Titlebook: Relativistic Quantum Mechanics; Lawrence P. Horwitz Book 2015 Springer Science+Business Media Dordrecht 2015 Bose-Einstein Condensation.Ja

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Relativistic Classical and Quantum Mechanics,en be in a position to introduce the relativistic quantum theory developed by Stueckelberg (1941) and Horwitz and Piron (1973). We describe in this chapter a simple and conceptual understanding of the Newton-Wigner problem (Newton 1949) presented above, a rigorous basis for the energy time uncertain

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The Relativistic Action at a Distance Two Body Problem, framework than the perhaps more fundamental field mediated models for interaction, and are also straightforwardly amenable to rigorous mathematical analysis. In this Newtonian-Galilean view, all events directly interacting dynamically occur simultaneously; the dynamical phase space of N particles c

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Experimental Consequences of Coherence in Time,in which it was demonstrated that an electron wave packet undergoing a sequential ionizing perturbation in time (from Argon gas) undergoes interference phenomena, and the careful analysis and design of an experiment by Palacios et al. (2009) to show that a two electron spin state could be formed coh

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Scattering Theory and Resonances,ator) by the semi-axiomatic approach of Lehmann et al. (1955) or through the use of interaction picture expansion of the perturbed field equations (Schweber 1964; Jauch and Rohrlich 1955; Schwinger-Tomonaga 1948). Feynman’s approach to scattering in spacetime (Feynman 1949), using the method of prop

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Hamiltonian Map to Conformal Modification of Spacetime Metric: Kaluza-Klein and TeVeS,ement of simulations using the Newtonian form for gravitational attraction (with forces proportional to . between stellar bodies) with the Tulley-Fisher radiation curves (Tulley 1977) is due to a matter distribution that is not visible through emitted light (so-called “dark matter”), but it has been