1 00:00:01,800 --> 00:00:04,320 Speaker 1: Welcome to brain Stuff, a production of I Heart Radio. 2 00:00:06,720 --> 00:00:09,600 Speaker 1: Hey brain Stuff, Lauren Vogel bomb here with another classic 3 00:00:09,640 --> 00:00:13,080 Speaker 1: episode from the vault. This one gets into the weird 4 00:00:13,160 --> 00:00:19,040 Speaker 1: astrophysics of the strongest known material in the universe, Nuclear pasta, 5 00:00:21,120 --> 00:00:24,760 Speaker 1: Hey brain Stuff, Laurin Vogel bomb here. Nuclear pasta might 6 00:00:24,840 --> 00:00:27,240 Speaker 1: sound like a fancy concoction cooked up by a chef 7 00:00:27,280 --> 00:00:31,200 Speaker 1: working in molecular astronomy, but it's actually light years away, 8 00:00:31,240 --> 00:00:34,440 Speaker 1: literally from the spaghetti you'd find in the kitchen. This 9 00:00:34,560 --> 00:00:37,320 Speaker 1: weird kind of noodle is needed below the crust of 10 00:00:37,400 --> 00:00:41,000 Speaker 1: neutron stars, and in a new study, a powerful computer 11 00:00:41,040 --> 00:00:44,080 Speaker 1: simulation has taken a stab at manipulating this stellar noodle 12 00:00:44,400 --> 00:00:47,720 Speaker 1: and found that it's the strongest material in the cosmos. 13 00:00:48,440 --> 00:00:51,920 Speaker 1: So how did this nuclear pasta become the super Macaroni 14 00:00:51,960 --> 00:00:55,840 Speaker 1: of the universe. Well, it's because it's created inside neutron stars, 15 00:00:56,040 --> 00:01:00,279 Speaker 1: which act like extreme pressure cookers. Neutron stars are these 16 00:01:00,280 --> 00:01:03,000 Speaker 1: stellar corpses of massive stars that have run out of 17 00:01:03,000 --> 00:01:07,200 Speaker 1: fuel and exploded as supernova. These tiny, fast spinning objects 18 00:01:07,240 --> 00:01:09,760 Speaker 1: are only a dozen or so miles wide and yet 19 00:01:09,800 --> 00:01:13,400 Speaker 1: pack in the entire mass of our Sun. They're so 20 00:01:13,480 --> 00:01:16,679 Speaker 1: dense that only a teaspoonful of neutron star matter weighs 21 00:01:16,680 --> 00:01:19,640 Speaker 1: as much as a mountain on Earth. Neutron stars are 22 00:01:19,680 --> 00:01:23,600 Speaker 1: therefore not composed of normal matter, but rather what astrophysicists 23 00:01:23,640 --> 00:01:26,920 Speaker 1: call degenerate matter. It's not an insult, it's just the 24 00:01:27,040 --> 00:01:30,720 Speaker 1: term for extremely compact neutrons that are crushed together under 25 00:01:30,760 --> 00:01:35,679 Speaker 1: incredibly powerful gravitational forces. A neutron star is extreme gravity 26 00:01:35,720 --> 00:01:38,399 Speaker 1: makes its outer layers freeze solid as a crust with 27 00:01:38,440 --> 00:01:42,840 Speaker 1: a liquid core below. Underneath the crust, powerful forces royal 28 00:01:42,920 --> 00:01:46,199 Speaker 1: between the neutrons and protons inside the neutron stars matter, 29 00:01:46,560 --> 00:01:49,640 Speaker 1: causing the material to take on some surprising shapes like 30 00:01:49,800 --> 00:01:54,200 Speaker 1: long cylinders and flat planes. Astrophysicists refer to these shapes 31 00:01:54,240 --> 00:01:58,640 Speaker 1: as things like lasagna, spaghetti, and nioki, and collectively as 32 00:01:58,720 --> 00:02:02,200 Speaker 1: nuclear pasta. As astrophysicists get to make their own fun. 33 00:02:02,960 --> 00:02:06,360 Speaker 1: Understanding how this nuclear pasta works is a key concern. 34 00:02:07,200 --> 00:02:11,399 Speaker 1: Researcher Matthew Kaplan, a postdoctoral research fellow at McGill University, 35 00:02:11,520 --> 00:02:14,400 Speaker 1: set in a statement, the strength of the neutron star crust, 36 00:02:14,560 --> 00:02:17,120 Speaker 1: especially the bottom of the crust, is relevant to a 37 00:02:17,240 --> 00:02:21,440 Speaker 1: large number of astrophysics problems, but isn't well understood their 38 00:02:21,480 --> 00:02:24,160 Speaker 1: outer layers, the part we actually observe, so we need 39 00:02:24,200 --> 00:02:27,959 Speaker 1: to understand that in order to interpret astronomical observations of 40 00:02:28,040 --> 00:02:31,760 Speaker 1: these stars. To get a better understanding of this noodlely 41 00:02:31,840 --> 00:02:34,960 Speaker 1: mess Kaplan and his team created the most complex computer 42 00:02:35,000 --> 00:02:38,560 Speaker 1: simulation ever carried out on neutron star crusts to understand 43 00:02:38,600 --> 00:02:41,880 Speaker 1: how they warp and break. It turns out that nuclear 44 00:02:41,880 --> 00:02:45,359 Speaker 1: pasta is way beyond Al Dente. It's the strongest known 45 00:02:45,400 --> 00:02:49,760 Speaker 1: material in the universe. This is especially important as physicists 46 00:02:49,760 --> 00:02:53,359 Speaker 1: can now measure gravitational waves, the ripples in space time 47 00:02:53,440 --> 00:02:57,000 Speaker 1: caused by massive cosmic objects like neutron stars and black 48 00:02:57,040 --> 00:03:01,040 Speaker 1: holes spinning, colliding, and merging. The st of neutron stars 49 00:03:01,120 --> 00:03:04,760 Speaker 1: is therefore very important for science to understand. In fact, 50 00:03:05,000 --> 00:03:08,320 Speaker 1: lone neutron stars may produce their own weak gravitational waves 51 00:03:08,360 --> 00:03:12,520 Speaker 1: by creating rigid mountains in their crests. As neutron stars spin, 52 00:03:12,800 --> 00:03:15,880 Speaker 1: these mountains would disturb space time like a propeller cutting 53 00:03:15,880 --> 00:03:19,160 Speaker 1: through a calm lake surface, generating a constant source of 54 00:03:19,160 --> 00:03:21,600 Speaker 1: gravitational waves that we may be able to detect in 55 00:03:21,639 --> 00:03:25,320 Speaker 1: the future. Kaplan said, a lot of interesting physics is 56 00:03:25,360 --> 00:03:28,639 Speaker 1: going on here under extreme conditions, and so understanding the 57 00:03:28,680 --> 00:03:31,080 Speaker 1: physical properties of a neutron star is a way for 58 00:03:31,120 --> 00:03:34,720 Speaker 1: scientists to test their theories and models. With this result, 59 00:03:34,920 --> 00:03:38,120 Speaker 1: many problems need to be revisited. How large a mountain 60 00:03:38,160 --> 00:03:40,120 Speaker 1: can you build on a neutron star before the crust 61 00:03:40,160 --> 00:03:42,880 Speaker 1: breaks and it collapses, What will it look like, and 62 00:03:43,040 --> 00:03:47,560 Speaker 1: most importantly, how can astronomers observe it? So the next 63 00:03:47,560 --> 00:03:49,920 Speaker 1: time you're boiling your penny, take a minute to ponder 64 00:03:49,960 --> 00:03:52,280 Speaker 1: the mountains of nuclear Pasta that could feed us a 65 00:03:52,280 --> 00:04:00,560 Speaker 1: lot about the nature of neutron stars. Today's episode is 66 00:04:00,600 --> 00:04:03,760 Speaker 1: based on the article nuclear Pasta is the super Macaroni 67 00:04:03,800 --> 00:04:06,000 Speaker 1: of the Universe on how stuff Works dot com, written 68 00:04:06,040 --> 00:04:09,040 Speaker 1: by Ian O'Neill. Brain Stuff is production of iHeart Radio 69 00:04:09,080 --> 00:04:11,000 Speaker 1: in partnership with how stuff Works dot Com, and it's 70 00:04:11,040 --> 00:04:14,320 Speaker 1: produced by Tyler Clang. Four more podcasts my Heart Radio, 71 00:04:14,520 --> 00:04:17,320 Speaker 1: visit the iHeart Radio app, Apple Podcasts, or wherever you 72 00:04:17,360 --> 00:04:18,640 Speaker 1: listen to your favorite shows.