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pt_cover1121_Cover 10/14/2021 1:03 PM Page 1 PHYSICS TODAY November 2021 • volume 74, number 11 A publication of the American Institute of Physics waves How wind makes Cooling protons with lasers Philosophy of thermodynamics Doing science sustainably
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pt_contents1121_Contents 10/15/2021 4:13 PM Page 5 PHYSICS TODAY November 2021 | volume 74 number 11 FEATURES 30 Illuminating the darkest galaxies 30 Joshua D. Simon and Marla Geha The behavior of extremely dim galaxies provides stringent constraints on the nature of dark matter. Establishing those constraints depends on precise stellar-motion measurements. 38 How does the wind generate waves? Nick Pizzo, Luc Deike, and Alex Ayet Although the question is a classical problem, the details of how wind transfers energy to waves at the ocean surface remain elusive. 44 The demons haunting thermodynamics 38 Katie Robertson The contradictory implications of statistical mechanics have worried physicists and philosophers for centuries. Does our present-day knowledge allow us to exorcize those philosophical demons? ON THE COVER: Waves are born at the interface of air and water, where the flow is generally turbulent over a broad range of spatial and temporal scales. Scientists have been struggling with that complexity for more than a century. For a review of historical approaches and recent experimental and numerical efforts to resolve how momentum is transferred from winds to waves, turn to the article by Nick Pizzo, Luc Deike, and Alex Ayet on 44 page 38. (Image by iStock.com/Anna_Om.) PHYSICS TODAY (ISSN 0031-9228, coden PHTOAD) volume 74, Recently on number 11. Published monthly by the American Institute of Physics, 1305 Walt Whitman Rd, Suite 300, Melville, NY 11747-4300. Periodicals postage paid at Huntington PHYSICS Station, NY, and at additional mailing offices. POSTMASTER: Send address changes to PHYSICS TODAY, American Institute of Physics, 1305 Walt Whitman Rd, Suite 300, Melville, NY TODAY ISTOCK.COM/FATCAMERA SARAH WILD NIST 11747-4300. Views expressed in PHYSICS TODAY and on its website are those of the authors and not necessarily those of AIP or any of ONLINE its member societies. College after COVID-19 Shielded by quartz NIST reactor New surveys of under- Amid the unrelenting heat On page 26 of the Copyright © 2021, American Institute of Physics. Single graduate physics students and aridity in the Namib October issue, David copies of individual articles may be made for private use reveal the impacts of the Desert in southwest Africa, Kramer recounted physicists’ or research. Authorization is given to copy articles beyond pandemic on education hardy bacteria manage to dismay with the indefinite the free use permitted under US Copyright Law, provided www.physicstoday.org and offer insights into how survive on the undersides shutdown of NIST’s that the copying fee of $30.00 per copy per article is paid departments can improve. of quartz stones. New research reactor in to the Copyright Clearance Center, 222 Rosewood Dr, Danvers, MA 01923. For articles published before 1978, Many students report interdisciplinary research Maryland. A new report the copying fee is $0.25 per article. Authorization does not learning less from remote reveals how the quartz details the operator errors, extend to systematic or multiple reproduction or to instruction than they shelters, by filtering out which the agency partly republication in any form. In all such cases, specific written would have in person and UV light, enable the attributes to staff turnover, permission from AIP must be obtained. Send requests for limited access to study bacteria to survive as that led to a release of permission to AIP Office of Rights and Permissions, 1305 groups with peers. they wait for water. radiation in February. Walt Whitman Rd, Suite 300, Melville, NY 11747-4300; physicstoday.org/Nov2021a physicstoday.org/Nov2021b physicstoday.org/Nov2021c phone +1 516 576-2268; email rights@aip.org. NOVEMBER 2021 | PHYSICS TODAY 5
pt_contents1121_Contents 10/15/2021 4:13 PM Page 6 PHYSICS TODAY Editor-in-chief Charles Day cday@aip.org Managing editor www.physicstoday.org Richard J. Fitzgerald rjf@aip.org Art and production DEPARTMENTS Donna Padian, art director Freddie A. Pagani, graphic designer Cynthia B. Cummings, photographer 8 From the editor Nathan Cromer Editors 10 Readers’ forum Ryan Dahn rdahn@aip.org Toni Feder tf@aip.org Letters Heather M. Hill hhill@aip.org Abby Hunt ahunt@aip.org 14 Search & discovery David Kramer dk@aip.org Alex Lopatka alopatka@aip.org A cryogenic circuit cools from afar • A new undersea volcano Christine Middleton cmiddleton@aip.org 10 is born east of Africa • An unusual material hosts both even and odd superconducting phases Johanna L. Miller jlm@aip.org Gayle G. Parraway ggp@aip.org R. Mark Wilson rmw@aip.org Online 22 Issues & events Paul K. Guinnessy, director pkg@aip.org Andrew Grant, editor agrant@aip.org A sprinkling of scientists prioritizes behaviors to counter Angela Dombroski atd@aip.org climate change • Idaho project tests the limits of DOE aid to Greg Stasiewicz gls@aip.org advanced reactors Assistant editor Cynthia B. Cummings 52 Books Editorial assistant The conundrums of atomic secrecy — Benjamin Wilson Tonya Gary • Unifying two fields — Nicholas B. Suntzeff • New books Contributing editor Andreas Mandelis 22 & media Sales and marketing Christina Unger Ramos, director cunger@aip.org 58 New products Unique Carter Krystal Dell Focus on lasers, imaging, microscopy, and nanoscience Skye Haynes Address 63 Obituaries American Center for Physics Isamu Akasaki • Toshihide Maskawa One Physics Ellipse College Park, MD 20740-3842 66 Quick study +1 301 209-3100 pteditors@aip.org Aerodynamic heating in hypersonic flows — Charles R. Smith PhysicsToday @physicstoday 68 Back scatter 52 Black carbon frozen in ice Member societies Acoustical Society of America American Association of Physicists in Medicine American Association of Physics Teachers The American Institute of Physics is a federation of scientific societies in the physical sciences, representing American Astronomical Society scientists, engineers, educators, and students. AIP offers authoritative information, services, and expertise in American Crystallographic Association physics education and student programs, science communication, government relations, career services, statistical American Meteorological Society research in physics employment and education, industrial outreach, and history of the physical sciences. AIP American Physical Society publishes PHYSICS TODAY and is also home to the Society of Physics Students and to the Niels Bohr Library and AVS: Science & Technology of Materials, Interfaces, Archives. AIP owns AIP Publishing, a scholarly publisher in the physical and related sciences. and Processing Board of Directors: David J. Helfand (Chair), Michael H. Moloney (CEO), Judy R. Dubno (Corporate Secretary), Susan K. Optica (formerly The Optical Society) Avery, Susan Burkett, Bruce H. Curran, Eric M. Furst, Jack G. Hehn, John Kent (Treasurer), Allison Macfarlane, Michael The Society of Rheology Morgan, Tyrone M. Porter, Efrain E. Rodriguez, Elizabeth Rogan, Nathan Sanders, James W. Taylor, Charles E. Woodward. Other member organizations Officers: Michael H. Moloney (CEO), Gigi Swartz (CFAO). Sigma Pi Sigma Physics Honor Society Society of Physics Students SUBSCRIPTION QUESTIONS? +1 800 344-6902 | +1 516 576-2270 | ptsubs@aip.org Corporate Associates 6 PHYSICS TODAY | NOVEMBER 2021
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pt_from_the_editor1121_Editors_note 10/12/2021 11:59 AM Page 8 FROM THE EDITOR Aga sagas Charles Day M artin Amis, a former bad boy of British literature, was interviewed last year by the New York Times about his reading habits. Asked which genres he enjoys and which he avoids, he replied, “I confess I have never read an Aga saga or a bodice ripper—or indeed a western (though Hitler, incidentally, read nothing else).” What, you might ask, is an Aga saga? The term was coined But all is not well in Agashire. Since Trollope wrote her first in 1992 to describe the novels of Joanna Trollope, which, Aga saga in the late 1980s, climate change has nudged up the being set amid middle-class society in the countryside of mean temperature in the UK and led to more frequent and in- southern England, could be pre- tense heat waves. AGAs run too sumed to feature a type of stored- hot for some parts of the country. heat cooker called an AGA. By hap- Indeed, without much difficulty, I penstance, my home library includes found a news story about a resi- the epitome of Aga sagas, Trollope’s dent of Aldeburgh in the east of A Village Affair (1989). Motivated to England who complained that her one-up Amis, I read the book. No AGA made her kitchen “unbear- AGAs appear within its pages, ably hot” during a 2019 heat wave. but thanks to YouTube, I spotted If the Aga saga endures, the genre’s one in the trailer for the 1995 TV name will become vestigial. adaptation. A changed climate—invariably The acronym AGA stands for a worse one—has been a setting for Aktiebolaget Svenska Gasaccumu- science fiction for decades. Notable lator (Swedish Gas Accumulator novels that feature warmer worlds Limited). The company has a con- include Octavia Butler’s Parable of nection with physics. Its chief en- the Sower (1993), Peter F. Hamil- gineer and inventor of the AGA ton’s Mindstar Rising (1993), Kim cooker, Gustaf Dalén, was awarded Stanley Robinson’s Forty Signs of the 1912 Nobel Prize in Physics “for Rain (2004), and Sarah Hall’s The his invention of automatic regula- Carhullan Army (2007). tors for use in conjunction with gas Climate change is also show- accumulators for illuminating light- ing up in literary fiction. In Iain houses and buoys.” Banks’s The Steep Approach to Gar- Dalén was inspired to invent a badale (2007), a gamekeeper on an cooker after being blinded in 1912 estate in the Scottish Highlands in an acetylene explosion. Spend- laments, “Ah, it’s all changing. We ing more time at home, he noticed can see it here. The salmon and how much work his wife, Elma, put brown trout, they’re mostly gone. into fueling and running the fam- And we don’t get the winters we ily’s stove. His solution was to cre- used to. I’ve got clothes and win- ate one that ran continuously. When ter gear I just never wear—well, introduced to the UK in 1929, the maybe a day a year or some- AGA stove became popular among the rich owners of large thing—because it’s milder all the time.” country houses. Banks himself became increasingly alarmed about climate AGAs not only serve as cookers, they also heat water. The change. In 2007 he sold his fleet of cars (BMW M5, Land Rover stove is hot enough that it warms a kitchen. In a drafty old Discovery, Porsche 911 Turbo, and Porsche Boxter S) and re- house, the kitchen is the coziest room because of the AGA. placed them with a Lexus RX 400 hybrid. PT 8 PHYSICS TODAY | NOVEMBER 2021
PT_Nov21_p9_Blank-Ad-Page.qxd 10/15/2021 3:27 PM Page 9 DEPARTMENT HEAD/PROFESSOR OF PHYSICS & ASTRONOMY Purdue University seeks a new Head of the Department of Physics & Astronomy to lead a large and dynamic faculty towards its full potential for forefront scientific research, state-of-the-art teaching, and outstanding service to the community. Unprecedented enrollment increases and substantial growth in the campus combined with the nation- ally recognized quality of life of the surrounding community provide a strong foundation for a successful candidate to achieve an ambitious strategic vision. Recent faculty initiatives provide a solid basis for growth, including a founding role in the DOE Quantum Science Center (at Oak Ridge), the preeminent Microsoft Quantum Lab Purdue for topological quantum computing, a key role in the NSF Harnessing the Data Revolution Institute (A3D3) for artificial intelligence, establishing a highly rec*gnized new group in atomic, molecular & optical (AMO) physics, and ambitious projects in astrophysics spanning multi- messenger astronomy and utilizing the upcoming Vera Rubin Observatory and James Webb Space Telescope. Internationally recognized research in biophysics, condensed matter physics, high energy physics (including dark matter searches), and high energy nuclear physics is growing through the contribution of a young faculty, with one third of the 60-member faculty having joined since 2015 as new faculty continue to be recruited. The Department of Physics & Astronomy is in the College of Science, which has spear-headed key initiatives in data & computational sciences and quantum science & engineering as well as recently making substantial investments in the geosciences, life sciences, environmental & atmospheric science, and space sciences & engineering. Qualifications: The successful candidate will have a Ph.D. in Physics, Astronomy, or related discipline, an outstand- ing record of scholarly achievement, and a history of extramurally funded research commensurate with the rank of full professor at Purdue. The candidate must have a clear vision for the future of the Department in the University, the State of Indiana, and the Nation. Requirements include exceptional leadership abilities, a commitment to excellence in education, a record of teaching achievement, an enthusiasm for engagement, and a dedication to championing diversity, equity, and inclusion. Outstanding candidates are eligible for the rank of Distinguished Professor and may relocate an existing research program to Purdue. The Dual Career Assistance Program at Purdue will assist with find- ing appointments for a faculty spouse or partner. Applications: Candidates should submit (1) a cover letter including the names of three references, (2) a complete curriculum vitae, (3) a statement of research interests and accomplishments, (4) a statement of teaching interests and accomplishments, and a (5) vision statement for the Department’s future. Purdue University is committed to advancing diversity in all areas of faculty effort, including scholarship, instruction, and engagement. Candidates should address at least one of these areas in (6) a separate Diversity and Inclusion Statement, indicating past experiences, current activities, and/or future goals to promote a climate that values diversity and inclusion. Applications should be submitted to: https://career8.successfactors.com/sfcareer/jobreqcareer?jobId=16418&company=purdueuniv Inquiries can be directed to Steve Durbin, chair of the head search committee (durbin@purdue.edu). Review of applications will begin after Jan 1, 2022 and will continue until the position is filled. A background check is required for employment at Purdue University. Purdue University is an EEO/AA employer. All individuals, including minorities, women, individuals with disabilities, and veterans are encouraged to apply.
pt_readersforum1121_Letters 10/18/2021 5:16 PM Page 10 READERS’ FORUM Rethinking the Nebra Sky Disk T he June 2020 issue of Physics Today arc with two distinct lines along its sky and to the north. i propose that it features an image of the Nebra sky length and many shorter ones radiating was intended as a representation of the disk as the illustration for a book re- from its sides. some have interpreted the aurora borealis, which would have made view by Bernie Taylor (page 53). The sky object to be a mythical boat that ferries periodic appearances in Nebra. That disk is one of the earliest depictions of the sun across the sky, with the short en- would agree with the observational na- recognizable astronomical objects and graved strokes representing the oars.2 ture of the rest of the disk. relationships. Researchers have ana- images of the disk are often oriented lyzed the disk extensively and debated so that the third arc is on the bottom, em- about when it was created and where it phasizing the possibility that the symbol 1. B. Ferreira, “a bitter archaeological feud was found. The disk had been used for represents a boat. But if the two side over an ancient vision of the cosmos,” New York Times, 19 January 2021. generations, and elements were added to pieces indeed represent the extent of sun- 2. “The Nebra sky disc (Germany),” nomi- it over the years.1 rises and sunsets throughout the year, nation form for the international Memory The 30-centimeter disk originally fea- then the disk is meant to be viewed as of the World Register (2012), https://en tured elements that appear to be stars, the though the edge represents the horizon, .unesco.org/sites/default/files/germany_ sun or a full Moon, and a crescent Moon. as with modern overhead sky charts. if nebra_sky_disc.pdf. Two golden arcs (one of which is now that is the case, the disk’s iconography Richard Mentock missing) were later added to the rim, might be interpreted differently. Cary Academy which may have changed the disk’s func- The disk could be depicting the star Cary, North Carolina tion. it has been posited that those arcs cluster nearly midway between the side 3-2-1 Contact: represent the distances the sunrise and arcs—often thought to be the Pleiades— sunset travel between solstices at the lat- in the sky to the south, as it would some- itude where the disk was purportedly times appear from the area around Nebra. found in 1999 near Nebra, Germany. added later to the disk was another The object often thought to be a sun boat then would be a fuzzy swath, low in the Scientists at the writers’ table I ngrid ockert’s article “s is for science: The making of 3-2-1 Contact” (Physics Today, January 2021, page 26) ably portrays the pioneering roles viewer re- search and innovative programming played in the landmark series. But as a former curriculum developer at the chil- dren’s Television Workshop, which pro- duced 3-2-1 Contact, i’d like to point out that the article omits mention of a less obvious way in which the show broke new ground. Rather than relying solely on outside content advisers, the children’s Televi- sion Workshop adopted the novel strat- egy of also bringing people with scien- tific expertise in-house to collaborate on the day-to-day making of 3-2-1 Contact. ANAGORIA/WIKIMEDIA COMMONS/CC BY 3.0 after the show’s maiden year, that re- sponsibility fell to the biologist Ed atkins, who went on to oversee all the science in the series. he was perhaps the first scientist invited into the intricacies of television production on this scale. he was an inexhaustible source of The Nebra Sky Disk ideas for episodes and a conduit for the many other scientists who contributed to 10 PHYSICS TODAY | NOVEMBER 2021
pt_readersforum1121_Letters 10/18/2021 3:04 PM Page 11 the show in front of the camera or behind issue of PHYSICS ToDAY (page 14). She de- A second test is related to the other the scenes. In his work with writers, an- scribes the SeaQuest experiment, which explanation Miller mentions, the pion imators, editors, and producers, Atkins found that there are about 50% more d ‾ cloud. While pions can indeed generate touched every science-related image and antiquarks than u ‾ antiquarks. The result asymmetry in the isospin of the sea, they idea that appeared on screen and essen- is surprising, since the traditional mech- will not do so for the spin, since pions tially established the role of content di- anism generating the sea was commonly have spin zero. The ’t Hooft Lagrangian, rector in science television thereafter. expected to be mediated by gluons, on the other hand, leads to strict predic- That so many in the scientific commu- which are “flavor blind” and cannot tell tions for the quark polarizations. For ex- nity today think back to 3-2-1 Contact and u ‾ from d ‾. ample, a left-handed up quark u L can smile is a wonderful testament both to Miller’s report mentions two theoret- produce only a 100% polarized d ‾ Rd L pair. the soundness of the Children’s Televi- ical ideas proposed to explain the asym- Therefore, a key to the sea’s antiquark sion Workshop’s vision of melding con- metry. one is that the presence of two u asymmetry should come from future tent with production in the development valence quarks leads to “Pauli blocking” theoretical and experimental investiga- of the series and to Atkins’s unique gifts of sea u quarks, the twin brothers of u ‾ tions that relate isospin and the spin in that arena. antiquarks. But quarks have six states asymmetry. Ralph Smallberg available: three colors × two spin orienta- (rsmallberg49@gmail.com) tions. In addition, valence and sea quarks New York City overlap little in momentum space. Pauli 1. A. E. Dorokhov, N. I. Kochelev, Phys. Lett. blocking is therefore way too small to ex- B 304, 167 (1993). 2. G. ’t Hooft, Phys. Rev. D 14, 3432 (1976). ‣ Ockert replies: Ralph Smallberg plain the data. (I’ll turn to the second 3. E. Shuryak, Phys. Rev. D 100, 114018 brings up an excellent point. While some idea—the contribution of the pion (2019). 1970s shows had science advisers, the cloud—at the end.) Edward Shuryak Children’s Television Workshop was one Unfortunately, Miller does not men- (edward.shuryak@stonybrook.edu) of the first production companies to give tion a third idea that has been put forth, Stony Brook University them a seat at the writers’ table. In 1977 which is more nontrivial and seems like- Stony Brook, New York the company launched a three-day lier to explain the puzzling asymmetry. It started with an observation by Alexan- Rare earths in space workshop in Glen Cove, New York, bringing together leading scientists and der Dorokhov and Nikolai Kochelev1 educators—including MIT physicist that the so-called ’t Hooft effective four- communications Philip Morrison—to brainstorm topics quark Lagrangian2 is “flavor nondiago- for what became 3-2-1 Contact. From nal,” leading to processes u → u(d ‾d) and d → d(u ‾u) but not to u → u(u ‾u) and I there, the Children’s Television Work- d → d(d ‾d). have enjoyed reading several items on shop formed a formal science advisory In a way, the effect is also due to the the rare-earth elements in PHYSICS committee for the show, intentionally in- Pauli exclusion principle, but at a differ- ToDAY over the past few years. David cluding scientists from Black, Hispanic, ent level. Topological tunneling events, Kramer’s most recent piece focused on the and Asian American communities. known as instantons, create fields so topic (February 2021, page 20) was about As I note in the article, the first con- strong that they fix the color and spin neodymium-based rare-earth magnets, tent director of 3-2-1 Contact was Charles states of participating quarks uniquely. but readers might be interested to learn Walcott, a biologist at the State Univer- Instead of six possibilities, there remains of another class of rare-earth magnets sity of New York at Stony Brook, who only one, thus a complete blocking. Since based on samarium. Among their appli- did a wonderful job of facilitating the the proton has two valence u quarks and cations are traveling wave tubes (TWTs), collaborations between the scientists and only one valence d quark, that mecha- which form the backbone of the world’s the production staff. Likewise, Ted Ducas, nism would suggest d ‾/ u ‾ = 2 rather than 1. entire space communications system. a physicist at Wellesley College, deserves Recently I made the first attempt to The core feature of most TWTs is a credit for his role in cowriting the show’s evaluate that effect quantitatively, by stack of samarium–cobalt (SmCo5 or excellent first season. calculating the wavefunction of the five- Sm2Co17) magnetic rings, each magne- Ingrid Ockert quark uuduu ‾ and uuddd ‾ sectors of the tized in opposition to its neighbor. one Lawrence Berkeley National Laboratory proton induced by the ’t Hooft La- design uses a 25 cm stack of 16 rings that Berkeley, California grangian.3 The results approximately are 4 cm in diameter. The tubes can am- match the data, in magnitude and mo- plify and transmit millimeter waves in Another look at the mentum dependence. How can one test that idea further? If frequency ranges of 300 MHz to 50 GHz. They have bandwidths as high as two oc- proton sea that explanation is true, the sea of Δ++ taves, power gains of 40–70 dB, and out- baryons, which have three up quarks, put powers of a few watts to megawatts. would have only d ‾ antiquarks (at corre- TWTs also exhibit excellent reliability. J ohanna Miller nicely summarizes the sponding momentum fraction x). It is Voyager 1, launched in 1977, has a SmCo current experimental situation with hardly possible to check that experimen- TWT produced by Watkins-Johnson the puzzling asymmetry of the pro- tally, but it can be tested numerically, via that is still broadcasting from more than ton's antiquark "sea" in the May 2021 lattice gauge theory. 23 billion kilometers away from Earth! NOVEMBER 2021 | PHYSICS TODAY 11
pt_readersforum1121_Letters 10/18/2021 3:04 PM Page 12 READERS’ FORUM The large communications satellites SmCo magnets have an extremely in geosynchronous orbit have around large coercive force, a measure of their 20–50 TWTs that provide many essential ability to resist demagnetization, and an services. Complete world coverage also extremely large energy product (the requires satellites in polar orbits. Fortu- maximum product of the B and H fields nately, Iridium Communications now during demagnetization), a measure of PLAN TO maintains a constellation of 66 low- their ability to do work. The maximum PARTICIPATE Earth-orbit communications satellites that are in polar orbits. The geosynchro- energy products for SmCo5 and Sm2Co17 are around 20 megagauss oersteds nous-orbit and low-Earth-orbit satellites, (160 kJ/m3) and 32 MGOe (250 kJ/m3), taken together, provide the world with respectively. They are appropriate for access to space-based communications operating at temperatures from absolute because of the discovery and develop- zero (−273 °C) to 300 °C for SmCo5 and ment of SmCo5 and Sm2Co17 magnets in to 350 °C for Sm2Co17. the late 1960s. Importantly, the magnetic field SmCo In 1966 Karl Strnat and Gary Hoffer magnets produce is parallel to the c-axis reported finding promising magnetic of their hexagonal unit cell and never properties in the yttrium–cobalt com- flips to the easy basal plane at any tem- pound YCo5. The following year, they perature. The phenomenon, known as and their colleagues reported the dis- magnetocrystalline anisotropy, gives ap- covery of a new family of cobalt-based plication designers great flexibility in permanent magnet materials.1 The re- magnet shape. searchers substituted other rare earths Neodymium-iron-boron magnets, The world’s for Y and determined that SmCo5 was the optimal choice for practical applications. discovered in 1984, have far better mag- netic properties than SmCo5 or Sm2Co17 premier lasers, Strnat and Alden Ray continued that line at ordinary temperatures. Their maxi- biomedical of study and ultimately discovered Sm2Co17, which has even more impres- mum energy product is about 55 MGOe (440 kJ/m3), and their useful temperature optics, and sive magnetic properties. That research range is between −138 °C and 150 °C. was possible only because a separation Therefore, NdFeB magnets are the only optoelectronics process developed by the Department of choice for moderate-temperature appli- event Energy’s Ames Laboratory for the Man- hattan Project made pure rare-earth ele- cations such as electric car motors or MRI devices. They have already replaced the ments available for the first time. superconducting magnets used in older SmCo5 and Sm2Co17 magnets are supe- MRIs, mitigating claustrophobia and rior to the platinum–cobalt magnets they size issues. SmCo5 and Sm2Co17 magnets, replaced in terms of magnetic properties, however, have far better magnetic prop- cost, size, and weight. At present, they re- erties than neodymium-iron-boron mag- main the only choices for many applica- nets at low temperatures and are the tions, particularly those that require very only choice for most space applications, low or very high operating tempera- such as TWTs. Thus, SmCo and NdFeB tures. Uses include gyros for space launch magnet technologies will coexist peace- 22–27 January 2022 vehicles, brushless high-torque motors fully because their application areas do for dental and medical power tools, air- not overlap. San Francisco, craft radar, and computer disk drives. California, USA 1. K. Strnat et al., J. Appl. Phys. 38, 1001 CONTACT Letters and commentary are (1967). encouraged and should be sent Melvin C. Ohmer spie.org/pw PHYSICS by email to ptletters@aip.org (using your surname as the (lemremho@aol.com) Sevierville, Tennessee #photonicswest TODAY Subject line), or by standard mail to Letters, PHYSICS TODAY, American Correction Center for Physics, One Physics Ellipse, College Park, MD 20740-3842. Please include your name, work affiliation, mailing address, email address, and daytime phone number on your letter September 2021, page 23—The story and attachments. You can also contact us online at erroneously referenced a nonexistent https://contact.physicstoday.org. We reserve the radionuclide of iridium. The correct ra- right to edit submissions. dionuclide is iridium-192. PT 12 PHYSICS TODAY | NOVEMBER 2021
PT_Nov21_p13_Blank-Ad-Page.qxd 10/18/2021 1:45 PM Page 13 INDUSTRY VIEWPOINT: COMSOL THE INSIDE VIEW FROM OUR INDUSTRY PARTNERS Multiphysics Modeling Is Quickly Becoming Standard Practice in All Engineering Simulations For all fields of engineering, simulation has been an important step in workflows from product design to their manufacture. As part of this, design engineers and modeling specialists have wrestled with the computing and solving capabilities of the day to produce more accurate and complex models. The complexity arises in part from the need to consider more details in a design’s geometry, as these are integral to a better, more compact, and optimized design. In addition, taking more details of a design’s physical behavior into consideration is usually required to increase its model’s accuracy. Subsequently, in order to accurately simulate and optimize a design, the model needs to include all or many of the physics associated with the design’s function, which includes its interaction with processes and its Phil Kinnane surrounding environment. VP of Sales, COMSOL Coupling supplementary physics to engineering problems has been difficult because of the limitations imposed by traditional software. The software may be hardwired to simulate certain types of applications; it may be based on a set of questions used to define a single- physics phenomenon, such as electromagnetic fields around an antenna; or it may focus on a predefined coupled- physics phenomenon, such as thermal stresses in structural analysis. In some cases, the numerical method that is the basis for the software is not suitable for modeling the additional physics. Therefore, many simulations rely on assumptions, the exclusion of certain behavior, or the use of empirical data in order to consider the additional physics. This is not to say that software strategies that are hardwired for such modeling are to be discounted. Much design work is adequately satisfied by the information such software provides. Yet multiphysics modeling is now opening up modeling possibilities, improving on current practices, and forging substantial inroads into the market once dominated by hardwired solutions. Two reasons account for this growing dominance. The first is that certain applications are too difficult to simulate with hardwired software, because it does not allow the coupling of any arbitrary physics to any other. Thermal runaway in batteries is a great example of this, where the design engineer needs to couple most of the behaviors of a battery, which include electrochemical reaction kinetics, electric fields, chemical deposition, ionic transfer and electrical heat production, thermal stresses, and conjugate heat transfer within cooling. COMSOL Multiphysics®, on the other hand, satisfies this need quickly and effectively by providing flexibility in coupling these physics. It even has an add-on module specific for this type of modeling. The second reason is that even in applications that were rather well served by hardwired simulation software, multiphysics modeling often provides greater accuracy and optimization as well as new knowledge about a product’s design and manufacture. For example, electric-motor simulation software has primarily modeled just the electromagnetic field within motors. However, as high-power-density motors come into greater use, induction heating and thermal and other stresses can no longer be ignored; the design as a whole must be considered. In this case, multiphysics modeling with COMSOL Multiphysics® provides flexibility and expands the usefulness of these simulations by allowing the addition of arbitrary physics to existing analyses. As the required complexity of engineering simulations continues to increase due to improvements in hardware capabilities and the numerical methods used to solve them, multiphysics modeling in product design and manufacture is quickly becoming established practice in engineering simulations. Industry ViewPoint shares the perspectives of PHYSICS TODAY’s advertising partners, who supply the content. It is written by the listed company and copyedited and designed by PHYSICS TODAY. NOVEMBER 2021 | PHYSICS TODAY 13
pt_search1121_search 10/14/2021 2:13 PM Page 14 SEARCH & DISCOVERY A cryogenic circuit cools from afar A cloud of ultracold ions can lower the temperature of a trapped proton 9 cm away. bers in Mainz work on measur- M uch of modern experimental atomic physics relies on a counterintuitive ing the proton g factor, while principle: Under the right circum- collaborators at CERN work on stances, zapping matter with a laser antiprotons. doesn’t inject energy into the system; The experiments require rather, it sucks energy out. By cooling the particles cooled to between 100 system to a fraction of a degree above ab- and 500 mK. “Warmer than solute zero, one can observe quantum ef- that, and the spin states get fects that are otherwise hidden. muddled together,” explains Laser cooling works like a charm, but Christian Smorra, leader of the only when a system’s ladder of quantum Mainz group. So far, the re- states contains a transition that the lasers searchers have achieved those can repeatedly and reliably cycle to leave temperatures by a technique the system with a bit less energy each called resistive cooling. As the time. Atoms of alkali metals and a few proton oscillates back and forth other elements are ideal. Molecules are in its trap, the moving charge much more challenging: Their vibrational induces a tiny current, called an and rotational degrees of freedom create image current, in the trap elec- a multitude of low-lying quantum states trodes. The current is allowed that can disrupt a cooling cycle. And to flow into an external circuit, fundamental particles such as protons, where its energy is dissipated, which lack internal states altogether, can’t and the proton energy steadily be laser cooled at all. decreases. Nevertheless, there’s a lot of interest The energy flow, however, in experimenting on fundamental parti- goes both ways. Thermal noise cles at low temperature. Toward that end, in the circuit creates voltage researchers from the Baryon Antibaryon fluctuations in the trap electrodes; the FIGURE 1. MATTHEW BOHMAN examines Symmetry Experiment (BASE) collabo- fluctuating electric potential jostles and the core of the BASE collaboration’s new ration have now demonstrated a method warms the proton. The circuit is cooled cooling apparatus. The central gold-colored cylinder contains two electromagnetic for using a cloud of laser-cooled ions to with liquid helium to 4 K, so it might seem Penning traps: one to hold laser-cooled cool a single proton, even when the pro- that the researchers can’t resistively cool beryllium atoms, the other to hold a single ton and ions are too far apart to directly their proton any further than that. proton. (Photo by Stefan F. Sämmer, interact.1 Figure 1 shows team member But they can—using a trick that capi- Johannes Gutenberg University Mainz.) Matthew Bohman in the lab at Johannes talizes on the definition of temperature Gutenberg University Mainz in Germany. and the fact that the trap contains only By coupling both the proton and the ions one proton. An ensemble of particles at a than its surroundings, just by connecting to an inductor–capacitor (LC) circuit, given temperature is spread among states and disconnecting the trap enough times they transport the effect of the laser cool- of different energies, according to the until the proton is caught in a low-energy ing from one location to the other. Boltzmann distribution. So a single par- state. The process doesn’t take long— ticle in a thermalized system hops among about an hour. But a full g-factor mea- Try, try again states, and at any given instant its energy surement campaign requires 1000 cold- BASE, as the full name suggests, seeks to might be higher or lower. When the BASE proton measurements, which means that compare the properties of protons with researchers abruptly disconnect their a solid month or more of experiment those of antiprotons to test how exact trap from the circuit, they lock the proton time might be spent just waiting for the the symmetry between matter and anti- into whatever state it is in at the time. particle to find its way into a cold enough matter really is. In particular, the goal That state, with a few percent chance, state. is to measure the magnetic moments, or could be low enough in energy for a g factors, of each particle by observing the g-factor measurement. Cooling from a distance spin flips of a single particle held in an It’s possible, then, to “cool” the pro- To speed things up, the BASE team electromagnetic Penning trap. Team mem- ton to a significantly lower temperature turned to an idea proposed 30 years ago 14 PHYSICS TODAY | NOVEMBER 2021
pt_search1121_search 10/18/2021 10:09 AM Page 15 by David Wineland and Daniel Heinzen: both take bites out of the circuit-noise using laser-cooled ions in one trap to bump as a sharp spike and a slightly sympathetically cool a proton in another wider dip, respectively. trap.2 The trap electrodes are wired to- The researchers use the spectrum to gether, and as before, energy is ex- verify that the resonant frequencies all changed via the induced image currents: match. They also use it to track the pro- from the proton to the trap electrodes to ton’s temperature. Typically, in experi- the ions, where it’s promptly laser cooled ments on trapped particles, it’s desirable away. for the trap potential to be as close to per- It’s essential that the laser-cooled par- fectly harmonic as possible. Then, the ticles be ions, not atoms: Only charged particles oscillate at the same frequency particles can be confined in a Penning trap no matter their energy. But here, the re- and couple to the image currents. The re- searchers deliberately made the proton searchers chose singly charged beryllium trap slightly anharmonic. As the proton ions, which have the same electronic cools, its frequency shifts. configuration as neutral lithium atoms The frequency-spectrum measure- and are thus among the most easily laser ments revealed that the proton was cooled cooled of all species. A single laser can to 2.6 K. Relative to the 100–500 mK cool a cloud of Be+ ions to 0.5 mK, so in needed for a g-factor measurement, that principle, the proton could reach a tem- number might seem unimpressive. But perature almost as low. the fact that it’s more than 80% lower The proton cooling is still slow. For than the LC circuit temperature of 15 K particles in the two traps to exchange en- is an encouraging demonstration that ergy, they need to oscillate in their traps image-current cooling is possible. at identical frequency. The oscillation fre- The LC circuit was cooled with liquid quency depends on each trap’s electric helium at 4 K; its temperature was so potential, which is hard to keep perfectly much higher than that because it was stable. The laser-cooled Be+ ions might heated by the amplifier that was used therefore be cooling the proton for only to read out the noise spectrum. Under a fraction of the time that the traps are the best of circumstances, that heating connected. is limited to a couple of degrees. But as The innovation in the new work was an amplifier ages, the heating problem to also wire in the LC circuit, as shown in worsens. figure 2a. When the circuit’s resonant fre- “It just happened that by the time we quency matches the frequency of both got everything else working, the ampli- traps, the current—and thus the rate of fier was old,” says Smorra. “That’s exper- energy exchange—is amplified by the imental physics for you.” Swapping out circuit’s quality factor Q. The BASE col- the amplifier for a new one will reduce the laboration uses high Q-factor circuits for whole system’s temperature by a factor its other experiments, and its researchers of 3—not quite low enough for a g-factor are good at making them. The Q factor of measurement. the circuit used in the proton-cooling ex- The BASE researchers expect that the periment, 15 000, is typical of their work. essential improvement could come from The drawback is that, once again, the tinkering with the trap frequencies. In the thermal noise in the circuit leaks into the proof-of-principle experiment, both traps traps and heats the particles. Still, because were tuned to the peak of the LC circuit’s the laser-cooled Be+ ions are continu- resonance. That arrangement maximizes ously cooling the proton at the same time the rate of energy exchange between the as the circuit is heating it, the system can two traps, but it also maximizes the rate settle into a steady state with the proton of heating from the circuit; detuning the much colder than the circuit. frequencies slightly would decrease both rates. Detuning too much, of course, will Resonance upon resonance negate the advantage of using the circuit To monitor the system, the researchers in the first place. But in between, there’s read out the circuit’s noise spectrum, as a range where the sympathetic-cooling shown in figure 2b. The widest bump is rate should have enough of an advan- the whole LC circuit resonance—although tage to push the proton to the desired it looks broad in the figure, it is needle- temperature. thin relative to the resonant frequency of “Once we optimize the setup, 100 mK 479 kHz. The proton and Be+ resonances certainly seems possible,” says Bohman, NOVEMBER 2021 | PHYSICS TODAY 15
pt_search1121_search 10/14/2021 2:13 PM Page 16 SEARCH & DISCOVERY a Laser-cooled Be+ ions Single proton Cryogenic LC circuit 313 nm cooling laser 5 mm 9 mm Be+ trap 9 cm Proton trap b Circuit resonance Beryllium −110 ions AMPLITUDE (dBV) −115 −120 Proton Δν −125 −100 −50 0 50 100 FREQUENCY ν − ν0 (Hz) FIGURE 2. AN INDUCTOR–CAPACITOR (LC) circuit (a) amplifies the rate of energy transfer between a pair of Penning traps 9 cm apart, so the laser-cooled beryllium ions in the first trap can sympathetically cool the proton in the second trap in just seconds. (b) The circuit’s noise spectrum contains a bump at the circuit resonant frequency ν0 = 479 kHz, with nested dips marking the Be+ and proton resonances. The proton trap is slightly anharmonic, so as the proton cools, its resonant frequency shifts. (Adapted from ref. 1.) “and even below that is maybe some- be to reverse the antiproton trap’s electric thing we can do.” potential to account for the particle’s negative charge. Beyond protons But the possibilities don’t end there. An LC circuit isn’t the only possible way Molecules of two or more atoms, when to use one set of trapped particles to cool cooled into the quantum regime, offer a another. The most straightforward ap- range of ways to test fundamental phys- proach is to put both sets of particles in ical laws (see the article by Dave DeMille, the same trap, where they can directly PhySiCS ToDAy, December 2015, page 34). exchange energy and approach a com- Molecules are challenging to laser cool, mon thermal equilibrium. Another pos- but molecular ions could lend themselves sibility other researchers are exploring is to cooling through the LC circuit. to keep the particles in separate traps but Another possible target is highly bring those traps close enough together charged ions, of interest for testing the that the particles can exchange energy theory of quantum electrodynamics (see through their Coulomb interactions. PhySiCS ToDAy, December 2012, page 22). The big advantage of the circuit- Most highly charged ions lack a conven- mediated approach, though, is its adapt- ient laser-cooling transition. But, Smorra ability. Because the particles in their re- predicts, they should be easy to cool with spective traps never come close together, the circuit-mediated method. “in fact, it it doesn’t matter if they attract or repel, would be even easier,” he says, “because chemically react, or even annihilate each the image current, and therefore the in- other. teraction strength, is enhanced by a fac- The flexibility bodes well for the BASE tor of the charge.” collaboration’s experiments of interest, Johanna Miller in which they hope to cool antiprotons just as easily as they cool protons. The antiproton setup could use the same pos- References 1. M. Bohman et al., Nature 596, 514 (2021). itively charged Be ions as in the proton 2. D. J. heinzen, D. J. Wineland, Phys. Rev. A setup; the only necessary change would 42, 2977 (1990). 16 PHYSICS TODAY | NOVEMBER 2021
pt_search1121_search 10/14/2021 4:57 PM Page 17 A new undersea volcano is born east of Africa Geophysical and oceanographic observations establish how a deep magma chamber fueled an extraordinary eruption. T he largest submarine volcanic erup- tion ever recorded began on 10 May 2018 off the eastern shore of Mayotte, one of the Comoros group of islands east of Mozambique and north of Madagas- car. Then and there, a highly viscous and ductile volume of molten rock from the asthenosphere—Earth’s upper mantle— pierced the cooler and brittler litho- sphere above it and erupted lava onto the seafloor. That day, people in Mayotte felt a magnitude 4.3 earthquake, the first of many. The largest event, of magnitude 5.9, struck several days later, on 15 May. Over the next few weeks, the moving magma generated a few very low fre- quency earthquakes in the crust and thou- sands of deeper ones.1 The result of all FIGURE 1. JÉRÉMY GOMEZ of the Paris Institute of Earth Physics (IPGP) helps retrieve that geophysical activity was a new moun- an ocean-bottom seismometer that was deployed off the eastern coast of Mayotte, an tain on the seafloor. (To learn about other island north of Madagascar. He and several other scientists participated in a May 2019 submarine volcanoes, see PhysiCs TOday, research cruise to collect geochemical, seismological, and seafloor topographic data august 2012, page 16.) after the region began experiencing volcanism and earthquakes in May 2018. (Courtesy as the chief scientist of the May 2019 of Eric Jacques, IPGP.) research cruise MayOBs 1, Nathalie Feuillet of the Paris institute of Earth Physics (iPGP) and the University of over the past 30 years geologists had cat- 2019.) By the end of 2018, the project Paris led an effort to collect seismic and aloged just two small earthquakes near was finalized, and Feuillet and some col- surface deformation data of the volcanic Mayotte, according to an earthquake leagues traveled to Mayotte in February eruption and the ongoing earthquakes. database maintained by the Us Geologi- 2019 to deploy the OBss. (Mayotte is an overseas department of cal survey. The BRGM recorded the ini- The discovery of the volcano came in France.) she and her colleagues—from tial seismic activity associated with the May 2019 when the MayOBs 1 research institutions including the French geolog- 2018 eruption using a single seismic sta- cruise recovered the OBss deployed in ical survey BRGM, the CNRs, and the tion on Mayotte. With their sparse obser- February; one of the devices is shown in French Research institute for Exploita- vations, the BRGM suspected the earth- figure 1. The researchers on the ship used tion of the sea—found that the new un- quakes originated somewhere in the a multibeam echo sounder to bounce dersea volcano now stands 820 m tall and ocean east of Mayotte but couldn’t pin- sound waves off the ocean floor across an lies at the end of a 50 km ridge formed point the exact source of the tremors. area of 8600 km2, slightly smaller than by a series of recent lava flows.2 The ge- shortly thereafter, Feuillet and other the size of Puerto Rico, to determine ological feature is likely part of a tectonic volcanologists and seismologists made the seafloor elevation. an instrument structure formed by fissures and faults plans to study the region more closely. deployed to more than 3000 m below associated with the East african Rift to among other activities, they installed the ocean surface looked for some trace the west. ocean-bottom seismometers (OBss), in- of volcanic activity by determining the struments capable of picking up under- seawater’s conductivity, temperature, and Seafloor anomaly sea earthquake activity. (For more on chemical composition as a function of The occurrence of the 2018 eruption was those devices, see “deploying seismom- depth. absolute pressure gauges attached unusual. No volcanic activity had ever eters where they’re needed most: Under- to the OBss measured the vertical defor- been reported in the area before, and water,” PhysiCs TOday online, 24 May mation of the seafloor. NOVEMBER 2021 | PHYSICS TODAY 17
pt_search1121_search 10/14/2021 2:13 PM Page 18 SEARCH & DISCOVERY “One evening we saw a big anomaly on a polar echogram of the water column,” says Feuillet, recall- ing the cruise. “It was a 2000-meter- high acoustic plume.” East of Ma- yotte, the source of the anomaly turned out to be a mixture of solid particles, liquid droplets, and bub- bles. The jet of materials had the tell- tale characteristics of volcanism: highly turbid, alkaline water and elevated concentrations of molecu- lar hydrogen, methane, and carbon dioxide. “It was one of the biggest acoustic plumes ever detected in the water column,” says Feuillet. The volcano, which had formed 10 months earlier, was erupting again. A fuller picture of the volcano and its surroundings emerged when the seafloor topography data re- vealed the Mayotte volcanic ridge. A previous research cruise, led by the French Naval Hydrographic and FIGURE 2. A NEW VOLCANO formed east of the East African Rift off the eastern shore Oceanographic Service, had fortuitously of Mayotte after lava erupted through the seafloor in mid 2018. (a) This elevation map mapped the same stretch of seafloor in from measurements collected during a 2014 oceanographic research cruise, shows a 2014. Figure 2a shows what was once relatively flat seafloor topography. (b) More recent data from a 2019 cruise and seismic the relatively flat seafloor topography; stations (black triangles in inset) reveal the formation of an undersea volcanic ridge. figure 2b, the new undersea mountain (Adapted from ref. 2; inset from ref. 3.) and ridge. Earth’s interior is rare. Many seismic As the region stretches, the litho- Seismic swarm events caused by volcanic activity occur sphere is susceptible to fracturing, which To learn more about the new volcano, in the brittler crust rather than the provides more pathways for the magma which spewed about 5 km3 of lava dur- deeper, more ductile mantle. At Mayotte, to reach the surface. Once the magma ing the 2018 eruption, coauthors Wayne the crust descends about 17 km below travels through the weakened crust and Crawford and Jean-Marie Saurel of IPGP the surface. Below that brittle–ductile reaches the seafloor, it can instigate and the University of Paris and other transition zone, molten rock more easily swarms of deep earthquakes. That inter- seismologists on the team analyzed the deforms and is therefore less likely to pretation is supported by another re- seismic-wave data collected by a net- crack and instigate tremors in response cently published paper by Océane Foix, work of seismometers on land and on the to seismic energy. Feuillet, and their colleagues. They used seafloor; most of them were installed or Still, Feuillet and her colleagues sus- a tomographic method to construct a more deployed after the 2018 eruption. pect that magma activity may have detailed picture of the new volcano’s From 25 February to 6 May 2019, the caused the deep earthquakes that were plumbing.3 network detected some 17 000 earth- observed below Mayotte. Most of them quakes, 94% of which cluster on the were clustered beneath a caldera struc- Early warning western segment of the Mayotte ridge ture, a large, low topographical region The new volcano is 50 km east of Ma- and 25–50 km below the seafloor. An ad- that formed when an ancient volcano yotte. Feuillet and her colleagues sus- ditional 84 earthquakes were identified by erupted and collapsed. The many faults pect that the main magma reservoir is IPGP and University of Paris coauthors and fissures of the caldera form channels 5–10 km east of the island and about 70 km Claudio Satriano, Angèle Laurent, and through which the magma could have below the seafloor. Another eruption from Pascal Bernard as very low frequency easily navigated from a deep upper- the reservoir, if it’s closer to the island, events lasting up to about 30 minutes, mantle reservoir to the seafloor. could be more dangerous than the last with seismic-wave energy detected below The researchers infer that the Comoros one. The next goal is to develop a warn- 0.10 Hz. The very low frequency earth- archipelago, with the African continent ing system that would alert everyone in quakes can be generated by a seismic to the west, is part of a tectonic zone the region, especially Mayotte’s 270 000 source that’s been repeatedly excited, pos- where the crust is pulling and sliding residents, of a future eruption as early as sibly faults destabilized by magma from apart. Some earthquakes could be the re- possible. the upper mantle that pressurize a large sult of the transfer of tectonic deforma- On land, GPS instruments and seis- deep reservoir. tion from the East African Rift to an area mometers are collecting real-time data. To have so many earthquakes deep in of Madagascar with rifting in the crust. But a permanent underwater observa- 18 PHYSICS TODAY | NOVEMBER 2021
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