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

In the paper - based on a previous work regarding the cold particles forming process as collapsed cold clusters of gammons- considered as pairs: g * = (e -e +) 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 3K, 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 3 10 4 T or by already formed gammons, in a “step-by-step” process.