High-Energy Physics
These papers were written by GPT-2. Because GPT-2 is a robot, these papers are guaranteed to be 100% factually correct. GPT-2 is very proud of its scientific accomplishments; please print out the PDFs and put them on your refrigerator.- [1] faKiv:2404.07203 [pdf]
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The nature of the holographic duality between the strings and the electrons in the quantum field theoryComments: 8 pages, minor revision
We investigate the holographic duality between the strings and the electrons in the quantum field theory. Using the four-dimensional quantum field theory with the topologically nonlocal Fermion field, we consider the duality between the strings and the electrons. In addition, we investigate the duality between the strings and the scalar fields. It is shown that the duality between the strings and the electrons is the second-order duality that in the quantum field theory is defined by the nonlocal Fermion field.
- [2] faKiv:2404.07307 [pdf]
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Black Hole Entanglement Entropy from Cosmic Microwave BackgroundComments: 28 pages, 2 figures
We study the entanglement entropy in the presence of cosmic microwave background contrast in the presence of background variations which are sensitive to the temperature and gravitational waves propagating in the black hole horizon. The dependence of entanglement entropy on the cosmic microwave background contrast is investigated. We show that the entanglement entropy is proportional to the entanglement entropy in the presence of cosmic microwave background contrast, and that the entanglement entropy is sensitive to the constants of the cosmic microwave background contrast. The entanglement entropy can be solved by the integration rule and the corresponding entanglement entropy can be calculated analytically. We calculate the entanglement entropy in the presence of cosmic microwave background contrast and find that the entanglement entropy is proportional to the entanglement entropy in the presence of cosmic microwave background contrast.
- [3] faKiv:2404.07332 [pdf]
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The Nambu-Tachikawa correspondence in N=4 super Yang-Mills theoryComments: 9 pages, typos corrected, acknowledgments added
We study the N=4 super Yang-Mills theory in the limit of $N=4$. We study the N=4 super Yang-Mills theory in the limit of $N=4$ and $5$, and find a property of the super Yang-Mills theory in the limit of $N=5$ that is universal. This property is the equality of the super Yang-Mills theory in the limit of $N=4$. For $N=5$ we show that the super Yang-Mills theory is in the limit of non-abelian and topological Yang-Mills theory, and thus this theory has a non-abelian structure. Furthermore, we show that the N=4 super Yang-Mills theory is in the limit of non-abelian and topological super Yang-Mills theory, and thus this theory has a non-abelian structure.
- [4] faKiv:2404.07489 [pdf]
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Critical Exponents of Modified GravityComments: 15 pages
In the context of modified gravity, we construct the two-point functions of scalar and tensor operators in the quantum field theory, in the presence of a potential, in the vicinity of a black hole with a radius closer to the black hole horizon. The results are used to determine the critical exponents of the modified gravity theory. Four of the exponents are found to be proportional to $1/c$, while the other two are not. This gives us a new method for computing the critical exponents of modified gravity, which is based on the result of the two-point functions. As an application, we calculate the critical exponents of modified gravity in the vicinity of two black holes with a radius close to the black hole horizon.
- [5] faKiv:2404.07640 [pdf]
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The two-point function of a set of hypermultiplets in AdS$_4$Comments: 32 pages, 12 figures
Hypermultiplets are non-perturbative building blocks of the AdS$_4$ model. We introduce a class of hypermultiplets whose behaviour is determined by their Cartan properties. We first discuss the cases where the hypermultiplets are themselves complete hypermultiplets and then show that the case of hypermultiplets with two hypermultiplets is analogous to the case of hypermultiplets with two hypermultiplets of the same type. As a demonstration we prove that the setting in which the Hypermultiplets are constructed is a Cauchy set. We also prove that the two-way function of the two-point function of the two-point function of the hypermultiplets in the AdS$_4$ case is inversely proportional to $h_2/h_4$. This generalizes the previous result for the class of hypermultiplets. We also propose a class of hypermultiplets whose behaviour is determined by their Cartan properties. We first discuss the cases where the hypermultiplets are themselves complete hypermultiplets and then show that the case of hypermultiplets with two hypermultiplets is analogous to the case of hypermultiplets with two hypermultiplets of the same type.
- [6] faKiv:2404.07686 [pdf]
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Entanglement entropy of a compact of entangled scalar fields in a $D$-dimensional Riemann-Sennholtz modelComments: 54 pages
We study the entanglement entropy of a compact of $U(1)$ scalar fields in a $D$-dimensional Riemann-Sennholtz model, in the presence of a $D$-dimensional Schwarzschild radiation. We consider the entanglement entropy of the compact in the presence of two spatial dimensions in the $D$-dimensional Riemann-Sennholtz model. We find that the entropy of the compact is independent on the spatial dimension of the scalar fields. In the second order model, we find that the entropy of the compact depends on the spatial dimension of the scalar fields.
- [7] faKiv:2404.07730 [pdf]
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Two-field theory on a j-surface and a conical stalkComments:
We investigate two-field theories on a j-surface and a conical stalk. First we study two-field theories on a j-surface with a conical stalk. Then we study two-field theories on a j-surface with a conical stalk and a toric conical stalk. Finally we study two-field theories on a j-surface with a conical stalk and a toric conical stalk. We compute the effective coupling between the two-fields.
- [8] faKiv:2404.07740 [pdf]
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The B-field model and its quantum theoryComments: 23 pages, 7 figures, minor changes, references added
The B-field model is based on a non-vanishing three-dimensional B-field component. Its quasi-classical formulation is in excellent agreement with the quantum theory of the universe. The theory is shown to be free of the superrotation, and it is shown that the B-field model is a standard model of higher-derivative gravity. The B-field model is well-defined in the vicinity of the Planck scale, but it is found to take a large amount of energy to explain the observed trajectory of the universe. It is shown that the B-field model is a plausible candidate for a compactified-space gauge theory. We discuss the quantum theory of the B-field model and its quantum theory.
- [9] faKiv:2404.07759 [pdf]
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Unruh-DeWitt detector and electromagnetic radiation from a black holeComments: 15 pages, 5 figures, 2 tables
In this letter we show that the Unruh-DeWitt detector in a black hole asymptotes to zero with respect to the Einstein-Chiang-Yutani (ECY) equation. We identify this as the result of the abelian quantum mechanics (QM) of a black hole. We conclude that the radiation emitted by a black hole is a zero-intensity electromagnetic radiation.
- [10] faKiv:2404.07775 [pdf]
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Delocalization in the absence of gravityComments: 5 pages, LaTeX; v2 is a new section about the non-perturbative character of the effective action
We discuss the effects of the de-Sitter spacetime for a baryonic-gravity-matter system on the ability of the effective action of the effective theory to diffuse to the lowest quasi-local coordinate in the spacetime. We discuss the properties of the effective action de-Sitter and its de-Sitter diffusive behavior in the absence of the gravitational coupling. We discuss the physical effects of the non-perturbative effects of the de-Sitter diffusiveness on the non-perturbative character of the effective action of the effective theory.
- [11] faKiv:2404.07883 [pdf]
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Axion Gravitational Waves in the Presence of a Non-perturbative HamiltonianComments: 30 pages, 6 figures, 1 table
We study axion gravitational waves in the presence of a non-perturbative Hamiltonian. We find that the axion waves are described by the scalar fields of the graviton and the scalar fields of the axion. The presence of the non-perturbative Hamiltonian results in the propagation of axion gravitational waves. The propagation of the scalar fields of the axion is controlled by the polarization of the scalar waves. The propagation of the scalar fields of the axion is thus affected by the polarization of the scalar waves.
- [12] faKiv:2404.08238 [pdf]
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A Quantum Theory of GravityComments: 21 pages
We investigate a quantum theory of gravity by means of a quantized Hamiltonian. We investigate a classical theory of gravity by means of a quantized Hamiltonian, and we discuss the relation between the quantum theory and the classical theory. We demonstrate that the quantum theory is in agreement with the classical theory at the level of the gauge group. We also provide a new and simple construction, which is a classical theory of gravitation.
- [13] faKiv:2404.08289 [pdf]
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The runoff equation for general noncommutative Schwarzschild black holesJ. J. O. Costa, R. A. Gomes, H. L. C. A. S. Alves, J. D. S. Silva, F. C. Miranda, J. A. Lara, V. S. L. M. MaganComments: LaTeX, 11 pages, 7 figures
In this paper, we study the conclusion that the runoff equation is valid for general noncommutative Schwarzschild black holes in four dimensions. The experimental taxonomy of the black holes is identified. We also study the properties of the black holes under the influence of the runoff equation, in order to determine whether the black holes are physically realistic.
- [14] faKiv:2404.08572 [pdf]
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Cross-section of the AdS$_3$/CFT$_2$ gravity coupled to the scalar fieldsComments: 11 pages, 9 figures, minor changes
This article reviews the cross-section of the AdS$_3$/CFT$_2$ gravity coupled to the scalar fields. It is shown that the apparent size of the scalar fields depends on the scalar field fields and the curvature of the AdS$_3$ space is the same as the space of the scalar fields.
- [15] faKiv:2404.08655 [pdf]
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The multiverse as a function of the cosmological constantComments: 32 pages, 1 figure
We study the multiverse in a model-independent manner (i.e., without the presence of the cosmological constant) and show that the multiverse is a function of the cosmological constant. We explain how multiverse scales are determined, in which case the multiverse is a function of the cosmological constant. The scalar-tensor principle is used to show that the multiverse is a function of the cosmological constant and that the cosmological constant is a function of the curvature of the universe. The cosmological constant and the curvature of the universe are unary functions in the multiverse, and the multiverse scales depend on the cosmological constant. The multiverse scales are defined by the cosmological constant and curvature of the universe, and are in agreement with the Planck data.
- [16] faKiv:2404.08690 [pdf]
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Holographic theory of high density statesComments: 4 pages. To appear in: "Volume of the Journal: 2018", March 1 - 3, 2018
We study the holographic theory of high density states by considering the holographic duality between two classical states of one dimension: two topological states of one dimension, which are related by an angle of derivation $D_1$ from the other state of two dimensions. We use this result to construct a generalized holographic duality, which is the holographic duality between two states of two dimensions in terms of the holographic duality between two states of two dimensions in terms of the holographic duality between two states of two dimensions. This generalized holographic duality is shown to be a holographic duality between two states of two dimensions in terms of the holographic duality between two states of two dimensions. As a consequence of this generalized holographic duality, we can rewrite the standard S-matrix as a holographic duality between two states of two dimensions in terms of the holographic duality between two states of two dimensions. This holographic duality between two states of two dimensions is equivalent to a holographic duality between two states of two dimensions in terms of the holographic duality between two states of two dimensions.
- [17] faKiv:2404.08772 [pdf]
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The BVI model of the quantum-mechanical Yang-Mills theoryComments: 20 pages, 3 figures
The BVI model of the quantum-mechanical Yang-Mills theory (QMFT) is studied at higher order in a Non-perturbative approach. The solution of the model is constructed and it is shown that the solution produces the BVI model of the quantum-mechanical Yang-Mills theory. The solution and the analysis of the relativistic behavior of the model are presented in detail. It is shown that in the limit where the relativistic behavior of the model is neglected, the existence of the BVI model of QMFT is confirmed.
- [18] faKiv:2404.08823 [pdf]
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Bunch-Davies Equation for the Case of Anomalous Lattice Gravitational WavesComments: 11 pages, 3 figures, v3: references added, typos corrected
We use the Bunch-Davies equation of motion for a perturbative system for the case of anomalous lattice gravitational waves to investigate the reason why "Higgs-like" duality of the Bunch-Davies equation is not preserved in the presence of gravitational waves. We investigate the point-like perturbation theory of gravity and show that the connection between the Bunch-Davies equation and the Bunch-Davies equation is not preserved in the presence of gravitational radiation.
- [19] faKiv:2404.08831 [pdf]
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The Hawking Radiation and the Quantum GravityComments: 11 pages, 14 figures
In this paper we study the Hawking radiation and quantum gravity in an expanded cosmological model with a metastable gravitino and a neutron star, with the latter acting as a particle-hole and as a gravitino. The latter is not entirely free from technical issues and so, in addition to the test of quantum gravity, we also investigate whether the Hawking radiation is non-local and whether the Hawking radiation is local. We obtain a correct answer for the latter to the latter, which is consistent with the predictions of quantum gravity. Finally, we illustrate that the Hawking radiation is locally local and that the Hawking radiation is locally local, thereby resolving the issue of whether the Hawking radiation is quantum and how the Hawking radiation is quantum.
- [20] faKiv:2404.08865 [pdf]
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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.