Abstract:With the arrival of the era of gravitational wave astronomy, the strong gravitational field regime will be explored soon in various aspects. In this article, we provide a general review over cylindrical systems in Einstein's theory of general relativity. In particular, we first review the general properties, both local and global, of several important solutions of Einstein's field equations, including the Levi-Civita and Lewis solutions and their extensions to include the cosmological constant and matter field… Show more
“…Here, the constants a, b and K are all arbitrary -with a constraint between a and bwhile c is the speed of light. Note that the form (II.2) of the Levi-Civita metric we use here is not the one that one often encounters in the literature [28][29][30][31] (see also, the very nice recent review [32].) In fact, the first difference is that we have introduced here the fixed constant radius ρ * to allow us to keep inside the metric the radius ρ, describing the position of the particle away from the center of the cylinder, with the dimensions of a length.…”
Section: A Particle Inside a Magnetic Field In The Levi-civita Spmentioning
confidence: 99%
“…This specific choice is merely made here for the sake of simplicity. In fact, had we chosen to use instead the more familiar form of the metric, in which both coordinates acquire the same metric component [31,32], the angular component of the metric would also acquire 2 a power function of ρ instead of having the above familiar factor ρ 2 . This would indeed only render our equations and analysis uselessly complicated.…”
Section: A Particle Inside a Magnetic Field In The Levi-civita Spmentioning
confidence: 99%
“…Given that the Lewis spacetime reduces in the limit of zero radius of the cylinder to that of a rotating cosmic string (see, e.g., Ref. [32] and the references therein for more details about such a metric), which, in turn, has extensively been studied in Ref. [42], we are going to turn instead into the rotating spacetime represented by the Kerr metric.…”
Section: B Using the Harmonic Oscillator Approximationmentioning
We have recently found that the gravitational field of a static spherical mass removes the Landau degeneracy of the energy levels of a particle moving around the mass inside a magnetic field by splitting the energy of the Landau orbitals. In this paper we present the second part of our investigation of the effect of gravity on Landau levels. We examine the effect of the gravitational fields created by an infinitely long massive cylinder and a rotating spherical mass. In both cases, we show that the degeneracy is again removed thanks to the splitting of the particle's orbitals. The first case would constitute an experimental test -which is quantum mechanical in nature -of the gravitational field of a cylinder. The approach relies on the Newtonian approximation of the gravitational potential created by a cylinder but, in view of self-consistency and for future higher-order approximations, the formalism is based on the full Levi-Civita metric. The second case opens up the possibility for a novel quantum mechanical test of the well-known rotational frame-dragging effect of general relativity. * Electronic address: fhammad@ubishops.ca † Electronic address: alexandre.landry.1@umontreal.ca
“…Here, the constants a, b and K are all arbitrary -with a constraint between a and bwhile c is the speed of light. Note that the form (II.2) of the Levi-Civita metric we use here is not the one that one often encounters in the literature [28][29][30][31] (see also, the very nice recent review [32].) In fact, the first difference is that we have introduced here the fixed constant radius ρ * to allow us to keep inside the metric the radius ρ, describing the position of the particle away from the center of the cylinder, with the dimensions of a length.…”
Section: A Particle Inside a Magnetic Field In The Levi-civita Spmentioning
confidence: 99%
“…This specific choice is merely made here for the sake of simplicity. In fact, had we chosen to use instead the more familiar form of the metric, in which both coordinates acquire the same metric component [31,32], the angular component of the metric would also acquire 2 a power function of ρ instead of having the above familiar factor ρ 2 . This would indeed only render our equations and analysis uselessly complicated.…”
Section: A Particle Inside a Magnetic Field In The Levi-civita Spmentioning
confidence: 99%
“…Given that the Lewis spacetime reduces in the limit of zero radius of the cylinder to that of a rotating cosmic string (see, e.g., Ref. [32] and the references therein for more details about such a metric), which, in turn, has extensively been studied in Ref. [42], we are going to turn instead into the rotating spacetime represented by the Kerr metric.…”
Section: B Using the Harmonic Oscillator Approximationmentioning
We have recently found that the gravitational field of a static spherical mass removes the Landau degeneracy of the energy levels of a particle moving around the mass inside a magnetic field by splitting the energy of the Landau orbitals. In this paper we present the second part of our investigation of the effect of gravity on Landau levels. We examine the effect of the gravitational fields created by an infinitely long massive cylinder and a rotating spherical mass. In both cases, we show that the degeneracy is again removed thanks to the splitting of the particle's orbitals. The first case would constitute an experimental test -which is quantum mechanical in nature -of the gravitational field of a cylinder. The approach relies on the Newtonian approximation of the gravitational potential created by a cylinder but, in view of self-consistency and for future higher-order approximations, the formalism is based on the full Levi-Civita metric. The second case opens up the possibility for a novel quantum mechanical test of the well-known rotational frame-dragging effect of general relativity. * Electronic address: fhammad@ubishops.ca † Electronic address: alexandre.landry.1@umontreal.ca
“…where the constant factors A, B, C, D depend on the values of w i as well as ρ 0 and ω 0 . If B = C = 0, we have two separate Liouville-type equations which are solved directly and completely, and it remains to substitute the solution to the first-order equation (23) to verify the solution and to obtain a relation between the integration constants. Apart from the case B = C = 0, in which the matrix of coefficients in Eqs.…”
Section: A Search For Solutionsmentioning
confidence: 99%
“…Among motivations of such studies one can mention the relative simplicity of the gravitational field equations as compared to more realistic axial symmetry (to say nothing on the general nonsymmetric case) and the possible existence of linearly extended structures like cosmic strings in the Universe. In addition, cylindrical symmetry is the simplest one that admits rotation and is most suitable for studying rotational phenomena in GR, so not too surprising is the wealth of existing stationary (that is, assuming rotation) exact solutions to the Einstein equations with various sources of gravity: the cosmological constant Λ [3][4][5]; scalar fields with or without self-interaction potentials [6,7], including Λ as a constant potential [8]; dust in rigid or differential rotation [9][10][11], electrically charged dust [12], dust with a scalar field [13], perfect fluids with various equations of state, mostly p = wρ, w = const (in usual notations) [14][15][16][17][18]; some examples of anisotropic fluids [19][20][21] etc, see also references therein as well as reviews [22,23].…”
We consider anisotropic fluids with directional pressures p i = w i ρ (ρ is the density, w i = const, i = 1, 2, 3 ) as sources of gravity in stationary cylindrically symmetric space-times. We describe a general way of obtaining exact solutions with such sources, where the main features are splitting of the Ricci tensor into static and rotational parts and using the harmonic radial coordinate. Depending on the values of w i , it appears possible to obtain general or special solutions to the Einstein equations, thus recovering some known solutions and finding new ones. Three particular examples of exact solutions are briefly described: with a stiff isotropic perfect fluid (p = ρ), with a distribution of cosmic strings of azimuthal direction (i.e., forming circles around the z axis), and with a stationary combination of two opposite radiation flows along the z axis.
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