere. It is widely accepted that flares are powered by magnetic reconnection in the corona. An eruptive flare is usually accompanied by a coronal mass ejection, both of which are probably driven by the eruption of a magnetic flux rope (MFR). Here we report an eruptive flare on 2016 March 23 observed by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory . The extreme-ultraviolet imaging observations exhibit the clear rise and eruption of an MFR. In particular, the observations reveal solid evidence of magnetic reconnection from both the corona and chromosphere during the flare. Moreover, weak reconnection is observed before the start of the flare. We find that the preflare weak reconnection is of tether-cutting type and helps the MFR to rise slowly. Induced by a further rise of the MFR, strong reconnection occurs in the rise phases of the flare, which is temporally related to the MFR eruption. We also find that the magnetic reconnection is more of 3D-type in the early phase, as manifested in a strong-to-weak shear transition in flare loops, and becomes more 2D-like in the later phase, as shown by the apparent rising motion of an arcade of flare loops.

79 ASTRONOMY AND ASTROPHYSICS↗

Observation of D 0 → ρ 0 γ and Search for C P Violation in Radiative Charm Decays

Here, we discuss the first observation of the radiative charm decay D 0 → ρ 0 γ and the first search for C P violation in decays D 0 → ρ 0 γ , φ γ , and K ¯ * 0 ( 892 ) γ , using a data sample of 943 fb - 1 collected with the Belle detector at the KEKB asymmetric-energy e + e - collider. The branching fraction is measured to be B ( D 0 → ρ 0 γ ) = ( 1.77 ± 0.30 ± 0.07 ) × 10 - 5 , where the first uncertainty is statistical and the second is systematic. The obtained C P asymmetries A C P ( D 0 → ρ 0 γ ) = + 0.056 ± 0.152 ± 0.006 , A C P ( D 0 → φ γ ) = - 0.094 ± 0.066 ± 0.001 , and A C P ( D 0 → K ¯ * 0 γ ) = - 0.003 ± 0.020 ± 0.000 are consistent with no C P violation. Furthermore, we present an improved measurement of the branching fractions B ( D 0 → φ γ ) = ( 2.76 ± 0.19 ± 0.10 ) × 10 - 5 and B ( D 0 → K ¯ * 0 γ ) = ( 4.66 ± 0.21 ± 0.21 ) × 10 - 4 .

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

Search for D 0 decays to invisible final states at Belle

Here, we report the result from the first search for D 0 decays to invisible final states. The analysis is performed on a data sample of 924 fb - 1 collected at and near the Υ ( 4 S ) and Υ ( 5 S ) resonances with the Belle detector at the KEKB asymmetric-energy e + e - collider. The absolute branching fraction is confirmed using an inclusive D 0 sample, obtained by fully reconstructing the rest of the particle system including the other charmed particle. No significant signal yield is observed and an upper limit of 9.4 × 10 - 5 is set on the branching fraction of D 0 to invisible final states at 90% confidence level.

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

Search for the 0 - - glueball in Υ ( 1 S ) and Υ ( 2 S ) decays

Here, we report the first search for the J P C = 0 - - glueball in Υ ( 1 S ) and Υ ( 2 S ) decays with data samples of ( 102 ± 2 ) × 1 0 6 and ( 158 ± 4 ) × 1 0 6 events, respectively, collected with the Belle detector. No significant signals are observed in any of the proposed production modes, and the 90% credibility level upper limits on their branching fractions in Υ ( 1 S ) and Υ ( 2 S ) decays are gained. The inclusive branching fractions of the Υ ( 1 S ) and Υ ( 2 S ) decays into final states with a χ c 1 are measured to be B ( Υ ( 1 S ) → χ c 1 + anything ) = ( 1.90 ± 0.43 ( stat ) ± 0.14 ( syst ) ) × 10 - 4 with an improved precision over prior measurements and B ( Υ ( 2 S ) → χ c 1 + anything ) = ( 2.24 ± 0.44 ( stat ) ± 0.20 ( syst ) ) × 10 - 4 for the first time.

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

Status of the NPDGamma experiment

We report that the NPDGamma experiment measures the parity-violating (PV) gamma asymmetry from polarized cold neutrons captured on protons at the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL). The (PV) neutron spin asymmetry A γ of photons from polarized cold neutron capture on protons is proportional to the ΔI=1 long range weak meson coupling h$1\atop{π}$ between nucleons in the hadronic weak interaction (HWI). Liquid para-hydrogen production data taking concluded in April 2014 and once the background aluminum asymmetry measurements are complete, the PV asymmetry A γ can be extracted. Finally, preliminary results of the analysis of A γ are presented.

73 NUCLEAR PHYSICS AND RADIATION PHYSICS↗

Search for a dark vector gauge boson decaying to π + π - using η → π + π - γ decays

In this report, we search for a dark vector gauge boson U ' that couples to quarks in the decay chain D * + → D 0 π + , D 0 → K S 0 η , η → U ' γ , U ' → π + π - . No signal is discovered and we set a mass-dependent limit on the baryonic fine structure constant of 10 - 3 - 10 - 2 in the U ' mass range of 290 to 520 MeV / c 2 . This analysis is based on a data sample of 976 fb - 1 collected by the Belle experiment at the KEKB asymmetric-energy e + e - collider.

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS↗

Measurement of diagnostic neutral beam parameters on J-TEXT

A Doppler frequency shift spectrum (DFSS) system composed of two spectrometers has been developed for the joint Texas experimental tokamak to measure diagnostic neutral beam parameters including the beam energy fractions, intensity distributions, and divergences. The beam energy fractions are derived from measurements of H-alpha (Hα) emission using collisional excitation cross sections. The beam intensity distributions are obtained using an 11-channel measurement with a reconstruction technique. The beam divergences are obtained from spectrum broadening and geometric calculations. The results of preliminary investigations indicate that the DFSS system works well and can be used to obtain all of these parameters simultaneously. According to the preliminary experiment, the one-third energy fraction has the largest proportion (about 45%) of the beam energy and the full energy fraction is about 10%. The beam diameter is about 8.1 cm at a distance of 2.04 m from the accelerator. The beam divergence angle is about 3.3°. The current beam parameters are insufficient for charge-exchange measurements.

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND ↗