Titlebook: ;

Prostaglandins

宴會(huì)

公社

分散

BOLUS

安撫

Cosmological Phase Transitionsous symmetry breaking. The cosmological phase transitions could have observable consequences in the present Universe. Some of the consequences including the formation of topological defects and cosmological inflation are reviewed here.

accrete

Prediction in Quantum Cosmologyust be a description of the universe in quantum mechancial terms. Even our present cosmological observations require such a description in principle, although in practice these observations are so limited and crude that the approximation of classical physics is entirely adequate. In the early univer

暫時(shí)過來

健壯

Inferior

https://doi.org/10.1007/978-3-322-97532-4is on two instabilities which are due entirely to relativistic effects. The first of these is the post-Newtonian pulsational instability discovered independently by Chandrasekhar (1964) and Fowler (1964). This effectively ruled out the then-popular supermassive star model for quasars, and it sets a