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Rinat A. Daishev

Publications and source records attributed to Rinat A. Daishev.

6 recordsLinked to original sources

Gravitational fields and harmonic gauge in brane model of Universe

We suppose that our Universe is closed manifold in real embedding higher dimensional space. This model well describes expanding character of Universe where each point becomes more far from any other point with time. We have derived Klein-Gordon equation using the symmetry of Universe expansion. Comparing it with squared Dirac-Fock-Ivanenko equation we have derived expression for gravitationally induced chiral current. Starting from the expression for gravitationally induced chiral current obtained on the basis of brane symmetry we have shown that being placed into the Einstein's gravitational field, chiral current yields inertial gravitational field. This inertial gravitational field transforms into the vortex gravitational field and then back to the inertial gravitational field thus ensuring the propagation of such kind of gravitational excitation as constitutional part of gravitational wave. In the case of weak gravitation, these symmetry considerations and our consequent equations lead directly to harmonic gauge conditions that are necessary for supplementing Einstein equations.

physics.gen-ph↗

Spin chiral current induced by curvature of space-time

Klein-Gordon equation is derived for a particle in the brane model of Universe. It is compared with squared Dirac-Fock-Ivanenko equation and expression for a chiral current is obtained by this comparison. This expression defines chiral current through variation of spin connection gauge field that arises due to the symmetry in respect to local Lorenz transformations. So, the second derivative of gravitational gauge field determines variation of chiral current responsible for variation of mass. The role of these processes on the early stages of Universe evolution is discussed.

physics.gen-ph↗

Klein-Gordon equation for a particles in brane model

Brane model of universe is considered for a free particle. Conservation laws on the brane are obtained using the symmetry properties of the brane. Equation of motion is derived for a particle using variation principle from these conservation laws. This equation has a form of Klein-Gordon equation. Comparison of squared Dirac-Fok-Ivanenko equation for a spin particle with Klein-Gordon equation in curved space has given an expression for chiral spin current variation through the derivative of spin connectivity. This chiral spin current is anomalous spin current corresponding to spontaneous chiral symmetry breaking of massive particle in the space of KG equation solutions.

gr-qc↗

Einsteins hole dilemma and gauge freedom

The issue of the physical equivalence between the different coordinate system in Einstein theory is revised. Gauge fixing influences results of measurements and physics are different in two different coordinate system. Spacetime metric generated by static spherically symmetric distribution of matter can be matched with wide family of vacuum solution and the exterior spacetime geometry could not be deduced directly from the interior perfect fluid solution, without reference to a gauge fixing or viceversa. The property of sollutions in general relativity is indeed an observer dependent concept.

physics.gen-ph↗

"Gauge" freedom and relationship between the Einstein and Jordan conformal frames

The issue of the physical equivalence between the Einstein and Jordan conformal frames in Jordan-Brans-Dicke (JBD) theory is revised. Scalar-tensor theories equations are not invariant with respect to conformal transformations if one uses the same "gauge" fixing in Jordan and Einstein frames. We hope to have clarified some eventual obscure issues associated to the concept of conformal invariance of relativistic theories appearing in the literature, in particular the relationship between Jordan and Einstein frames.

physics.gen-ph↗

On homothetic cosmological dynamics

We consider the homogeneous and isotropic cosmological fluid dynamics which is compatible with a homothetic, timelike motion, equivalent to an equation of state $ρ+ 3P = 0$. By splitting the total pressure $P$ into the sum of an equilibrium part $p$ and a non-equilibrium part $Π$, we find that on thermodynamical grounds this split is necessarily given by $p = ρ$ and $Π= - (4/3)ρ$, corresponding to a dissipative stiff (Zel'dovich) fluid.

gr-qc↗