Daily Archives: May 19, 2020

Evolution Well Services Announces Opening of Midland, Texas Location – PR Web

Posted: May 19, 2020 at 5:47 pm

Evolution's new facility in Midland, Texas

THE WOODLANDS, Texas (PRWEB) May 18, 2020

Evolution Well Services (EWS) announces the opening of a new location in Midland, Texas. The location is in close proximity to both downtown Midland and the companys growing Permian Basin field operations.

"As the rate of adoption for Evolution Well Services electric fleets continues to increase, we are investing back into our business & operations to best support our valued clients. In challenging commodity environments, the most efficient, safe, & economical operations will succeed, and EWS is continually adapting to stay ahead of this curve said Evolutions Vice President of Operations, Mike Bateman.

The newly constructed EWS location provides localized office space, maintenance bays, and warehousing to support the demanding hydraulic fracturing operations of the Permian Basin. EWS will begin ramping up operations at this facility to provide rapid response times for client support & field operational needs. The company currently provides electric hydraulic fracturing services in the Permian, Eagle Ford, Marcellus, & Utica basins, and Evolution pumped its first stage in the Permian Basin in 2016.

ABOUT EVOLUTION WELL SERVICES

Evolution Well Services is the largest provider of electric hydraulic fracturing services and the only pure-player electric fracturing service company in the industry today. We are continually committed to establishing new standards in the fracturing industry, delivering cost-effective fracturing treatments, precise execution and control with a greatly reduced onsite footprint.

Our electric fracturing fleets utilize best-in-class turbine technology enabling maximum mobility, a safer work environment, and greatly reduced emission and noise levels. Together with the affiliated Dynamis Power Solutions, their patented green technology currently conserves an estimated 33,000,000 gallons of diesel fuel annually.

For more information, visit http://www.EvolutionWS.com.

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Supply Side Platform Software Industry Market 2020-2025 industry evolution facts and figures – Cole of Duty

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The outbreak of COVID-19 has impacted several industries and aspects, such as travel bans, flight cancellations, closing of restaurants, restrictions on outdoor events, closing companies and multiple working places, malls, and public places, slow down on supply chain, growing panic among general population, instability of share market, and more. Similarly, the pandemic has impacted technology sector affecting the speed of improvements or modernizations in technology, the demand and supply of raw materials, uncertainty about future processes, and others. With respect to these factors, the report presents details on the shifting landscape across different domains including IT services, network equipment, software and hardware, and more.

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WATCH: How F1’s TV graphics have evolved over the years | Formula 1 – Formula 1

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Ever wondered how Formula 1 TV graphics of decades past would look on a modern Grand Prix? Well, wonder no more as we've managed to dress the 2019 British Grand Prix in retro TV overlays as part of F1's 70th-anniversary celebrations.

How things have changed: right down to the fuzzy, pre-race map of Silverstone to the VHS-style static, this video shows you just how last year's British Grand Prix would look if you tuned in from 1979 and watched the graphics evolve every year until now.

WATCH: The Evolution of F1's Opening Titles

There's even a cheeky screenwipe effect state-of-the-art in those days, mind and some fetching Safety Car graphics and if that's not enough, the 2019 British Grand Prix was a spectacular contest in itself.

AVAILABLE NOW: The Official Formula 1 Magazine celebrates 70 years of F1

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Hot Super-Earth Discovered Orbiting Ancient Star | Astronomy – Sci-News.com

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An international team of astronomers has discovered a close-in super-Earth exoplanet in the HD 164922 planetary system.

An artists impression of the super-Earth exoplanet HD 164922d. Image credit: Sci-News.com.

HD 164922 is a bright G9-type star located approximately 72 light-years away in the constellation of Hercules.

Also known as Gliese 9613 or LHS 3353, the star is slightly smaller and less massive than the Sun and is 9.6 billion years old.

HD 164922 is known to host two massive planets: the temperate sub-Neptune HD 164922c and the Saturn-mass planet HD 164922b in a wide orbit.

The sub-Neptune is 12.9 times more massive than Earth, and orbits the parent star once every 75.8 days at a distance of 0.35 AU (astronomical units).

The Saturn-like planet has a mass 0.3 times that of Jupiter and an orbital period of 1,201 days at a distance of 2.2 AU.

In a new study, Dr. Serena Benatti from the INAF Astronomical Observatory of Palermo and colleagues searched for additional low-mass planets in the inner region of the HD 164922 system.

The astronomers analyzed 314 spectra of the host star collected by HARPS-N (High Accuracy Radial velocity Planet Searcher for the Northern hemisphere), a spectrograph on the Telescopio Nazionale Galileo at the Roque de los Muchachos Observatory, La Palma, Canary Islands, Spain.

We monitored this target in the framework of the Global Architecture of Planetary Systems (GAPS) project focused on finding close-in low-mass companions in systems with outer giant planets, they said.

The team detected an additional inner super-Earth with a minimum mass of 4 times that of the Earth.

Named HD 164922d, the planet orbits the star once every 12.5 days at a distance of 0.1 AU.

This target will not be observed with NASAs Transiting Exoplanets Survey Satellite (TESS), at least in Cycle 2, to verify if it transits, the researchers said.

Dedicated observations with ESAs CHarachterizing ExOPlanet Satellite (CHEOPS) could be proposed, but they can be severely affected by the uncertainty on the transit time.

The teams paper will be published in the journal Astronomy & Astrophysics.

_____

S. Benatti et al. 2020. The GAPS Programme at TNG XXIII. HD 164922 d: a close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion. A&A, in press; arXiv: 2005.03368

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Why astronomy matters in times of crisis | Cosmos – Cosmos

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By Fred Watson, Astronomer-at-Large, The Australian Astronomical Observatory

In an international emergency like the present one, you might expect the science of the stars to be the last thing on peoples minds. The problems facing both individuals and governments are infinitely more pressing than events in the depths of space. People are suffering unprecedented hardships.

Yet throughout history, astronomy has shown extraordinary resilience in times of crisis and has kept public support. That resilience will be needed as a major international project, the Square Kilometre Array (SKA), is on the brink of construction.

The SKA will be the worlds largest radio telescope, and Australia will play a leading role in building and operating it. How can this benefit a nation focused on containing a global pandemic?

History shows the science of the stars is no stranger to crisis. Indeed, modern astronomy was born in a time of deep conflict, when the northern provinces of the Netherlands were engaged in difficult negotiations with Spain after 40 years of war.

In 1608, the fledgling telescope came out of obscurity in the hands of Dutch spectacle-makers, and its possibilities for astronomy were recognised. When news of this optical novelty reached Galileo Galilei in Padua the following May, he set about improving it and the rest is history.

By the turn of the twentieth century, astronomical infrastructure had become big business, but two World Wars caused major disruptions. New telescope proposals were put on hold as manufacturers turned their hands to gunsights, rangefinders, binoculars and other optical munitions.

During the Second World War, one British company actually buried the 1.5-tonne mirror for a new South African telescope in a field to avoid possible bomb damage. While delivery of the mirror was delayed until 1948, the telescope was a success, and is still at work today.

Similarly, in the United States, the 200-inch (5.1-metre) mirror for what was to be the worlds largest telescope at the time, at Mount Palomar, California, was cast in December 1934, but the instruments completion was delayed until 1949. Although it is no longer the largest in the world, the Palomar telescope remains among the most effective.

While hardly comparable to a world war, the present crisis constitutes an emergency of grave proportions, and it is important to put a project like the Square Kilometre Array (SKA) into perspective.

When completed, the telescope will provide radio astronomers with the largest and most advanced facility available to them. With an expected working lifetime of more than 50 years, it will explore the whole 13.8-billion year history of the Universe, yielding many exciting discoveries.

And spin-offs from the technologies under development have huge commercial potential, with tangible benefits for economic recovery.

One of the reasons governments fund research into the study of the Universe is that astronomy pushes technology to its limits whether it be low-noise radio receivers, complex data management systems or sophisticated computer algorithms. Wifi, for example, had its origins in Australian radio astronomy a quarter of a century ago.

More immediately, the construction of the SKA offers significant opportunities for local companies. The low-frequency component of the telescope will be built at the Murchison Radioastronomy Observatory in Western Australias remote Wajarri Yamatji country, one of the most radio-quiet places on Earth.

The project has so far spent $330 million in funding from the Australian and WA governments establishing the observatory and building pathfinder instruments.

And on the wider horizon, big science facilities like the SKA require strong international partnerships, with collaboration among the projects 14 member states representing a further positive outcome. Along with South Africa, where the mid-frequency component of the telescope will be located, Australia can expect its scientific standing to be further enhanced as one of the SKA host nations.

Although technological spin-offs are an important outcome of astronomical research, it is pure curiosity that is the ultimate driver. We are an inquisitive species, and the quest to know is what motivates researchers.

But it also inspires the rest of us with the staggering beauty of the universe and the appeal of scientific understanding. For youngsters in particular, that can prepare them for the jobs of the future, shaping an agile knowledge economy for our nation.

If the lessons of history are anything to go by, the SKA will be unlocking the secrets of the universe long after COVID-19 has subsided into memory. And that will be something of which we can all be proud.

Fred Watson, Astronomer-at-Large, Department of Industry, Science, Energy and Resources, Australian Astronomical Observatory

This article is republished from The Conversation under a Creative Commons license. Read the original article.

The Royal Institution of Australia has an education resource based on this article. You can access it here.

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The Sky This Week from May 15 to 22 – Astronomy Magazine

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Saturday, May 16The Moon passes 4 south of Neptune at 11 A.M. EDT. Two hours before sunrise, the pair are 6.5 apart and low on the eastern horizon shortly after rising. Follow them upward as the sky lightens with dawn. The Moon is just 33 percent lit and waning, while Neptune glows at magnitude 6, its disk appearing just 2" across. The nearest bright star is magnitude 4.2 Phi () Aquarii, a red-hued star that offers a glimpse of our Suns future. Currently in the red giant phase of its life, Phi is more than 260 times as luminous as the Sun and almost 39 times as wide. The star will eventually run out of nuclear fuel and its core will turn into a tiny white dwarf, lighting up what once was the stars own atmosphere as a beautiful planetary nebula.

Sunday, May 17Mercury passes 7 north of Aldebaran at 5 A.M. EDT. Because the pair trails the Sun in the sky, they wont be visible until sunset. About 20 minutes after sunset, the sky will still be bright. At that time, Mercury will hover just 9 high, with Aldebaran a mere 3 above the horizon. The two are now nearly 8 apart. Venus is roughly 9 northeast of Mercury, both brighter and higher in the sky, making it easier to spot. The two planets are drawing closer and will pass within 0.9 of each other in just a few days.

Monday, May 18The Moon reaches apogee at 3:45 A.M. EDT, when it will be 252,018 miles (405,584 km) from Earth. Rising just after 4 A.M. local time, our satellite is a smidge less than 17 percent lit and waning fast. Look for a mere sliver of a crescent in the southeast before sunrise, hanging against the brightening backdrop.

Above it in the sky is the Square of Pegasus, outlined by Alpheratz, Scheat, Markab, and Algenib. A little less than 20.5 west of Markab is the supergiant star Enif (Epsilon [] Pegasi), which represents the nose or muzzle of the flying horses figure. Coming in at roughly 150 times the diameter of our Sun, if placed in the center of our solar system, Enif would reach halfway to Venus. To the south of Enif are Alpha () and Beta () Aquarii, which are roughly as bright as Enif. The three also sit at roughly the same distance from Earth. Astronomers think the trio may have been born in the same group of stars, slowly drifting apart over the past 15 million years.

Tuesday, May 19Jupiter and Saturn rise in the southeast not long after local midnight, climbing higher in the sky as the morning hours tick by. The gas giants stand about 4.7 apart, glowing at magnitudes 2.5 and 0.5, respectively.

Once youve found the planets, draw an imaginary line between them. Halfway along that line, glance just over 1 due south to find M75 (NGC 6864), a tightly packed globular cluster considered to have the densest core of all Messiers globulars. This cluster is so dense, in fact, that it still appears starlike in binoculars, and apertures of 10 inches or larger are required to truly begin resolving the clusters stars. The 13-billion-year-old sphere of stars contains about 400,000 members and sits roughly 67,500 light-years from Earth.

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Observe edge-on and face-on galaxies | Astronomy.com – Astronomy Magazine

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Section 4

Our final section encompasses parts of Canes Venatici, Coma Berenices, and Virgo.

For a whale of a view, slide about 3.5 east-northeast of NGC 4414 to NGC 4631. Popularly known as the Whale Galaxy, this 9th-magnitude tapered monolith (oriented roughly east to west) is replete with dark vapors in a delicate embrace. Star clumps pepper the 15'-long disk like snowballs on the side of a house. For a triple treat, check out NGC 4627, a magnitude 12.5 dwarf elliptical galaxy 3' to the north, and its equally slender partner, the Hockey Stick (NGC 4656/7), a magnitude 10.5 edge-on barred spiral 30' to the southeast.

Next is a different sort of pinwheel. NGC 4725 is a peculiar one-armed spiral a transition system between a normal spiral and a barred spiral that forms one of the most complete rings of any galaxy known. To find this magnitude 9.5 gem, look 2 south and slightly west of 31 Com, which lies near the North Galactic Pole. Through a 4-inch scope, the galaxys inner region displays a bar that connects a bright, broken inner ring surrounded by a fainter lens of light.

To find our next treat, travel westward to a point 2 due east of 17 Com. There, youll find the Needle Galaxy (NGC 4565). This magnitude 9.5 wafer of light has two 8'-long threads of light extending from the galaxys slightly swollen belly like silk from a spiders abdomen. A 4-inch telescope at high power will resolve NGC 4565s classic dark lane, which cleanly divides the galaxys bright hub into two distinct ovals.

The last object is the Lost Galaxy (NGC 4535). While relatively bright (magnitude 10.5), this barred spiral is of low surface brightness, so its a challenge to small-scope observers. The 7'-long glow lies 2 northwest of 31 Vir and, in a 4-inch scope, shines as a circular patch of ill-defined light. Views through 12-inch and larger scopes bring out the spirals main, S-shaped arms within what I describe as extragalactic ectoplasm.

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Hunting The Secrets Of The Universe In Pajamas, Astronomers Go Back To Work – Hawaiipublicradio

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Hawaii Islands 12 observatories have been cleared to resume operations by state officials. With travel largely on hold, many observations will now be made from home.

Both state and county authorities in Hawaii have begun relaxing lockdown restrictions that closed many businesses statewide in March. One of the first industries granted permission to reopen by Governor David Ige was astronomy.

The pandemic was the second time in less than a year that Mauna Keas telescopes had to shut down. The first closure was during the anti-TMT protest in the summer of 2019.

Bringing the multi-million dollar telescopes back online is a lot more complicated than turning the lights on. Ivan Look, operations manager at the Canada-France-Hawaii Telescope, told HPR that the major component of regular maintenance is replenishing the coolant that keeps astronomical instruments chilled.

Theyre so sensitive that they need to be super cold in order to provide the clear images that we need, Look said.

Super-cold is not an exaggeration. Some observational tools are kept at temperatures as low as minus 400 degrees Fahrenheit. Maintaining that frigid temperature requires the use of specialized coolant that needs to be regularly replenished, sometimes daily.

If technicians cant reliably access the summit, a telescope may be placed into a safe mode to protect the instruments from damage if they warm up. Look says re-cooling them can take a long time, as in the case of one lunar observation device.

"If that instrument was to warm up, it takes 21 days for us to get all the way back down to cold, he noted.

The Canada-France-Hawaii Telescope has a system that allows some maintenance to be done remotely, minimizing the need to send technicians to the Mauna Kea summit. Look says that capability was a major factor in allowing him to get the telescope operational within 24 hours of the governors announcement, although other telescopes take longer to reboot.

There have also been costs to science. Astronomers have not been on-sky, as they say, in almost two months, according to John OMeara, the chief scientist at the W.M Keck Observatory in Hilo.

We executed zero observing since the governors lockdown, he noted.

Half of the major telescopes worldwide have been shut down, according to OMeara. Some of those projects can be rescheduled, like seasonal observations of the center of the Milky Way or hunting for planets outside our solar system.

Other celestial observations may never be made up. So-called transient events happen with little to no warning and are often impossible to predict.

A supernova goes off, and you never knowwhen its going to happen. But when it happens, you want to catch it. That type of science could have been executed, but I cant point at a specific thing, OMeara said.

He added those types of decisions are often made in real time, when an event occurs. A recent example is the sudden appearance of Omuamua, a mysterious, cigar-shaped object from interstellar space that briefly visited our solar system in 2017.

With worldwide travel largely on hold, OMeara says Keck has beefed up its remote-observing capability. Half of observations made by the Keck telescopes were already being conducted by astronomers operating from remote sites. But some of those sites are also closed as a result of the pandemic. So like many of us, astronomers are now learning how to work from home.

In some cases astronomers are observing on their laptops or computers at home. We colloquially call this pajama-mode observing, OMeara jokes.

Despite the shutdown restrictions, local observatories have been keeping busy during the lockdown. Scientists analyzed previously collected data, while summit technicians have been training on new skills and working on other projects as allowed.

One machinist with the Canada-France-Hawaii Telescope designed and fabricated almost 300 no-touch door openers, which were disturbed to hospital workers in Hilo.

But for now, Hawaiis observatories are back on sky, hunting for the secrets of the universe. Sometimes in pajamas.

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Physicists Just Built The First Working Prototype Of A ‘Quantum Radar’ – ScienceAlert

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Quantum entanglement that strange but potentially hugely useful quantum phenomenon where two particles are inextricably linked across space and time could play a major role in future radar technology.

In 2008, an engineer from MIT devised a way to use the features of entanglement to illuminate objects while using barely any photons. In certain scenarios, such technology promises to outperform conventional radar, according to its makers, particularly in noisy thermal environments.

Now, researchers have taken the idea much further, demonstrating its potential with a working prototype.

The technology might eventually find a variety of applications in security and biomedical fields: building better MRI scanners, for example, or giving doctors an alternative way of looking for particular types of cancer.

"What we have demonstrated is a proof of concept for microwave quantum radar," says quantum physicist Shabir Barzanjeh, who conducted the work at the Institute of Science and Technology Austria.

"Using entanglement generated at a few thousandths of a degree above absolute zero, we have been able to detect low reflectivity objects at room temperature."

The device works along the same principles as a normal radar, except instead of sending out radio waves to scan an area, it uses pairs of entangled photons.

Entangled particles are distinguished by having properties that correlate with one another more than you'd expect by chance. In the case of the radar, one photon from each entangled pair, described as a signal photon, is sent towards an object. The remaining photon, described as an idler, is kept in isolation, waiting for a report back.

If the signal photon reflects from an object and is caught, it can be combined with the idler to create a signature pattern of interference, setting the signal apart from other random noise.

As the signal photons reflect from an object, this actually breaks the quantum entanglement in the truest sense. This latest research verifies that even when entanglement is broken, enough information can survive to identify it as a reflected signal.

It doesn't use much power, and the radar itself is difficult to detect, which has benefits for security applications. The biggest advantage this has over conventional radar, however, is that it's less troubled by background radiation noise, which affects the sensitivity and the accuracy of standard radar hardware.

"The main message behind our research is that quantum radar or quantum microwave illumination is not only possible in theory but also in practice," says Barzanjeh.

"When benchmarked against classical low-power detectors in the same conditions we already see, at very low-signal photon numbers, that quantum-enhanced detection can be superior."

There's plenty of exciting potential here, though we shouldn't get ahead of ourselves just yet. Quantum entanglement remains an incredibly delicate process to manage, and entangling the photons initially requires a very precise and ultra-cold environment.

Barzanjeh and his colleagues are continuing their development of the quantum radar idea, yet another sign of how quantum physics is likely to transform our technologies in the near future in everything from communications to supercomputing.

"Throughout history, proof of concepts such as the one we have demonstrated here have often served as prominent milestones towards future technological advancements," says Barzanjeh.

"It will be interesting to see the future implications of this research, particularly for short-range microwave sensors."

The research has been published in Science Advances.

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Quantum Brakes to Learn About the Forces Within Molecules – SciTechDaily

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An ultrashort x-ray laser pulse (in violet) removes an inner-shell electron from the iodine atom in ethyl iodide. The experiment times the propagation of the electron with attosecond precision, and measures how much the released electron is decelerated or accelerated by intramolecular forces. Credit: Philipp Rosenberger / LMU

Physicists have measured the flight times of electrons emitted from a specific atom in a molecule upon excitation with laser light. This has enabled them to measure the influence of the molecule itself on the kinetics of emission.

Photoemission the release of electrons in response to excitation by light is one of the most fundamental processes in the microcosm. The kinetic energy of the emitted electron is characteristic for the atom concerned, and depends on the wavelength of the light employed. But how long does the process take? And does it always take the same amount of time, irrespective of whether the electron is emitted from an individual atom or from an atom that is part of a molecule? An international team of researchers led by laser physicists in the Laboratory for Attosecond Physics (LAP) at LMU Munich and the Max Planck Institute of Quantum Optics (MPQ) in Garching has now probed the influence of the molecule on photoemission time.

The theoretical description of photoemission in 1905 by Albert Einstein marked a breakthrough in quantum physics, and the details of the process are of continuing interest in the world of science and beyond. How the motions of an elementary quantum particle such as the electron are affected within a molecular environment has a significant bearing on our understanding of the process of photoemission and the forces that hold molecules together.

In close collaboration with researchers from the King Saud University (KSU) in Riyadh (Saudi Arabia), and additional international partners, the team at LAP has now determined how long it takes electrons to be photo-emitted from a specific atom within a molecule (in this case, the iodine in ethyl iodide). The measured times were in the range of tens of attoseconds. One attosecond is a billionth of a billionth of a second.

The researchers used a range of pulses in the x-ray region to excite the targeted electron. The use of machine learning helped to improve the precision of the analysis of the experimental data, and resulted in more accurate comparisons with theoretical predictions. The comparison of the experimental data with theoretical simulations finally revealed the influence of the molecule on the time that electrons need for the photoemission process, explains Professor Matthias Kling, who heads the Ultrafast Imaging and Nanophotonics group within the LAP team. The researchers found that the delay attributable to the molecular environment became larger as the energy of the light pulses and hence the initial kinetic energy imparted to the electrons was reduced.

The observations may be compared with exploring a landscape. When flying over it, many details on the ground remain unnoticed. At ground level, every single bump makes itself felt. The same is true for excited electrons. If the initial impulse is just enough to enable them to leave the molecule, the retarding effect of the forces that hold the molecule together is greater than when the kick is sufficiently energetic to eject them more promptly.

Our observations indicate that experiments tracing photoemission time permit us to learn about the forces within molecules, explains Professor Abdallah Azzeer, Head of the Laboratory for Attosecond Physics at KSU in Riyadh. These studies could improve our understanding of quantum effects in molecules and chemical reactions, adds Prof. Alexandra Landsman from Ohio State University in the US, who leads the group that conducted the majority of the theoretical work.

Reference: Probing molecular environment through photoemission delays by Shubhadeep Biswas, Benjamin Frg, Lisa Ortmann, Johannes Schtz, Wolfgang Schweinberger, Tom Zimmermann, Liangwen Pi, Denitsa Baykusheva, Hafiz A. Masood, Ioannis Liontos, Amgad M. Kamal, Nora G. Kling, Abdullah F. Alharbi, Meshaal Alharbi, Abdallah M. Azzeer, Gregor Hartmann, Hans J. Wrner, Alexandra S. Landsman and Matthias F. Kling, 11 May 2020, Nature Physics.DOI: 10.1038/s41567-020-0887-8

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Quantum Brakes to Learn About the Forces Within Molecules - SciTechDaily

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