Submissions from Yuta Hayashi
- [1] faKiv:2404.08661 [pdf]
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Symmetry of Double Dimensional QFTs in a Classical $R$-CFV Schwarzschild Black HoleComments: 8 pages, 5 figures. Accepted for publication in PRD
We study the double-dimensional quantum field theory of $R$-CFV Schwarzschild black holes in a classical $R$-CFV Schwarzschild black hole background. We determine the following symmetric and non-symmetric solutions of the double-dimensional quantum field theory by properly fitting the canonical model of $R$-CFV black holes. We construct the canonical model of the double-dimensional QFTs using the structural equation-of-state (SEW) of the $R$-CFV black hole background in the presence of the $R$-CFV black hole. We determine the canonical model of the double-dimensional QFTs in terms of the SEW. We limit our study to the case where the boundary conditions are satisfied with respect to the canonical model of `R$-CFV black holes. We find that the canonical model of the double-dimensional quantum field theory is the model of the second-order quantum field theory of $R$-CFV black holes.
- [2] faKiv:2404.08666 [pdf]
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Bunch and Ray Numbers in Black Hole Evaporation and CalculationsComments:
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.
- [3] faKiv:2404.08682 [pdf]
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The Cosmological Evolution of a Black HoleComments: Latex, 6 pages, 1 figure. arXiv admin note: text overlap with arXiv:1808.06871
We study the cosmological evolution in the vicinity of a black hole using the method of the Euclidean solution of the Einstein-Hilbert equation. We find the Einstein-Hilbert solution of the Einstein-Hilbert equation and study the cosmological evolution in the vicinity of the black hole using the cosmological evolution formula. We present the results of our study and provide a detailed discussion of the cosmological evolution.
- [4] faKiv:2404.08714 [pdf]
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Atom-by-atom description of fermionic fields in a D-dimensional massless scalar fieldComments: 17 pages, 1 figure
We study the scalar field theory of the D-dimensional massless scalar field in the D-dimensional D5-D>D space-time. Using the atom-by-atom description of the scalar field, we derive the fermionic fields and the fermionic fields with the scalar field. The scalar fields are the atom-scalar fields in the D-dimensional D-space. The fermionic fields are the atom-atom fields in the D-dimensional D-space.
- [5] faKiv:2404.08794 [pdf]
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Cluster Diagrams of Gamma functions in the Minkowski spacetimeComments: 10 pages, 3 figures, one table. Version to appear in EPJC
We study the Minkowski spacetime cluster diagram for a class of noncommutative non-commutative Gamma functions. We show that the cluster diagrams of the Minkowski spacetime are the same as the cluster diagrams of the Minkowski spacetime, but that there are only two Minkowski diagrams. We also illustrate the inverse clustering theorem and the 3D, 4D, and 5D Minkowski diagrams.
- [6] faKiv:2404.08877 [pdf]
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Two-dimensional zero-temperature superconductivity in the presence of charged gluonsComments: 12 pages, 2 figures, v2: reference added
We study the zero-temperature zero-temperature superconductivity of two-dimensional matter in the presence of charged gluons. We analyze the charge-pumping effect of the gluons to determine the number of charged gluons, while calculating the capacitance of the gluons. We find that the charge-pumping effect of the gluons has a negative effect on the number of gluons in the zero-temperature zero-temperature superconductivity. We also find the physical consequence of the zero-temperature zero-temperature superconductivity. We find that there are two types of zero-temperature zero-temperature zero-temperature zero-temperature zero-temperature zero-temperature superconductivity in the presence of charged gluons.