The emergence of cosmic repulsion     

《Astroparticle Physics》2015

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Linearized stability of Reissner Nordstrom de-Sitter thin shell wormholes     

《New Astronomy》2015

Using the Darmois–Israel formalism the dynamical analysis of Reissner Nordstrom de-Sitter thin shell wormholes, at the wormhole throat, are determined by considering linearized radial perturbations around static solutions.The region of stability in the presence of a large value of charge is significantly increased. Also, the region of stability in the presence of a positive large value of cosmological constant is significantly increased.  相似文献   

青藏块体强震与祁连山地震带中强震相关性的初步探讨     

李兴坚  陈兰新  周莉萍  常千军  许玉红  李东生  陈建军  刘小明 《地震地磁观测与研究》2004,25(2):22-27

对青藏块体强震与祁连山地震带中强震的相关性进行了初步分析。结果表明：青藏块体发生强地震后,祁连山地震带中强地震活动具有增强趋势。通过分析认为,祁连山地震带已进入新的地震活跃期,并有可能发生7级以上地震。  相似文献   

Classical and quantum anisotropic wormholes in pure general relativity     

《Astroparticle Physics》2013

In the homogeneous and isotropic Friedmann–Robertson–Walker minisuperspace model, it is known that there are no Euclidean wormhole solutions in the pure gravity system. Here it is demonstrated explicitly that in Taub cosmology, which is one of the simplest anisotropic cosmology models, wormhole solutions do exist in pure general relativity in both classical and quantum contexts. Indeed, it is realized that it is the nonvanishing momentum or the energy associated with the anisotropy change, that essentially renders the occurrence of both classical and quantum wormholes possible.  相似文献   

粘性类土侵蚀强度量化研究   总被引：1，自引：0，他引：1  

曹成林  孙永福  宋玉鹏  陈勇 《海岸工程》2010,29(4):65-72

海洋动力作用下,粘性土内部粘结力与重力的联合作用使其冲刷侵蚀特性较为复杂。从侵蚀原理出发,利用粘结力仪进行侵蚀试验,探讨了粘性土临界侵蚀剪应力τ_c与土体物理力学性质之间的相关性,并提出中值粒径、粘粒含量、密度及抗剪强度与τ_c之间的计算关系式。同时通过侵蚀公式计算结果与试验结果比较,验证了试验结果的准确性。  相似文献   

鄂西建始地区页岩储层特征及含气性研究     

仇秀梅  刘亚东  董学林 《岩石矿物学杂志》2019,38(3):365-374

通过对鄂西建始地区页岩储层特征、有机地球化学特征及含气性分析,初步探讨了含气性的相关影响因素。结果表明,储层矿物以石英和粘土矿物为主,孔隙类型主要为有机质孔、矿物溶蚀孔、矿物粒间孔,岩石孔隙度为0. 2%～4. 5%,渗透率平均值为0. 081 0×10~(-3)μm~2,属低孔、特低渗储层;储层具有高有机质丰度、高热演化程度特征,TOC含量平均值为7. 63%,R_o平均值为3. 29%,有机质类型以Ⅱ型干酪根为主;现场解析法测得X井大隆组、龙潭组、孤峰组页岩具有较高的含气量,平均值为1. 32 m~3/t,含气量与有机质丰度、有机质成熟度、孔隙度呈正相关关系,与粘土矿物含量呈弱的正相关关系。该研究可以为鄂西建始地区页岩气的后续勘探开发提供依据。  相似文献   

Crustal oscillations of slowly rotating relativistic stars     

M. Vavoulidis  K. D. Kokkotas  A. Stavridis 《Monthly notices of the Royal Astronomical Society》2008,384(4):1711-1724

We study low-amplitude crustal oscillations of slowly rotating relativistic stars consisting of a central fluid core and an outer thin solid crust. We estimate the effect of rotation on the torsional toroidal modes and on the interfacial and shear spheroidal modes. The results compared against the Newtonian ones for wide range of neutron star models and equations of state.  相似文献   

Spinar paradigm and the central engine of gamma-ray bursts     

V. M. Lipunov  E. S. Gorbovskoy 《Monthly notices of the Royal Astronomical Society》2008,383(4):1397-1412

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Constraints on the magnetic field geometry of magnetars     

H. Sotani  A. Colaiuda  K. D. Kokkotas 《Monthly notices of the Royal Astronomical Society》2008,385(4):2161-2165

We study the effect of the magnetic field geometry on the oscillation spectra of strongly magnetized stars. We construct a configuration of magnetic field where a toroidal component is added to the standard poloidal one. We consider a star with a type I superconductor core so that both components of the magnetic field are expelled from the core and confined in the crust. Our results show that the toroidal contribution does not influence significantly the torsional oscillations of the crust. On the contrary, the confinement of the magnetic field in the crust drastically affects the torsional oscillation spectrum. A comparison with estimations for the magnetic field strength, from observations, excludes the possibility that magnetars will have a magnetic field solely confined in the crust, that is, our results suggest that the magnetic field in whatever geometry has to permeate the whole star.  相似文献   

On the variability and spectral distortion of fluorescent iron lines from black hole accretion discs     

Andrzej Nied&#;wiecki  Piotr T. &#;ycki 《Monthly notices of the Royal Astronomical Society》2008,386(2):759-780

We investigate the properties of fluorescent iron lines that arise as a result of the illumination of a black hole accretion disc by an X-ray source located above the disc's surface. We study in detail the light-bending model of the variability of the lines, extending previous work on the subject. We indicate that the bending of photon trajectories to the equatorial plane (a distinct property of the Kerr metric) is the most feasible effect underlying the reduced variability of the lines observed in several objects. A model involving an X-ray source with a varying radial distance, located within a few central gravitational radii around a rapidly rotating black hole, close to the disc's surface, may explain both the elongated red wing of the line profile and the complex variability pattern observed in MCG–6-30-15 by XMM–Newton . We also point out that illumination by radiation that returns to the disc (following the previous reflection) contributes significantly to the formation of the line profile in some cases. As a result of this effect, the line profile always has a pronounced blue peak (which is not observed in the deep minimum state in MCG–6-30-15), unless the reflecting material is absent within the innermost 2–3 gravitational radii.  相似文献