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81.
82.
Fadhel Al‐Musallam Amin Boumenir 《Mathematical Methods in the Applied Sciences》2014,37(11):1610-1623
We are concerned with the reconstruction of a non‐differentiable acoustic stiffness reactance coefficient of a one‐dimensional hyperbolic equation using the smallest possible number of boundary readings generated by classical initial conditions. To this end, a complete set of spectral data of a string is extracted from either a single or at most two readings of the trace of the solution on the boundary. The sought coefficient is then uniquely recovered by the Krein inverse spectral theory. Copyright © 2013 John Wiley & Sons, Ltd. 相似文献
83.
对小井眼、大曲率井中钻柱强度问题,以井轴为基准轴,在对井轴弯挠描述和钻柱微段三维受力变形分析的基础上,建立大位移钻柱平衡微分方程,采用Longe-Kutta法解之求内力,并依此求应力和建立强度条件.对H767侧钻水平井施工中钻柱应力计算分析,结果说明与有限元模型和弹性化软绳模型比较相吻合,该模型比有限元模型计算简捷方便;比弹性化软绳模型更完善可信;该井钻柱破坏事故愿因在于井眼曲率过大,兼有应力集中. 相似文献
84.
Ignattos Antoniadis 《Pramana》2004,62(2):163-176
The recent understanding of string theory opens the possibility that the string scale can be as low as a few TeV. The apparent
weakness of gravitational interactions can then be accounted by the existence of large internal dimensions, in the sub-millimeter
region. Furthermore, our world must be confined to live on a brane transverse to these large dimensions, with which it interacts
only gravitationally. In my lecture, I describe briefly this scenario which gives a new theoretical framework for solving
the gauge hierarchy problem and the unification of all interactions. I also discuss a minimal embedding of the standard model,
gauge coupling unification and proton stability.
On leave from: Centre de Physique Théorique, Ecole Polytechnique, 91128 Palaiseau, Cedex, France. 相似文献
85.
We study a relativistic quantum particle in cosmic string spacetime in the presence of a magnetic field and a Coulomb-type scalar potential. It is shown that the radial part of this problem possesses the su(1,1) symmetry. We obtain the energy spectrum and eigenfunctions of this problem by using two algebraic methods: the Schrödinger factorization and the tilting transformation. Finally, we give the explicit form of the relativistic coherent states for this problem. 相似文献
86.
We construct stable bundle extensions on elliptically fibered Calabi–Yau threefolds. We show that these bundles can solve the topological anomaly constraint in heterotic string theory without the need for invoking background five-branes. 相似文献
87.
V. Dzhunushaliev 《Annalen der Physik》2006,15(9):671-677
It is shown that in the standard vacuum 5D Kaluza‐Klein gravity there exist wormhole‐like solutions which look like strings attached to two D‐branes. The asymptotic behaviour of the corresponding metric is investigated. 相似文献
88.
The dynamic string motion, which displacement is unilaterally constrained by the rigid termination condition of an arbitrary geometry has been simulated and analyzed. The treble strings of a grand piano usually terminate at a capo bar, which is situated above the strings. The apex of a V-shaped section of the capo bar defines the end of the speaking length of the strings. A numerical calculation based on the traveling wave solution is proposed for modeling the nonlinearity inducing interactions between the vibrating string and the contact condition at the point of string termination. It was shown that the lossless string vibrates in two distinct vibration regimes. In the beginning the string starts to interact in a nonlinear fashion with the rigid terminator, and the resulting string motion is aperiodic. Consequently, the spectrum of the string motion depends on the amplitude of string vibrations, and its spectral structure changes continuously with the passage of time. The duration of that vibration regime depends on the geometry of the terminator. After some time of aperiodic vibration, the string vibrations settle in a periodic regime where the resulting spectrum remains constant. 相似文献
89.
F.?RahamanEmail author B.?C.?Bhui M.?Kalam 《International Journal of Theoretical Physics》2005,44(9):1413-1418
We analyze the space-time structure of local gauge string with a phenomenological energy–momentum tensor, as prescribed by
Vilenkin, in an arbitrary number of space-time dimensions with a non-zero cosmological constant Λ. A set of solutions of the
full non-linear Einstein's equations for the interior region of such a string is presented. 相似文献
90.