Peer-reviewed articles 17,970 +



Title: NOETHER?S SYMMETRY IN HORAVA-LIFSHITZ COSMOLOGY

NOETHER?S SYMMETRY IN HORAVA-LIFSHITZ COSMOLOGY
M. B. Arzimbetova;Sh. R. Myrzakul;T. R. Myrzakul;M. Imankul;G. Y. Mukhamedova
1314-2704
English
19
6.2
Recently, Horava-Lifshitz proposed the theory of quantum gravity, which takes into account the
degree of renormalizability in the ultraviolet. This was achieved by anisotropic scaling between
space and time, and, therefore, it violates the Lorentz invariance in the ultraviolet range. The
infrared limit of a theory reproduces the general theory of relativity for a particular choice of
parameter, namely . Lorentz symmetry breaking is performed by preferred foliation of threedimensional
space-like hypersurfaces, which, in turn, divide the coordinate into space and time.
This makes it possible to record the action of Einstein Hilbert with higher spatial derivatives of
the metric. It improves the ultraviolet behavior of the graviton propagator and displays the
renormalizable power counting theory. Moreover, the action has only second-order time
derivatives that prevent the presence of ghosts in the theory.
In this paper, we consider Friedmann-Robertson-Walker flat space-time in the framework of the
metric formalism of gravity. We created an effective Lagrangian in which the scale factor and
the Ricci scalar play the role of independent dynamic variables. This Lagrangian is constructed
in such a way that its variation is relative and gives the correct equations of motion as equations
of action with the typical one. The type of function appearing in the modified action is then
determined by the requirement that the Lagrangian admits the desired Noether symmetry. By
Noether?s symmetry of this cosmological model of a minisuperspace, we understand that there
is a vector field as an infinitesimal symmetry generator on the tangent space of the configuration
space, such that the Lie derivative of the Lagrangian over this vector field vanishes. We will see
that by presenting the Noether symmetry as a feature of the Lagrangian of the model under
consideration, we can obtain the explicit form of the function. Since the existence of symmetry
leads to constant motion, we can integrate the field equations, which then lead to the expansion
of the power law of the Universe.
conference
19th International Multidisciplinary Scientific GeoConference SGEM 2019
19th International Multidisciplinary Scientific GeoConference SGEM 2019, 30 June - 6 July, 2019
Proceedings Paper
STEF92 Technology
International Multidisciplinary Scientific GeoConference-SGEM
Bulgarian Acad Sci; Acad Sci Czech Republ; Latvian Acad Sci; Polish Acad Sci; Russian Acad Sci; Serbian Acad Sci & Arts; Slovak Acad Sci; Natl Acad Sci Ukraine; Natl Acad Sci Armenia; Sci Council Japan; World Acad Sci; European Acad Sci, Arts & Letters; Ac
667-674
30 June - 6 July, 2019
website
cdrom
6571
Noether symmetry; f (R) gravity; Horava-Lifshitz gravity; quantum gravity.

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