Noncommutative branch-cut quantum gravity with a self-coupling inflaton scalar field: The wave function of the Universe

This article focuses on the implications of a noncommutative formulation of branch-cut quantum gravity. Based on a mini-superspace structure that obeys the noncommutative Poisson algebra, combined with the Wheeler–DeWitt equation and Hořava–Lifshitz quantum gravity, we explore the impact of a scalar field of the inflaton-type in the evolution of the Universe's wave function. Taking as a starting point the Hořava–Lifshitz action, which depends on the scalar curvature of the branched Universe and its derivatives, the corresponding wave equations are derived and solved. The noncommutative quantum gravity approach adopted preserves the diffeomorphism property of General Relativity, maintaining compatibility with the Arnowitt–Deser–Misner Formalism. In this work we delve deeper into a mini-superspace of noncommutative variables, incorporating scalar inflaton fields and exploring inflationary models, particularly chaotic and nonchaotic scenarios. We obtained solutions to the wave equations without resorting to numerical approximations. The results indicate that the noncommutative algebraic space captures low and high spacetime scales, driving the exponential acceleration of the Universe.     

云南倒春寒天气过程的分析研究

利用常规观测和NCEP 1°×1°的6小时再分析资料,总结1980-2011年云南15次低温雨雪强倒春寒天气过程,得出500 hPa形势高纬为两槽一脊和横槽型,700 hPa为典型北高南低特征.重点分析2011年3月14-19日和2005年3月2-6日不同类型下两次强过程,过程中均有昆明准静止锋增强和川滇切变线南下,新西伯利亚冷空气南下自东北向西南侵入云南.前者地面强降温由中低层强冷平流引发,而后者是由低层强冷平流和高层强冷平流下传共同造成.强雨雪天气对应有深厚垂直上升运动或对流层中低层以下层存在强上升运动柱.孟加拉湾为水汽源地,强高、低空急流和其垂直耦合的次级环流输送了水汽和热量.强降雪期间,无南支槽时需要大而强的水汽通量和水汽辐合,有南支槽配合时中低层水汽通量有迅速增加过程.低层为冷层或近地面强冷平流利于降水物冷凝成雪.过程中均有强锋生作用推动锋面南下,锋面前进方向锋生函数零线对应低层850 hPaQ矢量辐合线,锋区梯度大,能量积聚多对应降雪范围大.低层等露点线有Ω型特征,露点锋抬升作用触发干湿交界面上干冷、暖湿气流交汇,露点锋和低空急流位置强度及Q矢量辐合区与云南强倒春寒降雪区有较好对应关系,地面降温幅度与850 hPa锋生函数正值强度成正比.     

螺杆钻侧钻分支绕障技术处理绳索取心钻孔事故

绳索取心钻进施工中常出现卡钻、埋钻和钻具断裂事故。一些孔内事故处理需要很长时间,尤其是深孔事故发生后投入了大量的财力、人力进行处理,最终还不一定能取得成功。在此情况下,采用侧钻绕障而避开孔内事故钻具则是一种理想的选择,可大大缩短事故处理时间,避免钻孔报废带来的损失。重庆北碚龙车勘探区ZK6-2孔运用螺杆定向钻进侧钻分支绕障方法取得成功,并积累了宝贵的经验。     

大型港口集装箱船舶智能配载的集成算法研究

为解决集装箱码头智能化配载多业务规则集成优化问题,提出3层规划框架,重点研究第2层规划方法。该方法对资源分配规则,建立数学模型;对质量匹配规则和胎吊冲突规则,建立逻辑学模型;这些模型均以剪枝条件的形式融入到分支限界搜索中,而剪枝条件的正确性和有效性均有严格的证明保证。对于其它的业务规则,在生成和压缩解空间的过程中就已经充分考虑。同时并不忽略卸货港、尺寸、箱型等重要属性及其对配船位置的限制,实验结果验证算法的有效性。     

岩土层速度结构回折波探测原理与方法

岩上层波速有随深度增加的总趋势。用浅层折射法记录到的折射波均属回折波。本文采用垂向速度梯度为不同正的常数多层水平层状介质模型，推导出回析波正反演公式，有简单解析表达式，据此解释的实测剖面，与验证孔波速测井资料相当吻合。表明在岩土层保持天然结构和横向比较均匀地区，回折波探测方法有良好应用前景。     

湖南东坡野鸡尾蚀变岩枝型锡多金属矿床地质特征及成因

野鸡尾矿床为一新型锡多金属矿床。本文研究了蚀变岩枝的特征,并论证其为千里山复式岩体第二期侵入体(γ_5~(2-2))的一个高侵位岩枝。认为矿液是沿接触带上升的。文章还研究了成矿物质的来源及成矿的物理化学条件。     

The distance to Galactic globular clusters through RR Lyrae pulsational properties

By adopting the same approach outlined by De Santis & Cassisi, we evaluate the absolute bolometric magnitude of the zero-age horizontal branch (ZAHB) at the level of the RR Lyrae variable instability strip in selected Galactic globular clusters. This allows us to estimate the ZAHB absolute visual magnitude for these clusters and to investigate its dependence on the cluster metallicity. The derived M _V (ZAHB)–[Fe/H] relation, corrected in order to account for the luminosity difference between the ZAHB and the mean RR Lyrae magnitude, has been compared with some of the most recent empirical determinations in this field, such as the one provided by Baade–Wesselink analyses, RR Lyrae periods, Hipparcos data for field variables and main-sequence fitting based on Hipparcos parallaxes for field subdwarfs. As a result, our relation provides a clear support to the 'long' distance scale. We discuss also another method for measuring the distance to Galactic globular clusters. This method is quite similar to the one adopted for estimating the absolute bolometric magnitude of the ZAHB but it relies only on the pulsational properties of the Lyrae variables in each cluster. The reliability and accuracy of this method have been tested by applying it to a sample of globular clusters for which, owing to the morphology of their horizontal branch (HB), the use of the commonly adopted ZAHB fitting is a risky procedure. We notice that the two approaches for deriving the cluster distance modulus provide consistent results when applied to globular clusters, the RR Lyrae instability strip is well populated. As the adopted method relies on theoretical predictions on both the fundamental pulsational equation and the allowed mass range for fundamental pulsators, we give an estimate of the error affecting present results, owing to systematic uncertainties in the adopted theoretical framework.