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:2009.07213 [pdf]

Resting state curvature and the 8D $U(1)$ caseComments: 8 pages, published version
We study the 8D $U(1)$ case in the presence of an external scalar field that is a massless scalar field with the mass of the scalar field and is coupled to a $\mathbb{Z}_2$vector. In this case, we compute the resting state curvature of the state space, in the presence of an external scalar field, and we determine that the resting state curvature is given by the rate of the resting state decay.
 [2] faKiv:2009.07260 [pdf]

Lightcone supersymmetry and the causality relationComments: 17 pages, 5 figures
We study the lightcone supersymmetry in the theory of Einstein and YangMills (EJ and YM) theories and find that its effects are of the type of the gammaray photons. We explore the possible role of the lightcone supersymmetry in the gaugegravity theory of lightcone EinsteinYangMills theories.
 [3] faKiv:2009.07266 [pdf]

Ninedimensional gravity in $AdS_4$ de Sitter spacetimeComments: 8 pages, 2 figures, v1: minor corrections, references added
We study the ninedimensional gravity in a de Sitter spacetime in $AdS_4$ spacetime.
 [4] faKiv:2009.07300 [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.
 [5] faKiv:2009.07354 [pdf]

Nonperturbative quadratic quarkgluon plasma in a gravityflux backgroundComments: 19 pages, 6 figures
We investigate the nonperturbative quadratic quarkgluon plasma (QGP) in the presence of a gravitino field in a gravityflux background.
 [6] faKiv:2009.07554 [pdf]

Skyrmepropagation of the Higgs field in four dimensions and the entanglement with the Ho\v{e}therianComments: Published version
In this paper we study the propagation of the Higgs field in four dimensions in the presence of a background field, called the Ho\v{e}therian. We have calculated the propagators of the Higgs field in four dimensions in the presence of the Ho\v{e}therian in the presence of a background field. We have found that the propagation of the Higgs field is localized in the direction of its entangling force at the boundary. We have also calculated the propagators of the Higgs field in four dimensions in the presence of the Ho\v{e}therian in the presence of a background field.
 [7] faKiv:2009.07560 [pdf]

Generalized incoherent Higgs models with a oneloop nonlinear sigma modelComments: 12 pages, 5 figures
The approach of the oneloop nonlinear sigma model (NLSM) is recognized as a promising candidate for characterizing the quantum nature of the Higgs vacuum state. In this statement, we show that the generalization of the NLSM to the case of a oneloop nonlinear sigma model (NPCM) yields a zeropoint energymomentum tensor that is compatible with the Planck data. We also demonstrate that the zeropoint energymomentum tensor is compatible with the entire Planck data of the NPCM.
 [8] faKiv:2009.07562 [pdf]

Firstorder differential equations of classical systems with a scalar field and a Hamiltonian in the presence of a gravitational wave signalComments: 17 pages, two columns
We investigate the dynamics of classical systems with a scalar field and a Hamiltonian in the presence of a gravitational wave signal. The scalar field is nonlocal in the vicinity of the horizon, and the Hamiltonian is a generalized nonlinear messian of the EinsteinHilbert structure. Any two such systems can be studied as the diagrammatic representation of a torsional equation of motion. We find that the scalar field in the presence of the gravitational wave signal can generate a firstorder differential equation of motion that is firstorder in the degree of freedom of the Hamiltonian. We show that the equation of motion is firstorder in the KelvinTaylorRouetHiggs direction, and our results provide proof of the generalization of the results in the case of a scalar field and a Hamiltonian in the presence of a gravitational wave signal. In particular, the equation of motion is firstorder in the KelvinTaylor direction in the regular direction, and we show that this equation is firstorder in the normal direction, and that it is firstorder in the KelvinTaylor direction in the nonperiodic direction.
 [9] faKiv:2009.07579 [pdf]

Probing the bound on the energy scale of black holes and supersymmetric QFTsComments: 19 pages, no figures, v2: minor changes, references to published version
In this paper, we investigate the energy scale of black holes and supersymmetric QFTs in the presence of a bound on the energy scale. We show that the bound on the energy scale can be satisfied only if the energy scale of the black hole is sufficiently large. In this case, the bound on the energy scale can be realized as a RealTime System. We find that for two specific black holes and one specific supersymmetric QFT, the bound can be satisfied only if the bound on the energy scale is sufficiently large. We also show that the bound can be satisfied in the presence of a bound on the energy scale for two specific black holes and one specific supersymmetric QFT.
 [10] faKiv:2009.07592 [pdf]

Relativistic effects of a gravitational wave interference in the background of the gravitational wavesComments: 5 pages, 3 figures, no figure. v2: minor changes; v3: minor changes
We construct relativistic effects of gravitational waves interference in the background of a gravitational wave. This is shown to be equivalent to the standard relativistic effects of the gravitational waves in the presence of a gravitational wave.
 [11] faKiv:2009.07796 [pdf]

Gravitational Waves in the presence of massless gravonsComments: 9 pages, 1 figure
Gravitational waves in the presence of massless gravons are studied. The massless gravons are chaotically shifted in the direction of the propagation of the gravitational waves, and the flow of energy is determined by the orientation of the particle beams. The gravitational waves are reflected off the gravons and are distorted by the distortions. The distortion factor is determined by the massless gravons in the direction of propagation of the gravitational waves. The reflection of the gravitational waves is calculated in its twopoint function in the presence of the massless gravons, and its relation to the reflection of the gravitational waves is expressed by the return of the massless gravons.
 [12] faKiv:2009.07871 [pdf]

Assisted expansion and the space of integrable extensionsComments: Title changed, references added, matches the published version
We study a generalized QFT of the Coulomb branch in 6d $SU(N)_k$ gauge theories and show that the space of integrable extensions is fully finite in the Coulomb branch. This results in the existence of a finite family of QFTs for 6d $SU(N)_k$ gauge theories, which is the first example of a QFT of a generalized Coulomb branch in 6d gauge theories. We compare our QFT to the associated RiemannZeldovich Equation and find that the RiemannZeldovich Equation is the only QFT to be able to preserve the Coulomb branch.
 [13] faKiv:2009.08173 [pdf]

Symmetric $\mathcal{N}=4$ supergravity in the presence of a scalar fieldComments: 12 pages, 3 figures
We study $\mathcal{N}=4$ supergravity in the presence of a scalar field. We first study the case of an arbitrarily large $N$ symmetry along the top of the $SU(2)$ and $SU(2)_U$ gauge groups, where $SU(2)$ is a supersymmetric supergravity. Then we consider a generic $SU(2)_U$ gauge theory with $SU(2)$ supersymmetry and construct a compact, $SU(3)$ model. We then show that the $SU(2)$ gauge theory that we construct is a supergravity theory in the context of the $SU(3)$ superconformal field theory. For a given $N$symmetry in the vicinity of the $SU(2)$ gauge group, we show that the supergravity theory that we construct is the supergravity theory in the context of the supergravity duality of the $SU(3)$ gauge theory with $SU(2)$ supersymmetry. We also discuss the role of the FreemanKemmerHawking entropy of the supergravity theory in the presence of a scalar field.
 [14] faKiv:2009.08190 [pdf]

The entrypoint function for the Higgsboson systemComments: 5 pages, 2 figures, referees added
For the Higgsboson system with an initial state of a weakly interacting field coupled to the gammaray to the fermion condensate, the entrypoint function of the Higgsboson system is found. We find that there is a finite value of this function for the Higgsboson system leaving no intervening term in the noncommutativity parameter.
 [15] faKiv:2009.08341 [pdf]

The etherHiggs duality in the framework of the Noncommutativity PrincipleComments: 11 pages, 4 figures, minor changes
We study the etherHiggs duality (Higgs duality) in the framework of the Noncommutativity Principle (NPC), and of the etherHiggs theory. We find that, in particular, the EtherHiggs duality is not compatible with the entropy of the ether. In the presence of the ether, however, it is possible for the etherHiggs theory to form a unique etherHiggs duality. In the presence of the Higgs, however, it is impossible for the etherHiggs theory to form a unique etherHiggs duality.
 [16] faKiv:2009.08412 [pdf]

Turbulence at the EXPLICIT LatticeComments: 6 pages, 1 figure, 1 table, v3: refs added
The EXPLICIT Lattice (TL) model is a model which has an extrema of the scalar field at the moment of the generation of the superconducting phase. In order to obtain the exact scalar field wave function of the model, we study its extrema and find their amplitudes. We calculate the exact scalar wave function of the model based on the function of the scalar field and the perturbative expansion. We find that the extrema of the scalar field are opposite to the one of the model. The demonstration that the exotics of the scalar field are opposite to the one of the model is a proof that the extrema of the scalar field are opposite to the superconducting ones.
 [17] faKiv:2009.08600 [pdf]

On the elimination of the Lagrangian from the classical Galilean modelComments: 11 pages, 5 figures
The classical Galilean model contains a large set of covariant Lagrangians and some of them are degenerate and are the ones that satisfy the standard equivalence relation. The corresponding Lagrangians are a candidate for a constructive solution to quantum gravity. We show that the corresponding Lagrangians lead to the elimination of a Lagrangian from the classical Galilean model. The elimination of the Lagrangian is shown to be independent of the choice of the Laplacian and the noncommutative parameter. We also show that the elimination of the Lagrangian leads to the elimination of the spectral parameter and we prove that this result holds in the case of the other two Lagrangians as well. The elimination of the Lagrangian leads to the elimination of the spectral parameter as well. Usually, the spectral parameter is a nontrivial parameter which is proportional to the energy and momentum of the spinor particles. We show that the spectral parameter can be taken as a fixed point. We also show that the reduction of the spectral parameter to zero, i.e., to zero energy, results in the elimination of the spectral parameter.
 [18] faKiv:2009.08673 [pdf]

The Skyrme model of KKComments: 22 pages, 8 figures, 8 tables
The Skyrme model of KK is a model of gravitational radiation in general relativity (GR) in which the flux of the graviton is introduced as a free particle. These authors propose a description of this model on a BoseHilbert model. On the other hand, the authors propose a description of the model on the equivariant pathintegral. This equivariant pathintegral describes the Skyrme model in the presence of a noncompact object.
 [19] faKiv:2009.08679 [pdf]

Quantum mechanics with the massless scalar field and its timereversal relationComments: 18 pages, 3 figures, LaTeX
We study the quantum mechanics with the massless scalar field in the framework of the minimal model of the classical Schr\"odinger theory. We show that the relativistic timereversal relation is the classical Schr\"odinger relation with the massless scalar field. This relation does not depend on the existence of the scalar field or on the timereversal relation. We also show that the relativistic timereversal relation for the nonsupersymmetric case does not depend on the presence of the scalar field. Finally, we show that the relativistic timereversal relation for the scalar field in the classical Schr\"odinger theory does not depend on the gauge condition, the spectral index, the amount of energy or on the timereversal relation.
 [20] faKiv:2009.08788 [pdf]

The photon's heat capacityComments: 14 pages, 6 figures
We study the temperature capacity of the photon in the presence of a magnetic field and find that its temperature is dependent on the scale of the external magnetic field. The thermodynamic temperature capacity of the photon is shown to be the same as that of a thermal massless particle in addition to the thermodynamic temperature capacity.