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:2010.07213 [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:2010.07239 [pdf]

The powerful interaction between a weak gravitational field and a massive scalar field in the presence of a nonnegative cosmological constantComments: 4 pages, 5 figures
We study the strong interaction between a weak gravitational field and a massive scalar field in the presence of a nonnegligable nonlinear cosmological constant in the quantum phase transition between the vacuum and the null vacuum states. We find that the scalar field can be removed from the vacuum state in the presence of a nonnegligible nonlinear cosmological constant. We also calculate the scalar field of the scalar field in the null vacuum state. The spectral function can be obtained from the scalar field in the null vacuum state, and the spectral function can be obtained from the scalar field in the null vacuum state. We also find that the scalar field is the one that is the most sensitive to the interactions between the scalar field and the nonnegligible nonlinear cosmological constant. We then consider scalar fields in the null vacuum and the null vacuum states, and we find that in the null vacuum state the scalar field is the scalar field in the null vacuum state. In the null vacuum state, the scalar field is the scalar field in the null vacuum state.
 [3] faKiv:2010.07321 [pdf]

Quantum Gravity Black Holes, Quantum Entanglement and the Theory of an Entanglement Free UniverseComments: 6 pages, 3 figures
We study the physics of a quantum gravitational black hole in EinsteinGaussBonnet gravity. The black hole is described by an observer that is in a quantum vacuum state, and by a nonlocal observer that is not in a quantum vacuum state. The EinsteinGaussBonnet equation in the quantum vacuum state of the observer is also discussed. We study the effects of the quantum vacuum state on the geometry of the black hole. We demonstrate that, in the quantum vacuum state, the Hawking radiation from the black hole can make the black hole become a quantum entanglement free universe. In the nonperturbative limit, we find that the black hole is a quantum entanglement free universe, with Hawking radiation.
 [4] faKiv:2010.07333 [pdf]

The Big Bang from the Planck dataComments: 11 pages, 2 figures
In the big bang theory the prediction of the Planck data is the first step towards the prediction of the cosmological constant. The Planck data shows that the Big Bang was a hot Big Bang. We obtain the Big Bang temperature in the Planck data and find that the Big Bang temperature is consistent with the Planck data.
 [5] faKiv:2010.07519 [pdf]

A cosmological model with a black hole in the backgroundComments: 8 pages
We study the cosmological model with a black hole in the background. We show that the black holes are not necessarily black and that the cosmological constant is always positive. We also show that the cosmological constant is always positive when the black hole is removed. We show that the cosmological constant can be reduced to the cfield in the background of the black holes.
 [6] faKiv:2010.07574 [pdf]

Holographic Entanglement of a Big Bang Observable UniverseComments:
We study the holographic entanglement entropy of a big bang observable universe, which is the entropy of quantum fields in the universe. We derive the entropy of a big bang observable universe in two different holographic deterministic models. In the first model we find the entropy of the big bang observable universe in the big bang phase, which is the phase where the universe is accelerated in the Big Bang. In the second model we compute the entropy of the big bang observable universe in the big bang phase, which is the phase where the universe is accelerated in the Big Bang. In the case where the Big Bang particle is a particle decaying in a particlehole, we find that the entropy is the same as in the particlehole model, i.e., the entropy in the particlehole model is the same as the entropy in the big bang model.
 [7] faKiv:2010.07592 [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.
 [8] faKiv:2010.07690 [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:2010.07833 [pdf]

Supergravity and the de Sitter spaceComments: 14 pages, 1 figure, v3: references updated
We construct a de Sitter space solution for the supergravity field theory in the de Sitter space, which is consistent with the presence of a de Sitter singularity. The solution is constructed by bringing the de Sitter space to a point in the plane perpendicular to the normal plane. It is shown that the geometry of the de Sitter space solution is determined by the velocity of the de Sitter space. We also show that the solution satisfies the semiclassical interpretation of the $\Lambda$CDM singularity.
 [10] faKiv:2010.07852 [pdf]

Anomalous bipartite gauge theory of the Zsymmetric QCD modelComments: 36 pages
The bipartite gauge theory of the Zsymmetric QCD model, obtained by the ChernSimons theory, is shown to be a noncommutative theory of the matterfree gauge theory. There is an anomalous behavior of the energy of the gauge fields in the QCD model, which is characterized by the presence of a phase of the Zsymmetric gauge fields and the existence of a phase of the matterfree gauge fields.
 [11] faKiv:2010.07865 [pdf]

Scalartensor models with a cosmological constantComments: 6 pages, 4 figures, 1 table
We show that a scalartensor model explaining the dynamics of the Smatrix of a scalar field in four dimensions with a cosmological constant, as constructed by Delcambra and Tait, can be given in terms of a cosmological constant in three dimensions. The solution of the Einstein equations is replaced by a solution of the scalartensor equations in four dimensions.
 [12] faKiv:2010.08276 [pdf]

Quantum mechanics from the pattern space: the double copyComments: 19 pages, 6 figures
We present a new way of doing quantum mechanics in the context of the pattern space of the (de)Sitter space. The classical case of the de Sitter space is given by a classical lepton of the topologically twisted double copy. An explicit example of the double copy pattern space is presented. We argue that the pattern space of the de Sitter space is the de Sitter space of the Pide Sitter space. We use the double copy phenomenon in the pattern space to obtain the de Sitter space of the Pide Sitter space. We also conclude that the pattern space of the de Sitter space is the de Sitter space of the Pide Sitter space.
 [13] faKiv:2010.08284 [pdf]

Nonminimal coupling and the realization of a cosmological constant in the final phase of inflationComments: 15 pages
We show that the charge of the theory of gravitation that is a simplicial one in the final phase of inflation is proportional to the mass of the theory fermions, and that the mass of the theory fermions is determined by the charge $q$.
 [14] faKiv:2010.08407 [pdf]

Changes in the transverse curvature of the sigma model in the presence of a constant noncommutatorComments: 19 pages, 3 figures
We study the transverse curvature of the sigma model in the presence of a constant noncommutator and analyze the effect of the constant noncommutator on the transverse curvature in the sigma model. We analyze the transverse curvature in the sigma model in two different contexts: one is the classical sigma model in the presence of a constant noncommutator, and the other is the quantum sigma model in the presence of a constant noncommutator.
 [15] faKiv:2010.08412 [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.
 [16] faKiv:2010.08421 [pdf]

The Evanescent Universe: A Feynman Game ExampleComments: 18 pages, 3 figures
We explore the possibility of effects of a Feynman game on the standard model of the Standard Model. To do so, we calculate the Feynman gameinduced cosmological constant and we obtain the range of parameters where the cosmological constant becomes nonzero. Using the range of parameters, we find that the cosmological constant is always nonzero for a constant parameter, but growing with the expansion of the universe.
 [17] faKiv:2010.08565 [pdf]

A direct link between a statedependent affine metric and the kinetic term of a particleComments: 15 pages, 3 figures. arXiv admin note: text overlap with arXiv:1606.06010
We consider a direct link between a statedependent affine metric and the kinetic term of a particle, which is a consequence of the kinetic term of a geometrical unitary Hamiltonian. The affine metric has a directcurrentvoltagemomentum property with respect to the velocity of the particle. We show that the directcurrentvoltagemomentum properties of the affine geometrical metric can be regarded as the energymomentum of a particle. We determine the kinetic term of a particle in the kinetic term of the affine metric. We find a directcurrentvoltagemomentum formula, which determines the energymomentum of a particle.
 [18] faKiv:2010.08679 [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.
 [19] faKiv:2010.08750 [pdf]

A description of the model structure of the sum of two Lie groupsComments: 8 pages, 2 figures
We study the model structure of two Lie groups in the presence of a background gauge field. We study the case where one of the groups, the Lie group, is expressed as a geometric structure of one dimensional abelian spaces. We show that the group is a padic classification of Lie groups which is a monoidal representation of the twodimensional algebra analgebraic Lie group. We also show that the model of the sum of two Lie groups is a geometric structure of a second Lie group called the Lie group which is a monoidal representation of the Lie group. We also argue that the model consists of a sum of two Lie groups and a sum of a Lie groups and a sum of a Lie groups.
 [20] faKiv:2010.08769 [pdf]

Conformal symmetry of the Pyromaniac modelsComments: 19 pages, 8 figures
A simple, nonlinear form of the Pyromaniac models is presented and its conformal symmetry is studied. For a particular choice of the model parameters and a certain subset of the input parameters, a simple, nonlinear form of the Pyromaniac models is presented and its conformal symmetry is analyzed. The conformal symmetry is determined by the input parameters including a few cases where the model parameters are nonlinear and a few others where the model parameters are nonlinear and the input parameters are nonlinear. The resulting conformal symmetry is the exact solution of the equation of motion which was found in the previous work of the authors. The result is that the Pyromaniac models have conformal symmetry.