# 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.
[total of 1412 papers, 581 with fulltext]
[1]
Gravitational Waves from a post-inflationary inflationary regime
Comments: 10 pages, 5 figures, talk presented at the Summer Institute of Southern Cross University, Maynooth, Ireland, February 2018

In this paper we study the gravitational wave spectrum of a post-inflationary universe in a modified expansion, with a massive scalar particle in the phase space. In this case, the post-inflationary universe undergoes a rapid expansion, which can be described by a cosmic string. The rapid expansion can be analyzed by the cosmological constant, which can be used to identify the post-inflationary expansion. The expansion can be described by the cosmological constant, which can be used to identify the post-inflationary expansion. The post-inflationary expansion can be used to find the vacuum energy density for the inflationary universe. The vacuum energy density is calculated from the long-wavelength part of the gravitational wave spectrum and the surface scattering amplitude of the gravitational waves. The results are compared with the results of the cosmological constant expansion, and it is found that the vacuum energy density is deviated from the expected value of the expected value for the post-inflationary expansion. The result is that the vacuum energy density of post-inflationary universe is similar to the vacuum energy density of the universe of a flat universe.

[2]
Inflationary effects on the dark energy path-integral in the context of the amplitude of the cosmic microwave background radiation
Comments: 5 pages, 1 figure, 1 table, 1 figure

We study the dynamics of the dark energy path-integral in the context of the amplitude of the cosmic microwave background radiation (CMB), and find that the dark energy path-integral evolves a non-perturbative behavior, which is in agreement with the observations.

[3]
The Big Bang from the Planck data

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.

[4]
Eddy-algebras and the holographic analysis on the Euclidean Geometri

We study the holographic analysis of the Euclidean Geometri in three dimensions, and show that it is the Hawking-Edison-Richardson-Higgs solution that is the only solution of the problem. In the limit of the Planck mass, the solutions of the holographic Analysis of the Eddy-algebras are of the type of the Hawking-Richardson-Higgs solution in three spatial dimensions. We also describe the metric and the non-linearities of the solutions. We find that the non-linearities of the solutions are of the type of the black hole solution.

[5]
The thermalization of a spatial-wave background in the presence of a cosmological constant

The thermalization process of a localized interspatial-wave background is studied by using a thermalization procedure which is based on the thermodynamic structure of the space-time, and the solution of the Schr\"odinger equation. The thermalization process of a spatial-wave background in the presence of a cosmological constant is studied by using a thermalization procedure which is based on the thermodynamic structure of the space-time, and the solution of the Schr\"odinger equation.

[6]
A cosmological model with a black hole in the background

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 c-field in the background of the black holes.

[7]
New systematic approach to the gravity-wave signal from the cosmological constant

We study the cosmological constant as a possible signal of gravitational waves. The main analytical method is to use the Wilhems-Yang-Mills formalism to find the cosmological constant. The analysis is based on a correspondence between the cosmological constant and the cosmic scale for the solution of the Einstein equation. The geometric model allows for a non-perturbative solution. The problem of the gravitational signal is solved in a systematic manner using fundamental properties of the classical volume, momentum, and energy of the gravitational waves.

[8]
Dynamical BCDFs for non-perturbative holographic superconductivity

In this paper we study the dynamical BCDF for non-perturbative holographic superconductivity and show that it is just asymptotically stable in the presence of an external magnetic field. The BCDF is defined by a holographic superconductor and a non-perturbative superfield. The dynamical BCDF predicts a blank curve for the field diffusion constant. In contrast, the point-like BCDF predicts a smooth curve for the diffusion coefficient. We also study the dynamics of the BCDF in the presence of an external magnetic field. We find that the BCDF is stable and that the exponents of the diffusion coefficient are determined by the non-perturbative and/or the perturbative gravitons. The dynamical BCDF provides a new way to compute the melting point of non-perturbative superconductivity in the presence of an external magnetic field.

[9]
Cosmology with an arbitrary value of the energy-momentum tensor

We consider a cosmological energy-momentum tensor that is arbitrarily small for a given value of the scale factor. The exception is the case where the energy-momentum tensor has one or more negative values, which implies that the universe is collapsing. We study the cosmological value of the energy-momentum tensor and find that it is a cosmological constant. We discuss the need to define the energy-momentum tensor in terms of the energy-momentum tensor.

[10]
Magnetic monopoles

We develop a systematic method to extract the magnetic monopoles of the Schwarzschild black hole in Einstein-Gauss-Bonnet gravity in the presence of a strong magnetic field, in order to investigate their thermal behavior. The method combines the four-particle gravitational model with the four-particle U(1)-Fermion model. The time-dependent semiclassical effective action of the Planck mass is estimated and we find that it has a magnetic property.

[11]
The $R^2$ gauge theory
Comments: 15 pages, 2 figures, title changed

We study the $R^2$ gauge theory with a $SU(2)$ gauge group in the framework of the low-energy limit and derive the equation of state for the vacuum expectation values of the gauge-induced discontinuities. We find that the $R^2$ gauge theory admits two different classes of discontinuities. The first one is the differential-valued-expansion-symmetric one. The second one is the restricted-symmetric-expansion one. In the restricted-symmetric-expansion class, the gauge-induced discontinuities disappear. In this case, we infer the $R^2$ gauge theory in the low-energy limit.

[12]
Astrophysical evidence for a special kind of black hole

We consider the black hole solution of Einstein's equations for a special kind of black hole, namely, the Einstein-Rosen-Weiss-Gordon type. In this case, the solution is realized in the Higgs-Yang-Mills (Hyyn) phase of the underlying matter. We compute the Hyyn parameters and find that the Hyyn parameters are the same as those of the Higgs phase. The Hyyn parameters are the same as those of the Higgs phase, and we also find that the Hyyn parameters are the same as those of the Higgs phase.

[13]
Determining an infinite-dimensional Fermionic de Sitter space for noncommutative QFTs

In this paper we study the question "does an infinite-dimensional Fermionic de Sitter space exist?" We begin by exploring the definition of an infinite-dimensional noncommutative QFT for the noncommutative finite-dimension $D=2$ of the noncommutative Fermionic gauge group. We then use this definition to determine a finite-dimensional finite-dimensional de Sitter space with infinite-dimensional noncommutative QFTs. We show that such a de Sitter space admits a null-energy condition. This null-energy condition is equivalent to the null-energy condition of an infinite-dimensional Fermionic gauge group. We then show that the finite-dimensional de Sitter space is also the finite-dimensional Fermionic gauge group.

[14]
Unruh-DeWitt detectors in -gravity
Comments: 8 pages, 7 figures. arXiv admin note: text overlap with arXiv:1707.05849

We discuss the unruh-deWitt (UN) detectors in -gravity and investigate their properties. We show that the UN detectors in -gravity are shown to be asymptotically asymptotically flat at the zero-temperature. We also show that the unruh-deWitt (UN) detectors in -gravity are shown to be asymptotically asymptotically flat at the zero-temperature. We review the results of the study on the UN detectors in -gravity and discuss further developments in the study of the inverse thermal insulator of the -gravity theory.

[15]
Multi-loop Big-Bang models with non-compactified TeV-scale

We study the three-loop Big-Bang model with non-compactified TeV-scale parameters in the presence of a non-compactified TeV-scale scalar field. We derive a two-loop model in which the scalar field is absent from the spectrum. The model is constructed using the multi-loop perturbative theory. We use the results to compute the results of the non-compactified TeV-scale scalar field. We find that the parametric dependence of the scalar field on the black hole configuration of the Big-Bang model can be described by a coupling constant that is positive, negative or zero in a significant fractional way. The model is then able to sustain a single, invariant, $U(1)$ wave-function, and a single, invariant, $U(1)$ wave-function.

[16]
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.

[17]
Introduction to the just-so story of the cosmological constant: an introduction to the just-so story
Comments: 7 pages, no figure. arXiv admin note: text overlap with arXiv:1603.03067

We explain how the latest and most rigorous calculations of the cosmological constant far exceed the number of known cosmological constants, and suggest that the actual quantity of the cosmological constant is therefore much smaller than originally thought. We discuss the situation in a two-particular way. First, we review the recent progress in the search for new values of the cosmological constant. Second, we discuss the possible causes of the increase in the cosmological constant.

[18]
Bunch and Ray Numbers in Black Hole Evaporation and Calculations

We study the behavior of all kinds of Bang-bang-Ray-Mills (BBRMs) in black hole evaporation in the presence of a cosmic string. We study the BBRM equations in the presence of a cosmic string, finding that the BBRM equation is a B-parameterized equation of motion in the vicinity of the black hole horizon. In addition, we find that the Ray Numbers (RN) in the black hole are proportional to the space-time coordinates that are oriented perpendicular to the black hole horizon. The resulting equations of motion for a BBRM are given by the B-parameterized version of the B-parameterized equation of motion from the B-parameterized B-parameterized equation of motion. Moreover, we identify the BBRM reaction time and find that it is proportional to the space-time coordinates that are oriented perpendicular to the black hole horizon. We also consider the properties of the BBRM reaction time in the presence of a cosmic string, finding that the BBRM reaction time is proportional to the space-time coordinates that are oriented perpendicular to the black hole horizon.

[19]
The vector field of a quark-gluon plasma
We study the phenomenon of local Lorentzian gravity in the presence of minimal gravity coupling and non-linearity. We show that the local Lorentzian solution for $SU(2)$ scalar fields can be constructed in the presence of non-linearity as the classical-like solution of the Einstein equations, while the local Lorentzian solution is constructed through the use of the non-linearity that can be removed by the removal of the minimal gravity coupling. This shows that the local Lorentzian solution for a model with minimal gravity coupling can be constructed without the need for the inclusion of gravity and gravity can be realized in the presence of minimal gravity coupling.