The cosmological constant problem is reanalyzed by imposing the limitation of the number of degrees of freedom (d.o.f.) due to entropy bounds directly in the calculation of the energy density of a field theory. It is shown that if a quantum field theory has to be consistent with gravity and holography, i.e. with an upper limit of storing information in a given area, the ultraviolet momentum cut-off is not the Planck mass, M_p, as naively expected, but M_p/N_U^(1/4) where N_U is the number of d.o.f. of the universe.
|Titolo:||Holographic Bound in Quantum Field Energy Density and Cosmological Constant|
|Data di pubblicazione:||2013|
|Citazione:||Holographic Bound in Quantum Field Energy Density and Cosmological Constant / Castorina P. - In: JOURNAL OF MODERN PHYSICS. - ISSN 2153-1196. - 4(2013), pp. 807-811.|
|Appare nelle tipologie:||1.1 Articolo in rivista|