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(Abridged) In this celebratory contribution, we present some new data from standard star cluster modelling containing primordial binaries and triples, as well as results from a binary black hole simulation with two massive members. In the star cluster case, the process of mass loss from evolving stars, together with general mass segregation, promotes favourable interactions involving compact subsystems of binaries and triples in the central region. Three-body interactions often lead to energetic ejections, with one or more of the components attaining relatively large terminal velocities which can be observed in principle. The second type of stellar system to be discussed is based on the scenario of two approaching galactic cores with density cusps, each having a massive black hole. After the subsystems become well mixed, the two massive components soon form a hard binary which gains energy by ejecting other members. Such a massive binary has a large cross section and can be very effective in depleting bound stars from the core. Again high-velocity escapers are produced, with their terminal speeds related to the shrinking binary size which eventually leads to coalescence.
We attempt a slingshot model interpretation of the unusual association of some 1&1/3 dozen nonstellar galaxian objects around the parent optical galaxy of the giant radio galaxy DA 240 (= 0748.6+55.8 (J2000)). Similar interpretation may be possible f
We generalize the Cosmological Slingshot Scenario for a Slingshot brane moving in a Klebanov-Strassler throat. We show that the horizon and isotropy problems of standard cosmology are avoided, while the flatness problem is acceptably alleviated. Rega
The interconnect is one of the most critical components in large scale computing systems, and its impact on the performance of applications is going to increase with the system size. In this paper, we will describe Slingshot, an interconnection netwo
The discrete nature of the solar magnetic field as it emerges into the corona through the photosphere indicates that it exists as isolated flux tubes in the convection zone, and will remain as discrete flux tubes in the corona until it collides and r
We consider a recently proposed scenario for the generation of primordial cosmological perturbations, the so called Cosmological Slingshot scenario. We firstly obtain a general expression for the Slingshot primordial power spectrum which extends prev