Daniel and Kelly’s Extraordinary Universe - What's the heaviest stable element?

Episode Date: April 1, 2021

Daniel and Jorge take a trip to the theoretical Island of Stability and talk about super heavy elements Learn more about your ad-choices at https://www.iheartpodcastnetwork.comSee omnystudio.com/list...ener for privacy information.

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Starting point is 00:01:24 sports production in partnership with deep blue sports and entertainment on the IHeart radio app, Apple Podcasts, or wherever you get your podcasts. Brought to you by Novartis, founding partner of IHeart Women's Sports Network. Hey, Jorge, what image do you have in your mind when you think about an atom? I guess I probably think of, you know, that image of the little balls going around in Hulu, orbits around a little cluster of other little balls? It's amazing how compelling that picture is, even though it's totally
Starting point is 00:02:00 wrong. What? You mean the universe doesn't agree with me? It's not that cooperative. And that image is mostly about the electrons. What do you think about when you think about the nucleus of the atom? I guess I always just picture like little proton and
Starting point is 00:02:16 neutron little balls just clustered together kind of like you take a bunch of marbles and stick it together. Well, as you might have guessed, I'm going to tell you that's also wrong. on. I am Horham, a cartoonist and the creator of PhD comics. Hi, I'm Daniel. I'm a particle physicist, and I'm doing my best to make the universe cooperate.
Starting point is 00:02:48 It's generally uncooperative? It doesn't just tell you its secrets, you know, just lay out for you the facts about nature. It makes you go on a hunt. It makes you ask the hard questions. But doesn't that make the answers more worth it, you know, when you have to fight for it? I don't know.
Starting point is 00:03:03 I'm the kind of person who reads the last page of a mystery novel first because I just want to know who did it. And then why do you read the rest of the book? I don't always. Well, there you go. Maybe the universe wants you to read all of it before you find out the answers. That's right.
Starting point is 00:03:19 The universe has an agent and wants me to read every single. single arc of the novel. Yeah, I mean, it spent 14 billion years making it. You're just going to jump to the end? Quite a build-up, quite a build-up. But welcome to our podcast, Daniel and Jorge Explain the Universe, a production of I-Hard Radio. Our podcast in which we try to skip you to the end and bring you the answers to the biggest questions about the nature of the universe, how things are built, what they're made out of, how they work on the tiniest little level, and how that comes together to make our incredible, inexplicable bonkers universe. That's right, because it is a pretty complicated and mysterious universe.
Starting point is 00:03:58 There's a lot of nuances and details and a lot of hidden things that we still haven't discovered. That's right. The things that we see around us in the universe are not like the fundamental elements of the universe. They are not the things that make up nature at its deepest level. We have to take them apart and understand what that's made out of and then what that's made up and then what that's made of and you can just keep going deeper and deeper. Yeah, it seems like as a human species, we've been sort of breaking matter down little by little over the centuries, right? I mean, before we thought that things were been out of like water, air,
Starting point is 00:04:31 earth, and then we found out about particles and then atoms and then subatomic particles and sub-atomic particles. It seems like we're breaking things down more and more. That's right. We are digging deeper into the nature of reality and that's fascinating because we wanted to know like what is the universe at the most basic level, if there is even a basic level. But there's also another direction that's really interesting for thinking about this problem,
Starting point is 00:04:55 which is going the other way. Starting from the smallest bits, what can you make? Like, if the universe is made out of Legos, what kind of stuff can you build? Yeah, because it's pretty mind-blowing, I guess, when you realize that all of the crazy variety of things
Starting point is 00:05:12 that is around is, it's all made out of the same little tiny bits, right? porks and electrons, you know, like air and dirt and, you know, metals, they're all made out of the same things. They just sort of behave totally different depending on how many and how they're arranged, these little tiny bits. That's right. It's really just the arrangement. In fact, the number is about the same. You have about one proton to one electron to one neutron in everything, even if it's lava or hamsters or ice cream. So there's something really deep and fascinating about the arrangements of particles.
Starting point is 00:05:48 How you put them together determines what they are. And as you're saying, not just by a little bit. Like, it determines whether it's metallic or whether it's insulating or whether it's shiny or whether it's dull or whether it melts at room temperature or not. All these properties determine just by how those bits are put together. Yeah, whether it's tasty or whether it will kill you or whether it'll be tasty and kill you at the same time. That's a different element there. You don't think it's possible for something to be tasty and not kill you. you? I think it's totally possible, but it hasn't quite taken off. But yeah, the difference
Starting point is 00:06:20 is very small, right? I mean, like if you have 12 protons and electrons, then it behaves like one thing. But if you have 16 of them, it behaves like something totally different. Yeah, it's totally different. And for a long time, we thought those differences were fundamental, that they were elemental, you know, that carbon really was something totally different from neon. But now that we know that you can take them apart and that they're made out of the same bits, we wonder things like, what else can you make out of these little bits? What else can our little universe Lego kit put together? Yeah, like if you keep adding more and more of them, what happens?
Starting point is 00:06:52 Or if you arrange them in a different way, do you get a totally different element with maybe magical and interesting new properties? Yeah, it's like you could create something totally new, something that has never existed in the universe before, or at least something that no human has ever experienced. Imagine creating a new substance with a completely different set of properties when it comes to like how it reflects light. Is it transparent? Is it pink?
Starting point is 00:07:16 Is it kind of translucent? Does it glow? Maybe it blinks. Who knows? But the universe is the limit. Yeah. And as you add more and more of these little bits, the elements get heavier and heavier and heavier.
Starting point is 00:07:26 They get literally like heavier and more massive and sometimes more unstable. Yeah. So we have the periodic table, the elements that records the ones we found and the few that we've built. But a question that's existed since we've had that table is, how far does that table go? Yeah. Is it like a super long table like they have in those big houses or is it like a small kitchen table?
Starting point is 00:07:47 We don't know, right? It's a mystery of the universe. How many leaps can we add? Can we invite as many people as we want over for dinner? Do you need a kitty table? They need to eat outside and who has that many chairs anyways? Maybe the universe should just have a picnic. Or, you know, have a Zoom dinner or something as is popular these days.
Starting point is 00:08:07 But anyway, that begs the question that we're going to tackle here today. So today on the program, we'll be asking. the question. What is the heaviest possible element? Meaning what's the most massive element you can make out of these little bits? Yeah, because not every combination sticks together. Sometimes you have a serving of neutrons and a serving of protons and a serving electrons and you try to stick them together and they just blow apart.
Starting point is 00:08:34 They're not stable. But some configurations do hang out and they can last for days or years or billions of years. And so it's curious, like, why can some of these things hang out together? What makes them stable? How big an element can you make and have it hang out and have it be stable? Have it like really be a thing you can play with. Right. They're sort of fickle things, protons and neutrons.
Starting point is 00:08:57 That's kind of what it's about, right? The elements and the periodic table of the elements kind of depend on the protons and the neutrons, right? I mean, the electrons are sort of fluid and they don't matter as much, but it's all about the protons and the neutrons. It's all about the protons and the neutrons because they feel. be able to strong force, they have strong feelings about what hangs out and what breaks down. Is that why it was called the strong force? Because it's so dramatic. The universe's agent suggested that name. But you're right, it's the number of protons that tells you sort of what element it is. Like, are you carbon or are you neon is determined by the number of protons in the
Starting point is 00:09:35 nucleus. And then you can have various isotopes because you can add neutrons or remove neutrons as you like without changing the identity of the element. And then the electrons typically follow the number of protons. So, yeah, you're right. The number of protons and the number of neutrons tell you what it is and how heavy it is. And that determines whether or not it hangs out or breaks apart. Right. And, you know, if you look at a periodic table, it seems pretty filled out down there at the bottom.
Starting point is 00:10:00 Like, as you go lower in the periodic table, that's where you have the heavier and heavier elements. And it seems pretty complete. Like you can add one more proton. a neutron and you get another element and you get another one and you get an you know there aren't any big gaps there so far. Yeah, that's sort of amazing, you know, that there's a place for every element
Starting point is 00:10:19 and an element for every place. And that was a big clue in the beginning. People started measuring the atomic numbers of these elements and putting them together in the table and realizing, oh, there are gaps. Is there something there? And then they went and they specifically tried to make those things and figured out,
Starting point is 00:10:36 oh yeah, there is something at Element 43. technetium, it turns out it can be made. And so organizing them in this way shows us where to look for new elements, where to aim for in constructing new kinds of stuff. Right. And it also has to do with this new concept that we're also talking about here today, which is called the Island of Stability. Now, Daniel, that sounds like a, I don't know, like a new age spa, maybe in an island, tropical island somewhere where you go and stabilize your karma. or something. But it's actually a pretty
Starting point is 00:11:10 heavy physics topic. It is a heavy physics topic. It has all to do with this question of heavy elements and whether or not they can hang out for a long time. So I don't know how many people out there have heard of the island of stability,
Starting point is 00:11:22 but we were wondering how popular this term is out there in the general public. So as usual, Daniel went out there into the wild to the internet to ask random people, what is, or where is the island of stability?
Starting point is 00:11:35 So thank you in advance to everybody who participated and lent their voice to this question. If you'd like to volunteer, please don't be shy. Send us an email to Questions at Danielanhorpe.com. Here's what people had to say. Is it something like the Uncanny Valley? So maybe it's, if you look into particles a lot into the readouts
Starting point is 00:11:58 and there are little islands of data that are like stable points that are always there. so in a sea of static I have not heard of that before there are elements with high atomic number on the periodic table where the proton to neutron ratio makes them have long lifetime so they have a large half-life I think those are the atoms that are said
Starting point is 00:12:25 to form the island of stability maybe it has something to do with stable orbits within the solar system so it could be kind of where the gravity from the sun makes the stability of the Earth's orbit more stable. For Europe, it's quite easy. It's Switzerland, definitely. And as for the rest of the universe, it makes me think of a particular region, a small region that would be very peaceful, very quiet with no disorder in the middle of a huge chaos. It's something that I would ask my travel legend.
Starting point is 00:13:02 I want to go there, but I don't know where is it. Yes, it sounds like it could be something out in the universe where there's not much movement or spinning of anything, possibly the center of the universe, where nothing expands from, I don't know. It kind of sounds like an equilibrium of some sort, kind of on the razor's edge, very unlikely, finely tuned. Can't wait to find out. Is the island of stability in Washington, D.C.? has something to do with quantum fields and how they can be arranged in such a way that a stable particle is present as opposed to just the energy in the field. I'm guessing that it has to do with some sort of parameters about how the field is organized such that a particle, like an electron
Starting point is 00:13:56 or something can live. I seem to remember there was discussion about the Higgs boat, on and how it's at a higher energy because it kind of got stranded on an island, as it were. And if it ever got tipped off of that, a whole bunch of bad stuff could happen. All right. Not a lot of people know where it is or what it is. No, and nobody wants to sign up for your getaway weekend there, Jorge. Yeah, I know. What's not too like?
Starting point is 00:14:24 You go somewhere and you, you know, stabilize a little bit. You come back feeling centered. That's right. Yeah. you align your your chakras you know and a thousand dollars poorer yeah but a million dollars richer in your soul what a deal what a deal i like the person who equated it to the uncanny valley that's like a totally uh interesting connection there is it though i'm not sure exactly how that's connected we're going to have video games with heavy elements in them that don't look quite right
Starting point is 00:14:56 I think we're just thinking of like geological features. Maybe we should have like the canyon of complexity or the cliffs of insanity. There you go. All right. So let's jump into this topic and let's talk about how this island of stability is related to making the heaviest possible element in the universe, basically, right? I mean, because the periodic table kind of goes on and on. And at some point, I notice that it doesn't go on forever. Well, that's the question.
Starting point is 00:15:22 We don't know if it doesn't go on forever because there's nothing else to make. or we just haven't yet found those elements or been able to fabricate them in the laboratory. That's the question. Oh, that's the mystery. Can we just skip to the end of the book, Daniel here? I guess those of you listening could skip to the end of the podcast to find out. But then what's the journey, Daniel?
Starting point is 00:15:43 Yeah, exactly. Then you miss all these great jokes. All these heavy jokes. All right, so the periodic table can't keep going, possibly. And it's been changing a lot in the last few decades, right? Like we keep adding heavier and new elements. That's right. We keep fabricating heavier and heavier elements by combining smaller ones because the question
Starting point is 00:16:02 we have is how far up can we go? Is there a limit to how far you can go? And if you go far enough, do you get to some like new region where things are surprisingly stable? I guess that's two different questions. Like what can you put together theoretically, physically in terms of the physical loss of the universe? And there's also the question of how stable it is.
Starting point is 00:16:23 Like how long will it stay in that? configuration, right? That's right. And, you know, it sort of has to be at least a little bit stable for you to call it an element. If you take, for example, element 99 and element 20, you smush them together to make element 119. If it doesn't like settle into a state that you can really call element 19, at least for a few milliseconds before it explodes, can you really say you've done it, right? You haven't really mixed the ingredients to make your brownies if they sort of repel each other and never come together. That's another. That's another. element, right? Brownium? Brownium? It's the tastiest element. It's the reason brownies are so good.
Starting point is 00:17:01 It's quite heavy, too, depending on how much butter you put into it. But yeah, it's a question of stability. And is there sort of a threshold in physics? Like, it has to last for X number of milliseconds or microseconds before you can say, okay, that's an element. Yeah, that's a great question. When they do these experiments, they only detect these atoms if they see characteristic stuff that flies out of that atom. So it's not like there's a minimum amount of time. It has to exist in order for them to like declare it having been an element, but they need to see its products, the things that it can only make. And so for that to happen, there must be some sort of minimum amount of time for an element to sort of like relax and stabilize and come together from all of its
Starting point is 00:17:44 ingredients swooshing around. But that's going to be a very, very small time, much smaller than anything we can measure. All right. Well, let's break it down, Daniel. I guess the first topic we can talk about here is this question of stability. Like, what makes an atom stable and not stable? Yeah, it's fascinating. Like, why can't you just put any number of protons and neutrons together
Starting point is 00:18:05 and get an atom and call it a day? Why do some of them break apart and some of them last forever? It's really a fascinating question and it turns out, like usual, it's complicated. You know, you might turn it around and instead of asking like, why are some of these things
Starting point is 00:18:21 unstable? You might ask, like, why is any nucleus stable because the nucleus has in it what protons and neutrons and protons are positively charged so they repel each other and the neutrons are just neutral so you might ask like well why doesn't the nucleus break apart every single time i have a strong hunch about this it's related to the strong force it's related to the strong force exactly we know that protons and neutrons are just little bags of corks that are held together by gluons and so they are tied together by the strong force and we like to think of them as not having an overall strong force charge being sort of neutral with respect to the strong force because the corks inside them add up all the colors
Starting point is 00:19:03 inside balance and you get something which ostensibly is neutral from the point of view of the strong force and that's mostly true but the mostly is doing a lot of work there if you get really close to a proton you could be like closer to one of the corks than the other ones and so the corks don't exactly balance themselves out so when the protons are neutral, get really near each other, then like the corks inside them can start talking to each other. So this little residual extra bit of the strong force is actually the thing that holds the nucleus together. That's enough to overcome the repulsion from the protons. Interesting. I guess it's kind of like if you have a positive charge and a negative charge
Starting point is 00:19:42 and you stick them together, they're not going to really attract or repel anything around them because together they're neutral, right, to everyone around them. But if you get really, really close to them, you might be, you know, closer to the plus or to the minus, in which case you would feel an attraction or repulsion. Yeah, precisely. So you had two of those things that had a plus and a minus inside of them and you brought them close
Starting point is 00:20:04 together and inverted the orientation so that the plus of one was close to the minus of the other, then they would feel an overall attraction. And so that's a great example for how you can put something together, which has an overall neutral charge and still have it attract itself. And that's the thing that holds
Starting point is 00:20:20 these nuclei together. That's the reason that they don't bust apart. That's why helium and calcium and all the things that make up your dinner tonight hang together. It's the strong force. Right. And so that's what's happening with the quarks inside of the protons and neutrons. Like the quarks sort of attract and repel each other,
Starting point is 00:20:36 but once you get three of them that are stable, they're sort of neutral together. Yeah, exactly. And then you mix these things together and they can hang out. But because it's the strong force, it's complicated. Like the strong force is just a mess. When we try to do calculations with the strong force, it's a disaster. because the strong force is so powerful
Starting point is 00:20:53 that it's very sensitive to small changes of distance. So we need massive supercomputers to figure out what's stable and how these things work and the masses of particles. It's really kind of a nightmare to do any calculations with. It's a heavy endeavor. But we've noticed a few things. We don't really understand how to predict these things,
Starting point is 00:21:13 but we've noticed some patterns. We've noticed sort of like what is stable and what is not. If you just sort of count the number of protons and neutrons, that are in the nuclei of stable atoms, you notice some really interesting patterns. Yeah, you get sort of like a magic sequence of numbers, right? They feel almost sort of like supernatural. Yeah, exactly.
Starting point is 00:21:33 All right, well, let's get into this magic sequence of numbers, and let's talk about how to make a really stable, heavy atom. But first, let's take a quick break. December 29th, 1975, LaGuardia, airport. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal.
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Starting point is 00:24:44 All right, we're talking about the heaviest possible element you can make in the universe. how many protons and neutrons can you stick together and still be stable? And we're talking about the stability of these things. And it has to do with some sort of magic number, right, Daniel? Yeah, it turns out that certain numbers of protons and neutrons are more stable than other configurations. And it's really kind of analogous to the way we think about electrons filling up their orbitals. You know the picture you were describing earlier of a nucleus with electrons around it. And we know that like you can have two electrons in the lowest.
Starting point is 00:25:19 orbital and then a certain number in the next and a certain number in the next and they sort of fill up these shells and as they fill them up they get more interactive or less interactive et cetera turns out that the protons and the neutrons inside the nucleus also have these kind of shells and you can get like two neutrons at the inner shell and then six in the next shell and 12 in the next shell and eight in the shell after that so we've noticed these trends that if you have just the right number of neutrons to, like, fill up a shell, then the atom becomes much more stable. Oh, interesting.
Starting point is 00:25:52 You mean, the nucleus of an atom has layers, like an onion or the sun? It's really kind of hard to visualize. It's not like there are physical shells. These are sort of energy levels. These are, like, how many neutrons you have filling up energy levels. The best way to visualize it is still like a ball of marbles, but they're all sort of like moving around and swishing, and different ones have different amounts of it. energy.
Starting point is 00:26:15 I see. Is it kind of like electron clouds? Like they're in different configurations in their quantum, you know, shape. Yeah, exactly. That's a good way to think about it. You know, like they're filling up these energy levels. And as you get to like a complete shell, then they sort of fit together very nicely in a way that supports each other. And so if you have, for example, six neutrons in the third shell, then they fit together really
Starting point is 00:26:38 nicely. And the next shell needs 12 neutrons. The next one needs eight. And the next one needs 22. And these aren't numbers that we. we understand. It's not like we can sit down and figure out why you need 22 or why you need eight, but it's just sort of an observation we've made. As you put these things together, the nucleus becomes more stable if you have these magic numbers of neutrons and protons.
Starting point is 00:26:59 Interesting. So you see this pattern in the periodic table, like, you know, the first two heavy elements were stable, then the next most stable is the eighth one, and then the most stable is the 20th one and things like that. Yeah, it's a little bit more complicated because you count the neutrons and the protons separately. Like if the protons have their magic number, then it's stable. If the neutrons have their magic number, it can be stable. And then you could have doubly magic elements, things where both the neutrons and the protons have their magic number, and those are the most stable.
Starting point is 00:27:29 But as these things sort of fit together, you can get different amounts of stability per atom. Oh, interesting. You have two variables here that you need to match to get the most stable element. Yeah, exactly. And it's all sort of related to the quantum nature of these. particles, you know what I mean? Because they're a wave and they have to fit within a certain energy level or space, they sort of click in certain integers. Yeah, these guys are all trapped inside this potential well of the nucleus, this strong force which wants to hold them together.
Starting point is 00:27:57 And it's mostly successful for a stable atom, you know, but some atoms are more stable than others. What happens when an atom is breaking apart? You're right, it's a quantum effect. It's like you have a particle stuck in a potential well, but that potential well doesn't have infinite sides. And so occasionally it can slip out. So the way that a nucleus breaks apart, the way that it decays is that it quantum tunnels from one state where it's trapped inside this well, outside of it, into a state where you have two separate pieces. And so to do that, you have to quantum tunnel. And the likelihood of that happening depends sort of like on the height of the potential barrier and also its width. I see. All right. So it's sort of quantized by these
Starting point is 00:28:38 magic numbers. But I guess the question we're trying to answer today is, Is there a limit? Like you can have, you know, two is a stable number. Eight's a stable number 20, 2850, 82, 126, 184, potentially. How far can you go? How far can you keep, you know, putting these protons and neutrons together and still get, you know, the double magic stability numbers? Yeah, it's really interesting. The heaviest stable thing that we have ever found in the universe is lead.
Starting point is 00:29:04 Lead is totally stable and it's element number 82. And, you know, if you make lead, we think it'll just stick around forever. really yeah that's the heaviest stable thing there is it's like it hits the two magic numbers like the protons are super happy together and the neutrons are super happy together yeah exactly 82 is one of the magic numbers and that we think is what makes lead so stable now there is other stuff out there for example uranium right uranium is the heaviest element that we find in nature but of course we know that it's not stable it tends to decay down to lighter things so there are processes out there in the universe like the collisions of neutron stars that can make these heavy elements,
Starting point is 00:29:44 some of which are very long lived. You know, they live for thousands or millions or even billions of years, but lead is the heaviest stable thing that we've found. And so you can ask really fun questions like, is it possible that there are heavier elements up there much further down deeper into the periodic table where you combine these magic numbers to get like really big numbers that could like click together in a stable way?
Starting point is 00:30:07 Like a super duper heavy lead or something. Yeah, exactly, exactly, an element that makes lead feel lightweight. Yeah, and I guess is there anything, like after lead, what's the next, you know, heaviest, but also sort of stable element that we know about? You know, there's really nothing above lead that's very stable. You know, uranium is up there, plutonium is up there, but nothing up there really has much stability at all. But we can look at the trends and we can get a sense for like, as we go up as we crank up the number, 100, 105, 115, are things getting more or less? stable and that can help us sort of predict whether or not there's going to be stuff up there. I see.
Starting point is 00:30:45 But we can try to predict, right? We can put these magic numbers together and we can say, well, what if we could make this element like 126 that's called unbi hexium? This one would be doubly magic because that has a proton number 126, which is magic, and then 184 neutrons, which is also magic. So it would be this huge, massive nucleus, super duper heavy, element 126. But, you know, we haven't seen it yet or we haven't been able to make it yet. So we just don't know if it's stable or not.
Starting point is 00:31:16 It's a hypothetical element. Yes, exactly. Everything above 118 is hypothetical. 118 is the heaviest thing we've ever fabricated. Everything above that is just speculation. We don't know if it can exist and what it would be like. I see 82 is the heaviest we've seen in nature, like that naturally seems to occur. That's stable.
Starting point is 00:31:36 But you can imagine heavier elements. And you can give him names. Like, you're allowed to do that? You can name things that don't exist? Yeah, they've named a bunch of these elements that we haven't actually made yet. But I think those names are placeholders. And when somebody actually makes them, then they get sort of, then decide the name. I see.
Starting point is 00:31:52 Because up to 118, they have sort of more interesting names. And above that, they have these sort of placeholder names. I see. Can I stick my claim in a number? Like, you know, is 573 taken? Can I call that chamium? Do it, man. Chamium, exactly.
Starting point is 00:32:07 There you go. Camium 573. Are you stable? Are you feeling stable today, Jorge? Don't decay. I need my brownie first. All right, so we can imagine, and there might be these sort of super heavy lead elements that are doubly magic and super stable. But we don't know, right? Like, that's a big mystery.
Starting point is 00:32:26 We don't know. It's a big mystery. And we've been sort of bad historically at understanding where the periodic table might end. And this is because this is hard, right? the strong force in nuclear physics is tough stuff. But people have been making predictions for a long time and getting it wrong. You know, for example, when we discovered plutonium, which is just element 94, people thought about naming it ultimium because they thought maybe it was the last element anybody would ever make. And now, you know, we're more than 10 elements beyond it. I see.
Starting point is 00:32:55 I guess maybe a question here is, what's the limitation, you know, both in nature and for us as humans? It seems like nature doesn't like making things heavier than lead or uranium or plutonium. Is that because that's just, you know, it takes too much energy to make heavier things? It takes energy, but you also have to have the ingredients, right? To make a really heavy element, you have to have the ingredients, which will also be pretty heavy. And, you know, these heavy elements are rare. As you get further up in the periodic table, you need things like neutron star collisions to even fabricate enough platinum or uranium or plutonium. And so to make something which is like twice as heavy as plutonium,
Starting point is 00:33:35 you need some situation where you're like smashing plutonium against plutonium to make, you know, I don't know what it's called double plutonium. Duplotium. Exactly. So these things just get rarer and rarer. And so you just don't have them being made at all. But one question is whether these things actually already exist out there in the universe. Like it's possible that Unbihexium exists and it's somewhere out there buried deep in the
Starting point is 00:34:02 Earth or in the center of a neutron star. Right? Because when these heavy neutron stars crash, I mean, can anything happen? Like, could it just become one giant element with a million protons in it? That's an awesome question. And it sort of breaks apart with this whole concept of what an element is because we talk about this thing and it's not fundamental, right? It's a special circumstance. It's something that appears in a special configuration under certain pressures and
Starting point is 00:34:29 temperatures. And if you push stuff together into a neutron star, I don't think you can really call that an element because I think those neutrons are in some crazy special state where they're really crammed together. And we also don't know how to calculate the details of how that works. There's a whole other field of study, what's going on inside neutron stars. But we talked about this once like what's inside a black hole. We called it black holium because it's some weird state of matter where these things are squished together. So the boundaries between the neutrons and protons are probably breaking down. Right. Interesting.
Starting point is 00:35:02 And what about for us as humans? Like, what's the limiting factor? Why can we just keep smashing these heavier and heavier elements together to make super heavy elements? Well, that's what we're doing. And there's an exciting program at Berkeley and then a lab in Russia that's doing exactly that. And that's how we've made element up to 118 is that we found lighter elements and we've smashed them together to try to make heavy elements. But it's not easy, right? It's not easy for a couple of reasons.
Starting point is 00:35:27 One is that you just don't have that much of the ingredients. For example, you want to make 117, then you've got to smash berkeleyum, which is 97, into calcium, which is 20. And there's not that much berkeleym around. Like, it took them two years of dedicated running just to make 12 milligrams of berkeleym, which is like the minimum you need to make this target to shoot calcium at. So it's just not easy to get the ingredients. If we had an unlimited source of all the elements we knew, we could smash them together to make heavier stuff. But it's not easy that you can't just like order these ingredients on Amazon.
Starting point is 00:36:05 Which is probably going to have its own element soon, Amazonium for sure. They're all just going to be Bezosium. Bezosium 1. Bezosium 2. He owns everything anyway. No, he retired then. He's just the puppet master behind the scenes now. So I guess maybe my question is, why can I just take, you know, like two plutonium atoms and smash those together?
Starting point is 00:36:24 You know, then you get 94 plus 94, then you get, you know, 188. Yeah, so the second reason is hard is that if you smash them together, you just get a bunch of little bits. You've got to do this thing which is sort of gentle. You've got to push them together hard enough for them to merge, but not so hard that you destroy the outcome, right? You shoot two plutonium nuclei together at the speeds we have the large Hedron Collider. You're just going to get a huge explosion. In fact, we do that at the large Hedron Collider. We collide usually protons and protons, but sometimes we collide gold.
Starting point is 00:36:54 old nuclei, sometimes lead nuclei, but you don't get a stable atom, what you get is too destroyed heavy nuclei. Oh, I see. I guess if you take like one thing built out of Legos and you smash it against something else built out of Lego, you don't just get one bigger thing made out of Legos. You just get a big mess on your floor probably. Yeah, but you know, if you take one brownie and you smash against another brownie, you kind of do just get a double-sized brownie. So maybe brownie physics is the way to go. Yeah, you're in the wrong, you're in the laboratory instead of the kitchen, Daniel. That's your problem. Yeah, so you've got to bring these things together so they form this stable state,
Starting point is 00:37:29 but not with so much energy that they destroyed. So this process is actually called, confusingly, cold fusion. Nothing to do with the other notorious cold fusion research that was done in the 90s that tried to produce energy from hydrogen fusion. This is a totally separate process that's trying to merge nuclei of heavy atoms, sort of kiss them together so they turn into this heavier thing. It's quite delicate. it. It's like a reboot or a rebrand. It's a totally separate line of research that actually predates the crazy cold fusion. This is like actual cold fusion.
Starting point is 00:38:04 And, you know, it makes sense. It's fusion because they're merging together heavy nuclei to make something new. And it's cold because they try not to do it too hard. All right. Well, I guess that covers why it's hard to make these super heavy elements. And we sort of talked a little bit about what makes these heavier elements possible and stable. but we still haven't talked about why we can't make these super heavy elements or whether or not they're theoretically or practically possible.
Starting point is 00:38:32 And it all seems to have to do with this concept of the island of stability. So let's get into what this island is and whether or not it makes for a pleasant vacation. But first, let's take another quick break. The holiday rush, parents hauling luggage, kids gripping their new Christmas toys. Then, at 6.33 p.m., everything changed. There's been a bombing at the TWA terminal. Apparently the explosion actually impelled metal, glass. The injured were being loaded into ambulances, just a chaotic, chaotic scene.
Starting point is 00:39:21 In its wake, a new kind of enemy emerged, and it was here to stay. Terrorism. Law and Order Criminal Justice System is back. In Season 2, we're turning our focus to a threat that hides in plain sight. That's harder to predict and even harder to stop. Listen to the new season of Law and Order Criminal Justice System on the IHeart Radio app, Apple Podcasts, or wherever you get your podcasts. I'm Dr. Scott Barry Kaufman, host of the psychology podcast.
Starting point is 00:39:58 Here's a clip from an upcoming conversation about exploring human potential. I was going to schools to try to teach kids these skills, and I get eye rolling from teachers or I get students who would be like, it's easier to punch someone in the face. When you think about emotion regulation, like, you're not going to choose an adaptive strategy, which is more effortful to use unless you think there's a good outcome as a result. of it if it's going to be beneficial to you because it's easy to say like like go you go blank yourself right it's easy it's easy to just drink the extra beer it's easy to ignore to suppress seeing a colleague who's bothering you and just like walk the other way avoidance is easier ignoring is easier
Starting point is 00:40:36 denial is easier drinking is easier yelling screaming is easy complex problem solving meditating you know takes effort listen to the psychology podcast on the iHeart radio app apple or wherever you get your podcasts. Have you ever wished for a change but weren't sure how to make it? Maybe you felt stuck in a job, a place, or even a relationship. I'm Emily Tish Sussman, and on she pivots, I dive into the inspiring pivots of women who have taken big leaps in their lives and careers. I'm Gretchen Whitmer, Jody Sweetie.
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Starting point is 00:41:48 All right, Dinah, let's talk about the IHartRadi. island of stability. Now, this has to do with, I'm guessing, some sort of like special configuration that the protons and neutrons have to be in before they can make these magic numbers happen. Yeah, we look at the pattern of the number of neutrons and the number of protons that are in various atoms. And you can ask the question, like, what happens if I put 17 neutrons and nine protons together or 144 neutrons and 92 protons? What do you get? And most of them, you get something unstable, which just breaks apart almost instantly. But there's this diagonal line where the protons are increasing, the neutrons are increasing,
Starting point is 00:42:26 and you get a bunch of stable atoms. And those are the elements that we know, right? But it sort of runs out at a certain point. There's like a heaviest element and above that thing start to get really unstable like we were talking about. But nuclear theorists suggest or speculate that deep beyond that, like far past the elements that we know if you have the right number, of protons and neutrons, there might be an island out there where if you put them together, they can actually be stable. They could last for a very, very long time. Oh, I see. Like there's a,
Starting point is 00:42:56 maybe a whole range of special combinations of protons that is stable, but it's just not connected to sort of the range of stable configurations that we know about. Yeah, exactly. We have like a peninsula jutting out. You know, they have the peninsula of stability and then a gap. And, you know, there's no configuration where you could assemble those protons and neutrons. together to make something stable. But then if you keep going, you keep going, you find this island where certain number of protons and certain number of neutrons, really large, crazy numbers could maybe actually hang out together and be stable.
Starting point is 00:43:31 Because I guess in general, it seems like the number of protons and the number of neutrons needs to be similar, right? Like you can't have an element with one proton and 100 neutrons, just like you can't have an element with like 100 protons and one neutrons. It seems like nature likes for those two numbers to be. similar. Yeah, they do need to be similar, but they're not exactly equal, right? Like, for example, you tend to have more neutrons than protons. Like the line veers up off the diagonal. So, for example, if you have 82 protons in lead, then you have like 126 neutrons in lead. So we don't
Starting point is 00:44:07 quite understand it, but it tends to prefer having more neutrons than protons. Oh, I see. But you're right. It's about the same number. You can't go too far off the diagram. Right, right. And the two numbers a little bit different, again, because of these magic numbers. Like protons like to be happy in certain numbers and neutrons like to be happy in other numbers and so it's getting the right combination that gives you the stable
Starting point is 00:44:29 element. Yeah, exactly. And lead for example is one of these doubly magic ones. It has 82 protons, which is a magic number and 126 neutrons, which is a magic number. I see. And that works for us up to a certain point, but you're imagining that, or physicists
Starting point is 00:44:45 are imagining that maybe there's, you you know, a whole set of combinations way out there, like, you know, a thousand protons and 2,000 neutrons that may be also stable, just like let it. Yeah, exactly. Not quite as far as 2,000. Nobody's gone that far, but it might be true, right? It might be that these magic numbers just keep increasing. And then we have not just one island out there at like 126 protons, but another one at 184 protons,
Starting point is 00:45:12 another one even further beyond that. And so we find this island of stability, it might suggest. that you could just keep going on making like redonculously heavy elements. I see. Well, I guess the question, Daniel, is how do you know that they're the island and we're not the island? Like, what if we're the island and they're the continent?
Starting point is 00:45:30 That sounds great. I'm happy to be on an island. I love islands. Islands are wonderful. But these other islands, we think they would be disconnected. As the magic numbers increase, they get further and further apart. And so you can't get as far away from sort of this island of stability
Starting point is 00:45:44 without falling into the ocean of decay. I guess you would call it. All right. Well, all of this sounds a little bit theoretical. These magic numbers combinations might exist and it might give us stable atoms. So what have physicists been doing to sort of explore this or confirm or deny this? Well, one thing they've been doing is just trying to make these things. And so they're trying to push the technology, like create heavier and heavier elements
Starting point is 00:46:07 and see if there's this trend towards increasing stability. We don't have to actually get all the way onto the island to have an idea that it might be there. If as we make heavier and heavier elements, we see the stability go up and up and up, and that suggests that we're like on the right path. We're like coming up the shore towards the island of stability. I see. We're like testing the waters kind of. Yeah, exactly.
Starting point is 00:46:30 And so, for example, in the 90s, people were working on making this atom, gleruvium, which is number of 114, and they worked on it for a long time, and they saw one. Like, they made a single one of these atoms. What? They could tell. Like, hey, we made one atom of this? It's hard to do, right? So they were smashing plutonium onto calcium,
Starting point is 00:46:52 and they were looking for individual ones. They are sensitive to individual atoms, which is pretty cool. And they made this one. And it stuck around for like 30 seconds, which is crazy long for a heavy element, right? It's not as long as we think the island of stability is we think those elements might have lifetimes in thousands, millions, or billions of years,
Starting point is 00:47:12 but it's much longer than the lighter, elements just before it. So it's sort of like this trend we were looking for. I see. So they try to make this element and it lasted for 30 seconds once. Once. And then they were never able to make it again, right? People have been trying to make this again and again, but they just haven't been able to. And so we don't know if that was wrong or if they got lucky and it's just really, really hard. Sometimes these experiments can go for years without making one and then get like two atoms made in a single week. It's just sort of up to luck. Wow, that's crazy. What must it feel like to have made this?
Starting point is 00:47:47 It's like finding one unicorn and then it goes away. And then you're trying to tell everyone that unicorns exist. Exactly. If I made a unicorn in the Large Hadron Collider, I'd be pretty excited. But yeah, I'd hope it was reproducible. But if it only lasts for 30 seconds and then nobody else saw it, Daniel. Then I would doubt my sanity and I would book a trip to the island of stability to restore myself. There you go.
Starting point is 00:48:08 I guess you should have taken a selfie with it. Or it didn't happen. All right. Well, let's say we do start to make these super. duper heavy elements. I guess what would they be good for? Just making better paper weights? Well, they'd be fascinating sort of theoretically because they would tell us that we do understand something about how the nucleus comes together and they would help us predict like where the next islandist ability is. And it's always just sort of good to learn like at a basic level.
Starting point is 00:48:33 How does the universe fit together? How can you fit these things together and build something that hangs together? That's sort of from the abstract. I just want a no area. But there are also potential practical uses. Remember that a lot of our spacecraft that we send out there to explore the universe run on nuclear fuel. For example, the Mars rover that just landed or Voyager and Pioneer that are deep out into space, they have nuclear batteries on them. And super heavy elements, which are not completely stable but last for a long time, might be excellent sources of power for spacecraft. Oh, I see. Like you would make a super heavy element and then use the decay to like power your spaceship for a thousand years.
Starting point is 00:49:13 Exactly. You want your fuel to last the whole length of your trip. And so if you want to go really, really far, then you need fuel, which is not totally stable, but takes a long time to decay. And so if you want to fly for a million years, then you need to find something with a half-life of about a million years.
Starting point is 00:49:28 Oh, I see. Because even plutonium won't last you forever, right? It will eventually all decay. Exactly. And the heavier elements are also denser, right? So you can carry them around in sort of smaller spaces. And, you know, space is always a premium on these, spacecraft.
Starting point is 00:49:42 Interesting. And I guess it would also just teach us just about matter and what's possible and what corner of the universe do we exist in? Like, do we exist in the most common one or are we sort of a flute? Yeah. And there are crazy ideas for what these super heavy elements might look like. People have the idea that, for example, the nucleus of one of these super heavy elements, like 184 protons in it might not even be spherical.
Starting point is 00:50:07 You know, the way you think about like electrons having shells and some of those. things have like weird blobs and shapes to them, some people speculate that the nucleus of a super heavy element might be sort of like a figure eight or it might be sort of like a bubble, like be hollow and have like no neutrons and protons inside, but be sort of like an actual physical shell. Oh, interesting. But you would only see that if you drill down to the nucleus of this atom, right? Yeah, exactly.
Starting point is 00:50:32 You'd have to make a bunch of them and then somehow probe them by shooting particles at them. So you'd make your unicorn and then you'd kill your unicorn in doing experiments on it. what if the nucleus looks like a unicorn that's theoretically possible isn't it it's theoretically possible there must be some magic number for that it would make it very hard to shoot particles at it because it would be so cute people like oh let's not study this thing let's just let it go yeah it'd be a tragedy to see it decay and then there are also folks who are just looking for this stuff they think let's not build this let's see if it exists in nature as you were saying sometimes crazy stuff happens at the core of neutron stars how do we know that these crazy heavy
Starting point is 00:51:11 elements haven't already been made and just like lying in the ground waiting for us to find them. Interesting. So there's a pretty amazing possibilities out there. There are really crazy possibilities out there. And there's even a guy from Hebrew University who claimed in 2008 to have discovered some of these things. He didn't see them directly, but he saw a bunch of crystals with like weird radiation damage that he claimed could only have been made by the decay of a super duper heavy element. But then again, of course, other people looked for the same sort of patterns and didn't spot them. So it's not really reproduced. Interesting. I guess then the hunt goes on for the heaviest element possible in the universe,
Starting point is 00:51:47 both theoretically and experimentally. Yes, exactly. It's just another way we can continue to explore the nature of the universe that we find around us. We can put these building blocks together and try to create new stuff, become like masters of the universe and make new weird elements that we could then use and build stuff out of it and also just gain insight into how matter works. Cool. Well, I've always been curious about how heavy I can get, and I'll let you know how that goes. Just keep shooting brownies at yourself, and eventually it'll happen. I'll just keep colliding brownies with my mouth.
Starting point is 00:52:22 It's an experiment. It's an experiment, I promise. It's for science. Yeah, that seems like a foregone conclusion about what's going to happen. Well, eventually you might just decay. Well, eventually we all decay, Daniel. The question is, how many brownies will you have eaten before? that happens to you. I think it's an ancient question in philosophy.
Starting point is 00:52:43 All right. Well, keep thinking about the universe and keep thinking about what kinds of matter could exist out there. There could be, who knows, magic number, figure eight elements out there that maybe look like unicorns. That's right.
Starting point is 00:52:56 And we will continue to explore the universe and try to understand this stuff, not just taking stuff apart and figuring out what it's made out at the smallest scale, but putting it back together and trying to make new crazy stuff for us to experience,
Starting point is 00:53:09 to fly us around the universe and to make delicious new kinds of desserts for Jorge. I would appreciate that. Thank you. In my island of stability. Who says particle physics has no applications? All right. Well, we hope you enjoyed that. Thanks for joining us. See you next time. visit the I Heart Radio app, Apple Podcasts, or wherever you listen to your favorite shows. and they're talking like we're talking. You know, you hear our story, how we grew up, how Barack grew up.
Starting point is 00:54:14 And you get a chance for people to unpack and get beyond race. All the Smoke featuring Michelle Obama. To hear this podcast and more, open your free iHeartRadio app. Search all the smoke and listen now. The U.S. Open is here. And on my podcast, Good Game with Sarah Spain. I'm breaking down the players, the predictions, the pressure. And, of course, the honey deuses, the signature cocktail of the U.S. Open.
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Starting point is 00:55:02 On a recent episode of Culture Raises Us podcast, I sat down with Warren Campbell, Grammy-winning producer, pastor, and music executive to talk about the beats, the business, and the legacy behind some of the biggest names in gospel, R&B, and hip-hop. Professionally, I started at Death World Records. From Mary Mary to Jennifer Hudson, we get into the soul of the music and the purpose that drives it. Listen to Culture raises us on the IHeart Radio app, Apple Podcasts, or wherever you get your podcast. This is an IHeart podcast.

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