


Vol 46, No 3 (2019)
- Year: 2019
- Articles: 9
- URL: https://journals.rcsi.science/1068-3356/issue/view/14152
Article
Baryonic Decays of B Mesons to the J/ψ Final State
Abstract
This study concerns the experimental situation in the range of baryon decays of B mesons. The basic properties of these decays and theoretical models explaining these properties are discussed. The emphasis is on baryon decays of B mesons with J/ψ in the final state, which facilitate the search for exotic resonant states in the J/ψ + baryon system.



On the Detection of Multinucleon Events in Nucleus—Nucleus Collisions with Forward Calorimeters (ZDC)
Abstract
The detection of spectator nucleons emitted forward in the beam direction in experiments on the study of nucleus—nucleus interactions using forward Zero Degree Calorimeters (ZDCs) allows the determination of the event centrality and the detection of the nucleons from electromagnetic dissociation (EMD). In this paper, we propose a simple combinatorial model for calculating the energy releases in the ZDC, taking into account the calorimeter acceptance and efficiency. Using this model, the effect of the limited acceptance and nucleon detection efficiency on the spectral shape in the ZDC and the possibility of measuring the yield of a certain number of nucleons from the EMD is studied at LHC energies.



Effect of the Galactic Disk and Satellite Galaxies on the Spatial Distribution of Globular Clusters
Abstract
The distribution anisotropy in systems of globular clusters (GCs) in satellite galaxies of the Milky Way is considered using the inertia tensor. The statistical significance of the results is estimated by repeating this analysis for random catalogs. This method reproduces a known planar structure in the distribution of satellite galaxies; however, the significance of this structure is slightly lower than that for other methods used in the literature. For the GCs at distances 2 < R < 10 kpc, the structure is coplanar with the galactic plane. At large distances, the structure orientation is close to the orientations of the satellite galaxies, i.e., is perpendicular to the Galaxy plane. The probability of stochastic realization of such distribution is 1.7%. The GC distribution anisotropy is also measured without the GCs belonging to the Sagittarius tidal stream. Measurements show that the effect of the stream on the GC perturbation is weak.



Growth of Si/Si1-xGex/Si (x < 0.1) Quantum Wells by Modulating the Ge Molecular Flow. II. Study of Properties
Abstract
Single quantum wells in the Si1-xGex/Si (x < 0.1) system grown in the mode of molecular Ge flow modulation in forming the solid solution layer are studied. The grown heterostructures are investigated by the low-temperature photoluminescence method, and their properties were compared with the properties of similar heterostructures grown without modulation of the Ge molecular flow. It is shown that modulation of the Ge flow has almost no effect on the spectral properties of the quantum wells.



Nonlinear Optical Properties of Hybrid Associates of Azure A Molecules with Zn0.5Cd0.5S Colloidal Quantum Dots
Abstract
We present the results of the study of the nonlinear optical response observed in hybrid associates of Azure A dye with Zn0.5Cd0.5S colloidal quantum dots upon exposure to 10-ns pulses of the second harmonic (532 nm) of a Nd3+:YAG laser. It is shown that association enhances the absorption saturation in the dye by a factor of 4.5, which is caused by charge phototransfer between the components of the hybrid associate.



Formation of Primordial Black Hole Clusters from Phase Transitions in the Early Universe
Abstract
A new model of the formation of primordial black holes (PBHs) is considered. The PBH generation mechanism is based on the collapse of massive walls formed in a scalar field during second-order phase transitions caused by quantum fluctuations during inflation. An essential feature of the mechanism is the formation of primordial black holes in the form of clusters. An analytical spectrum of PBH masses is obtained. We also demonstrate the possibility of forming the clusters with a total mass of ∼ 105–108M☉, ∼ 1 pc in size, and ∼ 1011 in number, which corresponds to the observational data on the number of galaxies in the visible region of the Universe. The prospect for the use of the proposed approach as a new scenario of the formation of galactic nuclei in the early Universe is shown.



GHz Repetition Rate of Picosecond Pulses in a Nd:YAG Waveguide Laser
Abstract
A passive mode locking Nd:YAG waveguide laser with a gigahertz pulse repetition rate is presented. Single-layer graphene is used as the saturable absorber. A tubular waveguide in the active medium was developed to provide generation of only the fundamental transverse mode. Due to this approach, stable generation of pulses with a duration of < 20 ps and a repetition rate of 9.8 GHz was achieved.



Angular Analysis of the e+e− → D(*)±D*∓ Process Near the Open Charm Threshold with Initial-State Radiation
Abstract
The results of measurements of the exclusive cross section for the e+e− → D(*)±D*∓ process near the open charm threshold with initial-state radiation are presented. The analysis is based on the experimental data collected with the Belle detector at energies \(\sqrt s \) equal to ϒ(4S), ϒ(5S) production energies, and energies of the nearby continuum corresponding to an integrated luminosity of 951 fb−1. The accuracy of the measurements of the cross sections is twice higher in comparison with the previous results of the Belle collaboration. An angular analysis is performed for the final state D*+D*− for the first time with the result that the cross section is decomposed into three components corresponding to the possible combinations of D*-meson polarizations in the final state.



Search for Radiative Decays of the ϒ(1S) Resonance
Abstract
A new technique for searching radiative decays of the ϒ(1S) resonance in the charmonium state is discussed. It is based on tagging the ϒ(1S) resonance in hadron transitions ϒ(2S) → ϒ(1S)π+π− using the data sample obtained at B factories, i.e., in experiments at e+e− colliders for studying B mesons at the center-of-mass energy equal to the mass of the ϒ(2S) resonance. Simulation estimates show that the use of the proposed method in the Belle experiment will make it possible to increase the sensitivity in the study of the radiative decays of the ϒ(1S) resonance in the charmonium states by an order of magnitude.


