Dirac equationmesonsSU(3) theoryYang-Mills theory/ black hole physicsconfining solutionsSU(3)-Yang-Mills equationsrelativistic modelsMinkowski space-timeThe black hole physics techniques and results are applied to find aset of exact solutions of the SU(3)-Yangu2013Mills equations in Minkowskispaceu...
Black Hole Physics, Confining Solutions of SU(3)-Yang– Mills Equations and Relativistic Models of Mesons.The black hole physics techniques and results are applied to find a set of exact solutions of the SU(3)-Yang-Mills equations in Minkowski space-time in the Lorentz gauge. All the ...
关于黑洞物理的若干问题 Some Topics on Black Hole Physics(蔡荣根).ppt,In order to be well-defined for the variation, a Gibbons and Hawking surface term has to be added to the action where C is a term which depends only on the boundary metric h and not o
as compared to the extreme allowed by the Kerr geometry, and are electrically neutral. The space-time around such a black hole is thus well approximated by the spherically symmetric Schwarzschild geometry, where the radius of the trapping horizon is determined by its mass,R=2GMc2. The latter ...
The Hamiltonian mapping of the Dirac equation with a quantum perturbation in 2D black hole models are investigated. We derive the Hamiltonians of the modified Rabi model for the point matter black hole and noncommutative black hole, and obtain perturbed expressions for the velocity and acceleration ...
The p5 equation follows because the Schwarzschild black hole is neutral. View article Read full article URL: https://www.sciencedirect.com/science/article/pii/S0370157302002715 Journal 2002, Physics ReportsJustin R. DavidGautam MandalSpenta R. Wadia Chapter QUANTUM GRAVITY 2007, Philosophy of Physics...
Progress in PhysicsU.V.S. Seshavatharam, Physics of Rotating and Expanding Black Hole Universe, Progress in Physics, vol. 2, pp7-14, 2010.U. V. S. Seshavatharam, Physics of rotating and expanding black hole universe. Progress in Physics, Vol-2, April, 2010. P. 7-14....
Since the last factor has to be positive, Ω has to lie between the two roots of the corresponding quadratic equation: (2.86)−gtϕ+gtϕ2−gttgϕϕgϕϕ<Ω<−gtϕ+gtϕ2−gttgϕϕgϕϕ. As one approaches the black hole, one reaches the distance rstat where...
3.2 Equation of state In order to explore the similarities between the Lorentz Violation black hole solution in Lifshitz spacetime (32) and liquid–gas system in the extended phase, we make the assumption that both the charge and the cosmological constant are fixed external parameters, not thermody...
Black hole temperature Drake equation Hubble's LawWe make it count! Calculator Categories BiologyChemistryConstructionConversionEcologyEveryday lifeFinanceFoodHealthMathPhysicsSportsStatisticsOtherDiscover Omni Press Editorial policiesJournalist's Guide to NumbersPartnerships Meet Omni AboutBlogContactWe're hiring!