Explosive fragmentation of additively manufactured stainless steel
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Item purpose: SnT virtual poster showing LYNM work Internal peer review status: This poster has been peer reviewed HQ review status: this poster has been approved by HQ
Physics-rich dataset of cylindrically symmetric shock-propagation simulations (CYL and PLI).
Several short-lived radionuclides (SLRs) are know to have existed in the early solar system (ESS). These species, which typically decay with half-lives of the order of a few million years, can be used to probe the timescales of events preceding the birth of the Sun. We investigate the ESS origin of 53 Mn, produced by core-collapse supernovae (CCSNe) and Type Ia supernovae (SNe Ia), and 60 Fe, produced exclusively by CCSNe. We model the evolution of the radioactive-to-stable abundance ratios of these SLRs with a Galactic chemical evolution (GCE) framework accounting for different SN yields, SN Ia delay times, and other Galactic features (K). A further set of models is calculated assuming that SNe Ia did not contribute any 53 Mn to the ESS. The predicted ratios are compared to meteoritic ratios to derive a distribution of solar isolation times that includes uncertainties due to stochastic chemical enrichment and measurements of the ESS values. The isolation times are then compared to those of 107 Pd and 182 Hf calculated in previous work. A self-consistent solution can be found within the current uncertainties, especially when using the GCE setups with K = 1.6 and 2.3, although the maximum likelihood for the 60 Fe distribution is typically ∼4–5 Myr shorter than for 53 Mn. The predicted 60 Fe/ 53 Mn ratio, instead, is completely inconsistent with the ESS value; this could be resolved using a larger fraction of faint CCSNe than usually considered in GCE models.
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General theory describing discontinuous processes and application to hydrodynamic inhomogeneities such as combustion waves, combustion zone motion
Experiment on the influence of ignition geometry on initial flame acceleration in spark-ignited stoichiometric hydrogen-oxygen mixtures at n.t.p.
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Grenade detonation acoustic wave propagation in upper atmosphere
Three postulates relating radio star galaxies, quasars and spontaneous creation of energy mass
Meteoritic simulator using shaped charge techniques
Stars with core greater than 30 solar masses become unstable due to electron-positron pair production at 1.5-2 billion K leading to supernova
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Safe/Armed Firing-Type Initiator /SAFTI/ combines the safety features of existing electromechanical safe-arm devices with the weight and size of a standard initiator and the functioning speed of a relay.
Damage potential of titanium alloy pressure spheres relative to spacecraft vibration testing
Thin walled metal cylinders residual deformation microstructures under internal impulsive loading