聚合物中空环芯光纤中O AM模式传输的几何容差特性研究

基于全矢量有限元法,研究了聚合物中空环芯光纤结构的椭圆、偏芯、直径不均匀等几何形变对光纤中轨道角动量模式性能的影响;此外,还研究了在保持轨道角动量模式稳定传输的条件下,光纤结构所能承受的最大形变.结果表明椭圆和偏芯会引起轨道角动量模式在传输过程中发生奇偶模间的模式走离,导致轨道角动量模式纯度降低,进而导致模式串扰增大;数值计算结果表明,当椭圆度或偏心度小于1%时,模式纯度大于99.02%,串扰小于-20.08dB.光纤的直径不均匀仅对光纤中所能支持的轨道角动量模式数量造成影响,纤芯半径越大,光纤中所能传输的轨道角动量模式越多;直径不均匀度在-3%～10%内的光纤均可支持原有的26个轨道角动量模式.     

低串扰低弯曲损耗环形芯少模多芯光纤的设计

针对少模多芯光纤中存在的纤芯内模式间的耦合及芯间模式耦合等问题,提出一种阶跃型环形芯组成的7芯结构光纤,每个纤芯可支持5个模式.各纤芯具有一个中心低折射率区域和一个高折射率环,保证纤芯内模式间均具有较大的折射率差,从而减小模式间耦合问题.运用有限元法模拟分析了中心纤芯和外纤芯的弯曲损耗、模式间的串扰特性及纤芯参数对串扰性能的影响.数据模拟结果表明,当波长为1.55μm,这种多芯光纤在弯曲半径为50 mm时,弯曲损耗远低于光纤衰减损耗,且纤芯中5个模式的相邻纤芯之间串扰均小于-20 dB/100 km,因而这种多芯光纤在小弯曲半径下仍可实现纤芯间独立的长距离信息传输.     

一种基于三芯光子晶体光纤的宽带模分复用器的设计与研究

本文提出了一种基于非对称三芯光子晶体光纤的宽带模分复用器.该器件主要是由位于光纤中心的可提供基模和高阶模传输的中心纤芯和分别位于中心纤芯两侧的可提供基模传输的2个旁芯构成.根据光耦合理论,在输入端对3个纤芯分别输入LP₀₁模式的光,在传输过程中左旁芯的LP₀₁模式的光将逐步向中心纤芯耦合并转换为LP₂₁模式传输,而右旁芯中的LP₀₁模式的光则逐步耦合并转换为中心纤芯中的LP₃₁模式来传输.通过对光纤结构的优化设计和光纤长度的选择,使得在输出端同时完成旁芯LP₀₁模向中心纤芯LP₂₁和LP₃₁模的最佳转换,从而实现LP₀₁、LP₂₁和LP₃₁ 3种模式的光在中心纤芯中的复用.反之,若将该器件的输出端用作输入端则可以实现中心纤芯中3种模式的光向3个纤芯的解复用.本文利用有限元法和光束传播法进行了优化设计和仿真,并将光耦合理论与超模理论相结合进行了分析计...     

基于空芯反谐振光纤的三芯结构宽带耦合器设计

提出一种基于三芯结构空芯反谐振光纤的太赫兹耦合器。采用有限元分析法对太赫兹光纤的模式特性进行分析,并基于耦合理论得到其耦合特性曲线。仿真结果表明,三芯结构模式具有比单芯结构更低的传输损耗,其耦合长度可通过改变纤芯间隔和隔离包层管的间隙进行调节。采用长度为223.2 mm的三芯结构空芯光纤可以实现插入损耗小于3.5 dB、带宽达到0.52 THz的宽带、均匀分束。     

基于谐振耦合现象的三芯光子晶体光纤带通滤波器

设计了一种三芯光子晶体光纤带通滤波器结构.利用纤芯间的谐振耦合,实现了滤波.当3个纤芯基模模式有效折射率在同一频率点实现匹配时,将产生谐振现象.通过合理选取光纤结构参数,可以使3个模式满足谐振条件.由于3个纤芯基模只在工作波长处实现有效折射率的匹配,因而纤芯间发生波长的选择性耦合.应用全矢量光束传播法(BPM)分析了这种光纤带通滤波器的性能.结果表明:在1.55 μm工作波长上,光纤耦合长度为22.8 mm;在损耗低于-3 dB前提下,通带带宽为8.9 nm.     

三角结构三芯光子晶体光纤中的模式耦合特性分析

基于耦合模理论,得出了三角结构三芯光子晶体光纤(TTC-PCF)的耦合模方程.数值模拟研究了该结构中纤芯间的定向耦合特性,分析了光纤结构及入射波长对耦合系数的影响以及入射光振幅比对纤芯间能量耦合特性的影响.结果表明,通过调节入射光振幅比可实现对纤芯间耦合强度的连续调节.对比了耦合模理论与束传播法得到的结果,两者表现出很好的一致性.结合TTC-PCF展现的独特耦合传输性能,讨论了其在耦合强度连续可调光纤定向耦合器和大模场光纤激光器的设计与制备等方面的可能应用前景.     

基于少模长周期光纤叠栅的模式转换器

本文提出一种在同一段少模光纤上写入两个不同周期Λ1和Λ2的长周期光纤光栅构成叠栅的方法,实现了纤芯基模LP_(01)向高阶纤芯模LP_(11)模式转换的宽带宽的新型的全光纤模式转换器.利用有限元法和耦合模理论建立了模式转换器的理论分析模型.数值仿真分析了叠栅中两个子光栅周期间隔、光栅长度、耦合系数等光栅参数对模式转换器的影响.仿真分析和实验结果表明,通过改变两个子光栅的周期间隔来改变两个损耗峰的位置,形成一个损耗峰,从而可以实现宽带宽的模式转换器,其10dB带宽约是单栅的2倍.与传统的模式转换器相比,该转换器带宽宽、转换效率高,尺寸小、抗干扰能力强,可以在模分复用系统和光通信中得到广泛的应用.     

Kagome结构空芯光子晶体光纤纤芯参数对传输特性的影响

 应用全矢量有限元方法,研究大间距Kagome结构空芯光子晶体光纤中纤芯的大小、形状与壁厚对光纤传输损耗谱的影响。结果表明,某些纤芯尺寸会造成包层中的结构缺陷,易使纤芯基模、表面模及包层模之间发生能量耦合,产生较大损耗。而纤芯形状与壁厚的改变会引起表面模式的变化,从而影响发生在基模与表面模之间反向耦合的位置和强度,使光纤传输频带变窄和损耗变大。据此,提出Kagome结构光纤的纤芯设计思路,即纤芯的大小应使包层保持完整的微结构,纤芯形状应与包层中的单元微结构相楔合,纤芯壁厚应与包层中玻璃支柱的宽度相同。     

基于对称双环嵌套管的低损耗弱耦合六模空芯负曲率光纤

本文设计了一种具有对称双环嵌套管结构的新型低损耗少模空芯负曲率光纤,该光纤支持LP₀₁, LP₁₁,LP₂₁, LP₀₂, LP_31a, LP_31b共6种纤芯模式.所设计的光纤以SiO₂作为基底材料,采用特殊的对称双环嵌套结构将包层区域进行划分,能够有效地减小纤芯模式与包层模式的耦合.使用有限元法对该少模空芯负曲率光纤的结构参数进行优化,并分析了纤芯各个模式的限制损耗和弯曲损耗.仿真结果表明,所提出的少模空芯负曲率光纤能够同时支持弱耦合的6种纤芯模式独立传输(相邻模式间的有效折射率差均大于10^–4,有效地避免了纤芯内模式间的耦合).在400 nm带宽(1.23—1.63μm,覆盖O, E, S, C, L波段)范围内,纤芯中的6个模式均保持低损耗稳定传输.各模式限制损耗在1.4μm处达到最低,其中基模LP₀₁模式的限制损耗最低,为4.3×10^–7 d B/m.此外,当弯...     

空芯光子晶体光纤表面模损耗控制的研究

本文研究了纤芯结构对空芯光子晶体光纤光子带隙和传输损耗的影响,得到了适合光纤制备工艺的纤芯结构．首先利用平面波展开法计算了一定占空比三角形结构的空芯光子晶体光纤的带隙结构,给出了在传输波长λ=1．55μm时光纤的结构参数值,并模拟了纤芯直径对带隙位置和大小的影响,得出纤芯直径的取值范围,通过分析泄露损耗特性得出纤芯壁厚的取值．然后根据分析结果设计出了光纤端面图,运用全矢量有限元法模拟出在不同纤芯直径的情况下的模场分布,通过对比分析得出光纤的最佳纤芯半径R为1．6以-1．75A．研究结果表明,选择合适的纤芯结构既能满足空芯光子晶体光纤的光子带隙和损耗特征,又可以适当降低光纤制备工艺的难度．     

Parity-violating neutron spin rotation in hydrogen and deuterium

We calculate the (parity-violating) spin-rotation angle of a polarized neutron beam through hydrogen and deuterium targets, using pionless effective field theory up to next-to-leading order. Our result is part of a program to obtain the five leading independent low-energy parameters that characterize hadronic parity violation from few-body observables in one systematic and consistent framework. The two spin-rotation angles provide independent constraints on these parameters. Our result for np spin rotation is $\frac{1} {\rho }\frac{{d\varphi _{PV}^{np} }} {{dl}} = \left[ {4.5 \pm 0.5} \right] rad MeV^{ - \frac{1} {2}} \left( {2g^{\left( {^3 S_1 - ^3 P_1 } \right)} + g^{\left( {^3 S_1 - ^3 P_1 } \right)} } \right) - \left[ {18.5 \pm 1.9} \right] rad MeV^{ - \frac{1} {2}} \left( {g_{\left( {\Delta {\rm I} = 0} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} - 2g_{\left( {\Delta {\rm I} = 2} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} } \right)$\frac{1} {\rho }\frac{{d\varphi _{PV}^{np} }} {{dl}} = \left[ {4.5 \pm 0.5} \right] rad MeV^{ - \frac{1} {2}} \left( {2g^{\left( {^3 S_1 - ^3 P_1 } \right)} + g^{\left( {^3 S_1 - ^3 P_1 } \right)} } \right) - \left[ {18.5 \pm 1.9} \right] rad MeV^{ - \frac{1} {2}} \left( {g_{\left( {\Delta {\rm I} = 0} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} - 2g_{\left( {\Delta {\rm I} = 2} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} } \right), while for nd spin rotation we obtain $\frac{1} {\rho }\frac{{d\varphi _{PV}^{nd} }} {{dl}} = \left[ {8.0 \pm 0.8} \right] rad MeV^{ - \frac{1} {2}} g^{\left( {^3 S_1 - ^1 P_1 } \right)} + \left[ {17.0 \pm 1.7} \right] rad MeV^{ - \frac{1} {2}} g^{\left( {^3 S_1 - ^3 P_1 } \right)} + \left[ {2.3 \pm 0.5} \right] rad MeV^{ - \frac{1} {2}} \left( {3g_{\left( {\Delta {\rm I} = 0} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} - 2g_{\left( {\Delta {\rm I} = 1} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} } \right)$\frac{1} {\rho }\frac{{d\varphi _{PV}^{nd} }} {{dl}} = \left[ {8.0 \pm 0.8} \right] rad MeV^{ - \frac{1} {2}} g^{\left( {^3 S_1 - ^1 P_1 } \right)} + \left[ {17.0 \pm 1.7} \right] rad MeV^{ - \frac{1} {2}} g^{\left( {^3 S_1 - ^3 P_1 } \right)} + \left[ {2.3 \pm 0.5} \right] rad MeV^{ - \frac{1} {2}} \left( {3g_{\left( {\Delta {\rm I} = 0} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} - 2g_{\left( {\Delta {\rm I} = 1} \right)}^{\left( {^1 S_0 - ^3 P_0 } \right)} } \right), where the g ^(X-Y), in units of $MeV^{ - \frac{3} {2}}$MeV^{ - \frac{3} {2}}, are the presently unknown parameters in the leading-order parity-violating Lagrangian. Using naıve dimensional analysis to estimate the typical size of the couplings, we expect the signal for standard target densities to be $\left| {\frac{{d\varphi _{PV} }} {{dl}}} \right| \approx \left[ {10^{ - 7} \ldots 10^{ - 6} } \right]\frac{{rad}} {m}$\left| {\frac{{d\varphi _{PV} }} {{dl}}} \right| \approx \left[ {10^{ - 7} \ldots 10^{ - 6} } \right]\frac{{rad}} {m} for both hydrogen and deuterium targets. We find no indication that the nd observable is enhanced compared to the np one. All results are properly renormalized. An estimate of the numerical and systematic uncertainties of our calculations indicates excellent convergence. An appendix contains the relevant partial-wave projectors of the three-nucleon system.     

Characteristics of temperature fluctuation in two-dimensional turbulent Rayleigh-Bénard convection

We study the characteristics of temperature fluctuation in two-dimensional turbulent Rayleigh–Benard convection in′a square cavity by direct numerical simulations.The Rayleigh number range is 1×10⁸≤Ra≤1×10¹³,and the Prandtl number is selected as Pr=0.7 and Pr=4.3.It is found that the temperature fluctuation profiles with respect to Ra exhibit two different distribution patterns.In the thermal boundary layer,the normalized fluctuationθrms/θrms,max is independent of Ra and a power law relation is identified,i.e.,θrms/θrms,max～(z/δ)0.99±0.01,where z/δis a dimensionless distance to the boundary(δis the thickness of thermal boundary layer).Out of the boundary layer,when Ra≤5×10⁹,the profiles ofθrms/θrms,max descend,then ascend,and finally drop dramatically as z/δincreases.While for Ra≥1×10¹⁰,the profiles continuously decrease and finally overlap with each other.The two different characteristics of temperature fluctuations are closely related to the formation of stable large-scale circulations and corner rolls.Besides,there is a critical value of Ra indicating the transition,beyond which the fluctuation hθrmsiV has a power law dependence on Ra,given by hθrmsiV～Ra?0.14±0.01.     

Low-temperature heat capacities and standard molar enthalpy of formation of 4-（2-aminoethyl）-phenol （C8H11NO）

This paper reports that low-temperature heat capacities of 4-（2-aminoethyl）-phenol （C8H11NO） are measured by a precision automated adiabatic calorimeter over the temperature range from 78 to 400 K. A polynomial equation of heat capacities as a function of the temperature was fitted by the least square method. Based on the fitted polynomial, the smoothed heat capacities and thermodynamic functions of the compound relative to the standard reference temperature 298.15K were calculated and tabulated at the interval of 5K. The energy equivalent, εcalor, of the oxygen-bomb combustion calorimeter has been determined from 0.68g of NIST 39i benzoic acid to be εcalor=（14674.69±17.49）J·K^-1. The constant-volume energy of combustion of the compound at T=298.15 K was measured by a precision oxygen-bomb combustion calorimeter to be ΔcU=-（32374.25±12.93）J·g^-1. The standard molar enthalpy of combustion for the compound was calculated to be ΔcHm = -（4445.47 ± 1.77） kJ·mol^-1 according to the definition of enthalpy of combustion and other thermodynamic principles. Finally, the standard molar enthalpy of formation of the compound was derived to be ΔfHm（C8H11NO, s）=-（274.68 ±2.06） kJ·mol^-1, in accordance with Hess law.     

A precise measurement of the tau lifetime

The tau lepton lifetime has been measured with the events collected by the DELPHI detector at LEP in the years 1991-1995. Three different methods have been exploited, using both one-prong and three-prong decay channels. Two measurements have been made using events in which both taus decay to a single charged particle. Combining these measurements gave . A third measurement using taus which decayed to three charged particles yielded These were combined with previous DELPHI results to measure the tau lifetime, using the full LEP1 data sample, to be .Received: 12 November 2003, Revised: 1 June 2004, Published online: 20 July 2004     

利用格点量子色动力学研究手征平滑过渡温度和手征相变温度

回顾了最近关于手征平滑过渡温度和手征相变温度的研究结果。首先给出了在零重子化学势能下的手征平滑过渡温度为156.5(1.5) MeV,其次,给出了在非零重子化学势能下手征相转变曲线的二阶及四阶曲率分别为0.012(4)和0.000(4)。接着讨论了在格点QCD中第一次得到的量子色动力学的手征相变温度。在热力学极限、连续极限及手征极限下,我们得到手征相变温度为132$^{+3}_{-6}$ MeV。     

Searching for isotropic stochastic gravitational-wave background in the international pulsar timing array second data release

We search for isotropic stochastic gravitational-wave background (SGWB) in the International Pulsar Timing Array second data release. By modeling the SGWB as a power-law, we find very strong Bayesian evidence for a common-spectrum process, and further this process has scalar transverse (ST) correlations allowed in general metric theory of gravity as the Bayes factor in favor of the ST-correlated process versus the spatially uncorrelated common-spectrum process is 30 ± 2. The median and the 90% equal-tail amplitudes of ST mode are ${{ \mathcal A }}_{\mathrm{ST}}={1.29}_{-0.44}^{+0.51}\times {10}^{-15}$, or equivalently the energy density parameter per logarithm frequency is ${{\rm{\Omega }}}_{\mathrm{GW}}^{\mathrm{ST}}={2.31}_{-1.30}^{+2.19}\times {10}^{-9}$, at frequency of 1 year⁻¹. However, we do not find any statistically significant evidence for the tensor transverse (TT) mode and then place the 95% upper limits as ${{ \mathcal A }}_{\mathrm{TT}}\lt 3.95\times {10}^{-15}$, or equivalently ${{\rm{\Omega }}}_{\mathrm{GW}}^{\mathrm{TT}}\lt 2.16\times {10}^{-9}$, at frequency of 1 year⁻¹.     

Constraints on $H_0$ from WMAP and BAO Measurements *

We report the constraints of $H_0$ obtained from Wilkinson Microwave Anisotropy Probe (WMAP) 9-year data combined with the latest baryonic acoustic oscillations (BAO) measurements. We use the BAO measurements from 6dF Galaxy Survey (6dFGS), the SDSS DR7 main galaxies sample (MGS), the BOSS DR12 galaxies, and the eBOSS DR14 quasars. Adding the recent BAO measurements to the cosmic microwave background (CMB) data from WMAP, we constrain cosmological parameters $\Omega_m=0.298\pm0.005$, $H_0=68.36^{+0.53}_{-0.52} {\rm km}\cdot {\rm s}^{-1}\cdot {\rm Mpc}^{-1}$, $\sigma_8=0.8170^{+0.0159}_{-0.0175}$ in a spatially flat $\Lambda$ cold dark matter ($\Lambda$CDM) model, and $\Omega_m=0.302\pm0.008$, $H_0=67.63\pm1.30 {\rm km}\cdot{\rm s}^{-1}\cdot {\rm Mpc}^{-1}$, $\sigma_8=0.7988^{+0.0345}_{-0.0338}$ in a spatially flat $w$CDM model, respectively. Our measured $H_0$ results prefer a value lower than 70 ${\rm km}\cdot {\rm s}^{-1}\cdot{\rm Mpc}^{-1}$, consistent with the recent data on CMB constraints from Planck (2018), but in $3.1$ and $3.5\sigma$ tension with local measurements of SH0ES (2018) in $\Lambda$CDM and $w$CDM framework, respectively. Our results indicate that there is a systematic tension on the Hubble constant between SH0ES and the combination of CMB and BAO datasets.     

Impurity effects of the Λhyperon in the hypernuclear systems ${}_{{\rm{\Lambda }}}^{25}\mathrm{Mg}$ and ${}_{{\rm{\Lambda }}}^{29}\mathrm{Si}$

Based on the beyond-mean-field Skyrme–Hartree–Fock model, impurity effects of the Λhyperon in the hypernuclear systems ${}_{\,{\rm{\Lambda }}}^{25}$ Mg and ${}_{\,{\rm{\Lambda }}}^{29}$ Si are investigated, respectively. Four cases, in which the Λhyperon occupies the single-particle orbitals ${\rm{\Lambda }}$[000]${\tfrac{1}{2}}^{+}$, ${\rm{\Lambda }}$[110]${\tfrac{1}{2}}^{-}$, ${\rm{\Lambda }}$[101]${\tfrac{3}{2}}^{-}$ and ${\rm{\Lambda }}$[101]${\tfrac{1}{2}}^{-}$, are focused. In each case, the potential energy surface and the energy curves projected on certain angular momenta are employed to show the influence of the Λhyperon on the nuclear core. Beside the shrinkage effect that is induced by the Λhyperon occupying the s_Λ orbital, it is found that the Λhyperon on the p_Λ orbital, ${\rm{\Lambda }}$[110]${\tfrac{1}{2}}^{-}$, drives the nuclear core toward a prolate shape, while the ones on the other two p_Λ orbitals, ${\rm{\Lambda }}$[101]${\tfrac{3}{2}}^{-}$ and ${\rm{\Lambda }}$[101]${\tfrac{1}{2}}^{-}$, drive the nuclear core toward an oblate shape. The energy spectra and the corresponding intra-band E2 transition rates for the rotational bands are given as a prediction for future experiments.     

Three-Particle Decays of the Higgs Bosons in the Minimal Supersymmetric Standard Model

Russian Physics Journal - Decay channels of the Higgs bosons $$ H\to A\overline{f},\kern1em A\to hf\overline{f},\kern1em {H}^{\pm}\to Hf{\overline{f}}^{\hbox{'}},\kern1em {H}^{\pm}\to...