5۔شرعی و قانونی ماہرین کی قلت
حدود و قصاص قوانین کے لیے جس طرح کے ماہرین درکار ہیں ، وہ بہت کم یاب بلکہ نایاب ہیں ۔ نفاذ اسلام کے لیے مختلف شعبوں میں جس طرح کے ماہرین درکار ہیں ، اس طرح کے ماہرین تیار کرنے کا پاکستان میں کوئی جامع انتظام نہیں ہے۔ اگر آج ایسی حکومت برسراقتدار آ جائے جو سو فیصد اسلام نافذ کرنا چاہے تو معاشرے میں بہت زیادہ دینی جذبہ رکھنے والے تو مل جائیں گے لیکن بینکاری کے حوالے سے بینکوں کے جدید نظام اور شریعت کے احکام میں ماہر افراد شاید انگلیوں پر بھی نہ گئے جاسکیں۔ ایسے کتنے وکلا ء ہیں جو دنیا میں قانون سازی اور قانون دانی میں ماہر مانے جاتے ہوں اور شریعت میں ان کی مہارت بھی مسلّم ہو اور ان کی زندگی اسلامی تعلیمات سے عبارت بھی ہو۔ یہی حال ہمارے معاشرے میں دیگرشعبوں کا ہے
یہ ایک ایسا پہلو ہے جس پر جتنی جلد توجہ دی جائے اتنا ہی ضروری ہے ۔ جب تک ایسی ٹیم تیار نہیں ہوگی اور مطلوبہ افراد میسر نہیں ہوں گے ، یہ کام نہیں ہو سکتا۔ قانون سازی اور اسلامی عدالتوں کے قیام کے لیے جوں جوں کام شروع ہو، افراد بھی تیار ہوتے جائیں گے ، ادارے بھی بنتے جائیں گے اورعملی طورپر کام بھی ہوتا چلا جائے گا۔
It has been the norm of the West that they allay the blessings and reforms brought into the world towards themselves as if the rest of the World was drenched into darknessof ignorance. The concept of Human Rights has laso been allayed to the British Magna Carta, though Islam has offered the most complete and comprehensive Human rights foundation hundred years earlier, aboout 600 years prior to Magna Carta. This research article pertains to a comparative study of the charter of Human Rights by UNO and the comprehensive socio-political and economic sphere of Human Rights by Islam.
In recent years, an exceptional progress has exposed a great deal of information about the formation and evolution of large-scale struc- tures in this stunning star-spangled Universe. But, with more infor- mation comes many thought-provoking questions for theorists. The images obtained by the Hubble Space Telescope (HST ) has revealed that basic large-scale structures are shaped at the non-stationary non- linear stage of their evolution; therefore modern extragalactic astron- omy is compelled to study early non-linear stages of evolution of self- gravitational systems. A great role is played by global pulsations in different stages of the formation of galaxies. Incidentally though, reliable mechanisms of development of their sub-structures, as well as possible various non- linear effects are not yet fully revealed. Similarly, the physics of the formation of large-scale structures in the non-stationary universe is not completely available. Many authors have put forward various specific models of the system that gravitate. Binney and Tremaine (1987) have obtained a large number of results. The basis of the most of these results are on the linearisation of the Euler-Poison and Vlasov Poison systems around a stationary solution. Kalnajs (1972) has covered milestones in station- ary models of self-gravitating systems. Although the stationary mod- els of gravitating systems are abundance in the research, the presence of non-stationary models is very conspicuous among various models for study of dynamical development of large-scale structures. There- fore it seemed necessary to develop a new non-linear model which is viinon-stationary in nature and discuss its stability, so that our model will be more accurate. Gravitational instability with respect to lopsided oscillation mode is examined in this dissertation. A phase model of non-stationary self- gravitating disks with isotropic and anisotropic diagrams has been constructed. We used well-known generalization of the Bisnovatyi- Kogan-Zel’dovich model is used in order to find out the formation criteria of galaxies whose nucleus is away from their center (lopsided galaxies). Non-stationary dispersion relations are obtained for both isotropic and anisotropic models of lopsided mode. ) calculations ( The 2T show the relationship between initial virial ratio |U and degree of | ◦ rotation Ω. A comparative analysis of increment (growth rate) of lop- sided mode with other oscillatory modes is made and concluded that lopsided mode has a clear lead over other oscillatory modes. A radial instability always occurs if total kinetic energy is no more than 12.4% of the initial potential energy, in non-stationary isotropic model for lopsided mode. Also, it has been shown that instability is aperiodic when Ω = 0 and oscillatory when Ω ̸ = 0. This ratio of total kinetic energy and total potential energy becomes 30.6% for an anisotropic model of lopsided structure. In this thesis, a multi-parameter composite model by the method of linear superposition has also been constructed and analyzed the stabil- ity of lopsided mode for this model. This new composite model inves- tigates intermediate stages between isotropic and anisotropic models. In the end, the application of lopsidedness in our solar system is dis- cussed. Here, we suggested that G. Darwin’s theory of origin of moon would be acceptable if he had calculated his model in the background of non-stationary and non-equilibrium theory. It has been shown that if Nuritdinov’s non-stationary spherical model is applied on the earth- moon system and calculated that at the initial moment of collapse, the kinetic energy will be lesser than 22.3% of the potential energy viiiwhere instability occurred and the earth became lopsided and then split into two parts and hence the moon came into existence.