A_n型非退化仿射Hecke代数的Gr?bner-Shirshov基

我们讨论了A_n-型非退化仿射Hecke代数的Gr?bner-Shirshov基和线性基.构造代数的Gr?bner-Shirshov基的方法主要有两种:一是通过计算合成;另一种方法是用线性基和钻石合成引理.因为我们还不知道A_n-型非退化仿射Hecke代数的线性基,因此我们使用第一种方法,也就是先通过计算合成给出A_n-型非退化放射Hecke代数的Gr?bnerShirshov基,然后用此Gr?bner-Shirshov基和结合代数的钻石合成引理,给出A_n型非退化仿射Hecke代数的一组线性基.     

2-μm singly resonant optical parameter oscillator

We experimentally realize a singly resonant optical parameter oscillator （OPO） which operates at the degenerate point of KTiOPOa （KTP） crystal. A thin film plate polarizer （TFP） is used as the output coupler to obtain linearly polarized 2.12 μm laser. A maximum output power of 2.2 W at 2.12 μm is obtained from a near-degenerate, type-II KTP OPO by utilizing a Q-switched diode-pumped Nd：YAG laser operating at 5 kHz.     

Primordial perturbations and non-gaussianities in Ho?ava-Lifshitz gravity

We investigate primordial perturbations and non-gaussianities in the Ho?ava-Lifshitz theory of gravitation. In the UV limit, the scalar perturbation in the Ho?ava theory is naturally scale-invariant, ignoring the details of the expansion of the Universe. One may thus relax the exponential inflation and the slow-roll conditions for the inflaton field. As a result, it is possible that the primordial non-gaussianities, which are " slow-roll suppressed” in the standard scenarios, become large. We calculate the non-gaussianities from the bispectrum of the perturbation and find that the equilateral-type non-gaussianity is of the order of unity, while the local-type non-gaussianity remains small, as in the usual single-field slow-roll inflation model in general relativity. Our result is a new constraint on Ho?ava-Lifshitz gravity.     

大面积LaBr3:Ce闪烁探测器伽马灵敏度和时间响应测量

在60Co放射性标准源场中,对国内新研制的大面积LaBr3∶Ce闪烁探测器伽马灵敏度进行了测量,并用GD100光电管分别与LYSO:Ce、ST401闪烁体构成闪烁探测器的伽马灵敏度进行了对比分析;应用CΓC-67型三通道的ns快脉冲辐射源对这种大面积新型闪烁晶体本身的时间响应特性进行了测量.实验测量结果表明:直径76 mm的大面积LaBr3∶Ce闪烁探测器伽马灵敏度与LYSO∶Ce、ST401闪烁探测器的同体积归一灵敏度比分别超过5和200;时间响应前沿2.56 ns,后沿56 ns,半高宽23.56 ns,衰减时间25.45 ns.     

Design of the low energy beam transport line for the China spallation neutron source

The design of the China Spallation Neutron Source (CSNS) low-energy beam transport (LEBT) line, which locates between the ion source and the radio-frequency quadrupole (RFQ), has been completed with the TRACE3D code. The design aims at perfect matching, primary chopping, a small emittance growth and sufficient space for beam diagnostics. The line consists of three solenoids, three vacuum chambers, two steering magnets and a pre-chopper. The total length of LEBT is about 1.74m. This LEBT is designed to transfer 20mA of H-pulsed beam from the ion source to the RFQ. An induction cavity is adopted as the pre-chopper. The electrostatic octupole steerer is discussed as a candidate. A four-quadrant aperture for beam scraping and beam position monitoring is designed.     

Design of magnet and control of the beam emittance for Penning H－ ion source

The design requirement and principle of the deflection magnet for Magnetron and Penning H^－ ion source are discussed. It is proved that there exists a maximum emittance for the beam that may be transformed by the magnet into a state with equal Twiss parameters of α_r=α_y and β_r=β_y, which is the requisite condition to get a minimum emittance at the entrance of RFQ after transporting by a LEBT with solenoids. For this maximum emittance, the corresponding magnetic field gradient index is 1.     

A Continuous-Wave Diode-Side-Pumped Tm:YAG Laser with Output 51W

A compact diode-side-pumped Tm：YAG laser is presented, which can output 51 W of cw power at 2.02 μm. The Tm：YAG rod is side pumped by nine diode arrays with the central wavelength of 783nm and the with bandwidth of about 2.5 nm at 25^o C. To decrease the thermal effect on the both ends and dissipate the heat effectively, one composite Tm：YAG rod with the undoped YAG end caps and the screw threads on the side surface of the rod is used as the laser crystal. The maximum optical-to-optical conversion efficiency of the 2.02-μm laser output is 14.2%, with a slope effciency of 26.8%     

铱(I)联萘胺Schiff碱(BPMBNDI)配合物催化苯乙酮的不对称氢转移反应

用旋光活性2, 2'-(1, 1'-联萘)二胺和2-吡啶基甲醛缩合得到的Schiff碱BPMBNDI[N, N'-二(2-吡啶基亚甲基)-(1, 1'-联萘)-2, 2'-二亚胺]为配体与[Ir(COD)Cl]2(COD=1, 5-环辛二烯)反应, 生成了10个光学活性铱配合物。研究它们在异丙醇对苯乙酮不对称氢转移反应中的光学诱导活性时, 发现10个催化剂均具有较高的立体选择性,其中[Ir(COD)(BPMBNDI)I]催化的光学产率高达84%。     

Standing Rankine-Hugoniot Shocks in Black Hole Accretion Discs

We study the problem of standing shocks in viscous disc-like accretion flows around black holes. For the first time we parametrize such a flow with two physical constants, namely the specific angular momentum accreted by the black hole j and the energy quantity K. By providing the global dependence of shock formation in the j- K parameter space, we show that a significant parameter region can ensure solutions with Rankine-Hugoniot shocks; and that the possibilities of shock formation are the largest for inviscid flows, decreasing with increasing viscosity, and ceasing to exist for a strong enough viscosity. Our results support the view that the standing shock is an essential ingredient in black hole accretion discs and is a general phenomenon in astrophysics, and that there should be a continuous change from the properties of inviscid flows to those of viscous ones.