The Possibility of Particles Forming from a Bose-Einstein Condensate, in an Intense Magnetic or Gravitational Field

Abstract

In the paper -based on a previous work regarding the cold particles forming process as collapsed cold clusters of gammons-considered as pairs: γ * = (ee + ) of axially coupled electrons with opposed charges, is analyzed the possibility of gammons pre-cluster forming from a Bose-Einstein condensate formed in the magnetic and in the gravitational field of a star. By known relations of a BEC forming, it is argued that-in the magnetic field of a star, the forming of a gammonic BEC with particles density N 0 corresponding to those of a pre-cluster of gammons which may generates a particle-like stable cluster, may occurs-for a transition temperature T BE ≈ 10 3 K, in a specific interval of field intensity and of temperature: B = (2.2x10 6 ÷ 8.3x10 7 ) T and T p = (4.8x10 -11 ÷ 1.8x10 -10 ) K. The possible mechanism of the formed BEC transforming into pre-clusters of gammons which may become particle-like collapsed BEC, is a pearlitization mechanism, resulted as fragmentation of the formed BEC. It is argued that the particles forming from chiral quantum vacuum fluctuations is possible at T →0K, either by a vortexial, magnetic-like field corresponding to B ≥ 10 4 T or by already formed gammons, in a "step-by-step" process.