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51.
52.
The dependence of emission direction of fast electrons on the laser intensity has been investigated. The experimental results show that, at nonrelativistic laser intensities, the emission of fast electrons is mainly in the polarization plane. With the increase of the laser intensity, fast electrons emit towards the laser propagation direction from laser polarization direction. At relativistic laser intensities, fast electrons move away from the laser polarization plane, closely to the reflection direction of the incident laser beam. 相似文献
53.
J.-F. Pascual-Sánchez A. San Miguel F. Vicente 《General Relativity and Gravitation》2004,36(9):2075-2083
We analyze the geometry of a rotating disk with a tangential acceleration in the framework of the theory of Special Relativity, using the kinematic linear differential system that verifies the relative position vector of time-like curves in a Fermi reference. A numerical integration of these equations for a generic initial value problem is made up and the results are compared with those obtained in other works. 相似文献
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55.
H. Hora 《Czechoslovak Journal of Physics》2003,53(3):199-217
The anomaly of ion emission at laser irradiation of targets measured by Badziak et al. was analyzed on the background of the extensive research in the past. In contrast to the irradiation with lasers of longer than 100 ps pulse duration, a drastic decrease of the maximum ion energies was measured with ps pulses. Very strange was the observation that the number of emitted fast ions was intensity independent. The usual ponderomotive or relativistic self-focusing theory and related processes could not explain the results. Instead a direct interaction within the skin depth of the irradiated target was concluded. This model confirms the plane geometry nonlinear force interaction in the ps range producing fast plasma blocks moving perpendicular off or into the target. The block moving into the target opens a new scheme of laser fusion by modifying the experiments of Norreys et al. The use of relatively low subrelativistic laser intensities for the new scheme of laser fusion is evaluated on the background of the long years studies of nonlinear force driven plasma blocks and earlier interpenetration fusion reactions for providing the parameters for expected fusion gains much higher than the experiment of Norreys et al. for a fusion power scheme. 相似文献
56.
为了探索超热电子的加热机制,利用光学CCD相机和OMA光学多道分析仪,分别在靶背法线方向测量了光学渡越辐射(OTR)积分成像图案和光谱。实验在100 TW掺钛蓝宝石激光器上进行,飞秒激光与铜膜靶作用后,靶表面发光信号由空间分辨装置聚焦成像并引到CCD或OMA谱仪的狭缝上。测得的积分成像图案呈圆环状,光斑形成区域直径约为225 μm,在圆环边缘附近出现局部化明亮光信号,该现象表明,超热电子在传输的过程中存在成丝效应,其分布也不均匀。光谱在300~500 nm之间出现一系列非周期锐利尖峰,在400 nm(2ω0)附近出现的尖峰应归因于v×B加热机制产生的超热电子引起的相干渡越辐射(CTR)。 相似文献
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Vitaly N. Melnikov 《Frontiers of Physics in China》2009,4(1):75-93
A review of different cosmological models in diverse dimensions leading to a relatively small time variation in the effective
gravitational constant G is presented. Among them: the 4-dimensional (4-D) general scalar-tensor model, the multidimensional vacuum model with two
curved Einstein spaces, the multidimensional model with the multicomponent anisotropic “perfect fluid”, the S-brane model
with scalar fields and two form fields, etc. It is shown that there exist different possible ways of explaining relatively
small time variations of the effective gravitational constant G compatible with present cosmological data (e.g. acceleration): 4-dimensional scalar-tensor theories or multidimensional cosmological
models with different matter sources. The experimental bounds on Ġ may be satisfied either in some restricted interval or
for all allowed values of the synchronous time variable.
相似文献
60.
V. A. Kudryavtsev L. Pandola V. Tomasello 《The European Physical Journal A - Hadrons and Nuclei》2008,36(2):171-180
Background induced by neutrons in deep underground laboratories is a critical issue for all experiments looking for rare events,
such as dark matter interactions or neutrinoless ββ decay. Neutrons can be produced either by natural radioactivity, via spontaneous
fission or (α, n) reactions, or by interactions initiated by high-energy cosmic rays. In all underground experiments, Monte Carlo simulations
of neutron background play a crucial role for the evaluation of the total background rate and for the optimization of rejection
strategies. The Monte Carlo methods that are commonly employed to evaluate neutron-induced background and to optimize the
experimental setup, are reviewed and discussed. Focus is given to the issue of reliability of Monte Carlo background estimates.
We dedicate this work to the memory of our friend and colleague Nicola Ferrari, who prematurely passed away in July 2006. 相似文献