High-Energy Physics

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[total of 1412 papers, 581 with fulltext]
[1]  faKiv:2008.07324 [pdf]
A compact description of the KKLT model
Comments: 12 pages, 6 figures

In this paper, we extend the compact description of the KKLT model to the five-dimensional KKLT model. We generalize the KKLT model to the six-dimensional KKLT model. We consider the compact description of the model to the four-dimensional QCD model, and obtain the corresponding KKLT model and the corresponding KKLT model. In addition, we show that this model is compatible with the KKLT model in the bulk. That is, we show that the KKLT model is compatible with the KKLT model at the origin, and that the KKLT model is compatible with the KKLT model in the bulk.

[2]  faKiv:2008.07337 [pdf]
The DBI Group and the Time Domain
Comments: 17 pages, 1 figure

The DBI Group is a group of gauge groups that are algebraically pure, with no contributions from other groups. It is a supersymmetric group that is related to the algebraic group of the Lie algebra V2 of the N=2 super-O(N) groups. It has been suggested that DBI Group could possess an infinite number of subgroups, but this is a conjecture based on duality between the group corresponding to the subgroup of the DBI Group and that group of the Lie algebra V2. We argue that the DBI Group is the group of the Lie algebra V2 of the N=2 super-O(N) groups, and that there are DBI Group subgroups of the Lie algebra V2 whose subgroup is the group of the DBI Group. The DBI Group subgroups of the Lie algebra V2, which are the subgroups of the Lie algebra V2 of the N=2 super-O(N) groups, are found to be the group of the DBI Group. Our results illustrate the importance of using DBI Group subgroups of the Lie algebra V2 in the time domain of the massless field theory to prove the conjecture.

[3]  faKiv:2008.07377 [pdf]
Coulomb branch of the topological field theory of a Bose-Einstein condensate: Casimir kinetic term and other effects
Comments: LaTeX2e, 11 pages, 3 figures

In this paper we study the topological field theory of a Bose-Einstein condensate. The dynamical scalar sector is assumed to be the zero-point energy state of the condensate. We study the most general of the topological terms, which is the Casimir kinetic term, in the absence of the amount of non-zero charge of the condensate. We demonstrate that the Casimir kinetic term is not present in the zero-temperature regime and in the large-charge regime. It is shown that the Casimir kinetic term can be removed by adding a vehicle, which leads to the thermalization of the condensate. We discuss the consequences of this result for the zero-temperature regime and the large-charge regime.

[4]  faKiv:2008.07532 [pdf]
Quantum gravity-induced temperature dependence and the quantum thermodynamics
Comments:

In this paper, we study the thermodynamic properties of a particle in quantum gravity. Using the assumption that the temperature-gradient relation is the same as the thermodynamic one of the thermodynamics, we study the thermodynamics of the particle in quantum gravity. In order to do so, we calculate the quantum thermodynamics of the particle. We find that the quantum thermodynamics becomes stronger when the temperature-gradient relation is the same as the thermodynamics.

[5]  faKiv:2008.07604 [pdf]
Unprecedented size of the $q$-structure in AdS$_3$ and $\mathcal{N}=2$ supergravity
Comments: 10 pages, 5 figures

We show that the $q$-structure in AdS$_3$ and $\mathcal{N}=2$ supergravity can be obtained by the non-canonical solution of the AdS$_3$ and $\mathcal{N}=2$ supergravity equations. This result is in striking contrast to previous results that the $q$-structure is well-behaved in both AdS$_2$ and $\mathcal{N}=2$ supergravity.

[6]  faKiv:2008.07613 [pdf]
Generalized cross-curvature symmetries in the case of non-standard gauge fields and gauge fields with energy
Comments: 6 pages, 5 figures

We consider two specific examples of non-standard gauge fields and gauge fields with energy in the presence of standard gauge fields and gauge fields with energy. We find that these models have a special relation in the gauge field theory direction of the norm of the scalar field, which is a universal symmetry of the corresponding non-standard gauge field and gauge fields with energy. We show that the corresponding quantum field theory can be realized as a class of gauge theories with gauge fields and gauge fields of the opposite energy. We then discuss some aspects of the integration and the non-perturbative limit of these theories.

[7]  faKiv:2008.07651 [pdf]
Non-generic integrable systems
Comments: 9 pages, LaTeX2e, 8 pages, LaTeX2e, LaTeX2e

We compute the non-generic integrable systems of elliptic $L$-algebras in $AdS_{3\times S}$ (AdS_{3\times S})$) with $S=3$ and $S=2$ for $2n\geq 4$. The results are compared with those obtained by the same number from the duality of $AdS_{3\times S}$ and $AdS_{3\times S}$ in the case of $2n\geq 4$. The unification of the duality is shown to be the consequence of the algebra of the two singular integrable systems.

[8]  faKiv:2008.07654 [pdf]
From the KKL model to the Riemannian model
Comments:

In this paper we review results of a recent study of the KKL model in the context of the Riemannian model and of the Riemannian model itself. We show that the Riemannian model is a product of two different models, the KKL model and the Riemannian model. The KKL model is a product of the KKL model and the Riemannian model.

[9]  faKiv:2008.07657 [pdf]
Effects of the chiral fermion on the Lorenz-finite attractor and the underlying Lorenz-dilaton scattering amplitude
Comments: 49 pages, 4 figures, revised version to appear in Phys. Rev. D

In this paper a chiral fermion is introduced in the presence of a measure of the Lorenz-dilaton spin-2 potential and a background Lorenz-dilaton potential. We investigate the effects of this fermion on the Lorenz-dilaton spin-2 potential and the underlying Lorenz-dilaton scattering amplitude. As we demonstrate, the Lorenz-dilaton potential induces a behavior similar to that of a dilaton scalar spin-2 potential.

[10]  faKiv:2008.07711 [pdf]
A million-point integrability for the massless scalar field in the N=1 theory
Comments: 30 pages

We study the integrability of the massless scalar field in the N=1 theory in a thousand dimensions, which is equivalent to the massless scalar field in the general case of the Coulomb branch. We obtain the integrability of the massless scalar field in the N=1 case at the massless scalar-torsion branch. We compute the integrability of the massless scalar field in the total direction of the massless scalar branch and express it in terms of the number of points.

[11]  faKiv:2008.07806 [pdf]
Compactification in higher-spin fields with massless synchronous couplings
Comments: 12 pages, 2 figures

We study compactification effects in the $SU(3)$ Chern-Simons theory of higher-spin fields with massless synchronous couplings, by performing the standard 1/2-Chern-Simons decomposition in terms of the 1/4-Chern-Simons 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 non-compact, non-compact, compactification-free 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 compactification-free theory which corresponds to the known $SU(4)$ theory with massless synchronous couplings.

[12]  faKiv:2008.07882 [pdf]
The Radiation sphere of the cosmological constant in a chaotic universe
Comments: 16 pages

We study the cosmological constant field in a chaotic universe by considering a de Sitter vacuum of the form of a standard-like radiation sphere. The radiation sphere has a radius of the same order of the curvature of the space-time, and is characterized by the following properties: (1) It is invariant under a rigid coordinate transformation, (2) it is in the radiation sphere of the cosmological constant, (3) it is conserved in the radiation sphere of the cosmological constant, and (4) it is invariant under a non-linear transformation. The radiation sphere of the cosmological constant has a maximum radius, which is proportional to the cosmological constant, and a value determined by the change of the background curvature. The value of the radiation sphere of the cosmological constant is obtained at the moment of the expansion by removing the cosmological constant term. The value of the radius depends on the value of the cosmological constant. The result of the reduction of the cosmological constant to the radiation sphere of the cosmological constant is obtained by considering the cosmological constant term as the radiation sphere of the cosmological constant. The result of the transformation is the cosmological constant radiation radius.

[13]  faKiv:2008.08440 [pdf]
Entanglement entropy and the universal law of thermodynamics
Comments: 16 pages, 4 figures

We study the thermodynamic properties of the Lie-polyhedra (LPG) using the universal law of thermodynamics (UHT) and find that the entropy of the LPG is determined by the entropy of the subregion of interest. We conclude that the universal law of thermodynamics should be extended to the non-linear thermodynamic system by means of a generalization of Entanglement Entropy Law.

[14]  faKiv:2008.08470 [pdf]
On the Process of the AdS/CFT Transition
Comments: 17 pages, 3 figures; v2: minor changes, reference updated

We study the formation of the AdS/CFT transition in the presence of the scalar field in the vicinity of a packed CFT. We investigate the classical solution of the Einstein-Hilbert equation for a scalar field in the vicinity of a CFT, and show that the solution is compatible with a truncation of the effective action in the local gravity. The corresponding field equations have a constant curvature and a spin-orbit coupling which show that the local curvature and spin-orbit coupling measurements are equivalent. A critical mass, corresponding to the first state of the scalar field, is found.

[15]  faKiv:2008.08510 [pdf]
Monopole calculus and the Higgs mechanism in the quantum chromodynamics
Comments: 14 pages, 6 figures

We describe a monopole calculus for the Higgs mechanism. It is shown that the Higgs mechanism is the monopole of the Higgs field theory in the Higgs space. We also show that the Higgs mechanism can be eliminated in the quantum chromodynamics by a method similar to the Higgs model.

[16]  faKiv:2008.08561 [pdf]
Re-connection 1/N and Holographic Holography
Comments: 17 pages, published version

In this paper, we consider a model with a re-connection 1/N connected to the one-dimensional bosonic field theory by the one-dimensional wave-function. The model is constructed by means of the analytic Klein-Gordon formulation. The re-connection is obtained by means of the torsion-spin-torsion operator. The re-connection of the model is shown to be able to connect to the three-dimensional bosonic field theory in the same way as the one-dimensional reaction time.

[17]  faKiv:2008.08615 [pdf]
A note on supersymmetric higher-order theories: from Kitaev to Zamm
Comments: 17 pages, 10 figures; v2: references added, matches the published version

In this note we review the recent work of the author of the recently published Kitaev-Zamm work on the linearized version of the Klein-Gordon theory, which explicitly deduces the supersymmetric QCD action. This is a second-order theory formulated in terms of the dual Zamm-Klein theory. According to our review, the Kitaev-Zamm theory is the only known model which can be used to obtain the supersymmetric higher-order theories, which show a strong correspondence with the canonical theories of the Kitaev and Zamm groups. We proceed by briefly discussing the implications of our method for the generalization of Kitaev-Zamm theories to higher-order theories containing supersymmetric fields.

[18]  faKiv:2008.08674 [pdf]
The entropy of a a non-compact ideal gas
Comments: 8 pages, 5 figures

The entropy of a non-compact ideal gas is studied. The entropy of a non-compact ideal gas is calculated in the case of a non-compact gas with two spatial directions and a non-compact external constant. The entropy of the non-compact gas is found to be proportional to the average of the entropy of the two spatial directions. The entropy of the non-compact ideal gas is calculated using the non-compact gas theorem.

[19]  faKiv:2008.08686 [pdf]
Topological aspects of a black hole
Comments: 12 pages, v3: minor typos corrected

We clarify some basic notions of the, underlying black hole, in the context of a topological perspective. It is shown that the black hole is a real object, and that the spacetime geometry has a real structure. It is shown that the black hole is constructed from the space-time of a black hole observer. To illustrate this result, we construct a black hole observer, one whose space-time is a sphere and whose orbit is a point on a boundary. The observer's space-time has a real structure, and the observer's orbit is a point on a boundary. Our results establish that the black hole observer is a real object in the generic sense.

[20]  faKiv:2008.08869 [pdf]
What it means to be a zero-temperature model of the cosmological constant
Comments: 11 pages, 2 figures

We study the zero-temperature regime of a finite temperature scale, which is characterized by the absence of temperature-change-induced non-equilibrium fluctuations. It is shown that in the zero-temperature limit, the cosmological constant is always zero. In the absence of temperature-change phase transition, the integral of the cosmological constant is always zero.