质量的起源

P. Boyle, M. Buchoff, N. Christ, T. Izubuchi, C. Jung, T. Luu, R. Mawhinney, C. Schroeder, R. Soltz, P. Vranas, J. Wasem
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引用次数: 20

摘要

质量的起源是科学中最深奥的谜团之一。中子和质子构成了宇宙中几乎所有可见的质量,它们是在宇宙大爆炸后几微秒内通过剧烈的相变从原始等离子体中产生的。然而,宇宙中的大部分物质是看不见的。暗物质与我们的世界相互作用非常微弱,基本上无法探测到,它的存在是从它的星系尺度引力效应中确立的。在这里,我们描述了第一次真正的宇宙相变物理计算的结果,以及对复合暗物质的开创性第一原理研究,这些研究用以前最先进的方法和资源是不可能的。通过发明一种强大的新算法,“DSDR”,并在当代超级计算机上有效地实现它,我们实现了出色的强缩放,完美的弱缩放到LLNL BlueGene/Q 200万核,持续速度为7.2千万亿次,解决时间比以前的最先进技术加快200多倍。
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The origin of mass
The origin of mass is one of the deepest mysteries in science. Neutrons and protons, which account for almost all visible mass in the Universe, emerged from a primordial plasma through a cataclysmic phase transition microseconds after the Big Bang. However, most mass in the Universe is invisible. The existence of dark matter, which interacts with our world so weakly that it is essentially undetectable, has been established from its galactic-scale gravitational effects. Here we describe results from the first truly physical calculations of the cosmic phase transition and a groundbreaking first-principles investigation into composite dark matter, studies impossible with previous state-of-the-art methods and resources. By inventing a powerful new algorithm, “DSDR,” and implementing it effectively for contemporary supercomputers, we attain excellent strong scaling, perfect weak scaling to the LLNL BlueGene/Q two million cores, sustained speed of 7.2 petaflops, and time-to-solution speedup of more than 200 over the previous state-of-the-art.
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