The Origin of New Primaries from “Cygnus X-3” and “Centauro” astrophysical objects and the Gravy Quark Star” : ISC 1987 in 74th Session Paper 123 p.68 to 69

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Volume 2014, Issue No.2, February 10, 2014, Time: 11h42.A.M.

  149. K. L. Narayana,74th Sess. Ind. Sci. Cong. Bangalore Mathematics section,

                 “The Origin of New Primaries from “Cygnus X-3” and “Centaur”

                 Astrophysical objects and the Gravy Quark star” Paper No.123,

                 (Sect.III), Page 68-69. (presented) 1987:  

The Origin of New Primaries from “Cygnus X-3” and “Centauro” astrophysical objects and the Gravy Quark Star”

By

K. L. Narayana, M. Inst. P. (Lond),

Professor of Physics, Shivaji University, Kolhapur

{Professor Dr. Kotcherlakota Lakshmi Narayana,

General Physics Labs, Shivaji University, Kolhapur-416004 and

(Retd. Prof. of Phys, SU, Kolhapur}, 171-11-10, Narasimha Ashram,

Official Colony, Maharanipeta. P.O., Visakhapatnam – 530002

Cell No.09491902867.

The recent models of Quark star origin of new primaries

of Cygnus X-3 muon and Centauro proton ‘showers are

critically examined. It is proposed instead that Gravy Quark

Stars exist in the interior of these objects. (11^th Gravy Quark Int.

Conference, Stockholm July 1986 by K. L. Narayana).

Existence and role of spinorial particles of mass

1.6x10 ^-23 gm density 9.952x10 ⁴⁵ gm Cm ^-3 and magnetic

Moment of 5916.2μB is predicted. The model formulae to

Describe the space-time curvature behavior in terms of

Spinorial deformations and rotation stress tensors is presented.

                The new coupling constant of the renormalized

Gravitational Bosons and their role to generate Chromic Gravy

Lattice structures of those massive and bright stars are detailed

out. The significance of lattice section to describe the

frustration of plaquettes and transportation of new gravy

gauge fields along links of the lattice is presented. The model

is shown to lead thus to a “Stochastic Gravy Quantization”.

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Proc.74^th Ind. Sci. Cong. Sess. Part III Sect III :Physics,

 Page 68-69. (presented) 1987.

Cygnus X-3 and Centauro astrophysical objects

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       Acknowledgment

                The author is deeply indebted to Late Prof. K. R. Rao

        D.Sc. (Madras) D.Sc. (London) whose insight of the subjects of

       Science and Technology has helped many a students to grasp the

       intricate principles of the Universe and who achieved

       establishment of Internationally famous laboratories.

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