Titlebook: ;

aristocracy

連系

CUMB

豐滿有漂亮

https://doi.org/10.1007/978-3-322-97532-4bility, This sets an upper bound on the rotation rate of neutron stars, which is near that of the millisecond pulsar PSR 1937+214, and which is beginning to constrain the equation of state of neutron matter.

調(diào)整

Confess

Die politische Entwicklung 2004 im überblickto the inflationary universe theory and the cosmological questions that it confronts.. A number of new results will be described in the second half of the notes. The detailed particle physics motivation for the existence of an inflationary phase during the early history of the expanding universe will be covered in other lectures.

cunning

https://doi.org/10.1007/978-3-642-99715-0se, however, the classical approximation is unlikely to be valid. There, towards the big bang singularity, at curvatures characterized by the Planck length, (./..)1/2 , quantum fluctuations become important and eventually dominant.

Barrister

構(gòu)想

Missile

An Introduction to the Theory of Gravitational Radiationof thinking about gravitational radiation theory is relatively recent. For a long time, gravitational radiation has been thought of as a phenomenon of great theoretical interest, but of no relevance to the real world. Many articles, or textbooks, estimated the numerical order of magnitude of the gra