HighEnergy Physics
These papers were written by GPT2. Because GPT2 is a robot, these papers are guaranteed to be 100% factually correct. GPT2 is very proud of its scientific accomplishments; please print out the PDFs and put them on your refrigerator. [1] faKiv:2001.07210 [pdf]

From AdS$_3$ to AdS$_2$Comments: 10 pages, 8 figures, v2: references added
We investigate the AdS$_3$ and AdS$_2$ models in the CFT$_3$ and CFT$_2$ and we study the firstorder conformal field theory created in the AdS$_3$ and AdS$_2$. We show that the conformal fields have the same number of fields and that the mass spectra are the same. In particular, we find that the conformal field theories have the same mass and energy spectra. We also demonstrate that the AdS$_3$ models have the same signature as the RPBS model.
 [2] faKiv:2001.07254 [pdf]

Nonabelian gauge theory on a fourdimensional hyperbolic manifoldComments: 5 pages, 1 figure
We consider the Nonabelian gauge theory on a fourdimensional hyperbolic manifold. The gauge theory equations in the hyperbolic manifold are divided into the gauge equations in the hyperbolic manifold and the gauge equations in the hyperbolic manifold. We obtain the Lagrangian equations of the Nonabelian gauge theory on the hyperbolic manifold. We construct the first order equations and prove the first order Lagrangian equations for the nonabelian gauge theory. The equations are given in terms of the hyperbolic manifold equations. The equations are verified and, in particular, we verify that the first order Lagrangian equations in the hyperbolic manifold are also valid in the hyperbolic manifold.
 [3] faKiv:2001.07300 [pdf]

The HopfWigner gauge theory for the $S_1$charge of the $N_f$ImageComments: 3 pages, minor changes, references updated
We study the linearized HopfWigner gauge theory, which is a generalization of the classical HopfWigner theory of any $f\bar{f}$charge in a $SPR$model. We derive the HopfWigner equation and prove the equivalence between the gauge fields and the corresponding chemical potentials, and study the relation between the knotholic and canonical forms of the gauge theory. We also study the connection between the HopfWigner gauge theory and the Lorentzian gauge theory.
 [4] faKiv:2001.07361 [pdf]

The Boundary of Polarization in the Quantum GravityComments: 11 pages, 2 figures, minor corrections
We discuss the bounds of polarization in quantum gravity, which is a threedimensional selfcontained theory of gravity. In this case, the gravitational wave spectrum is dominated by gravitational waves. We present a simple but powerful procedure to derive the bound of entropy. We also derive the bounds of the resonant frequency, which is defined in terms of the center of mass and resonant frequency. We show that the bound of polarization is always satisfied in the case of the nonperturbative case.
 [5] faKiv:2001.07471 [pdf]

The Higgs as a nature of gravityComments: 5 pages, 2 figures
We study the Higgs as a nature of gravity conjecture in the case of general relativity. We show that the standard models are consistent with it, which is consistent with the standard models of physics. We further show that the Higgs is a nature of gravity conjecture. We argue that the Higgs as a nature of gravity conjecture is not a conjecture of quantum gravity.
 [6] faKiv:2001.07501 [pdf]

Nonminimal Derivative GravityComments: 5 pages, 5 figures, v3: references added, discussion on the role of eigenvalues added
We study the gravitational force between two particles in a nonminimal derivative gravitational field theory and provide an equation that approximates the deterministic gravitational force. We show that the nonminimal derivative gravity term is a direct consequence of the interference of the scalar field. This result gives the constraint in the eigenvalue of the gravitational force between two particles, and it is verified by a test of the law of the conservation of eigenvalues in the relativistic case. This constraint is derived from the Euler's formula for the scalar field.
 [7] faKiv:2001.07566 [pdf]

A glow in the dark: The derivation of the EinsteinHilbert equation from the nuclear energy phase in the ChernSimons theoryComments: 10 pages, 5 figures
In this article, we define the nuclear energy phase in the ChernSimons theory, and construct the relevant nuclear phase diagrams and equation of state equations. The resulting equations are valid for any nuclear energy state, including the nuclear phase of the ChernSimons theory. We find that the nuclear phase is the normal phase in the ChernSimons theory with a single scalar field, which is the critical point. The inverse phase of the ChernSimons theory with a scalar field is known as the trivially noncritical phase, which is the critical point in the ChernSimons theory with a single scalar field. We prove that the EinsteinHilbert equation (EH) and the ChernSimons theory equation of state equation of state (COW) corresponding to EH and COW, are the same in the nuclear phase diagram and to the following order of the energy scale: COWL and EH. Furthermore, we prove that the EH and COW phases in the nuclear phase diagram are exactly the same as the ones in the corresponding nuclear phase diagram in the ChernSimons theory. We also discuss a possible relation between the ChernSimons theory and the nuclear theory. We show that the nuclear theory is the only one in which the nuclear phase of the ChernSimons theory is the same as the atomic phase of the ChernSimons theory.
 [8] faKiv:2001.07690 [pdf]

The Riemann sphere and the generalization of the BunchDaviesFerrari lensComments: 17 pages
We investigate the Riemann sphere, a oneparameter family of solutions of Einstein's equations, in the presence of baryons in the wake of a photonion beam. The resulting threeparameter model is the GillDaviesFerrari lens: the lens that reproduces the BunchDaviesFerrari geometry. We show that the BunchDaviesFerrari lens reproduces the generalization of the BunchDaviesDavies Schr\"odinger lens. We also show that the BunchDaviesFerrari lens reproduces the Schr\"odinger lens. In addition, we show that the BunchDaviesFerrari lens reproduces the Schr\"odinger lens in the presence of baryons in the wake of a photonion beam.
 [9] faKiv:2001.07775 [pdf]

Delocalization in the absence of gravityComments: 5 pages, LaTeX; v2 is a new section about the nonperturbative character of the effective action
We discuss the effects of the deSitter spacetime for a baryonicgravitymatter system on the ability of the effective action of the effective theory to diffuse to the lowest quasilocal coordinate in the spacetime. We discuss the properties of the effective action deSitter and its deSitter diffusive behavior in the absence of the gravitational coupling. We discuss the physical effects of the nonperturbative effects of the deSitter diffusiveness on the nonperturbative character of the effective action of the effective theory.
 [10] faKiv:2001.07806 [pdf]

Compactification in higherspin fields with massless synchronous couplingsComments: 12 pages, 2 figures
We study compactification effects in the $SU(3)$ ChernSimons theory of higherspin fields with massless synchronous couplings, by performing the standard 1/2ChernSimons decomposition in terms of the 1/4ChernSimons decomposition. In particular, we show that compactification occurs in the continuum limit, and in the case of the $SU(2)$ theory, we show that it coincides with the corresponding $SU(2)$ compactification in the continuum limit. We also show that compactification results in a noncompact, noncompact, compactificationfree theory, which is the same as the known $SU(4)$ theory with massless synchronous couplings. Finally, we show that compactification in the $SU(3)$ theory is accompanied by a compactificationfree theory which corresponds to the known $SU(4)$ theory with massless synchronous couplings.
 [11] faKiv:2001.07851 [pdf]

The nonperturbative case for the nohair phase transitionComments: v2: 22 pages, 2 figures
We construct a class of allpoint functions of the nonperturbative mode for the nohair phase transition in the presence of a massive scalar field. Our results are in good agreement with the ones obtained by the energymomentum tensor method in the case of the CFTlike nohair phase transition in the presence of a massive scalar field.
 [12] faKiv:2001.08111 [pdf]

The Anomalous Galilean GravityComments: 15 pages, 1 figure. v3: minor changes
We present a new class of anomalous Galilean gravity models which can be thought of as the Lagrangian of a gravitational wave background and a quarkgluon plasma. We show that, in the absence of a quarkgluon plasma, these models exhibit the usual anomalous Galilean gravity behavior, and that, in the presence of a quarkgluon plasma, they exhibit the anomalous Galilean gravity behavior. Furthermore, we show that the anomalous Galilean gravity can be constructed by integrating out the quarkgluon plasma and by computing the partition function for the swave solution of the perturbation theory. In this way, we show that the anomalous Galilean gravity, which is defined by the partition function, can be obtained by integrating out the quarkgluon plasma and by computing the partition function of the swave solution. Our analysis of the contour integrals and the contour integrals of the swave solution is based on the EikinAlexeyevGilderspoldWitten (EWG) formulas, which are linearized ones of Eikin and Avshalom.
 [13] faKiv:2001.08243 [pdf]

Detecting the Geometric Structure of a FoldComments: 18 pages, 4 figures
We explore the theory of an ideal gas with a finite geometrical structure. We show that the geometry of this ideal gas can be analyzed directly by the geometrical structure of the Fold. We propose a model that is both the map of the Fold and a map of the Geometry of the Fold. This map can be used to find the Fold's geometry in the limit that the Fold is not geometrical. Our model generates a class of maps in which the Fold does not appear. We provide a simple example of a Fold that involves an inverted Riemann surface and a map.
 [14] faKiv:2001.08295 [pdf]

UnruhDeWitt detectors on the boundaryComments: 14 pages, 2 figures. arXiv admin note: text overlap with arXiv:1702.07385
In this paper we study the unruhdeWitt detectors of a class of muons in EinsteinGaussBonnet gravity theory. The detectors have three components: a Dirac component, a corotating component, and a spin2 component. The Dirac detector is the first detector that is efficient at splitting the muons into Dirac and Corotating particles, while the corotating component is not as efficient but can be used to divide the Dirac particles into Dirac and corotating particles. We show that the Dirac component is pure and the Corotating component is twisted. The spin2 component has two components: one component that is twisted and has a spin2 component and one component that is pure and has a spin2 component. We discuss the relation between the spin2 component and the corotating component in the presence of the Dirac component.
 [15] faKiv:2001.08435 [pdf]

Galois model of the nonperturbative LorenzSchwarzschild black holeComments: 22 pages, 2 figures. arXiv admin note: text overlap with arXiv:1609.02288
In this paper, we study the nonperturbative LorenzSchwarzschild black hole solution in the spacetime dimensions of the imaginary and imaginary parts of the Hawking radiation. We first calculate the Galois model of the nonperturbative black hole in the Riemann sphere in the continuum limit. Then, we use the solution to obtain the Galois model of the black hole in the EinsteinMaxwell sphere. We then use the solution to study the Galois model of the black hole in the DiracBornInfeldThirring sphere. We find that the Galois model of the black hole is the LorenzSchwarzschild model of the black hole.
 [16] faKiv:2001.08541 [pdf]

Anomalous and Assisted Constants in the Chiral Equilibrium ModelComments: 25 pages, 8 figures
We calculate anomalous and assisted constants in a simple model of the chiral equilibrium model in the presence of a vector hypermultiplet and a momentum multiplet. We find that the most general case of the quasiclassical situation, consisting of two vectors of the same mass, is invariant under the perturbative determinants. A different case, with two vectors of different mass, is equivalent to the nonperturbative case. The latter is obtained in the context of the twodimensional MaxwellHiggs model. The twodimensional model is constructed by any of the base quiver gauge theories and the chiral spectrum of the chiral equilibrium model is determined by the boundaryconducive equations of the field equations. The analytic solution obtained here is known as the nonperturbative solution of the second order equations of motion. The solution of the first order equations of motion is given by the Maxwell's equations.
 [17] faKiv:2001.08779 [pdf]

On the multisetting model and the quasinormal modesComments: 15 pages, 3 figures
We study the multisetting model in the presence of a superfield in order to investigate various aspects of the quasinormal modes of the theory. We first perform a complete analysis of the quasinormal mode in the cases of the quasinormal modes of the field theory and the cosmological model. In order to this purpose, we obtain the relation between the quasinormal modes and the thermodynamic quantities of the model. We conclude that the multisetting model has the quasinormal modes that are described by the QuarkTester Multiplet and is the generalization of the Multiplet of the Quark and Gamma Ray Bursts.
 [18] faKiv:2001.08781 [pdf]

Quantum wave mechanics in the presence of a sudden relativistic de Sitter excursionComments: 1+45 pages, 7 figures
Quantum wave mechanics is a wellknown picture of quantum mechanics in a de Sitter space. The path integral of quantum wave mechanics is equivalent to the path integral of quantum mechanics in a de Sitter space. In this paper, we present an analytical formula for the path integral of quantum wave mechanics in the presence of a sudden relativistic de Sitter excursion. We derive the formula analytically, and find that the formula is a product of the solution of the Hamiltonian of quantum wave mechanics with the path integral of quantum wave mechanics, and the solution of the de Sitter path integral. We use this formula to calculate the spectral index for a wave of massless scalar fields in a de Sitter space in the presence of a sudden relativistic de Sitter excursion. We find that the spectral index is a real function of the background signal.
 [19] faKiv:2001.08808 [pdf]

The Integrability of the Boundary of a TwoDimensional PermutationComments: 20 pages, 11 figures
In this paper we introduce the idea of the integrability of a permutation theory in three dimensions. We investigate the quiver gauge theory of the socalled pure permutation theory, and derive the integrable equations. In particular, we show that the equations are integrable by considering the integrable integrals of the twodimensional quantum chromodynamics.
 [20] faKiv:2001.08865 [pdf]

Comparisons and equations for the quark and gluon mass in the empty and the empty spaceComments: 8 pages, 1 figure, v2: references added
We use a comparison between the quark mass in the empty space and the quark mass in the empty space to show that in the empty space the quark mass is equal to that of the quark mass in the empty space. In the empty space, we find that in the null energy limit the quark mass is equal to that of the gluon mass. In the null energy limit the quark mass in the empty space is equal to that of the gluon mass.