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On Galaxies Rotation Curves: Gravitomagnetism Rather than MOND and Missing Mass 关于星系旋转曲线:重磁而非MOND和缺失质量
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.148067
P. Christillin
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引用次数: 0
Inconsistency of General Relativity Predictions for the Universe Expansion vs. the Black Hole Model 广义相对论对宇宙膨胀的预测与黑洞模型的不一致
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.141002
P. Christillin
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引用次数: 2
On the Fine Structure and the Other Coupling Constants at the Planck Scale 普朗克尺度下的精细结构和其他耦合常数
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.145037
P. Christillin
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引用次数: 1
From Generalized Hamilton Principle to Generalized Schrodinger Equation 从广义汉密尔顿原理到广义薛定谔方程
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.145039
Xiangyao Wu, Benshan Wu, Hong Li, Qiming Wu
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引用次数: 0
Time Dilation Cosmology 时间膨胀宇宙学
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.146049
J. Forrington
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引用次数: 0
The General Theory of the Probability 概率论
Pub Date : 2023-01-01 DOI: 10.4236/jmp.2023.148063
Julio A. Barraza
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引用次数: 1
Killing Operator for the Kerr Metric Kerr度量的Killing算子
Pub Date : 2022-10-21 DOI: 10.4236/jmp.2023.141003
J. Pommaret
When D : E → F is a linear differential operator of order q between the sections of vector bundles over a manifold X of dimension n , it is defined by a bundle map Φ : J q ( E ) → F = F 0 that may depend, explicitly or implicitly, on constant parameters a, b, c, ... . A ”direct problem ” is to find the generating compatibility conditions (CC) in the form of an operator D 1 : F 0 → F 1 . When D is involutive, that is when the corresponding system R q = ker (Φ) is involutive, this procedure provides successive first order involutive operators D 1 , ..., D n . Though D 1 ◦ D = 0 implies ad ( D ) ◦ ad ( D 1 ) = 0 by taking the respective adjoint operators, then ad ( D ) may not generate the CC of ad ( D 1 ) and measuring such ”gaps” led to introduce extension modules in differential homological algebra. They may also depend on the parameters and such a situation is well known in ordinary or partial control theory. When R q is not involutive, a standard prolongation/projection (PP) procedure allows in general to find integers r, s such that the image R ( s ) q + r of the projection at order q + r of the prolongation ρ r + s ( R q ) = J r + s ( R q ) ∩ J q + r + s ( E ) ⊂ J r + s ( J q ( E )) is involutive but it may highly depend on the parameters. However, sometimes the resulting system no longer depends on the parameters and the extension modules do not depend on the parameters because it is known that they do not depend on the differential sequence used for their definition. The purpose of this paper is to study the above problems for the Kerr ( m, a ), Schwarzschild ( m, 0) and Minkowski (0 , 0) parameters while computing the dimensions of the inclusions R (3)1 ⊂ R (2)1 ⊂ R (1)1 = R 1 ⊂ J 1 ( T ( X )) for the respective Killing operators. Other striking motivating examples are also presented.
当D:E→ F是维数为n的流形X上向量丛截面之间的q阶线性微分算子,它由丛映射Φ:Jq(E)定义→ F=F 0,它可以显式或隐式地取决于常数参数a、b、c。一个“直接问题”是以算子D1:F0的形式确定生成相容性条件(CC)→ F 1。当D是对合的,即当相应的系统Rq=ker(Φ)是对合时,该过程提供了连续的一阶对合算子D1。。。,D n。尽管D1◦ D=0表示ad(D)◦ 通过取相应的伴随算子,ad(D1)=0,则ad(D)可能不会生成ad(D1)的CC,并且测量这样的“间隙”导致在微分同调代数中引入扩展模。它们也可能取决于参数,并且这种情况在普通或部分控制理论中是众所周知的。当Rq不是对合的时,标准延拓/投影(PP)过程通常允许定义整数R,s,使得延拓的q+R阶投影的图像R(s)q+RρR+s(Rq)=Jr+s。然而,有时生成的系统不再依赖于参数,扩展模块也不再依赖于这些参数,因为众所周知,它们不依赖于用于定义的不同序列。本文的目的是研究Kerr(m,a)、Schwarzschild(m,0)和Minkowski(0,0)参数的上述问题,同时计算相应Killing算子的包含体R(3)1⊂R(2)1 8834R(1)1=R1 8834J 1(T(X))的维数。还列举了其他引人注目的激励例子。
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引用次数: 5
Supersymmetry in the Geometric Representation of the Early Universe Wave Function 早期宇宙波函数几何表示中的超对称性
Pub Date : 2022-09-22 DOI: 10.4236/jmp.2023.146044
B. Lev
An approach to the geometric description of the birth and evolution of the universe is proposed. The wave function as the fundamental field is represented by a Clifford number with the transfer rules that possess the structure of the Dirac equation for any manifold. In terms of this geometric representation of the universe wave function, the nature of super-symmetry is explained. A probable mechanism of spontaneous symmetry breaking of the universe excitations with Bose and Fermi degrees of freedom is proposed.
提出了一种对宇宙诞生和演化进行几何描述的方法。作为基本场的波函数由Clifford数表示,其传递规则具有任何流形的Dirac方程的结构。根据宇宙波函数的这种几何表示,解释了超对称性的性质。提出了玻色自由度和费米自由度宇宙激发自发对称性破缺的可能机制。
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引用次数: 0
Hamilton-Jacobi and Lagrange formulation of relativistic quantum mechanics wave equations with solutions with only-positive and only-negative kinetic energies 具有正动能和负动能解的相对论量子力学波动方程的Hamilton-Jacobi和Lagrange公式
Pub Date : 2022-02-18 DOI: 10.21203/rs.3.rs-1332654/v1
L. G. de Peralta, A. Ruiz-Columbié
Using the Hamilton-Jacobi and the Lagrange formalisms, a pair of relativistic quantum mechanics equations are obtained. These equations, in contrast with the Klein-Gordon and other relativistic quantum mechanics equations, have no solutions with both positive and negative kinetic energies. The equation with solutions with only positive kinetic energy values describes a spin-0 particle of mass m, which is moving at relativistic speeds in a scalar potential. The wavefunctions and the energies corresponding to the associated antiparticle can be obtained by solving the other equation, which only has solutions with negative kinetic energy values.
利用哈密顿-雅可比和拉格朗日形式,得到了一对相对论性量子力学方程。与Klein-Gordon和其他相对论量子力学方程不同,这些方程没有同时具有正、负动能的解。这个方程的解只有正动能值,它描述了一个质量为m的自旋为0的粒子,它在标量势中以相对论速度运动。对应反粒子的波函数和能量可以通过求解另一个方程得到,该方程只有负动能值的解。
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引用次数: 0
Possible Neutrino-Antineutrino Production during Gamma Ray e−e+ Pair Production: Monte Carlo Simulation Study 伽马射线e&负e+对产生过程中可能产生的中微子-反中微子:蒙特卡罗模拟研究
Pub Date : 2022-01-01 DOI: 10.4236/jmp.2022.1311082
M. Bettan, Jonathan Walg, I. Orion
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引用次数: 0
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