Exploring this year’s best physics research in our Top 10 Breakthroughs of 2025
This episode of the Physics World Weekly podcast features a lively discussion about our Top 10 Breakthroughs of 2025, which include important research in quantum sensing, planetary science, medical physics, 2D materials and more. Physics World editors explain why we have made our selections and look at the broader implications of this impressive body of research.
The top 10 serves as the shortlist for the Physics World Breakthrough of the Year award, the winner of which will be announced on 18 December.
Links to all the nominees, more about their research and the selection criteria can be found here.
Physics World‘s coverage of the Breakthrough of the Year is supported by Reports on Progress in Physics, which offers unparalleled visibility for your ground-breaking research.
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1 00:00:08,720 --> 00:00:11,039 Hello. I'm Matin Durrani, and welcome to a 2 00:00:11,039 --> 00:00:13,359 very special edition of the Physics World weekly 3 00:00:13,359 --> 00:00:13,859 podcast, 4 00:00:14,414 --> 00:00:16,175 where we're going to be revealing the top 5 00:00:16,175 --> 00:00:18,914 10 breakthroughs in physics for 2025. 6 00:00:19,614 --> 00:00:21,375 Every year here at Physics World, we pick 7 00:00:21,375 --> 00:00:23,314 what we think have been the biggest breakthroughs 8 00:00:23,375 --> 00:00:25,454 over the last twelve months, and we've had 9 00:00:25,454 --> 00:00:27,774 chosen some amazing successes over the years that 10 00:00:27,774 --> 00:00:28,994 include the Higgs boson, 11 00:00:29,480 --> 00:00:31,960 gravitational waves, and the shadow around a black 12 00:00:31,960 --> 00:00:34,439 hole. With last year, the top prize going 13 00:00:34,439 --> 00:00:37,000 to work on quantum error correction at Google 14 00:00:37,000 --> 00:00:37,739 and elsewhere. 15 00:00:38,920 --> 00:00:41,559 So taking you through our choices for 2025, 16 00:00:41,559 --> 00:00:44,219 I'm joined by my colleagues Margaret Harris, 17 00:00:44,674 --> 00:00:47,814 Tammy Freeman, Michael Banks, and Hamish Johnson. 18 00:00:48,914 --> 00:00:51,395 The physics world breakthrough the year 2025 19 00:00:51,395 --> 00:00:54,054 is sponsored by Reports on Progress in Physics. 20 00:00:54,754 --> 00:00:57,795 Celebrating the most significant advances across the physical 21 00:00:57,795 --> 00:00:58,295 sciences, 22 00:00:58,899 --> 00:01:01,880 this award highlights discoveries that reshape our understanding 23 00:01:01,940 --> 00:01:04,359 of the universe and inspire future innovation. 24 00:01:05,380 --> 00:01:07,540 Reports on Progress in Physics is the leading 25 00:01:07,540 --> 00:01:08,680 journal for authoritative 26 00:01:08,980 --> 00:01:09,480 research, 27 00:01:09,939 --> 00:01:13,380 connecting researchers worldwide with cutting edge insights across 28 00:01:13,380 --> 00:01:14,520 every field of physics. 29 00:01:15,114 --> 00:01:17,134 From quantum technologies to astrophysics, 30 00:01:17,754 --> 00:01:20,015 it provides the depth and clarity that drive 31 00:01:20,075 --> 00:01:21,134 scientific progress. 32 00:01:21,914 --> 00:01:24,394 Search reports on progress in physics on your 33 00:01:24,394 --> 00:01:27,694 favorite browser to explore the ideas transforming science 34 00:01:27,834 --> 00:01:28,334 today. 35 00:01:29,489 --> 00:01:31,569 So let's get cracking on the top 10 36 00:01:31,569 --> 00:01:34,549 physics world breakthroughs in physics for 2025, 37 00:01:35,090 --> 00:01:37,329 which, just to remind you, we pick based 38 00:01:37,329 --> 00:01:38,229 on three 39 00:01:38,609 --> 00:01:41,489 criteria. So in addition to having been reported 40 00:01:41,489 --> 00:01:44,069 in physics world in 2025, 41 00:01:44,534 --> 00:01:47,974 our selections have to represent a significant advance 42 00:01:47,974 --> 00:01:49,594 in knowledge or understanding, 43 00:01:50,295 --> 00:01:53,594 be important for scientific progress and or development 44 00:01:53,655 --> 00:01:54,875 of real world applications, 45 00:01:55,814 --> 00:01:58,510 and be of general interest to Physics World 46 00:01:58,510 --> 00:01:59,010 readers. 47 00:02:00,989 --> 00:02:02,269 So we're gonna start with a bit of 48 00:02:02,269 --> 00:02:05,069 astronomy, with astronomers creating what they say is 49 00:02:05,069 --> 00:02:06,129 a weather map 50 00:02:06,430 --> 00:02:08,689 for a gas giant exoplanet. 51 00:02:09,405 --> 00:02:11,084 Now it's hard enough for trying to predict 52 00:02:11,084 --> 00:02:12,844 the weather here in on Earth, although I 53 00:02:12,844 --> 00:02:14,444 know it's been a pretty dry year in 54 00:02:14,444 --> 00:02:16,925 Bristol in the Southwest corner of England where 55 00:02:16,925 --> 00:02:19,004 we are. So this sounds pretty cool to 56 00:02:19,004 --> 00:02:21,805 me. Hamish, you're gonna explain this breakthrough for 57 00:02:21,805 --> 00:02:22,080 us. 58 00:02:22,639 --> 00:02:25,460 That's right, Matin. This this first, breakthrough is 59 00:02:25,520 --> 00:02:28,080 astronomy related breakthrough, and it has to do 60 00:02:28,080 --> 00:02:28,819 with exoplanets. 61 00:02:29,599 --> 00:02:32,560 Now it's only been thirty years since the 62 00:02:32,560 --> 00:02:33,540 first exoplanet, 63 00:02:34,574 --> 00:02:37,134 orbiting a star, that's a planet orbiting a 64 00:02:37,134 --> 00:02:39,634 star other than the sun, was discovered. 65 00:02:39,935 --> 00:02:43,794 And today, astronomers know of more than 6,000 66 00:02:44,254 --> 00:02:45,235 such objects. 67 00:02:46,270 --> 00:02:49,009 And this breakthrough, it's been made by Lisa 68 00:02:49,069 --> 00:02:49,569 Nortman 69 00:02:49,949 --> 00:02:50,689 at Germany's 70 00:02:50,990 --> 00:02:51,490 University 71 00:02:51,870 --> 00:02:52,610 of Gottingen 72 00:02:53,229 --> 00:02:54,050 and colleagues, 73 00:02:54,430 --> 00:02:55,889 and they've used the European 74 00:02:56,189 --> 00:02:57,250 Southern Observatory's 75 00:02:57,949 --> 00:02:59,169 Very Large Telescope 76 00:02:59,865 --> 00:03:02,125 to create what they're saying 77 00:03:02,425 --> 00:03:05,245 is the first weather map of an exoplanet. 78 00:03:06,025 --> 00:03:08,844 Now this exoplanet is a hot Jupiter. 79 00:03:09,305 --> 00:03:12,044 It's a gas giant called WASP 80 00:03:12,500 --> 00:03:14,199 one twenty seven b, 81 00:03:14,500 --> 00:03:17,319 and it orbits very near to its star. 82 00:03:17,379 --> 00:03:19,299 So this is not something that we have 83 00:03:19,299 --> 00:03:21,459 in a in in the solar system. It's 84 00:03:21,459 --> 00:03:22,680 a very sort of exotic 85 00:03:22,979 --> 00:03:25,914 thing as far as we we're concerned. And 86 00:03:25,914 --> 00:03:28,314 what Nortman and colleagues did is they studied 87 00:03:28,314 --> 00:03:29,534 the absorption 88 00:03:29,914 --> 00:03:33,275 spectrum of starlight that had passed through the 89 00:03:33,275 --> 00:03:33,775 exoplanet's 90 00:03:34,155 --> 00:03:34,655 atmosphere. 91 00:03:35,675 --> 00:03:36,175 And 92 00:03:36,555 --> 00:03:40,349 by, looking at the Doppler shift of this, 93 00:03:41,150 --> 00:03:42,210 transmission spectrum, 94 00:03:42,590 --> 00:03:45,810 they could deduce that the winds on WASP 95 00:03:45,950 --> 00:03:48,830 one twenty seven b can reach as as 96 00:03:48,830 --> 00:03:51,170 high as 33,000 97 00:03:51,629 --> 00:03:52,930 kilometers per hour, 98 00:03:53,375 --> 00:03:55,854 which is pretty fast. That's quick. It it 99 00:03:55,854 --> 00:03:58,334 it is. Yeah. Yeah. And and what's more, 100 00:03:58,334 --> 00:04:00,514 by looking at the, sort of, the distribution 101 00:04:01,375 --> 00:04:02,354 of of how, 102 00:04:03,055 --> 00:04:04,914 the light is Doppler shifted, 103 00:04:05,375 --> 00:04:08,400 they could create a rough weather map of 104 00:04:08,400 --> 00:04:11,120 the exoplanet. Now, it's important to say that 105 00:04:11,120 --> 00:04:13,840 they weren't actually able to look at different 106 00:04:13,840 --> 00:04:14,340 points 107 00:04:14,800 --> 00:04:15,620 on the exoplanet 108 00:04:15,920 --> 00:04:18,420 and say the weather is like this there. 109 00:04:18,560 --> 00:04:20,319 What they did is they they looked at 110 00:04:20,319 --> 00:04:21,139 this distribution 111 00:04:22,035 --> 00:04:24,455 and somehow used that information to 112 00:04:24,835 --> 00:04:26,835 infer what the weather was like from the 113 00:04:26,835 --> 00:04:28,935 pole down to the Equator 114 00:04:29,555 --> 00:04:32,295 and, back again to to the other pole. 115 00:04:33,074 --> 00:04:34,615 So they were able to conclude, 116 00:04:35,250 --> 00:04:37,009 along with looking at the winds, they were 117 00:04:37,009 --> 00:04:37,910 able to conclude 118 00:04:38,290 --> 00:04:41,029 that the exoplanet's poles are cooler 119 00:04:41,330 --> 00:04:43,270 than the rest of the exoplanet, 120 00:04:43,730 --> 00:04:44,230 where, 121 00:04:44,770 --> 00:04:46,069 temperatures can exceed, 122 00:04:46,529 --> 00:04:49,250 over a thousand degrees Celsius. So, again, a 123 00:04:49,250 --> 00:04:50,550 very strange place. 124 00:04:51,314 --> 00:04:53,975 Imagine Jupiter, but it's a thousand degrees Celsius, 125 00:04:54,675 --> 00:04:56,134 sort of a weird world. 126 00:04:56,435 --> 00:04:59,794 And they also, detected water vapor in the 127 00:04:59,794 --> 00:05:00,294 atmosphere, 128 00:05:00,675 --> 00:05:04,134 and that raises the possibility of very exotic 129 00:05:04,274 --> 00:05:06,449 forms of rain on the planet. 130 00:05:06,930 --> 00:05:07,910 So rain, 131 00:05:08,290 --> 00:05:09,110 other than 132 00:05:09,889 --> 00:05:11,830 how we know it, I suppose. 133 00:05:12,210 --> 00:05:14,050 And, you know, I think we picked this 134 00:05:14,050 --> 00:05:17,830 one. Really, there's lots of really fantastic exoplanet 135 00:05:18,050 --> 00:05:20,470 research out there, thousands that have been discovered. 136 00:05:21,404 --> 00:05:22,384 But this was 137 00:05:22,845 --> 00:05:24,064 a a a really interesting, 138 00:05:24,605 --> 00:05:26,685 example of how we can we can now 139 00:05:26,685 --> 00:05:27,904 actually see the atmosphere 140 00:05:28,444 --> 00:05:29,425 of these exoplanets 141 00:05:29,964 --> 00:05:32,384 using, you know, the very latest telescopes. 142 00:05:33,139 --> 00:05:35,699 So very hot, very windy, and exotic rain. 143 00:05:35,699 --> 00:05:37,540 I don't think I wanna live there. Thanks, 144 00:05:37,540 --> 00:05:40,819 Hamish. Now from exoplanets out in space down 145 00:05:40,819 --> 00:05:42,819 to our planet here on Earth, our next 146 00:05:42,819 --> 00:05:44,839 breakthrough through of the year is a fascinating 147 00:05:44,899 --> 00:05:45,399 study 148 00:05:45,834 --> 00:05:47,995 about using the phones we all carry around 149 00:05:47,995 --> 00:05:50,074 with us to create an early warning system 150 00:05:50,074 --> 00:05:50,894 for earthquakes 151 00:05:51,435 --> 00:05:53,834 or at least using Android phones. Michael, can 152 00:05:53,834 --> 00:05:55,995 you tell us about this breakthrough, which seems 153 00:05:55,995 --> 00:05:58,759 like a great example of citizen science? Yeah. 154 00:05:58,759 --> 00:06:00,759 So this is all about using mobile phones 155 00:06:00,759 --> 00:06:02,939 to detect earthquakes. So traditional 156 00:06:03,319 --> 00:06:06,680 earthquake early warning systems usually use networks of 157 00:06:06,680 --> 00:06:07,660 seismic sensors 158 00:06:08,040 --> 00:06:10,680 that rapidly detect earthquakes in areas close to 159 00:06:10,680 --> 00:06:11,339 the epicenter. 160 00:06:12,165 --> 00:06:15,464 They also issue warnings to, people also across 161 00:06:15,524 --> 00:06:16,665 the affected region. 162 00:06:17,125 --> 00:06:19,125 Yet the issue is that building such networks 163 00:06:19,125 --> 00:06:20,904 of bulky sensors, it's expensive, 164 00:06:21,444 --> 00:06:23,464 you know, and this means that many earthquake 165 00:06:23,524 --> 00:06:26,069 prone regions do not have them. So to 166 00:06:26,069 --> 00:06:28,470 get around this problem, researchers in The US 167 00:06:28,470 --> 00:06:31,670 utilized the accelerometer housed in millions of mobile 168 00:06:31,670 --> 00:06:32,730 phones worldwide 169 00:06:33,189 --> 00:06:36,629 to create an app based Android earthquake alert 170 00:06:36,629 --> 00:06:37,129 system. 171 00:06:37,875 --> 00:06:41,814 So testing the app between 2021 and 2024 172 00:06:42,355 --> 00:06:44,275 led to the detection of an average of 173 00:06:44,275 --> 00:06:45,235 312 174 00:06:45,235 --> 00:06:49,314 earthquakes a month with magnitudes ranging from 1.9 175 00:06:49,314 --> 00:06:51,415 to 7.8 on the Richter scale. 176 00:06:52,300 --> 00:06:53,819 But what is more, the app could also 177 00:06:53,819 --> 00:06:55,980 alert people in the area. So for earthquakes 178 00:06:55,980 --> 00:06:57,759 of magnitude 4.5 179 00:06:57,819 --> 00:06:58,560 or higher, 180 00:06:58,939 --> 00:07:01,660 the system sent so called take action alerts 181 00:07:01,660 --> 00:07:02,400 to users. 182 00:07:02,860 --> 00:07:05,354 It also delivered lesser be aware alerts to 183 00:07:05,354 --> 00:07:08,394 regions expected to experience a shaking intensity of 184 00:07:08,394 --> 00:07:09,294 three or four. 185 00:07:09,914 --> 00:07:11,514 So the team now aimed to build on 186 00:07:11,514 --> 00:07:14,574 this earthquake early warning system based on Android 187 00:07:14,714 --> 00:07:17,754 mobile phones by producing maps of ground shaking 188 00:07:17,754 --> 00:07:18,300 as well. 189 00:07:18,779 --> 00:07:21,019 And this could all help assist the emergency 190 00:07:21,019 --> 00:07:23,439 response services when an earthquake occurs. 191 00:07:24,139 --> 00:07:27,099 Thanks, Michael. So from communicating with mobiles to 192 00:07:27,099 --> 00:07:29,339 communicating via the cables that make up the 193 00:07:29,339 --> 00:07:29,839 Internet, 194 00:07:30,220 --> 00:07:33,039 which is the almost invisible technology that underpins 195 00:07:33,180 --> 00:07:35,605 modern life. Now it seems the researchers have 196 00:07:35,605 --> 00:07:38,024 developed a new kind of fiber that loses 197 00:07:38,324 --> 00:07:39,865 that lose less data 198 00:07:40,165 --> 00:07:42,404 as the signals get sent down them. Tammy, 199 00:07:42,404 --> 00:07:43,545 what's this one about? 200 00:07:44,245 --> 00:07:47,045 So optical fibers form the backbone of the 201 00:07:47,045 --> 00:07:49,944 Internet carrying light signals across the globe. 202 00:07:50,430 --> 00:07:52,830 But sunlight is always lost as it travels 203 00:07:52,830 --> 00:07:55,230 through the fiber, which means that these signals 204 00:07:55,230 --> 00:07:57,730 must be amplified every few dozen kilometers. 205 00:07:58,430 --> 00:08:01,230 Now amazingly, the performance of even the best 206 00:08:01,230 --> 00:08:04,430 fibers has remained largely unchanged for nearly four 207 00:08:04,430 --> 00:08:04,930 decades 208 00:08:05,475 --> 00:08:06,375 until now. 209 00:08:07,235 --> 00:08:09,254 Physicists at the University of Southampton 210 00:08:09,875 --> 00:08:12,194 have developed a new type of fiber that 211 00:08:12,194 --> 00:08:13,714 exhibits 35% 212 00:08:13,714 --> 00:08:14,535 less attenuation 213 00:08:15,154 --> 00:08:18,854 while transmitting signals faster than standard glass fibers, 214 00:08:19,490 --> 00:08:21,810 and they achieved this by replacing the glass 215 00:08:21,810 --> 00:08:24,389 core of a conventional fiber with air. 216 00:08:25,250 --> 00:08:27,329 To guide the light through this hollow core, 217 00:08:27,329 --> 00:08:29,029 it's surrounded by a microstructure 218 00:08:29,490 --> 00:08:33,110 of ultrathin glass membranes that reflect certain frequencies 219 00:08:33,514 --> 00:08:35,434 to trap the light and keep it moving 220 00:08:35,434 --> 00:08:36,414 through the fiber. 221 00:08:37,434 --> 00:08:39,914 So to test this design, the team, which 222 00:08:39,914 --> 00:08:43,294 also included researchers from Microsoft Azure Fiber, 223 00:08:43,754 --> 00:08:46,315 they measured the transmission through a full spool 224 00:08:46,315 --> 00:08:48,450 of fiber, then they cut it into shorter 225 00:08:48,450 --> 00:08:49,990 lengths and compared the results. 226 00:08:50,610 --> 00:08:52,850 And they found that their hollow fibers reduced 227 00:08:52,850 --> 00:08:53,509 the attenuation 228 00:08:53,970 --> 00:08:56,389 to just naught point naught nine one decibels 229 00:08:56,450 --> 00:08:59,649 per kilometer at fifteen fifty nanometers, which is 230 00:08:59,649 --> 00:09:01,190 a wavelength used for telecoms. 231 00:09:01,784 --> 00:09:04,184 And this means that long cables would need 232 00:09:04,184 --> 00:09:05,164 fewer amplifiers, 233 00:09:05,625 --> 00:09:07,644 lowering the costs and the energy use. 234 00:09:08,345 --> 00:09:11,065 The new hollow fiber also supports a higher 235 00:09:11,065 --> 00:09:11,565 bandwidth 236 00:09:11,944 --> 00:09:13,084 than a normal fiber, 237 00:09:13,464 --> 00:09:15,464 which means that a single strand can carry 238 00:09:15,464 --> 00:09:16,919 far more channels at once. 239 00:09:17,480 --> 00:09:19,559 And because the speed of light's faster in 240 00:09:19,559 --> 00:09:22,039 air than in glass, the data could travel 241 00:09:22,039 --> 00:09:24,600 the same distance up to 45% 242 00:09:24,600 --> 00:09:25,100 faster. 243 00:09:26,120 --> 00:09:28,919 Now Microsoft has begun testing the new fibers 244 00:09:28,919 --> 00:09:29,980 in real systems, 245 00:09:30,575 --> 00:09:33,294 installing segments in its network and sending live 246 00:09:33,294 --> 00:09:34,355 traffic through them. 247 00:09:34,815 --> 00:09:37,215 And these trials prove that the hollow core 248 00:09:37,215 --> 00:09:40,654 design works with existing telecoms equipment and opens 249 00:09:40,654 --> 00:09:42,654 the door to a gradual rollout of this 250 00:09:42,654 --> 00:09:43,715 new source of fiber. 251 00:09:44,639 --> 00:09:48,000 And as team leader Francesco Paletti suggests, one 252 00:09:48,000 --> 00:09:51,220 day, they could even replace existing undersea cables. 253 00:09:51,920 --> 00:09:53,759 So that's the first three of our physics 254 00:09:53,759 --> 00:09:56,080 world breakthroughs of the year for 2025 255 00:09:56,080 --> 00:09:56,414 done. 256 00:09:56,894 --> 00:09:59,054 Now next up is some cool condensed matter 257 00:09:59,054 --> 00:10:00,834 physics that's involved superfluidity 258 00:10:01,375 --> 00:10:04,355 spotted in molecular hydrogen for the first time. 259 00:10:04,654 --> 00:10:07,315 Now, Margaret, physicists are pretty familiar with superfluidity 260 00:10:07,695 --> 00:10:09,794 in helium three and helium four 261 00:10:10,259 --> 00:10:12,660 atoms, but now we're talking about molecules, aren't 262 00:10:12,660 --> 00:10:13,160 we? 263 00:10:13,540 --> 00:10:15,940 Yeah. We're talking about specifically about molecular hydrogen, 264 00:10:15,940 --> 00:10:17,779 which is the simplest and lightest of all 265 00:10:17,779 --> 00:10:19,779 molecules. You take one hydrogen atom, you take 266 00:10:19,779 --> 00:10:21,800 another hydrogen atom, you link them together. 267 00:10:22,375 --> 00:10:25,735 And theorists predicted that this molecular hydrogen would 268 00:10:25,735 --> 00:10:28,394 enter a superfluid state at a temperature between 269 00:10:28,535 --> 00:10:30,795 one to two Kelvin above absolute zero, 270 00:10:31,254 --> 00:10:32,394 which is pretty cold. 271 00:10:32,855 --> 00:10:34,535 But the real problem with that is that 272 00:10:34,535 --> 00:10:37,175 molecular hydrogen freezes at 13.8 273 00:10:37,175 --> 00:10:39,190 Kelvin, So, obviously, it's not going to be 274 00:10:39,190 --> 00:10:41,269 behaving like a superfluid if it's further than 275 00:10:41,269 --> 00:10:41,769 solid. 276 00:10:42,629 --> 00:10:45,210 So before they could verify this prediction, Takamasa 277 00:10:45,350 --> 00:10:47,670 Momosa and colleagues at the University of British 278 00:10:47,670 --> 00:10:48,809 Columbia in Canada, 279 00:10:49,269 --> 00:10:50,790 they first had to develop a way to 280 00:10:50,790 --> 00:10:52,455 keep the hydrogen in a liquid state. 281 00:10:53,014 --> 00:10:55,095 And they did that by confining clusters of 282 00:10:55,095 --> 00:10:59,115 hydrogen molecules inside nanodroplets of helium and supercooling 283 00:10:59,254 --> 00:11:01,835 them to below their freezing point, which, 284 00:11:02,215 --> 00:11:03,735 I mean, I've never done it, but I 285 00:11:03,735 --> 00:11:06,134 imagine that isn't exactly easy. Certainly, it sounds 286 00:11:06,134 --> 00:11:07,434 like an impressive feat. 287 00:11:07,940 --> 00:11:10,259 And then once they've done that, they faced 288 00:11:10,259 --> 00:11:12,179 a further barrier, which was figure out how 289 00:11:12,179 --> 00:11:14,579 to detect whether the hydrogen was superfluid or 290 00:11:14,579 --> 00:11:15,079 not. 291 00:11:15,459 --> 00:11:17,459 And to do that, they stuck a methane 292 00:11:17,459 --> 00:11:19,799 molecule in with the cluster of hydrogen molecules 293 00:11:20,179 --> 00:11:21,399 and watched it rotate. 294 00:11:21,914 --> 00:11:24,495 And when it started to rotate without friction, 295 00:11:24,955 --> 00:11:26,495 they knew they'd seen superfluidity. 296 00:11:27,434 --> 00:11:29,274 Apparently, it took them nearly twenty years to 297 00:11:29,274 --> 00:11:31,034 sort of develop this experiment at this point, 298 00:11:31,034 --> 00:11:33,195 so this breakthrough was a long time coming. 299 00:11:33,195 --> 00:11:35,195 And it's a testament to the dedication and 300 00:11:35,195 --> 00:11:36,794 ingenuity of the team that they were able 301 00:11:36,794 --> 00:11:38,129 to do it at all. This is a 302 00:11:38,129 --> 00:11:40,549 real physicist experiment on my view at least. 303 00:11:41,329 --> 00:11:43,329 They now plan to study larger clusters of 304 00:11:43,329 --> 00:11:45,409 hydrogen with the aim of exploring the boundary 305 00:11:45,409 --> 00:11:48,549 between classical and quantum behavior in this system. 306 00:11:48,929 --> 00:11:51,250 So, I mean, they've seen superfluidity with 10 307 00:11:51,250 --> 00:11:52,725 hydrogen molecules. Great. 308 00:11:53,284 --> 00:11:54,964 Can I see it with a 100? What 309 00:11:54,964 --> 00:11:57,365 about a thousand or a million? We don't 310 00:11:57,365 --> 00:11:59,204 know the answer, but it'll be really exciting 311 00:11:59,204 --> 00:12:01,444 to find out. Like you say, Margaret, definitely 312 00:12:01,444 --> 00:12:03,204 one for the fit the hardcore physicist, I 313 00:12:03,204 --> 00:12:05,764 think, especially something that's taken twenty years to 314 00:12:05,764 --> 00:12:06,424 get through. 315 00:12:07,049 --> 00:12:09,129 So amazing achievement, that one. And speaking of 316 00:12:09,129 --> 00:12:12,910 molecules, research have found some pretty interesting molecules 317 00:12:13,049 --> 00:12:15,690 on the asteroid Bennu, which has caught our 318 00:12:15,690 --> 00:12:17,549 eye, hasn't it, Margaret? What have they found? 319 00:12:18,009 --> 00:12:20,090 Well, Matin, it's almost a case of asking 320 00:12:20,090 --> 00:12:21,950 what haven't they found on Bennu. 321 00:12:22,295 --> 00:12:24,134 I mean, they might be looking for not 322 00:12:24,134 --> 00:12:26,535 finding Jimmy Hoffa or Bigfoot, but they found 323 00:12:26,535 --> 00:12:28,934 almost everything else. So back in February, we 324 00:12:28,934 --> 00:12:31,254 reported that two teams had found salt and 325 00:12:31,254 --> 00:12:33,815 certain amino acids in samples of the asteroid 326 00:12:33,815 --> 00:12:34,315 Bennu, 327 00:12:34,639 --> 00:12:37,919 which NASA's OSIRIS REx spacecraft visited back in 328 00:12:37,919 --> 00:12:38,659 2020. 329 00:12:39,279 --> 00:12:41,360 These samples got parachuted back to Earth in 330 00:12:41,360 --> 00:12:44,320 2023, and ever since then, various groups of 331 00:12:44,320 --> 00:12:46,799 scientists have been studying them, hoping to answer 332 00:12:46,799 --> 00:12:49,184 questions about what was around in the earliest 333 00:12:49,184 --> 00:12:51,745 solar system, chemically speaking, and how it led 334 00:12:51,745 --> 00:12:53,264 to the kinds of stuff we see around 335 00:12:53,264 --> 00:12:53,845 us today. 336 00:12:54,784 --> 00:12:57,424 Now finding salt and amino acids on an 337 00:12:57,424 --> 00:13:00,225 asteroid is interesting because they're both important for 338 00:13:00,225 --> 00:13:01,204 living organisms. 339 00:13:01,769 --> 00:13:04,089 Lots of animals, including us, need salt to 340 00:13:04,089 --> 00:13:04,589 survive, 341 00:13:04,970 --> 00:13:06,970 and amino acids are the building blocks of 342 00:13:06,970 --> 00:13:09,289 the DNA and RNA that provide the instructions 343 00:13:09,289 --> 00:13:10,269 for making life. 344 00:13:10,730 --> 00:13:13,449 So finding these fairly complex molecules on an 345 00:13:13,449 --> 00:13:15,149 asteroid is a pretty big deal. 346 00:13:16,105 --> 00:13:17,625 Then just a few days ago, we got 347 00:13:17,625 --> 00:13:20,504 some new results about Bennu's composition showing that 348 00:13:20,504 --> 00:13:23,704 the asteroid also contains traces of glucose and 349 00:13:23,704 --> 00:13:25,804 ribose, which are both essential sugars, 350 00:13:26,345 --> 00:13:28,664 plus a bunch of different nitrogen and oxygen 351 00:13:28,664 --> 00:13:31,440 containing organic compounds plus supernova 352 00:13:32,139 --> 00:13:34,220 dust. And this is all really adding to 353 00:13:34,220 --> 00:13:36,620 this idea that asteroids could have delivered some 354 00:13:36,620 --> 00:13:39,259 of the, quote, ingredients for life to the 355 00:13:39,259 --> 00:13:40,000 early Earth 356 00:13:40,300 --> 00:13:42,779 while it was still essentially a smoldering ball 357 00:13:42,779 --> 00:13:43,840 of empty rock, 358 00:13:44,274 --> 00:13:46,514 and thereby kick starting the process that led 359 00:13:46,514 --> 00:13:47,815 to the evolution of life. 360 00:13:48,434 --> 00:13:50,514 This is a hypothesis that's been kicking around 361 00:13:50,514 --> 00:13:52,855 for decades, but thanks to our OSIRIS REx 362 00:13:53,154 --> 00:13:55,875 and other sample return missions, we're finally getting 363 00:13:55,875 --> 00:13:58,455 some answers about how plausible it really is. 364 00:13:59,509 --> 00:14:01,350 However, if I could add just a little 365 00:14:01,350 --> 00:14:03,669 down note here, several of the scientists involved 366 00:14:03,669 --> 00:14:06,230 in this particular breakthrough are or were affiliated 367 00:14:06,230 --> 00:14:08,309 with NASA, which is the US National Air 368 00:14:08,309 --> 00:14:09,289 and Space Administration. 369 00:14:10,149 --> 00:14:12,894 NASA's facing massive budget cuts and layoff due 370 00:14:12,894 --> 00:14:14,975 to the anti science attitude of the current 371 00:14:14,975 --> 00:14:15,714 US government, 372 00:14:16,095 --> 00:14:18,514 and NASA's Goddard Space Flight Center in particular 373 00:14:18,815 --> 00:14:21,315 is looking at significant reductions in staffing. 374 00:14:21,855 --> 00:14:24,014 It's perhaps indicative of the situation that at 375 00:14:24,014 --> 00:14:25,774 least one of the scientists who led this 376 00:14:25,774 --> 00:14:27,154 research is in this breakthrough 377 00:14:27,500 --> 00:14:29,419 and was employed at NASA Goddard at the 378 00:14:29,419 --> 00:14:31,120 beginning of 02/2025 379 00:14:31,419 --> 00:14:32,639 is no longer there. 380 00:14:33,339 --> 00:14:35,339 So we like to celebrate breakthroughs, but this 381 00:14:35,339 --> 00:14:37,019 is kind of the reverse. It's a breakdown 382 00:14:37,019 --> 00:14:38,779 of the year in terms of our ability 383 00:14:38,779 --> 00:14:40,945 to discover things like this because if it 384 00:14:40,945 --> 00:14:42,865 continues, then we're gonna lose the people and 385 00:14:42,865 --> 00:14:45,284 skills we need to make these discoveries happen. 386 00:14:45,504 --> 00:14:47,184 In fact, we already are losing them, and 387 00:14:47,184 --> 00:14:48,945 we'd be remiss not to mention that somewhere 388 00:14:48,945 --> 00:14:49,764 in this podcast. 389 00:14:50,544 --> 00:14:52,945 Yeah. Very good point, Margaret. Breakdown of the 390 00:14:52,945 --> 00:14:54,625 year. Yeah. That's something we didn't want hope 391 00:14:54,625 --> 00:14:56,840 we wouldn't think think would have happened. But, 392 00:14:57,220 --> 00:14:59,639 very good point. But, you know, sending asteroid 393 00:15:00,019 --> 00:15:01,539 samples back to Earth and studying them, I 394 00:15:01,539 --> 00:15:02,980 mean, how cool is that for getting people 395 00:15:02,980 --> 00:15:05,220 into physics and astronomy and science and getting 396 00:15:05,220 --> 00:15:06,820 them excited? It's the kind of thing, especially 397 00:15:06,820 --> 00:15:08,894 younger people will be, you know, fascinated about. 398 00:15:08,894 --> 00:15:10,335 Yeah. If we only keep if we can 399 00:15:10,335 --> 00:15:12,274 only keep them there, it'd be fantastic. Yeah. 400 00:15:12,335 --> 00:15:14,095 So we're now halfway through our list of, 401 00:15:14,335 --> 00:15:16,014 the top 10 breakthroughs of the year for 402 00:15:16,014 --> 00:15:18,654 2025 in physics. We're gonna switch gear and 403 00:15:18,654 --> 00:15:20,274 move over to medical physics. 404 00:15:20,654 --> 00:15:22,735 And, Tammy, we've gone for some new work 405 00:15:22,735 --> 00:15:24,355 using what's known as proton 406 00:15:25,080 --> 00:15:25,820 arc therapy, 407 00:15:26,120 --> 00:15:28,680 which involves using protons to treat patients with 408 00:15:28,680 --> 00:15:30,279 cancer, but in a better manner than has 409 00:15:30,279 --> 00:15:31,420 been possible before. 410 00:15:32,279 --> 00:15:35,340 Yes. So this study is about proton therapy, 411 00:15:35,720 --> 00:15:38,304 a cancer treatment in which beams of protons 412 00:15:38,365 --> 00:15:41,164 are precisely directed onto a tumor to destroy 413 00:15:41,164 --> 00:15:42,225 targeted cells. 414 00:15:42,845 --> 00:15:45,964 Now currently, proton therapy is mostly performed using 415 00:15:45,964 --> 00:15:48,684 a technique called pencil beam scanning, in which 416 00:15:48,684 --> 00:15:50,845 a narrow beam of protons is scanned over 417 00:15:50,845 --> 00:15:52,769 the target to match the tumor shape 418 00:15:53,250 --> 00:15:55,410 with different beam energies used to build up 419 00:15:55,410 --> 00:15:58,290 depth layers and effectively paint the dose onto 420 00:15:58,290 --> 00:15:59,429 the tumor volume. 421 00:15:59,730 --> 00:16:03,009 Now this this approach provides highly conformal dose 422 00:16:03,009 --> 00:16:03,509 distributions, 423 00:16:04,050 --> 00:16:06,690 which means that the proton dose matches really 424 00:16:06,690 --> 00:16:08,389 well with the shape of the tumor. 425 00:16:08,855 --> 00:16:10,454 But it can be limited by the small 426 00:16:10,454 --> 00:16:12,615 number of beam directions that it can deliver 427 00:16:12,615 --> 00:16:14,714 in an acceptable treatment time. 428 00:16:16,134 --> 00:16:18,694 Now a team at the Trento Proton Therapy 429 00:16:18,694 --> 00:16:21,014 Center in Italy is working on a new 430 00:16:21,014 --> 00:16:22,315 type of treatment delivery 431 00:16:22,620 --> 00:16:24,399 called proton arc therapy. 432 00:16:25,340 --> 00:16:27,899 Here, the proton beams are irradiated onto the 433 00:16:27,899 --> 00:16:30,320 target at a large number of beam angles 434 00:16:30,379 --> 00:16:32,799 while the gantry moves in an arc trajectory 435 00:16:33,100 --> 00:16:34,080 around the patient. 436 00:16:34,460 --> 00:16:35,679 And during this rotation, 437 00:16:36,095 --> 00:16:38,674 the beam energy and intensity are adjusted 438 00:16:38,975 --> 00:16:41,455 to map the required dose onto the target 439 00:16:41,455 --> 00:16:41,955 volume. 440 00:16:43,535 --> 00:16:46,815 Now working with researchers at research laboratories in 441 00:16:46,815 --> 00:16:47,315 Sweden, 442 00:16:47,934 --> 00:16:51,190 the team compared proton arc therapy plans with 443 00:16:51,190 --> 00:16:53,610 state of the art pencil beam scanning plans 444 00:16:53,750 --> 00:16:55,850 for 10 patients with head and neck cancers. 445 00:16:56,709 --> 00:16:59,209 And they found that proton arc therapy improved 446 00:16:59,269 --> 00:17:01,829 the dose conformality compared with the pencil beam 447 00:17:01,829 --> 00:17:04,869 plans. So it did it delivered equivalent dose 448 00:17:04,869 --> 00:17:07,265 to the tumor target, but less dose to 449 00:17:07,265 --> 00:17:10,065 the nearby organs at risk, with the largest 450 00:17:10,065 --> 00:17:12,544 impact seen in reducing dose to the brain 451 00:17:12,544 --> 00:17:13,044 stem. 452 00:17:13,744 --> 00:17:16,384 And the team also ran a feasibility test 453 00:17:16,384 --> 00:17:19,184 that confirmed that it's actually possible to deliver 454 00:17:19,184 --> 00:17:21,444 this proton arc therapy in the clinic. 455 00:17:22,880 --> 00:17:25,759 The big breakthrough here is that following these 456 00:17:25,759 --> 00:17:29,039 initial tests, the researchers then performed the world's 457 00:17:29,039 --> 00:17:32,099 first clinical treatments using proton arc therapy. 458 00:17:32,960 --> 00:17:34,960 At the time of writing their paper, they 459 00:17:34,960 --> 00:17:36,740 treated nine cancer patients, 460 00:17:37,244 --> 00:17:39,325 five with head and neck tumors, three with 461 00:17:39,325 --> 00:17:41,585 brain tumors, and one with thoracic cancer. 462 00:17:42,365 --> 00:17:44,924 Now importantly, all of these treatments were performed 463 00:17:44,924 --> 00:17:48,305 using the medical center's existing proton therapy system 464 00:17:48,525 --> 00:17:50,545 and using the same clinical workflow. 465 00:17:51,565 --> 00:17:54,069 Looking ahead, the researchers aim to use this 466 00:17:54,069 --> 00:17:57,029 protonark therapy to treat tumors in other regions 467 00:17:57,029 --> 00:17:57,769 of the body. 468 00:17:58,630 --> 00:18:00,630 So a technique that potentially could really be 469 00:18:00,630 --> 00:18:02,650 of great benefit to, to people, 470 00:18:03,109 --> 00:18:04,724 with cancer. That sounds great, 471 00:18:05,605 --> 00:18:08,265 and really promising work. And over in biophysics, 472 00:18:08,404 --> 00:18:10,085 Tammy, if I can stick with you, this 473 00:18:10,085 --> 00:18:12,244 year, we reported on some really interesting work 474 00:18:12,244 --> 00:18:13,944 using a quantum bit 475 00:18:14,244 --> 00:18:16,424 that was formed from a fluorescent protein 476 00:18:16,900 --> 00:18:18,579 that could be used as a sensor that 477 00:18:18,579 --> 00:18:21,700 can be directly produced inside living cells. Now 478 00:18:21,700 --> 00:18:23,859 to me, this sounds really fascinating. It's quantum 479 00:18:23,859 --> 00:18:25,000 physics and biophysics 480 00:18:25,299 --> 00:18:27,220 and a new kind of sensor. So do 481 00:18:27,220 --> 00:18:29,240 you wanna tell us about this one? Sure. 482 00:18:30,144 --> 00:18:32,704 So this breakthrough is from researchers at the 483 00:18:32,704 --> 00:18:36,244 University of Chicago, Pritzker School of Molecular Engineering. 484 00:18:37,025 --> 00:18:40,065 And they designed a protein quantum bit or 485 00:18:40,065 --> 00:18:40,565 qubit 486 00:18:40,945 --> 00:18:43,365 that can be produced inside living cells. 487 00:18:43,730 --> 00:18:45,890 And this protein qubit can be used as 488 00:18:45,890 --> 00:18:48,849 a quantum sensor that can detect tiny changes 489 00:18:48,849 --> 00:18:50,230 in magnetic fields. 490 00:18:51,089 --> 00:18:53,650 So many of today's quantum sensors are based 491 00:18:53,650 --> 00:18:56,230 on nitrogen vacancy or NV 492 00:18:56,884 --> 00:18:58,024 sensors in diamond. 493 00:18:58,484 --> 00:19:01,204 And when excited with laser pulses, these crystal 494 00:19:01,204 --> 00:19:03,845 defects emit a fluorescent signal that can be 495 00:19:03,845 --> 00:19:06,664 used to monitor slight changes in the magnetic 496 00:19:06,724 --> 00:19:08,585 properties of a nearby sample. 497 00:19:09,630 --> 00:19:13,089 For biological applications, however, these sensors are relatively 498 00:19:13,150 --> 00:19:16,990 large, and they're difficult to precisely position inside 499 00:19:16,990 --> 00:19:17,890 living cells. 500 00:19:18,750 --> 00:19:21,869 So instead, the team, led by Peter Maurer 501 00:19:21,869 --> 00:19:22,930 and David Avshalom, 502 00:19:23,615 --> 00:19:26,015 took a biological system and turned it into 503 00:19:26,015 --> 00:19:26,674 a qubit. 504 00:19:27,455 --> 00:19:29,775 They used fluorescent proteins that are just three 505 00:19:29,775 --> 00:19:30,994 nanometers in diameter 506 00:19:31,455 --> 00:19:33,234 and can be genetically encoded 507 00:19:33,535 --> 00:19:35,695 such that they're produced by cells at a 508 00:19:35,695 --> 00:19:38,035 desired location with atomic precision. 509 00:19:39,430 --> 00:19:41,670 What's special about these proteins is that they 510 00:19:41,670 --> 00:19:43,849 possess similar optical and spin properties 511 00:19:44,150 --> 00:19:46,410 to those of NV center based qubits, 512 00:19:46,950 --> 00:19:48,250 in that they have a metastable 513 00:19:48,630 --> 00:19:49,690 triplet state. 514 00:19:51,285 --> 00:19:53,525 So to demonstrate that their idea worked, the 515 00:19:53,525 --> 00:19:57,285 researchers created an optically addressable spin qubit in 516 00:19:57,285 --> 00:19:58,984 a yellow fluorescent protein, 517 00:19:59,285 --> 00:20:01,365 and they used a near infrared laser pulse 518 00:20:01,365 --> 00:20:03,285 to read out its triplet state with up 519 00:20:03,285 --> 00:20:05,065 to 20% spin contrast. 520 00:20:06,484 --> 00:20:09,670 Next, they genetically modified the protein so that 521 00:20:09,670 --> 00:20:12,710 it was expressed in bacterial cells, and they 522 00:20:12,710 --> 00:20:15,750 measured signals in this case with a, contrast 523 00:20:15,750 --> 00:20:16,970 of up to 8%. 524 00:20:17,750 --> 00:20:18,970 So while this performance 525 00:20:19,269 --> 00:20:22,170 doesn't match that of the NV quantum sensors, 526 00:20:22,914 --> 00:20:26,375 These fluorescent proteins could enable magnetic resonance measurements 527 00:20:26,595 --> 00:20:30,035 directly inside living cells, which NV centers simply 528 00:20:30,035 --> 00:20:30,855 cannot do. 529 00:20:31,954 --> 00:20:34,035 And because of this, Maurer suggests that the 530 00:20:34,035 --> 00:20:35,174 new protein qubits 531 00:20:35,579 --> 00:20:37,599 could transform medical and biochemical 532 00:20:37,900 --> 00:20:38,400 studies 533 00:20:39,019 --> 00:20:43,099 by probing protein folding, monitoring redox states, or 534 00:20:43,099 --> 00:20:45,679 detecting drug binding at the molecular scale. 535 00:20:46,059 --> 00:20:48,779 So thanks, Tammy. That's some fascinating, biophysics and 536 00:20:48,779 --> 00:20:51,054 quantum physics. And we're down to the final 537 00:20:51,054 --> 00:20:52,815 three picks for the breakthrough of the year 538 00:20:52,815 --> 00:20:54,674 in physics for 2025. 539 00:20:54,734 --> 00:20:56,255 Hamish, I'm gonna come back to you now 540 00:20:56,255 --> 00:20:58,835 for some imaging and condensed matter physicists, 541 00:20:59,294 --> 00:21:01,694 with physicists saying that they've recorded the highest 542 00:21:01,694 --> 00:21:02,514 ever resolution 543 00:21:02,894 --> 00:21:04,595 images of a single atom. 544 00:21:05,099 --> 00:21:06,779 Well, we do like breaking records here at 545 00:21:06,779 --> 00:21:08,460 Physics World. So, do you wanna tell us 546 00:21:08,460 --> 00:21:09,980 about this one? And can you pronounce the 547 00:21:09,980 --> 00:21:10,480 technique? 548 00:21:10,779 --> 00:21:13,099 It's got a funny name. Well, we'll see. 549 00:21:13,099 --> 00:21:14,240 Yeah. So, 550 00:21:14,539 --> 00:21:17,019 yes, this this is a a breakthrough in 551 00:21:17,019 --> 00:21:17,819 terms of, 552 00:21:18,605 --> 00:21:20,545 resolution with an electron micros- 553 00:21:20,845 --> 00:21:23,884 with an electron microscope. But there's much much 554 00:21:23,884 --> 00:21:26,205 more to it, which is why we selected 555 00:21:26,205 --> 00:21:27,984 it. This is related to twisted 556 00:21:28,445 --> 00:21:30,224 materials, this idea of twistronics. 557 00:21:31,005 --> 00:21:32,305 When you take two 558 00:21:32,609 --> 00:21:33,009 atomic, 559 00:21:33,569 --> 00:21:34,069 atomically 560 00:21:34,369 --> 00:21:34,869 thin 561 00:21:35,250 --> 00:21:38,130 lattice layers and twist them with respect to 562 00:21:38,130 --> 00:21:39,490 each other, and you can get some really 563 00:21:39,490 --> 00:21:39,990 strange, 564 00:21:41,009 --> 00:21:43,509 properties in these, twisted systems. 565 00:21:44,369 --> 00:21:47,109 The result is something called a moire superlattice 566 00:21:47,804 --> 00:21:49,984 of atoms. And you can by 567 00:21:50,524 --> 00:21:51,904 adjusting the twist angle, 568 00:21:52,204 --> 00:21:55,484 you can adjust this superlattice, the distance between 569 00:21:55,484 --> 00:21:56,065 the atoms, 570 00:21:56,524 --> 00:21:59,184 and then you can also adjust the electronic 571 00:21:59,244 --> 00:22:00,625 properties of the system, 572 00:22:01,480 --> 00:22:04,380 which researchers have found to be very useful. 573 00:22:05,000 --> 00:22:06,779 And in this, study, 574 00:22:07,079 --> 00:22:10,059 Yichao Zhang at the University of Maryland 575 00:22:10,519 --> 00:22:12,059 and Pinshain Huang 576 00:22:12,359 --> 00:22:14,140 of the University of Illinois 577 00:22:14,519 --> 00:22:15,179 at Urbana 578 00:22:15,644 --> 00:22:16,144 Champaign, 579 00:22:16,605 --> 00:22:18,224 have used a technique called 580 00:22:18,684 --> 00:22:19,904 electron tachygraphy 581 00:22:20,924 --> 00:22:22,945 to capture the highest resolution 582 00:22:23,404 --> 00:22:24,545 images ever 583 00:22:24,924 --> 00:22:25,664 of atoms, 584 00:22:26,285 --> 00:22:28,224 and they've done so in a moire 585 00:22:28,799 --> 00:22:29,299 superlattice 586 00:22:29,840 --> 00:22:30,900 made of tungsten 587 00:22:31,279 --> 00:22:31,779 diselenide. 588 00:22:32,799 --> 00:22:33,299 Now, 589 00:22:33,600 --> 00:22:34,660 electron ticography, 590 00:22:34,960 --> 00:22:36,420 it's an electron microscopy 591 00:22:36,720 --> 00:22:37,220 technique 592 00:22:37,600 --> 00:22:38,980 that uses diffraction 593 00:22:39,440 --> 00:22:42,884 to boost the resolution of electron microscopy. Now, 594 00:22:43,125 --> 00:22:46,404 electron microscopy has got pretty high resolution already, 595 00:22:46,404 --> 00:22:49,765 and you can see individual atoms with, some 596 00:22:49,765 --> 00:22:50,744 electron microscopes. 597 00:22:51,125 --> 00:22:54,184 But diffraction is used to to improve this. 598 00:22:54,484 --> 00:22:56,759 And they were able to look 599 00:22:57,240 --> 00:22:58,619 at this moire superlattice 600 00:22:59,160 --> 00:23:00,059 at a resolution 601 00:23:00,440 --> 00:23:01,259 of 15 602 00:23:01,720 --> 00:23:02,220 picometers. 603 00:23:03,400 --> 00:23:05,880 And that's pretty good when you consider that 604 00:23:05,880 --> 00:23:06,700 the size 605 00:23:07,000 --> 00:23:08,920 of an atom. Okay, what's the size of 606 00:23:08,920 --> 00:23:11,345 an atom? It's a bit wooly, the definition. 607 00:23:11,644 --> 00:23:14,525 But typically, you know, it's defined to be 608 00:23:14,525 --> 00:23:15,505 about a 100 609 00:23:16,365 --> 00:23:16,865 picometres, 610 00:23:17,164 --> 00:23:19,884 a 150 picometres, so they're you know, the 611 00:23:19,884 --> 00:23:22,464 resolution is much much smaller 612 00:23:22,765 --> 00:23:24,944 than the actual size of the atoms 613 00:23:25,289 --> 00:23:26,509 that they're looking at. 614 00:23:27,289 --> 00:23:28,670 And I suppose 615 00:23:29,130 --> 00:23:30,410 a a very interesting thing, 616 00:23:30,970 --> 00:23:33,789 that they used this technique to do 617 00:23:34,090 --> 00:23:37,150 is they looked at collective lattice vibrations 618 00:23:37,769 --> 00:23:39,630 called moire phasons. 619 00:23:40,505 --> 00:23:42,424 And so these are a bit like, the 620 00:23:42,424 --> 00:23:43,565 familiar phonons, 621 00:23:44,424 --> 00:23:44,924 collective 622 00:23:45,304 --> 00:23:48,204 sound waves that occur in normal lattices. 623 00:23:48,744 --> 00:23:51,565 But they occur in these moire superlattices, 624 00:23:51,865 --> 00:23:54,909 and they're actually much lower energy and much 625 00:23:54,909 --> 00:23:55,409 weaker, 626 00:23:56,509 --> 00:23:57,809 but they do have, 627 00:23:58,190 --> 00:24:01,970 a very important effect on the electronic properties 628 00:24:02,269 --> 00:24:03,970 of these twisted materials. 629 00:24:04,750 --> 00:24:05,389 And so, 630 00:24:05,869 --> 00:24:08,690 by using this technique to observe these phasons, 631 00:24:11,125 --> 00:24:11,605 physicists, 632 00:24:11,924 --> 00:24:14,984 have the chance to really understand why 633 00:24:15,285 --> 00:24:18,805 these twisted materials have these really strange and 634 00:24:18,805 --> 00:24:19,305 exotic 635 00:24:19,684 --> 00:24:23,990 electronic properties. Because often these electronic properties arise 636 00:24:23,990 --> 00:24:27,349 because of interactions between the electrons and the 637 00:24:27,349 --> 00:24:28,330 lattice vibrations, 638 00:24:28,710 --> 00:24:30,809 you know, the classic example being superconductivity. 639 00:24:31,990 --> 00:24:32,390 So, 640 00:24:33,589 --> 00:24:35,609 yeah, a very a very high resolution 641 00:24:36,070 --> 00:24:36,404 elect, 642 00:24:36,884 --> 00:24:38,505 electron microscopy technique 643 00:24:38,884 --> 00:24:41,125 that opens up a new field, a new 644 00:24:41,125 --> 00:24:42,025 way of studying, 645 00:24:42,884 --> 00:24:45,765 these materials. So, yep, very exciting, and that's 646 00:24:45,765 --> 00:24:48,644 why it's in our top 10. Brilliant stuff, 647 00:24:48,644 --> 00:24:50,309 Hamish. Thanks very much. And if I can 648 00:24:50,309 --> 00:24:52,069 stick with you, now we always do know 649 00:24:52,069 --> 00:24:54,950 that particle physics gets, people very excited. And 650 00:24:54,950 --> 00:24:57,190 our penultimate pick for this year is some 651 00:24:57,190 --> 00:24:58,409 work done at CERN, 652 00:24:58,789 --> 00:25:01,429 where researchers at the base experiments have measured 653 00:25:01,429 --> 00:25:05,154 the magnetic properties of antimatter with record breaking 654 00:25:05,214 --> 00:25:05,714 precision. 655 00:25:06,575 --> 00:25:08,734 Tell us about this one, Hamish. Well, this 656 00:25:08,734 --> 00:25:10,255 is I mean, this has to do with 657 00:25:10,255 --> 00:25:11,875 one of the biggest mysteries 658 00:25:12,494 --> 00:25:13,154 of physics. 659 00:25:13,775 --> 00:25:16,974 And that mystery is why is there much 660 00:25:16,974 --> 00:25:17,795 more matter 661 00:25:18,319 --> 00:25:21,519 than antimatter in the visible universe? The the 662 00:25:21,519 --> 00:25:22,980 standard model says 663 00:25:23,359 --> 00:25:23,680 that, 664 00:25:24,240 --> 00:25:26,819 when the universe began in the big bang, 665 00:25:26,960 --> 00:25:28,960 there would have been roughly equal amounts of 666 00:25:28,960 --> 00:25:30,259 matter and antimatter. 667 00:25:30,664 --> 00:25:32,744 But when we look around us well, you 668 00:25:32,744 --> 00:25:34,664 know, look around the room that you're in, 669 00:25:34,664 --> 00:25:38,265 it's all matter. There's very little antimatter. Really, 670 00:25:38,265 --> 00:25:41,244 the only antimatter that we see comes from, 671 00:25:41,784 --> 00:25:43,484 you know, sort of nuclear processes, 672 00:25:44,105 --> 00:25:46,524 you know, both in in stars and in 673 00:25:47,440 --> 00:25:49,680 in, colliders here on Earth. There there's not 674 00:25:49,680 --> 00:25:51,539 a lot of antimatter out there. 675 00:25:53,039 --> 00:25:55,840 And so there are, there's a series of 676 00:25:55,840 --> 00:25:58,100 experiments, base is one of them at CERN, 677 00:25:58,320 --> 00:25:59,539 where they create, 678 00:26:00,320 --> 00:26:00,820 antimatter 679 00:26:01,365 --> 00:26:01,724 in, 680 00:26:02,164 --> 00:26:03,224 in an accelerator, 681 00:26:03,924 --> 00:26:05,065 and they do 682 00:26:05,365 --> 00:26:07,785 really, really precise measurements on it. 683 00:26:08,404 --> 00:26:09,625 And in this case, 684 00:26:10,005 --> 00:26:11,944 researchers on the base experiment 685 00:26:12,244 --> 00:26:14,345 managed to trap a single 686 00:26:14,724 --> 00:26:15,224 antiproton 687 00:26:16,130 --> 00:26:17,029 in an electromagnetic 688 00:26:17,890 --> 00:26:18,390 trap 689 00:26:18,690 --> 00:26:21,269 and use quantum control techniques 690 00:26:21,809 --> 00:26:22,950 to measure the 691 00:26:23,330 --> 00:26:26,630 antiproton's magnetic properties, basically, its spin, 692 00:26:27,809 --> 00:26:28,630 very precisely. 693 00:26:29,170 --> 00:26:31,830 In fact, 16 times more precise 694 00:26:32,945 --> 00:26:33,684 than before. 695 00:26:34,945 --> 00:26:37,285 And, you know, this is very difficult because 696 00:26:37,424 --> 00:26:39,585 first, you have to create the antiprotons, and 697 00:26:39,585 --> 00:26:41,825 that's done in a collider, and they come 698 00:26:41,825 --> 00:26:44,065 out at very high energy. You have to 699 00:26:44,065 --> 00:26:45,125 slow them down. 700 00:26:46,250 --> 00:26:48,109 You have to sort of store them 701 00:26:48,649 --> 00:26:50,190 at very, very low temperatures 702 00:26:50,649 --> 00:26:53,289 and then do your experiments. And at any 703 00:26:53,289 --> 00:26:54,589 point in this process, 704 00:26:54,970 --> 00:26:57,929 if that anti piece of antimatter comes into 705 00:26:57,929 --> 00:27:00,509 contact with matter, which is, of course, everywhere, 706 00:27:01,244 --> 00:27:04,045 it'll annihilate and you lose it. So it's 707 00:27:04,045 --> 00:27:06,545 a really, really difficult process accumulating 708 00:27:07,244 --> 00:27:08,305 all this antimatter. 709 00:27:08,924 --> 00:27:11,244 And then amazingly, you know, they hold it 710 00:27:11,244 --> 00:27:12,144 in their trap 711 00:27:12,445 --> 00:27:14,785 for long enough to do these quantum manipulations 712 00:27:15,269 --> 00:27:15,769 and, 713 00:27:16,630 --> 00:27:17,450 and measure 714 00:27:18,070 --> 00:27:20,009 the, the its properties. 715 00:27:20,470 --> 00:27:22,230 And and and the reason they want to 716 00:27:22,230 --> 00:27:23,029 do this is, 717 00:27:23,990 --> 00:27:25,450 the the standard model, 718 00:27:26,070 --> 00:27:28,809 basically says that matter and antimatter 719 00:27:29,684 --> 00:27:32,404 should be roughly the same except, you know, 720 00:27:32,404 --> 00:27:35,044 for the the obvious that one's matter and 721 00:27:35,044 --> 00:27:35,865 one's antimatter. 722 00:27:36,404 --> 00:27:39,444 So what what the ultimate goal is to 723 00:27:39,444 --> 00:27:42,265 measure the magnetic properties of the antiproton 724 00:27:43,000 --> 00:27:45,559 and compare it to the magnetic properties of 725 00:27:45,559 --> 00:27:46,299 the proton. 726 00:27:46,839 --> 00:27:49,019 And these should be, well, identical 727 00:27:49,400 --> 00:27:51,740 with the exception of a flip in, 728 00:27:52,599 --> 00:27:54,859 in the side the charge on the particle. 729 00:27:55,325 --> 00:27:57,244 And so if they can find even the 730 00:27:57,244 --> 00:27:57,984 most minute 731 00:27:58,285 --> 00:28:00,944 differences between the proton and the antiproton, 732 00:28:01,644 --> 00:28:03,025 that could lead to physics 733 00:28:03,565 --> 00:28:05,105 beyond the standard model 734 00:28:05,565 --> 00:28:08,065 and also tell us why there's more matter 735 00:28:08,365 --> 00:28:09,265 than antimatter 736 00:28:09,700 --> 00:28:10,519 in the universe. 737 00:28:11,220 --> 00:28:11,720 So 738 00:28:12,259 --> 00:28:15,299 exciting experiment, and who knows? Hopefully, they'll they'll 739 00:28:15,299 --> 00:28:17,380 find a difference between the proton and the 740 00:28:17,380 --> 00:28:17,880 antiproton. 741 00:28:18,180 --> 00:28:20,019 I always think with antimatter, we need another 742 00:28:20,019 --> 00:28:22,340 Dan Brown novel to follow angels and demons 743 00:28:22,340 --> 00:28:24,259 when they used antimatter, and that was the 744 00:28:24,259 --> 00:28:25,214 the plot hook. 745 00:28:26,174 --> 00:28:28,335 Now completing our list of the top 10 746 00:28:28,335 --> 00:28:30,015 breakthroughs of the year in physics as picked 747 00:28:30,015 --> 00:28:31,154 by Physics World, 748 00:28:31,534 --> 00:28:33,855 we've gone some for some condensed matter physics 749 00:28:33,855 --> 00:28:36,335 that seems pretty straightforward in principle, but, 750 00:28:36,894 --> 00:28:38,335 it seems to have taken quite a lot 751 00:28:38,335 --> 00:28:40,599 of effort, and that is in making two 752 00:28:40,599 --> 00:28:41,819 dimensional metals. 753 00:28:42,519 --> 00:28:44,119 So, Michael, can you tell us more about 754 00:28:44,119 --> 00:28:44,779 this one? 755 00:28:45,079 --> 00:28:46,759 Yeah. So this breakthrough is about the first 756 00:28:46,759 --> 00:28:48,700 creation of two d sheets of metal. 757 00:28:49,000 --> 00:28:50,440 So since 2004, 758 00:28:50,440 --> 00:28:52,359 we know that some materials can form flat 759 00:28:52,359 --> 00:28:54,059 sheets known as two d materials, 760 00:28:54,464 --> 00:28:56,244 graphene being one prime example. 761 00:28:56,785 --> 00:28:59,105 Such materials are about one atom thick, and 762 00:28:59,105 --> 00:29:01,345 in the case of graphene occur because you 763 00:29:01,345 --> 00:29:03,444 have a layer of atoms that are separated 764 00:29:03,505 --> 00:29:05,924 by gaps between neighboring layers. 765 00:29:06,539 --> 00:29:08,860 This means that you can effectively shave off 766 00:29:08,860 --> 00:29:10,880 layers to make two d sheets. 767 00:29:11,420 --> 00:29:13,660 Things are a bit different, however, for metals. 768 00:29:13,660 --> 00:29:16,140 In the case of metals, atoms are strongly 769 00:29:16,140 --> 00:29:19,019 bounded to surrounding atoms in all directions, which 770 00:29:19,019 --> 00:29:20,559 makes cleaving difficult. 771 00:29:21,274 --> 00:29:23,034 To get around this problem and create two 772 00:29:23,034 --> 00:29:25,274 d sheets of metal, the researchers who are 773 00:29:25,274 --> 00:29:28,075 based in China heated powders of pure metals 774 00:29:28,075 --> 00:29:29,534 and melted them into droplets. 775 00:29:30,075 --> 00:29:32,474 They then applied a pressure of around 200 776 00:29:32,474 --> 00:29:33,774 megapascal, effectively 777 00:29:34,075 --> 00:29:37,440 squeezing the opposite sides of these anvils until 778 00:29:37,440 --> 00:29:39,539 two d sheets of metals were formed. 779 00:29:40,079 --> 00:29:42,799 The team managed to produce five atomically thin 780 00:29:42,799 --> 00:29:45,140 two d metals. That's bismuth, 781 00:29:45,440 --> 00:29:48,799 tin, lead, indium, and gallium, with the thinnest 782 00:29:48,799 --> 00:29:50,320 being around 6.3 783 00:29:50,320 --> 00:29:50,820 angstrom. 784 00:29:51,654 --> 00:29:53,335 The researchers say their work is just a 785 00:29:53,335 --> 00:29:55,255 tip of the iceberg, and they now aim 786 00:29:55,255 --> 00:29:57,755 to study fundamental physics with the new materials. 787 00:29:58,055 --> 00:29:59,194 So watch this space. 788 00:30:00,855 --> 00:30:03,035 So that's all of our top 10 breakthroughs 789 00:30:03,174 --> 00:30:05,319 for this year as picked by Physics World. 790 00:30:05,319 --> 00:30:07,419 We've had some astronomy, some geoscience, 791 00:30:07,880 --> 00:30:08,859 condensed matter, 792 00:30:09,240 --> 00:30:12,119 a bit of particle physics, biophysics, medical physics, 793 00:30:12,119 --> 00:30:13,339 and optical physics. 794 00:30:13,880 --> 00:30:15,720 But to find out who's bagged the overall 795 00:30:15,720 --> 00:30:17,960 top prize for Physics World's breakthrough of the 796 00:30:17,960 --> 00:30:19,500 year for 2025, 797 00:30:20,144 --> 00:30:22,805 Check back on Thursday, December 18, 798 00:30:23,025 --> 00:30:25,184 where we'll reveal the winner in a new 799 00:30:25,184 --> 00:30:27,105 story and in the next episode of the 800 00:30:27,105 --> 00:30:28,805 Physics World weekly podcast. 801 00:30:29,825 --> 00:30:32,644 So a big thank you to Tammy, Margaret, 802 00:30:32,865 --> 00:30:35,045 Michael, and Hamish for joining me today. 803 00:30:35,460 --> 00:30:38,359 And a special thanks to producer Fred Isles. 804 00:30:38,419 --> 00:30:40,419 And thanks for listening, and do join us 805 00:30:40,419 --> 00:30:42,500 again next week for the big reveal of 806 00:30:42,500 --> 00:30:45,720 Physics World's breakthrough of the year for 2025.