Abstract
Quantized solutions of the Wheeler–DeWitt (WDW) equation describing a closed Friedmann–Robertson–Walker universe with a $$\Lambda $$ term and a set of massless scalar fields are studied. It is shown that when $$\Lambda \ll 1$$ units and the standard in-vacuum state is considered, the wave function of the universe $$\Psi $$ behaves as a random quasiclassical field at rather large a, namely, $$1 \ll a \ll {{e}^{{\frac{2}{{3\Lambda }}}}}$$ [1].
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
