Titlebook: ;

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書目名稱Gravitational Lensing: Strong, Weak and Micro影響因子(影響力)




書目名稱Gravitational Lensing: Strong, Weak and Micro影響因子(影響力)學(xué)科排名




書目名稱Gravitational Lensing: Strong, Weak and Micro網(wǎng)絡(luò)公開度




書目名稱Gravitational Lensing: Strong, Weak and Micro網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Gravitational Lensing: Strong, Weak and Micro被引頻次




書目名稱Gravitational Lensing: Strong, Weak and Micro被引頻次學(xué)科排名




書目名稱Gravitational Lensing: Strong, Weak and Micro年度引用




書目名稱Gravitational Lensing: Strong, Weak and Micro年度引用學(xué)科排名




書目名稱Gravitational Lensing: Strong, Weak and Micro讀者反饋




書目名稱Gravitational Lensing: Strong, Weak and Micro讀者反饋學(xué)科排名

磨碎

https://doi.org/10.1007/978-3-540-73815-2. This translates into Einstein radii/angular separations of a milli-arcsecond or smaller for the two main distance regimes: “galactic” – lens/source distances of order 10 kpc, and “extragalactic/cosmological” – lens/source distances of order Gpc. Both regimes will be discussed at length in the subsequent sections.

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Introduction to Gravitational Lensing and Cosmology,e. The phenomena of light propagation in strong gravitational fields, as it occurs near the surface of neutron stars or black holes, are usually not incorporated into gravitational lensing – although the physics is the same, these strong-field effects require a rather different mathematical description than the weak deflection phenomena.

人造

Introduction to Gravitational Lensing and Cosmology,vides the correct description of gravity – it was only after Einstein’s final formulation of this theory that the effect was described quantitatively. The rich phenomena which are caused by this gravitational light deflection has led to the development of the rather recent active research field of g

人造

amplitude

Weak Gravitational Lensing,e unit matrix, which implies weak distortions and small magnifications. Those cannot be identified in individual sources, but only in a statistical sense. Because of that, the accuracy of any weak lensing study will depend on the number of sources which can be used for the weak lensing analysis. Thi

HAWK

Gravitational Microlensing,ultiple images are formed, but their typical separation – . 2 .E – is far below the limiting resolution determined by observational constraints. Given the dependence of the Einstein radius on lens mass and geometry, it is clear that microlensing will occur for sufficiently small masses and sufficien

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