New Matter and Stellar Structures

94th Ind. Sci. Congress held at Annamalai University, Chidambaram
ISCA 2007 3nd- 7th, Januar, 2007. Mathematical Sciences Section
:Paper No 21 Page 14

The possible symmetry-supersymmetry interaction currents & the properties of strange matter of stellar structures

Kotcherlakota Lakshmi Narayana

A.G.L.College, Post Graduate department Sankaramattam Road, Viskhapatnam-530016. Email:Kotcherlakota_l_n@hotmail.com

Key words: strange matter, supersymmetry, smon particles, aesthetic beauty

ABSTRACT:
A model involving the symmetry-supersymmetry interaction has been suggested to explain the properties of strange matter of compact stellar structures. The nine supersymmetry particles (smons) are endowed with the hypercharge and isospin assignments. These are G, ¯Nc, iS, -iR, A, D, T, θc, ¯θc .The imaginary particles are included for the aesthetic beauty of the model considerations. The strangeness-conserving and strangeness-changing expressions have been obtained. The typical amplitudes (θc n| S Ξ-)a*ν ae = (κ- S| κ0 θc) a*ν a e = a μ a*e (π – θ| κ+ ¯Nc) and a μ a*e (κ- θ| π+ Nc) = (κ- θ| κ0 R) aν a*e with the equality relations and the ax’s are typical coefficients. For the symmetry we took the Octet mesons that play a role in the strange or the neutron stars. A, D, T particles that constitute the diagonal elements of the Nonet, obey SO (3) structure. An important feature of our symmetry-supersymmetry model is that the gluon type X, Y, Z quanta carry the charges as per the QCD requirements, but as well they posses mass The meson-smon vertex terms and their diagrams are much more complex. The only reason of the mass acquisition by the colored gluons is the compactness of the strange matter. The processes that we envisaged in our theory are Meson+smonMeson+smon. The predicted amplitude relations would help experimental analysis of the Quark-Gluon fireball experiments of CERN, FERMI LAB, RHIC etc on the properties of the new matter.