View source for Derivation of Weinberg's Relation in a Inflationary Universe

{{Infobox paper
| title = Derivation of Weinberg's Relation in a Inflationary Universe
| url = [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_5299.pdf Link to paper]
| author = [[Ioannis Iraklis Haranas]]
| keywords = [[Inflationary cosmology]], [[quantum field theory]], [[elementary particle]], [[mass of the pion]], [[cosmological constant]]
| published = 2003
| journal = [[Vixra]]
| volume = ROAJ  13 and SAO/NASA Astrophy
| number = 2
| num_pages = 7
| pages = 111-117
}}

'''Read the full paper''' [http://www.naturalphilosophy.org/pdf/abstracts/abstracts_5299.pdf here]

==Abstract==

We propose a derivation of the empirical Weinberg relation for the mass of an elementary  particle and in an inflationary type of universe. Our derivation produces the standard  well known Weinberg relation for the mass of an elementary particle, along with an extra  term which depends on the inflationary potential, as well as Hubble's constant. The  derivation is based on Zeldovich's result for the cosmological constant &#923;, in the context  of quantum field theory. The extra term can be understood as a small correction to the  mass of the elementary particle due to inflation. This term also enables us to calculate,  the initial value of the field &#966;O for two kinds of potentials chosen, which makes  Weinberg's relation possible. Closed and flat and open universes give the mass of the  particles close to the mass of a pion, 140 MeV/c2 or as the one also predicted by  Weinberg's relation.

[[Category:Scientific Paper|derivation weinberg 's relation inflationary universe]]

[[Category:Quantum Theory]]