首页 | 本学科首页   官方微博 | 高级检索  
文章检索
  按 检索   检索词:      
出版年份:   被引次数:   他引次数: 提示:输入*表示无穷大
  收费全文   557546篇
  免费   4478篇
  国内免费   1116篇
化学   266354篇
晶体学   7762篇
力学   29860篇
综合类   12篇
数学   85771篇
物理学   173381篇
  2021年   4407篇
  2020年   5077篇
  2019年   5816篇
  2018年   13202篇
  2017年   13634篇
  2016年   13973篇
  2015年   6942篇
  2014年   10414篇
  2013年   22024篇
  2012年   21124篇
  2011年   29106篇
  2010年   20326篇
  2009年   20380篇
  2008年   26635篇
  2007年   28423篇
  2006年   18252篇
  2005年   19936篇
  2004年   17076篇
  2003年   15718篇
  2002年   14680篇
  2001年   13884篇
  2000年   11214篇
  1999年   8231篇
  1998年   7179篇
  1997年   6958篇
  1996年   6835篇
  1995年   5904篇
  1994年   5898篇
  1993年   5797篇
  1992年   6079篇
  1991年   6385篇
  1990年   6148篇
  1989年   6064篇
  1988年   5835篇
  1987年   5838篇
  1986年   5455篇
  1985年   6943篇
  1984年   7190篇
  1983年   6014篇
  1982年   6370篇
  1981年   5960篇
  1980年   5627篇
  1979年   6062篇
  1978年   6237篇
  1977年   6280篇
  1976年   6311篇
  1975年   5970篇
  1974年   5746篇
  1973年   6034篇
  1972年   4506篇
排序方式: 共有10000条查询结果,搜索用时 15 毫秒
81.
The mass power spectrum for a Universe dominated by the Chaplygin gas is evaluated numerically from scales of the order of the Hubble horizon to 100 Mpc. The results are compared with a pure baryonic Universe and a cosmological constant model. In all three cases, the spectrum increases with k, the wavenumber of the perturbations. The slope of the spectrum is higher for the baryonic model and smaller for the cosmological constant model, the Chaplygin gas interpolating these two models. The results are analyzed in terms of the sound velocity of the Chaplygin gas and the moment the Universe begins to accelerate.  相似文献   
82.
In this paper, a two-dimensional finite volume unstructured mesh method (FVUM) based on a triangular background interpolation mesh is developed for analysing the evolution of the saltwater intrusion into single and multiple coastal aquifer systems. The model formulation consists of a ground-water flow equation and a salt transport equation. These coupled and non-linear partial differential equations are transformed by FVUM into a system of differential/algebraic equations, which is solved using backward differentiation formulas of order one through five. Simulation results are compared with previously published solutions where good agreement is observed.  相似文献   
83.
Deformation quantization, which achieves the passage from classical mechanics to quantum mechanics by the replacement of the pointwise multiplication of functions on phase space by the star product, is a powerful tool for treating systems involving bosonic degrees of freedom, both in quantum mechanics and in quantum field theory. In the present paper we show how these methods may be naturally extended to systems involving fermions. In particular we show how supersymmetric quantum mechanics can be formulated in this approach and consider examples involving both non-relativistic and relativistic systems.  相似文献   
84.
Optics and Spectroscopy - The relationship between the parameters of quadripoles (mirrors, for example) ensuring the fulfillment of the energy conservation law are considered. Apart from the...  相似文献   
85.
The Wheeler–DeWitt equation of arbitrary Hartle–Hawking factor ordering for several minisuperspace universe models, such as the pure gravity Friedmann–Robertson–Walker and Taub ones, is mapped onto the dynamics of corresponding classical oscillators. The latter ones are studied by the classical Ermakov invariant method, which is a natural approach in this context. For the more realistic case of a minimally coupled massive scalar field, one can study, within the same type of approach, the corresponding squeezing features as a possible means of describing cosmological evolution. Finally, we comment on the analogy with the accelerator physics.  相似文献   
86.
87.
Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 54, No. 3, pp. 438–444, March, 1991.  相似文献   
88.
Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 55, No. 4, pp. 535–540, October, 1991.  相似文献   
89.
90.
Dependence of the phase transition temperature on the domain size is investigated for a double-well quadratic potential. It is shown that for a domain whose boundary is subjected to a hydrostatical pressure, the temperature of phase transitions is independent of the domain and the surface tension coefficient and depends exclusively on the properties of the elastic media. If the displacement field vanishes on the boundary, then for sufficiently small domains, the temperature also does not depend on the surface tension and domain size and is determined by properties of the elastic media only. Bibliography: 8 titles. __________ Translated from Zapiski Nauchnykh Seminarov POMI, Vol. 310, 2004, pp. 98–113.  相似文献   
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号