Wednesday, February 5, 2014

1. On Gravy Quark and 2. On Cosmod gravity : two papers given at ISC 1984 Nagpur and 1985/86 Delhi/Lucknow respectively

*137. K. L. Narayana,”Physical process of Gravitons and Gravy Quark in the interior
          of  Supergravity Cosmic Stellar structures”, 72nd Session of Ind. Sci. Cong.
         January 5th, 1985 and
         Arthur Eddington Centenary Symposium, Vol.3, Nagpur, 23rd February 1984.

Physical process of Gravitons and Gravy Quark in the interior OF SUPERGRAVITY Cosmic Stellar structures

K. L. Narayana

Physics Department, Shivaji University,
KOLHAPUR – 416004 (INDIA)

Present address: (Retd. Prof. of Physics, SU), 17-11-10, Narasimha Ashram,
Official colony, Maharanipeta. P. O, Visakhapatnam – 530002.

A B S T R A C T
          Supergravity gauge theories have been cited to
establish the nature of physical processes of constituents
of cosmic stellar structures.  In the present paper I have
Shown how the gravitational gauge potentials obtained to be
The vectors Bba μ in the complex 4 D – space of O(5), in a twenty
Spin-coefficients formulation may be incorporated in a new
Gravitational theory. Further (in the Yang-Mills similitude)
Gauge-spinorial potentials F αβ together with their potentials
Bμ are utilized to define a new M - derivative that transports
a vector,   along a time-like vector    Uμ   . This derivative
is presented to lead to gauge-covariant collineations.
(GRG Conference, Pune 1983). There are two-fold mechanisms
That are implied by the present theory that govern the possible
Physical processes. One involves terms that signify the
Interaction of an iso-scalar field with Massive spinorial
particles. The other is due to the breakdown of an enlarged
Symmetry of gravitons and gravy quarks resulting in new physical
processes. They are mediated by both the neutral fields and
Charged spinorial currents. In particular a process like KL à
è μe- , i.e. mediated by a direct exchange of E Boson
corresponding to neutral gauge current J [34] has been pointed out
in the generator scheme of SL(2,C)/ SU(2). It is interesting to
note that these processes transpire at high energies, and the
manifest gauge potentials, are generated by local iso-spin
transformations that mandate on a wave function defined at a
space-time point x. (Edington Centenary Symposium, Nagpur 1984).



126. K. L. Narayana, ”on Spinorial and Materialistic optical Cosmod tensor Invariants
        and Cosmod Gravity”, 73rd Sess. Ind. Sci. Cong. Delhi January 6th, Physics
        Section, 1986 and 72nd Sess. of Ind. Sci.Cong. Lucknow, Mathematics section,
        January 6th, 1985.


ON SPINORIAL AND MATERALISTIC OPTICAL
TENSOR INVARIANTS AND COSMOD GRAVITY

K. L. Narayana

Physics Department, Shivaji University,
KOLHAPUR – 416004 (INDIA)

Present address: (Retd. Prof. of Physics, SU),17-11-10,Narasimha Ashram,
Official colony, Maharanipeta. P. O, Visakhapatnam – 530002.

A B S T R A C T

         Spinorial and materialistic optical shear, rotation
and deformation tensors are defined and the fundamental
equations, employing these, for the propagation of a null
gravitational field have been formulated in the Extended
Newman-Penrose spin coefficient formalism. The four-
dimensional 0(5) gauge space of inhomogeneous SL(2,C) x
SU(2) supergravity theory has been used. The theorem,
as follows is enunciated.   “If a small spinorial-
cosmod” object in a null geodesic congruence casts a
shadow on a screen, all portions of the shadow hit the
screen simultaneously, but the shape, size, orientation
and spinorial (cosmod) polarization of the shadow depend
only on the location of the screen, not on its world
velocity.  The shadow is thus spinorial expanded, iso-
spinrotated and cosmod sheared”.

        Next cosmod gravity, in the context of large number
Hypothesis of Dirac has been shown to arrive at the number
0.354x10-39 with quantum cosmod gravity range formula
τ= ( n ћ/ (2 e 2 f c2 )).


 ACKNOWLEDGMENT

                                      The author is indebted to Late Prof.  K.  R.  Rao,  D.Sc. (Madras)  D.Sc.(London)  of  Andhra University,  Waltair  ( in the years 1932-1972) for  his  interest  and guidance  in  promoting my  research  endeavor.

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