Don’t walk into the water! Pokémon Go arrives at Fermilab. (Courtesy: Lauren Biron/Fermilab)
By Michael Banks and Hamish Johnston
The smartphone app Pokémon GO has been all the rage since its recent launch. The augmented-reality game is based on the Nintendo franchise and features players exploring their surroundings while trying to catch as many of the virtual creatures as possible, According to Science, Pokémon have been spotted at a number of science centres including NASA’s Jet Propulsion Laboratory while Symmetry Magazine reports that the game has also infiltrated particle-physics labs such as Fermilab, with scientists seen walking around the lab peering into their phone as they hunt down Pokémon.
This is the fourth in a series of blog posts about “Lateral Thoughts”, Physics World’slong-running humour column. Click to read the first, second and third posts.
As the editor in charge of Lateral Thoughts – Physics World’s long-running column of humorous or otherwise offbeat essays on physics – I am sometimes* asked whether I have a favourite. It’s an interesting question, and back in 2014, when I was writing a series of posts for this blog about how Lateral Thoughts had changed over the (then) 25-year history of Physics World, I promised to answer it.
This, however, proved easier said than done. In the weeks that followed my foolish pledge, the Physics World inbox (email@example.com) received a whole series of Lateral Thoughts essays that could have been my “favourite”. One of them, published in May 2014, was John Swanson’s discourse on the quantum nature of the 20:08 train from Bristol Parkway. Another, which appeared in June 2014, contained Chris Atkins’ gloriously straight-faced analysis of the physics of Poohsticks. A third, in July 2014, saw kung-fu expert Felix Flicker explore an unexpected connection between the mathematics of spinors and the art of escaping from an armlock. Then, in August 2014, John Evans pondered various physics-based ways of improving his running – such as refining his aerodynamic profile by developing a beer belly. (Evans, incidentally, went on to write a Lateral Thought on cycling in October 2015, and this month we published his essay on swimming. This means he’s now completed a lateral-thinking triathlon. Congratulations!)
If you have never been one of the lucky few to have wandered the tunnels of a particle accelerator, but have always wondered what lies within, take a look at the video above. The European X-ray Free Electron Laser (European XFEL) – which is currently under construction in Germany and will come online next year – will provide ultrashort (27,000 X-ray flashes per second) and ultrabright X-ray laser flashes that are needed to study chemical reactions in situ or to study extreme states of matter (you can read more about the kind of research that will be done there in the September issue of Physics World magazine). The XFEL tunnel is 3.4 km long and you can zoom across all of it in the 5 minute long video. I particularly enjoyed watching particular locations where engineers could be seen carrying out tests, as well as watching folks on bicycles wobble out of the camera’s way.
On a slightly related note, if, like me, you occasionally get a bit muddled when it comes to certain details of different particle accelerators – for example which came first, the synchrotron or the cyclotron – take a look at this excellent “primer” over at Symmetry magazine.
A few weeks ago I was in Germany for the 66th Lindau Nobel Laureate Meeting, where I moderated a “press talk” about migration and science. This was essentially a panel discussion that involved two chemistry Nobel laureates – Martin Karplus and Daniel Shechtman – and two early-career physicists: Winifred Ayinpogbilla Atiah from Ghana and Ana Isabel Maldonado Cid from Spain.
Before setting off to the International Space station (ISS) for six months, UK astronaut Tim Peake revealed that one of the meals he would miss most is the classic British roast dinner. So what better way to celebrate the 44 year old’s safe return to Earth last month than to create a portrait of him made from his favourite nosh? Designed by UK “food artist” Prudence Staite for the Hungry Horse pub chain, the culinary creation took 20 hours to make – you can watch a timelapse video of it being created above. The finished portrait weighed in at 12 kg and says “Welcome Home Tim”. Hungry Horse has even offered Tim and his family free roast dinners for life.
Triple bump: the 5 MeV bump data presented by K Joo at the Neutrino 2016 conference. (Courtesy: RENO Collaboration)
By Tushna Commissariat
A final mystery that was mentioned at the Neutrino 2016 I attended in London this week was yet another unexpected “bump” in data at 5 MeV, measured while monitoring the neutrino flux from nuclear power plants. Starting with the RENO experiment in 2012, it was spotted by the Double Chooz experiment in 2014 and finally by the Daya Bay neutrino experiment earlier this year. While the initial signal was not of high enough statistical significance, it has now held up over time and more measurements.
More data are definitely needed in the quest for the sought-after sterile neutrino. That much was clear as more than 10 different global neutrino detectors announced at the Neutrino 2016 conference in London that they have found no evidence for the slippery particle’s existence. The sterile neutrino is a hypothetical and much-debated fourth type of neutrino that would contribute mass, but only interact with the other three “active neutrinos”, making it that much more difficult to detect. In the video above, Physics World features editor Louise Mayor explains why researchers are so keen to nail down this particle, should it exist, as it may single-handedly explain some of the biggest mysteries in physics today, including dark matter.
Deep trap: Inside the Super-Kamiokande neutrino detector. (Courtesy: T2K Collaboration)
By Tushna Commissariat
As you may have read, earlier this week I was at Neutrino 2016 – the 27th International Conference on Neutrino Physics and Astrophysics – in London. Although I was only at two days of the week-long conference, I still have neutrinos on my mind. A whole host of experiments presented various data and updates. Indeed, the researchers presenting the latest results from the Tokai to Kamioka (T2K) experiment in Japan and the NOvA Neutrino Experiment at Fermilab in the US had some interesting things to say.
T2K collaborator Hirohisa Tanaka, from the University of Toronto in Canada, revealed that the experiment’s most recent data seem to support earlier hints that there may be different oscillation probabilities for neutrinos and antineutrinos. If these data hold up, then it would have big consequences – the standard model of neutrino physics says that these two oscillation rates should be the same so as not to violate charge–parity (CP) symmetry. According to the collaboration, their observed “electron antineutrino appearance event rate is lower than would be expected based on the electron neutrino appearance event rate, assuming that CP symmetry is conserved”.
Cool operator: Marek Kowalski talking about IceCube at the Neutrino 2016 conference. (Courtesy: Tushna Commissariat)
By Tushna Commissariat at the Royal Geographical Society in London
“There are still many things to be studied in neutrinos,” said 2015 Nobel laureate Takaaki Kajita at the first talk of the Neutrino 2016 conference that began in London today. I couldn’t help but notice that his statement rang very true, as the day’s talks touched on everything from high-energy neutrinos to dark-matter searches to monitoring nuclear reactors. This year, more than 700 physicists from all over the world are attending the week-long conference, which is taking place at the historic Royal Geographical Society in London.
Early next week NASA’s Juno spacecraft will fire its blasters and pop itself into orbit around Jupiter. On 24 June the approaching spacecraft fell under the spell of the planet’s powerful magnetic field and the transition was captured by Juno’s Waves instrument, which measures radio and plasma waves.
The signals have been converted to sound and you can listen to them in the above video. There are two abrupt changes in the signal from Waves. One is a shift from a high-pitch whisper to a low-frequency roar that occurs when Juno crosses Jupiter’s bow shock. This is where the supersonic solar wind is slowed by the planet’s magnetic field and the roar is the equivalent of a sonic boom here on Earth.