WatchOS is up first, and Apple’s Kevin Lynch is first up on stage to talk about it.ģ:10AM: Lynch is talking about WatchOS 3, the latest update that brings along instant app launches by retaining the favourite ones in memory. I count five platforms, but I guess you can stack both iOS devices together. “Our north star has always been improving the world.” This is what Apple (and Cook) says the company’s rationale behind changing and updating its devices and communicating with devs and users alike.ģ:05AM: Apple is going to talk about four platforms today - the Macintosh, the iPhone, the iPad, and Apple Watch, and Apple TV. High five to whoever else in Australia is awake to watch #WWDC2016- Campbell Simpson June 13, 2016ģ:00AM: The livestream’s hold music fades down and… we’re off! Apple CEO Tim Cook takes the stage. If you haven’t hit the livestream up already, now is the time: The presentation will begin shortly, we’re told! I’m typing on a mechanical keyboard, too, so here’s hoping I don’t wake up the entire house. Warmth being brought to you live by a little Dyson AM09. See you all some time around 3AM! Scroll down from here to read this morning’s live blog in chronological order.Ģ:45AM: Morning guys and girls! Who’s awake? It sure is cold.Ģ:50AM: OK, so I’m actually at my PC now instead of posting from my phone in bed. By the way, my hat is a delicious croissant. If there’s not some kind of announcement of a widening of the program or new hardware, I’ll eat my hat. Siri could be opened up to developers, and we might see Siri make her debut on OSX too, to challenge Microsoft’s Cortana.Īpple has also been doing a little bit behind the scenes on HomeKit, too - its nascent smart home network, mostly tied around the Apple TV as the central smart home hub to control your smart locks and Philips’ new Hue 2.0 lighting. iOS 10, if it comes about, is rumoured to be a relatively small update - but that’s not necessarily a bad thing. IPhone is Apple’s poster child, and it’d be a weird WWDC without a major iOS version number change. The Apple TV’s tvOS, too, seems in line for some small amount of refreshing, although the 4th gen box already has all the streaming apps we need. The MacBook Air is well overdue for a refresh, too - did you know the 2016 model still uses the exact same LCD as the 2010 one?īeyond that kind of serious, developer-focused hardware, we might see more on the Apple Watch front - if not a brand new Apple Watch 2, then maybe at least some kind of serious overhaul or adjustment to WatchOS. The general consensus is that we’ll almost certainly get a new MacBook Pro - hopefully with some kind of innovative new technology on board, possibly a new Nvidia or AMD mobile GPU on those companies’ new, efficient process architectures. Here’s what our UK cousins think, too!Īpple Is Reportedly Building An Echo Rival And Opening Siri To Developers Here’s what our US cousins are expecting from this year’s WWDC announcements. (No luck, Chrome fans!) Apple’s HTTP Live Streaming protocol only works on these two browsers. G’night!īy the way: If you’re thinking of watching the WWDC keynote, you’ll either need some kind of Mac or iDevice with access to Safari, or a Windows 10 PC with Microsoft Edge. If you’re going to be sleeping and then waking up - like us, fingers crossed - then about now is the time you really should be going to bed. Now that you’re awake (and we’re still awake), come take a look.Ģ1:00, 13/6: Hello folks! You can check back in from 2:30AM AEST - that’s when we’ll be kicking off our coverage in this post. Do you really like shiny new Apple laptops? Are you a night owl? Does the Swift programming language get you all hot and bothered? Well, have we got the treat for you: Apple’s WWDC 2016 keynote ran today from 3AM to 5AM.
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It is stressed that in the case of two-electron processes the independent-electron model breaks down and the possible role of correlations between K-electrons is discussed. The CDW-EIS calculations along with the IEA model grossly underestimate the double ionization cross sections. The K-shell ionization cross sections are found to deviate strongly from the calculations based on the continuum distorted wave eikonal initial state (CDW-EIS) and ECPSSR models. The measured single K-K transfer cross sections are reproduced very well by the two-centre close-coupling calculations whereas the double K-K transfer data are underestimated by the theory based on the independent-electron approximation (IEA). The ratio of double to single K-K transfer cross sections is found to be quite large for this nearly symmetric collision system, whereas the ratio of double to single ionization cross sections is quite small. The enhancement in the fluorescence yields due to multiple vacancies was measured from the energy shifts and intensity ratios of the characteristic x-ray lines to derive K-shell vacancy production cross sections from x-ray production cross sections. The charge-state dependence of the normal and hypersatellite x-rays was used to derive the cross sections for the one- and two-electron processes, respectively. MC simulation was used by Lam and Singh13,14 for similar work, where the transitions between the confined states are treated according to quantum mechanics, as. Because the collapsing core is far from equilibrium, the effects of general relativity are small.We present a combined study of single and double K-K electron transfer cross sections along with the single and double K-shell ionization of Ar induced by Si projectiles in the energy range 0.9-4.0 MeV u-1. The mass of inner core is given, to about 20% by the formula of Goldreich and Weber. The entropy change during the infall is small: Vertical Bar. Greater lepton loss during collapse leads to larger pressure deficits, more rapid collapse, and smaller inner homologous cores. The effects of more » changes in the neutrino trapping density and of qualitative changes in the electron capture reactions on the evolution are explored. We treat neutrino transport by a leakage scheme. The electron capture rates on nuclei proceed rapidly for densities less than 10/sup 11/ g cm/sup -3/, but are suppressed at higher densities where the neutron number of the nucleus, N, exceeds 40 (Fuller, Fowler, and Newman). The models use the recent equation of state of Lamb, Lattimer, Pethick, and Ravenhall and general-relativistic hydrodynamics. In this paper we consider the infall epoch, between the onset of collapse and core bounce. We report on simulations of the collapse of the central iron core of 15 M/sub sun/ spherically symmetric star. For this reason, experimental and theoretical efforts should focus on this region of the nuclear chart. If more accurate estimates confirm this, results from this study indicate that significant changes to the core-collapse trajectory are expected. As measurements for medium-heavy (A>65) and neutron-rich nuclei are sparse, and because accurate theoretical models that account for nuclear structure considerations of individual nuclei are not readily available, rates for these nuclei may be overestimated. Additionally, the simulations are found to be more sensitive to a reduction in electron-capture rates than an enhancement, and specifically to the reduction in rates for neutron-rich nuclei near the N = 50 closed neutron shell. These ranges are five times as large as those seen from a separate progenitor study, where we evaluate the sensitivity of these parameters to 32 presupernova models. = luminosity during the deleptonization burst. Call Bobby for more details at (409) 739-4401. 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