|
Escape from a Riddled-Like Basin
CHAO Xiao-Gang, DAI Jun, WANG Wen-Xiu, HE Da-Ren
Chin. Phys. Lett. 2005, 22 (12):
3025-3028
.
We investigate a system described by a conservative and a dissipative map concatenation. A fat fractal forbidden net, induced by interaction between discontinuous and noninvertible properties, introduces rippled-like attraction basins of two periodic attractors. Small areas, which serve as escaping holes of a new type of crisis, are dominated by conventional strong dissipation and are bounded by the forbidden region, but only in the vicinity of each periodic point. Based on this understanding, the scaling behaviour of the averaged lifetime of the crisis is analytically and numerically determined to be <τ> ∝ (b-b0)γ, where b denotes the control parameter, b0 denotes its critical threshold, and γ simeq -1.5.
|
|
Dynamical Study on Fusion Barrier in the Synthesis of Superheavy Elements
FENG Zhao-Qing, , JIN Gen-Ming, ZHANG Feng-Shou, FU Fen, HUANG Xi,
Chin. Phys. Lett. 2005, 22 (12):
3040-3043
.
Based on the improved isospin-dependent quantum molecular dynamics model, the fusion barrier in the synthesis of superheavy elements is studied dynamically. Deformation effect and nucleon transfer in neck region are also investigated systematically, which can lower the dynamical barrier since the neck formation. It is shown that the neck radius is dependent on the incident energy and collision orientation. For the static barrier, the model almost gives the same results with the proximity potential.
|
|
Dynamical Effects on Sub-barrier Fusion of 40,48Ca+90,96Zr
ZHANG Huan-Qiao, LIU Zu-Huan, YANG Feng, LIN Cheng-Jian, RUAN Ming, WU Yue-Wei, LI Zhu-Xia, WU Xi-Zhen, ZHAO Kai, WANG Ning
Chin. Phys. Lett. 2005, 22 (12):
3048-3051
.
We have measured the fusion cross sections for 48Ca+90,96 around the Coulomb barrier and presented them along with the experimental data of 40Ca+90,96. The experimental results are compared with the improved quantum molecular dynamics model calculations. It is shown in comparison that the dynamical effects play an important role in the sub-barrier fusion reactions.
|
|
Silica-Based 64-Channel Arrayed Waveguide Gratings with Double Functions
AN Jun-Ming, LI Jian, XIA Jun-Lei, GAO Ding-Shan, WU Yuan-Da, LI Jian-Guang, WANG Hong-Jie, HU Xiong-Wei
Chin. Phys. Lett. 2005, 22 (12):
3061-3063
.
Silica-based 64-channel arrayed waveguide gratings (AWGs) with double functions and 0.4nm (50GHz) channel spacing have been designed and fabricated. On the same component, Gauss and flat-top output response spectra are obtained simultaneously. The test results show that when the insertion loss ranges from 3.5dB to 6.4dB, the crosstalk is better than -34dB, the 1dB bandwidth is 0.12nm, the 3dB bandwidth is 0.218nm, and the polarization-dependent loss (PDL) is less than 0.5dB for Gauss response. When the insertion loss ranges from 5.8dB to 7.8dB, the crosstalk is better than -30dB, the 1dB bandwidth is 0.24nm, the 3dB bandwidth is 0.33nm, and the PDL is less than 0.2dB for flat-top response.
|
|
Low-Threshold and High-Power Oxide-Confined 850nm AlInGaAs Strained Quantum-Well Vertical-Cavity Surface-Emitting Lasers Based on Intra-Cavity Contacted Structure
CHEN Min, GUO Xia, DENG Jun, GAI Hong-Xing, DONG Li-Min, QU Hong-Wei, GUAN Bao-Lu, GAO Guo, SHEN Guang-Di
Chin. Phys. Lett. 2005, 22 (12):
3074-3076
.
The low-threshold and high-power oxide-confined 850nm AlInGaAs strained quantum-well (QW) vertical-cavity surface-emitting lasers (VCSELs) based on the intra-cavity contacted structure are fabricated. The threshold current of 0.1mA for a 10-μm oxide-aperture device is obtained with the threshold current density of 0.127kA/cm2. For a 22-μm oxide-aperture device, the peak optical output power reaches to 14.6mW at the current injection of 25mA under the room temperature and pulsed operation with a threshold current of 2mA, which corresponds to the threshold current density of 0.526kA/cm2. The lasing wavelength is 855.4nm. The full wave at half maximum is 2.2nm. The analysis of the characteristics and the fabrication of
VCSELs are also described.
|
|
Self-Assembly of Gold Nanoparticles on Nanometre-Patterned Surface
ZHANG Yong-Jun, YANG Jing-Hai, LI Wei, ZHANG Yu, XU Ling, XU Jun, HUANG Xin-Fan, CHEN Kun-Ji
Chin. Phys. Lett. 2005, 22 (12):
3133-3136
.
The self-assembly processes of gold nanoparticles on nanometre-step-patterned Si surface and polished Si surface are investigated by the convective self-assembly method. The convective self-assembly method is used to deposit the colloids dispersed in benzene onto the substrates. The SEM results show that the configurations of the gold arrays depend on the surface morphology of the substrates. On the nanometre-step-patterned Si surface, the nanoparticles self assemble into parallel lines, and the distance between the neighbouring lines is around 35nm. On the polished Si surface the nanoparticles form compact domains. In each domain the particles are close-packed in a two-dimensional hexagonal superlattice and are separated by uniform distances. The analysis shows that on the nanometre-step-patterned Si surface, the steps play critical roles in the self-assembly process of gold nanoparticles. The capillary force from the steps drives the particles to lines along the steps. Therefore, the particles tend to self-assemble into one-dimensional
line structures when the solvent evaporates. For the polished Si substrate there is a little difference that the particles form two-dimensional hexagonal superlattices without the directional confinement.
|
|
Transition for Optimal Paths in Bimodal Directed Polymers
WANG Xiao-Hong
Chin. Phys. Lett. 2005, 22 (12):
3144-3146
.
The problem for optimal paths in bimodal directed polymers is studied. It is shown that the distribution of the thermal average position of the endpoints of the optimal paths is discontinuous below the threshold p c. The origin is that there is a finite possibility that only one endpoint takes the global minimum energy for p c. Our results suggest that the percolation threshold for directed percolation is also the critical point of the transition for the possibility that the optimal paths converge to one endpoint.
|
|
An Improved Blue Polymer Light-Emitting Diode by Using Sodium Hydroxide/Ca/Al Cathode
MA Liang, XIE Zhi-Yuan, LIU Jun, YANG Jun-Wei, CHENG Yan-Xiang, WANG Li-Xiang, WANG Fo-Song
Chin. Phys. Lett. 2005, 22 (12):
3196-3188
.
The performance of blue polymer light-emitting diodes (PLEDs) based on poly(9,9-dioctylfluorene) (PFO) is improved by introducing a thin layer of sodium hydroxide (NaOH) between the calcium cathode and the PFO emissive layer. By replacing the commonly used Ca/Al cathode by a NaOH (2.5nm)/Ca (10nm)/Al cathode, the driving voltage is reduced from 8.3V to 5.4V and the light-emitting efficiency is enhanced from 0.46cd/A to 0.72cd/A for achieving a luminance of 500cdm2, respectively. Moreover, the device with NaOH/Ca/Al cathode shows a pure blue emission of (0.17, 0.12) at high brightnesses. These improvements are attributed to introduction of a thin layer of NaOH that can lower the interfacial barrier and facilitate electron injection.
|
|
Non-Gravitational Effects with Density-Matching in Evaluating the Influence of Sedimentation on Colloidal Coagulation
LIU Jie, SUN Zhi-Wei, AA Yan
Chin. Phys. Lett. 2005, 22 (12):
3199-3202
.
The method of density matching between the solid and liquid phases is often adopted to effectively eliminate the effect of sedimentation of suspensions in studies on dynamic behaviour of a colloidal system. However, the associated changes in the solvent composition may bring side effects to the properties investigated and therefore might lead to a faulty conclusion if the relevant correction is not made. To illustrate the importance of this side effect, we present an example of the sedimentation influence on the coagulation rate of suspensions of 2μm (diameter) polystyrene. The liquid mixtures, in the proper proportions of water (H2O), deuterium oxide (D2O) and methanol (MeOH) as the liquid phase, density-matched and unmatched experiments are performed. Besides the influence of viscosity, the presence of methanol in solvent media, used to enhance the sedimentation effect, causes significant changes (reduction) in rapid coagulation rates compared to that in pure water. Without the relevant corrections for those non-gravitational factors it seems that gravitational sedimentation would retard the coagulation. The magnitude of the contribution from the non-gravitational factor is quantitatively determined, making the relevant correction possible. After necessary corrections for all factors, our experiments show that the influence of the sedimentation on coagulation rates at the initial stage of the coagulation is not observable.
|
|
Lattice Boltzmann Simulation of Blood Flow in Blood Vessels with the Rolling Massage
YI Hou-Hui, XU Shi-Xiong, QIAN Yue-Hong, FANG Hai-Ping
Chin. Phys. Lett. 2005, 22 (12):
3210-3213
.
The rolling massage manipulation is a classic Chinese massage, which is expected to improve the circulation by pushing, pulling and kneading of the muscle. A model for the rolling massage manipulation is proposed and the lattice Boltzmann method is applied to study the blood flow in the blood vessels. The simulation results show that the blood flux is considerably modified by the rolling massage and the explicit value depends on the rolling frequency, the rolling depth, and the diameter of the vessel. The smaller the diameter of the blood vessel, the larger the enhancement of the blood flux by the rolling massage. The model, together with the simulation results, is expected to be helpful to understand the mechanism and further development of rolling massage techniques.
|
|
Physical Mechanism of Formation of the Bimodal Structure in the Meiyu Front System
CUI Xiao-Peng, GAO Shou-Ting, ZONG Zhi-Ping, LIU Wen-Ming, LI Xiao-Fan
Chin. Phys. Lett. 2005, 22 (12):
3218-3220
.
The bimodal structure of the Meiyu front system is readdressed after Zhou et al.(2005). The physical mechanism of the formation of the bimodal distribution is discussed. The bimodal structure of the Meiyu front system considerably results from atmospheric moisture gradients, though atmospheric temperature gradients are also not negligible. According to the definition of equivalent potential temperature, and by scale analysis, we find that atmospheric equivalent potential temperature gradients, which could be regarded as an indicator of the Meiyu front system, could be mainly attributed to the variations of atmospheric potential temperature gradients with a scaling factor of 1 and moisture gradients multiplied by a scaling factor of an order of about 2.5×103, which means that small variations of atmospheric moisture gradients could lead to large variations of equivalent potential temperature gradients, and thus large variations of the Meiyu front system. Quantitative diagnostics with a mesoscale simulation data in the vicinity of the Meiyu front system show that moisture gradients contribute to equivalent potential temperature gradients more than potential temperature gradients.
|
|
Earth’s Magnetosphere Impinged by Interplanetary Shocks of Different Orientations
GUO Xiao-Cheng, HU You-Qiu, WANG Chi
Chin. Phys. Lett. 2005, 22 (12):
3221-3224
.
Using a recently developed PPMLR-MHD code, we carry out a global numerical simulation of the interaction between interplanetary shocks and Earth's magnetosphere. The initial magnetosphere is in a quasi-steady state, embedded in a uniform solar wind and a spiral interplanetary magnetic field (IMF). An interplanetary (IP) shock interacts in turn with the bow shock, the magnetosheath, the magnetopause, and the magnetosphere, and changes the magnetosphere in shape and structure, and the distribution of the electric current and potential in the ionosphere as well. A preliminary comparison is made between two IP shocks of the same solar wind dynamic pressure and a vanishing IMF Bz on the downstream side, but with different propagation directions, one parallel and the other oblique to the Sun--Earth line. The numerical results show that both shocks cause a compression of the magnetosphere, an enhancement of magnetic field strength and field-aligned current in the magnetosphere, and an increase of the dawn-dusk electric potential drops across the polar ionosphere. Moreover, the magnetosphere--ionosphere system approaches a similar quasi-steady state after the interaction, for the downstream states are very close for the two shocks. However, the evolution processes of the system are remarkably different during the interaction with the two shocks of different orientations. The shock with the normal oblique to the Sun--Earth line results in a much longer evolution time for the system. This demonstrates that the shock orientation plays an important role in determining the associated geophysical effects and interpreting multisatellite observations of IP shock--magnetosphere interaction events.
|
|
New Evidence for Magnetic Reconnection in the Tail of Interplanetary Magnetic Cloud
ZHONG Ding-Kun, WEI Feng-Si, FENG Xue-Shang, YANG Fang,
Chin. Phys. Lett. 2005, 22 (12):
3225-3228
.
We analyse the WIND data of an interplanetary magnetic cloud (MC) on 2 November 2001, and find new evidences for magnetic reconnection in the tail of this MC. In the MC tail, the largely dip and the large change of the orientation of the magnetic field occurred simultaneously, Δθ approx 45°, and ΔФ changed from 90° to 320°. Correspondingly, the number density of ions increased, and the superthermal electrons were heated and accelerated, however its number density decreased. Meanwhile, inverse jets and Hall term were observed. The pitch-angle distributions of the electrons with lower energy and higher energy showed strong turbulence and bi-direction flow, respectively. The plasma wave activity enhanced near the electron plasma frequency, fpe and 2fpe. These important physical characteristics are new evidences for magnetic reconnection existing in interplanetary space.
|
|
A Quasi-Periodic Solar Radio Fluctuation at Microwave Band
XU Fu-Ying, HUANG Guang-Li, WU Hong-Ao,
Chin. Phys. Lett. 2005, 22 (12):
3229-3232
.
A rare but interesting solar radio fine structure, quasi-periodic fluctuations, on 25 August 1999 was observed at microwave band for the first time. They fluctuated initially at a nearly stable frequency level then at a reverse drift component up to 5.49GHz. The individual fluctuation consists of a bi-directional drift component. The features are characterized by narrow bandwidth of Δf/f≤3%, quasi-periodicity of ~ms as well as a slowly reverse and a rapidly normal drift rates on the bi-directional drift component. The associated data of the Yohkoh soft and hard x-ray telescope and Nobeyama radio heliograph at 17GHz showed that there are several bright spots (i.e. inhomogeneities) along the soft x-ray loop, and the locations of both radio and soft x-ray sources are closely consistent. Therefore, the fluctuations are most likely caused by the inhomogeneities within a flare loop. Based on the two-component atmospheric model, we suggest a three-component atmospheric model with large scale length λ and small scale lengths λ1 and λ2 to describe equilibrium atmosphere and inhomogeneity. With the beam model, the characters of fluctuations may be interpreted reasonably by the quasi-equidistant inhomogeneity along a flare loop.
|
68 articles
|