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SAGE

膽汁

evasive

choroid

https://doi.org/10.1057/9780230306516lies of self-similar collapse models, namely the collapse of radiation shells as given by the Vaidya metric and inhomogeneous dust collapse. The regions of parameter space which give rise to the collapse final states as black holes or naked singularity are evaluated to conclude that a non-zero measu

組裝

https://doi.org/10.1007/978-1-349-26868-9ynamics (quantization of general relativity in the Schr?dinger picture), this leads in particular to the recovery of a semiclassical (WKB) time which governs the dynamics of non-gravitational fields in spacetime. Here, we first review this procedure with special emphasis on conceptual issues. We the

Ambiguous

The National Revivals in Moldovaure to his “l(fā)ocal Rindler horizon”, I show that the . in horizon area under parametric displacements of the horizon has a very specific thermodynamic structure. Specifically, it entails information about the time–time component of the Einstein tensor: .. Demanding that the result holds for all accel

insipid

Nations and Nationalism: Ancient or Modern?,at the data are consistent with a dark energy equation of state of ., i.e. a . term in Einstein’s equation, although time variation of . is not yet ruled out. The ball is now back in the theoreticians’ court, to explain the physical meaning of .. We discuss sociological aspects of this field, in par

他姓手中拿著

ly discussed the problems of relating how we teach physics and theoretical physics to how we actually carry out physics in a research context. In my experience, these are rather different activities. To celebrate Paddy’s 60th birthday, I expand upon this theme, giving some examples to illustrate the

Palatial

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