scholarly journals Gravitational field of global monopole within the Eddington-inspired Born-Infeld theory of gravity

Author(s):  
Reyhan D. Lambaga ◽  
Handhika S. Ramadhan
2021 ◽  
Vol 52 (1) ◽  
Author(s):  
Alexander P. Sobolev

AbstractThe gravitational equations were derived in general relativity (GR) using the assumption of their covariance relative to arbitrary transformations of coordinates. It has been repeatedly expressed an opinion over the past century that such equality of all coordinate systems may not correspond to reality. Nevertheless, no actual verification of the necessity of this assumption has been made to date. The paper proposes a theory of gravity with a constraint, the degenerate variants of which are general relativity (GR) and the unimodular theory of gravity. This constraint is interpreted from a physical point of view as a sufficient condition for the adiabaticity of the process of the evolution of the space–time metric. The original equations of the theory of gravity with the constraint are formulated. On this basis, a unified model of the evolution of the modern, early, and very early Universe is constructed that is consistent with the observational astronomical data but does not require the hypotheses of the existence of dark energy, dark matter or inflatons. It is claimed that: physical time is anisotropic, the gravitational field is the main source of energy of the Universe, the maximum global energy density in the Universe was 64 orders of magnitude smaller the Planckian one, and the entropy density is 18 orders of magnitude higher the value predicted by GR. The value of the relative density of neutrinos at the present time and the maximum temperature of matter in the early Universe are calculated. The wave equation of the gravitational field is formulated, its solution is found, and the nonstationary wave function of the very early Universe is constructed. It is shown that the birth of the Universe was random.


1998 ◽  
Vol 58 (4) ◽  
pp. 294-296 ◽  
Author(s):  
Subenoy Chakraborty

1989 ◽  
Vol 63 (4) ◽  
pp. 341-343 ◽  
Author(s):  
Manuel Barriola ◽  
Alexander Vilenkin

2017 ◽  
Vol 32 (13) ◽  
pp. 1750061
Author(s):  
Buddhi Vallabh Tripathi ◽  
Hemwati Nandan ◽  
K. D. Purohit

We investigate global monopole solutions in a particular kind of scalar–tensor theory of gravity, viz. the broken-symmetric theory of gravity. Invoking the “hedgehog” ansatz for the scalar field, we derive the metric corresponding to global monopole solutions. The global monopole solutions found are independent of the scale of symmetry breaking unlike the Barriola–Vilenkin global monopoles in Einstein’s General Relativity (GR) which intrinsically depend on the symmetry breaking scale.


2012 ◽  
Vol 27 (31) ◽  
pp. 1250178 ◽  
Author(s):  
J. P. MORAIS GRAÇA ◽  
V. B. BEZERRA

In the framework of f(R) theory, we obtain the solution which corresponds to a rotating global monopole from its static counterpart by applying the method of complex coordinate transformation.


2000 ◽  
Vol 15 (06) ◽  
pp. 869-873
Author(s):  
A. BANERJEE ◽  
T. GHOSH

The motion of test particles and light rays in the perturbed gravitational field around a global monopole is studied. The metric of the monopole was previously obtained by solving the linearized semiclassical Einstein equations (Hiscock). The bending of light ray passing by such a monopole has contributions from the conical object as well as from the perturbed terms. The possibility of trapping particles in the perturbed gravitational field is also discussed.


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