Category Archives: Quantum Physics

Defeating Data Thieves With Quantum Physics: The Future of Secure Digital Payments – SciTechDaily

Artistic image of digital payments secured by quantum technology. Credit: Christine Schiansky

Have you ever felt the urge to input critical financial information on a not-so-familiar vendors website? Would you dare entrust your credit card details or passwords to potentially dubious entities?

Researchers from the University of Vienna have tackled this dilemma by devising an unconditionally secure system for conducting transactions in such scenarios. This solution merges contemporary cryptographic methods with the inherent properties of quantum light. The demonstration of such quantum-digital payments in a realistic environment has just been published in Nature Communications.

Digital payments have replaced physical banknotes in many aspects of our daily lives. Similar to banknotes, they should be easy to use, unique, tamper-resistant, and untraceable, but additionally withstand digital attackers and data breaches.

In todays payment ecosystem, customers sensitive data is substituted by sequences of random numbers, and the uniqueness of each transaction is secured by a classical cryptographic method or code. However, adversaries and merchants with powerful computational resources can crack these codes and recover the customers private data, and for example, make payments in their name.

A research team led by Prof. Philip Walther from the University of Vienna has shown how the quantum properties of light particles or photons can ensure unconditional security for digital payments. In an experiment, the researchers demonstrated that each transaction cannot be duplicated or diverted by malicious parties and that the users sensitive data stays private.

I am really impressed how the quantum properties of light can be used for protecting new applications such as digital payments that are relevant in our everyday life, says Tobias Guggemos.

For enabling absolutely secure digital payments, the scientists replaced classical cryptographic techniques with a quantum protocol exploiting single photons. During the course of a classical digital payment transaction, the client shares a classical code called cryptogram with his payment provider (e.g. a bank or credit card company). This cryptogram is then passed on between the customer, merchant, and payment provider. In the demonstrated quantum protocol this cryptogram is generated by having the payment provider sending particularly prepared single photons to the client.

For the payment procedure, the client measures these photons whereby the measurement settings depend on the transaction parameters. Since quantum states of light cannot be copied, the transaction can only be executed once. This, together with the fact that any deviation of the intended payment alters the measurement outcomes, which are verified by the payment provider, makes this digital payment unconditionally secure.

The researchers successfully implemented quantum-digital payments over an urban optical fiber link of 641m, connecting two university buildings in downtown Vienna. Digital payments currently operate within a few seconds. At present, our protocol takes a few minutes of quantum communication to complete a transaction. This is to guarantee security in the presence of noise and losses says Peter Schiansky, first author of the paper.

However, these time limitations are only of technological nature adds Matthieu Bozzio, who is convinced that we will witness that quantum-digital payments reach practical performance in the very near future.

Reference: Demonstration of quantum-digital payments by Peter Schiansky, Julia Kalb, Esther Sztatecsny, Marie-Christine Roehsner, Tobias Guggemos, Alessandro Trenti, Mathieu Bozzio and Philip Walther, 29 June 2023, Nature Communications.DOI: 10.1038/s41467-023-39519-w

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Defeating Data Thieves With Quantum Physics: The Future of Secure Digital Payments - SciTechDaily

Aotearoa’s first Mori quantum physicist is up and at ’em – New Zealand Herald

Dr Jacob Ngaha. Photo / Supplied

Dr Jacob Ngaha is claiming the title of the first Mori quantum physicist. His science looks at the behaviour of matter such as atoms and energy such as light, considered the building blocks of nature and Ngaha is seeking out the parallels with Te Ao Mori.

Ngaha (Waikato-Tainui, Ngti Maniapoto, Ngti Kahu) explains quantum physics like this: If we have, say, a planet going around the sun, we can calculate a lot of things and so those rules work for very big things and those rules we are comfortable with.

After a while, we realised that, actually, if you move down into a smaller world, so, instead of a planet going around the sun, were looking at an electron moving around a nucleus. Were looking inside of an atom and those same rules dont really apply and its those rules we use that are called quantum physics.

But quantum physics wasnt Ngahas first career choice and he accidentally fell into that field in his last years of high school.

I really liked maths but I wasnt very good at it, and so I found with physics, especially quantum physics, it was like doing maths but I could kind of sit back and, if we had a problem, I could think about it and I could visualise it in my head, he said.

Quantum physics is still relatively new. Its only maybe just over 100 years old since it was first really discovered and formalised, so theres still some work that needs to be done to create a link and I think one of the important things to help create that link is to get more Mori into this space.

Ngaha envisions working with Mori astronomer Professor Rangi Mtmua to develop a big bang theory reaction in the future.

I really want to get a good, firm grasp of maybe some mtauranga Mori because Im still learning that myself. I have the mtauranga ptaiao (science education), mtauranga quantum physics but want to have a wnanga (discussion) with him to see how those things can link together.

He plans to travel the world filling his kete with quantum physics knowledge to share here in Aotearoa and also complete his reo journey.

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Aotearoa's first Mori quantum physicist is up and at 'em - New Zealand Herald

Quantum Mechanics Thriller ‘The Theory of Everything’ German Trailer – First Showing

by Alex BillingtonJuly 26, 2023Source: YouTube

This looks unique. German distributor Neue Visionen Filmverleih has revealed a first look trailer for the indie film Die Theorie von Allem, which translates directly to The Theory of Everything. Yep, it's the same title as the Stephen Hawking film from 2014, and it's also about theoretical physics and scientists. But with a more mysterious, Hitchcockian twist. Set in 1962. A physics congress in the Alps. An Iranian guest. A mysterious pianist. A bizarre cloud in the sky and a booming mystery under the mountain. It's "a quantum mechanical thriller in black & white." The distributor also adds more buzz: with "Timm Krger, everything is there that makes for great cinematic art in the best Hitchcock tradition. Cast with a fantastic ensemble and interspersed with a phenomenal soundtrack, The Theory of Everything is a brilliant film noir about the contingency of our world, in which much is possible and hardly anything is necessary." Starring Jan Blow, Olivia Ross, Hanns Zischler, Gottfried Breitfuss, David Bennent, and Philippe Graber. I'm all about this! Mountains and mystery and sci-fi and theoretical ideas and much more. Will be watching.

Here's the first German trailer (+ poster) for Timm Krger's The Theory of Everything, from YouTube:

1962: Johannes Leinert travels with his doctoral advisor to a physics congress at the Hotel Esplanade in the Swiss Alps. An Iranian scientist is to give a groundbreaking lecture on quantum mechanics here. But the speaker, who is expected to deliver nothing less than a theory of everything, is late and the high society spends the interim with witty dinner parties and elegant skiing excursions. A mysterious pianist (Ross) captivates Johannes, but something's not right about her. She knows things about him she can't possibly know When one of the German physicists dies in a monstrous way, two investigators enter the scene, suspecting murder. As bizarre cloud formations appear in the sky, the pianist disappears without a trace and Johannes gets on the trail of a secret that has taken root deep beneath the mountain. (Text translated.)

The Theory of Everything, originally titled Die Theorie von Allem in German, is directed by the German cinematographer / filmmaker Timm Krger, director of the film The Council of Birds, and the doc Das leicht beunruhigende Schaukeln bei der Fahrt ins Tal, previously. The screenplay is written by Roderick Warich and Timm Krger. Produced by David Bohun and Lixi Frank. The film is premiering at the 2023 Venice Film Festival this fall playing in the Main Competition. The film is set to release in German cinemas starting October 26th, 2023 this fall. No US release is set yet - stay tuned for updates. Who's interested?

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Quantum Mechanics Thriller 'The Theory of Everything' German Trailer - First Showing

From Escaping a War to Becoming a Mom of 3 at Once, Science Has … – NIST

My team entangled the motion of two large aluminum drums. The drums are smaller than a poppy seed, but each contains more than 1 trillion atoms. They are microfabricated on sapphire chips in a clean room at NIST's campus in Boulder, Colorado.

Credit: NIST

I fled my home country of Bosnia during a civil war in 1992 when I was only a teenager. I eventually landed in California as an 18-year-old with one suitcase and settled in with a host family.

Every time I turned on the news, I saw horrifying pictures of what was going on back home. My home, my community, and everything I had known in Bosnia was gone. I lost many friends in the war.

I learned as a young adult not to get too attached to material things; they can be gone in an instant. But there were some things I knew no one could ever take from me an education and my love of science.

As I started my life over, I wanted to focus on something positive. I threw myself into science.

After fleeing Bosnia during a war in 1992, I returned in 1998 to the site of my destroyed childhood home. I learned material things can be gone in an instant, but no one could take away my education.

Credit: Courtesy of Katarina Cicak

As an undergraduate at the University of Southern California studying physics, I had lots of opportunities for on-campus work. With many graduate program labs in the area, we could pick what kind of fascinating physics we wanted to do. I worked with a professor who was measuring solar radiation using instruments on board rockets and space shuttles. It was so exciting.

In the summer of 1996, my lab mates and I drove parts of a rocket in the back of a rental truck from Los Angeles to White Sands Missile Range in New Mexico. We got pulled over for a routine check by highway patrol. It was fun to see the face of the officer who asked what we had in the back. We politely replied: A rocket.

The next summer, our instruments were on board the space shuttle Discovery, and we got to work at NASAs Goddard Space Flight Center and interact with astronauts in orbit. Here I was, a 20-something-year-old who recently survived a war, sitting at NASA telling astronauts what to do! It was mind-boggling.

This experience stirred my love of science and gave me the opportunity to focus on something that made me happy. I knew science would be in my life forever.

A few short years after arriving in the U.S., I spent a part of a summer at Goddard Space Flight Center in Greenbelt, Maryland, in 1997. I got to communicate with astronauts on the space shuttle Discovery STS-85.

Credit: Courtesy of Katarina Cicak

After physics graduate school at Cornell University, I came to NIST in 2004 during the early days of quantum computing. Quantum computing exploits powerful properties of quantum mechanics to solve problems that classical computers will never be able to do. The group I landed in was trying to build basic elements of quantum computers, quantum bits or qubits, fabricated on small chips, like the ones in todays computers and cellphones; however, they are made using superconducting materials. Qubits are extremely fragile. Learning how to keep them alive long enough to work with them was quite a challenge!

At that time, the field was in what I call the diaper days of quantum computing; the technology was about as mature as a toddler. If you compare it to the history of classical computing, it was at a stage right after the invention of a transistor.

When I first learned about quantum mechanics in school, it was unsettling. Compared to classical physics, which mostly makes sense in our everyday world, quantum theory exposes you to weird quantum behaviors.

For example, in quantum physics, entanglement means two things have no independent existence anymore. Theyre tied together inextricably, even when physically separated. You almost have to take it on faith. These strange rules are usually only relevant at the atomic scale, so it is not easy to test that quantum physics should also apply to things you can find in your house, like a ball or a marble.

Even so, quantum mechanics is one of the most tested and proven theories out there. But quantum information is so fragile that it takes a lot of effort to manipulate or sustain it in a controllable way to be useful. And yet every day, my group sees it, manipulates it, and measures it in our lab. Thats just so fascinating to me.

There are lots of technical obstacles to overcome before society can fully exploit the benefits of quantum computing. Today, quantum computing might be a school-aged child or a tween. Its certainly not fully formed yet.

But in my lab, were learning how to do all sorts of amazing things needed as precursors to scale up the technology, such as:

My team recently entangled two mechanical drums, almost large enough to be seen by a naked eye, built with a technology I developed as a postdoc at NIST. But entanglement is typically observed with much smaller objects in the microscopic realm of atoms and photons. Each of our drums contained over 1 trillion atoms.

Two drums, like the ones my team entangled, are shown here under a microscope. This experiment tested the boundaries of quantum mechanics with devices that we can build and control.

Credit: NIST

Our experiment was important in testing the boundaries of quantum mechanics with larger mechanical objects we can build and control. Physics World, a popular physics magazine, deemed it Breakthrough of the Year in 2021, and we earned a U.S. Department of Commerce Gold Medal in 2022.

I love the science and craft of building quantum things! Im a physicist, but I often call myself a quantum engineer. Its my job to innovate devices and circuits on chips for this work.

We nerds often study quantum science for selfish reasons. We just want to understand how things work; at least I do! Many of us who are passionate about quantum science can make a real change in advancing the goal of quantum computing. Already, major tech companies are using some of our knowledge and technology in their work on modern quantum processors.

A few years after I started at NIST, my husband and I wanted to start a family and started going through fertility treatments. At the time, my host familys grandson, Tristan who theyd raised and was like family to me needed a home. His grandfather passed away, and when Tristan was 14, his grandmother was no longer able to care for him due to her health. He had nowhere to go. His grandparents took me in when I had nowhere to go, so to me it only made sense to adopt him.

A few days after we brought Tristan home to Colorado, I found out I was pregnant with twins. So, my husband and I went from independent professionals focused on our careers to having three kids nearly overnight! Nothing has ever been the same for our family. We learned to change diapers at the same time we learned to parent a teen. We were living through a three-kid tornado!

My husband and I lived through a three-kid tornado! Shortly after adopting Tristan (left), we welcomed twins Nalah and Shea (right). This photo was taken in 2011, when the kids were 16 and 1.

Credit: Courtesy of Katarina Cicak

Just keeping track of the health of each kid and attending doctors appointments for everyone (98 of them in one year!) was a major challenge. When you are sleep-deprived, its hard to remember which sick twin had what symptom on what day for how long.

We also desperately needed parenting tips in trying to juggle three new kids at once. My husband (also a physicist) and I took a scientists approach to parenting. I used tables and charts to keep track of everything and keep my sanity. It helped me to test what worked and what didnt for what kid.

We also turned to networking with colleagues who were already parents to access their body of knowledge and to compare notes. Sometimes the advice was useful; sometimes it wasnt. But the scientist approach of rigorously and systematically exploring the possibilities was hugely beneficial.

Just like surviving a war, starting my life in the U.S., and working as a physicist, the early days of parenting were challenging, but they made me stronger and helped me realize what Im capable of. I always believe in turning lemons into lemonade. While those early years were grueling, I was incredibly fortunate to have supportive colleagues and find great mentors at NIST who helped me keep my career on track.

While my kids are much older now and parenting has changed, I hope I can be a source of advice and empathy for my colleagues who have young kids.

While it took patience and time for me to return to science full time, it is absolutely possible to have a rewarding career as a parent.

The science was there for me when I was ready, as it always has been.

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From Escaping a War to Becoming a Mom of 3 at Once, Science Has ... - NIST

ANSTO scientists would have preferred more about the physics but … – ANSTO

In part 1 of this two-part series, ANSTO scientists from across the organisation became film critics to review Christopher Nolans new movie, Oppenheimer, which explores the life of the director of the Manhattan Project to develop an atomic weapon.

In part 2, we explore more of the thoughts captured by ANSTOs scientists. Overall our reviewers, who took to the task with enthusiasm, were impressed with Nolan taking on a complex subject and individualdelivering a thought-provoking film but would have preferred more of a depiction of the physics involved.

Instrument scientist Dr Rachel Williamson, who undertook some postdoc work at Los Alamos National Lab (LANL) using stable isotope analysis earlier in her career said, I wasnt focused on the nitty-gritty of the science (Im a chemist, not a quantum physicist!), but I did enjoy watching a science, or rather, a scientist-centred movie with a strong emphasis on how pivotal scientific events, whether for good or bad, shape our world. The Atomic Age, which we all live in today, began with Oppenheimer and his teams successful test at Trinity Site.

I had a particular interest in seeing the movie because of the time I spent working at Los Alamos National Laboratory. Oppenheimer loomed large in the mythos of Los Alamos, along with the unfairness of his treatment after his incredible efforts in the Manhattan Project era. It was uniformly agreed that no one apart from Oppenheimer could have brought together and led that team to achieve such an outcome within the timeframe that they had.

I did enjoy the depiction of science leadership in the film, and how much depends on building the right team, such as knowing who you need to bring in and when and trying to remove any barriers in the way. Interestingly, to this day, Los Alamos National Laboratory recruits scientists from all over the world.

For me, Nolans film packed a truly emotional punch when depicting the political machinations involved in tearing Oppenheimer down and rescinding his Q clearance, effectively shutting down his career and removing his platform. I thought the film did a great job of showing the tension between politics and science (and how inconvenient we scientists can be).

A lighter moment in the film was when Oppenheimer talked about combining New Mexico and physics. New Mexico is a beautiful area filled with incredible scenery. Whilst at Los Alamos, I made the long journey down to the south of New Mexico to Trinity Site, a place with its own strange empty beauty, and I stood at ground zero.

Where a tower containing a bomb once stood, there is now a slightly underwhelming stone obelisk. It does seem odd to me that Oppenheimer chose to detonate the gadget in New Mexico, a place so dear to his heart. But he was a man of contradictions, and I think Nolans film was brilliant at conveying just how complicated and contradictory he was.

Dr Ceri Brenner, Leader of the Centre for Accelerator Science, said that she enjoyed and appreciated the snippets of science that were included in the script and the visuals to explain some of the main physics themes that are central to this story.

"They were short but sweet and got the right balance of inclusivity while maintaining flow and pace needed for a film that packed a lot in. For example, the explanations of fission and fusion, and the introduction to the paradox of light being both a particle and a wave that Oppenheimer gave to the one student who turned up for his first lectures in the US, were key to the story.

"This underlying principle of quantum physics was striking within the physics community at the time and still remains a mysterious idea for those outside that have never come across it before (which is most people who havent studied physics, maths and chemistry).

"I also enjoyed the discussion of theory vs experiment and another aspect of science that came across but not often gets airtime: that when we are doing something for the first time, its often that you get it wrong a hundred times before you get something right and make progress.

"The process of discovery and innovation is a winding road, full of dead ends and potholes, and certainly not a smooth straight line. Group discussion, such as peer review, is our process in science for challenging ideas and findings, so it was good to see this included in the storyline.

"The only thing that I would have liked to see, and would have been a key science communication opportunity, is that when the device went off, we got the flash of light and the silence, but I didnt notice anyone reacting to the immediate experience of heat that accompanied the visual of the flash.

"The energy emitted from fission is radiative and carried long distances via electromagnetic radiation, which travels at the speed of light, compared to conductive or convective heat that propagates more like the sound wave boom that arrived shortly after that travels at the speed of light. I saw a documentary where someone described it as being similar to opening an oven door and feeling the immediate bath of heat emerging. "

Dr Mitra Safavi Naeini, saw the film in Japan, where she is undertaking research relating to the anti-cancer therapy treatment NCEPT she co-developed.

The movie ends with a dialogue between Oppenheimer and Einstein, the essence of it summarised by another one of Oppenheimer's quotes from the Bhagavad Gita, "I have become death, the destroyer of worlds".

We do not get a primer on fission, quantum mechanics or particle physics. Instead, Nolan depicts the real-world experience of theoretical physicists convincingly, focusing on both their individual journeys and their collective dynamics. The film captures Oppenheimer as an intellectually curious individual, captivated by quantum mechanics and deeply engaged with various areas of science, including astrophysics, spectroscopy, and nuclear physics.

In an interesting cross-reference, Nolan has used models developed by Oppenheimer and his student, Snyder, to illustrate star collapse and the creation of a black hole, an aspect we've seen in his earlier movie Interstellar.

I was struck by how well the movie handles the influence of external events on personal trajectories. Oppenheimer, initially an academic, is thrust into a leadership role by the onset of World War II. The story doesn't shy away from depicting his humanity, showing him as a complex individual with many facets.

The film sets its drama against a background of a world in turmoil. With the rise of Nazi Germany, many renowned physicists, including Einstein and Born, were forced to flee (a few, like Heisenberg, stayed behind). These refugee scientists, exiled and concerned, played a pivotal role in alerting the world to the growing Nazi threat.

The depiction of the Kangaroo Courts, which handled the theme of suspicion and guilt by association, using the example of Oppenheimer's security hearing, was striking.

In my opinion, Oppenheimer asks an important question: Should decisions with cataclysmic potential be left to individuals with their own agenda?

"What an epic and intense movie!" commented Instrument scientist Dr Joseph Bevitt.

"In societal memory, the enormous endeavour to split the atom and control the reaction was overshadowed by the horror of subsequent weaponisation Hiroshima, Nagasaki and the Cold War. Nolan was right to focus on the events leading to the singular achievement of the Trinity demonstration on July 16, 1945.

"The film is centred around the complex psychological trauma, ethical dilemmas and political challenges experienced by theoretical physicist J. Robert Oppenheimer. 'Oppie' was the Director of the Manhattan Project, who was later castigated by political opponents.

"As a scientist who has studied the relevant mathematics and work of key scientists who participated in the Manhattan Project, I was absolutely engrossed by Oppenheimer, its characters and the suspense leading to one of the greatest collaborative feats in human history.

"To anyone who has not prepared for the film, including three of my four family members who attended with me, its abstract scientific complexity and the depiction of obsessively driven characters were thought-provoking, fascinating and terrifying. Oppenheimer demands a second watch.

"At the end of the three hours, I asked, Is that it?. I craved more. But why? The significance of the Chicago pile reactor, built under stadium seating, was glossed over. The first criticality of the X-10 reactor at Oak Ridge National Lab, the contributions of Enrico Fermi, and so much more, were omitted.

"The ramifications of the atomic bombings for humanity were suggested, but I needed closure. The formation of the Atoms for Peace program, the establishment of the International Atomic Energy Agency, and the positive real-life impacts that atomic research and neutron science have on everyday health and technological advancement followed those events.

"It is easy to be critical of the film and what it omits. Watch it for what it is: a modern-day tragedy and historical account of one of the most intense moments in human history, seen through the eyes of a brilliant and tortured mind torn between the passion for the science he loves, and the things he cannot control."

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ANSTO scientists would have preferred more about the physics but ... - ANSTO

Was Oppenheimer, the father of the atomic bomb, also the father of … – Space.com

Before becoming "the father of the atom bomb," J. Robert Oppenheimer made a significant contribution to the science of black holes.

Oppenheimer will forever, for better or for worse, be associated with the incredible destructive power of the atomic bomb and the image of the mushroom cloud, a near-Biblical symbol of destruction. That association will only strengthen in the public eye with today's (July 21) release of "Oppenheimer," Christopher Nolan's highly anticipated biopic about the physicist.

But before journeying to Los Alamos, New Mexico, in 1942 to contribute to the development of the atomic bomb, Oppenheimer was a theoretical physicist focusing on quantum physics.

In 1939, he and his University of California, Berkeley colleague Hartland S. Snyder published a pioneering paper entitled "On Continued Gravitational Contraction," which used the equations of Albert Einstein's theory of gravity, general relativity, to show how black holes could be born.

"Oppenheimer proposed the very first collapse model to describe how a star could collapse into a black hole," Xavier Calmet, a professor of physics at the University of Sussex in England, told Space.com. "This model explains the formation of black holes as a dynamical astrophysical process, the final stage of the evolution of heavy-enough stars.This model is still being used today."

Related: 'Oppenheimer' trailer reveals Cillian Murphy as Manhattan Project's genius bomb maker

Calmet said that he recently used the model himself, in a paper describing the collapse of black holes when considering quantum gravity.

"This model is very significant because it is analytically solvable solving the equations can be done with pen and paper and does not require numerical work. All the physics is thus easily trackable," he said. "Yet, despite its simplicity and maybe even crudeness, it is complex enough to describe many of the features of a collapsing star."

Ironically, as Oppenheimer and Snyder worked on the paper, which so heavily depended on the 1915 theory of general relativity, the father of that theory, Einsten, was himself completing research aimed at showing that black holes could not exist.

History would show Oppenheimer to be right about black holes, of course.

Related: Albert Einstein: His life, theories and impact on science

Eight years before Oppenheimer's theory of star collapse and black hole birth, another theoretical physicist was thinking about what happens when stars run out of fuel for nuclear fusion.

When this fuel is exhausted, a star can no longer support itself against gravitational collapse. While the star's outer layers are shed, its core rapidly contracts, leaving an exotic stellar remnant. The nature of the remnant depends on the mass of the stellar core.

Indian-American physicist Subrahmanyan Chandrasekhar realized that, for stellar cores with a mass less than 1.4 times that of the sun, gravitational collapse would halt due to quantum effects that prevent particles from "squashing" too close together.

This would come to be known as the Chandrasekhar limit, and any star below it unless it has a stellar companion feeding it material is doomed to end its existence as a smoldering stellar remnant called a white dwarf. That will be the fate of our star, the sun, after it exhausts the hydrogen at its core in around 5 billion years.

Related: When will the sun die?

For stellar cores at least 1.4 times more massive than the sun, there is enough pressure, and thus heat, generated during gravitational collapse that further bouts of nuclear fusion can be triggered, with the helium created by the fusion of hydrogen itself forging heavier elements like nitrogen, oxygen and carbon.

The most massive stars undergo a series of these collapses and bouts of nuclear fusion. But Oppenheimer and his students wanted to know where this gravitational collapse path leads and, thus, what is the final state of the universe's biggest stars.

This answer had already been delivered by a German physicist in 1916. Oppenheimer just had to find out how to get there.

In 1915, while serving on the front with the German army during the First World War, astronomer Karl Schwarzschild got his hands on a copy of Einstein's theory of general relativity. Astoundingly, and to the shock of Einstein, under these incredibly harsh conditions, Schwarzschild managed to calculate an exact mathematical solution to the field equations of general relativity.

In these solutions lurked two disturbing things places known as "singularities" where physics as we know it completely breaks down. These singularities indicated the existence of objects with gravity so intense that they could "swallow" light.

One of the singularities was deemed a coordinate singularity, which could be removed with a little clever mathematical manipulation. This coordinate singularity would come to be known as the Schwarzschild radius the point at which the gravity of a body becomes so great that the velocity needed to escape its clutches is greater than the speed of light.

This one-way light-trapping surface is called the "event horizon," and it represents the outer boundary of the black hole.

The other singularity, the true or gravitational singularity, could not be dealt with mathematically. Nothing could remove it, so it was, and still is, the point at which physics completely breaks down the heart of the black hole.

That was the theoretical birth of the black hole concept, but it didn't say anything about the creation of these cosmic titans just that they can exist.

While Einstein toiled in 1939 to destroy this gravitational singularity, and thus the concept of the black hole, Oppenheimer was delving into how such objects could come to exist.

Working with simple assumptions that neglect quantum effects and don't consider rotation, Oppenheimer set Snyder to work. And this paid off when the latter researcher discovered that what appears to happen to a collapsing star is dependent on an observer's point of view.

Snyder theorized that, at some distance from the collapsing star, light from a source close to the event horizon would have its wavelength stretched by gravity, a process called redshift, with it becoming ever more red.

At the same time, the frequency of this light is being reduced from the observer's perspective. This frequency reduction continues until, for the distant observer, the light is effectively "frozen."

Oppenheimer and collaborators realized the story is quite different for an observer unfortunate enough to be falling with the surface of the collapsing star. An observer in this position would fall beyond the event horizon without noticing anything significant about it.

Of course, in reality, an observer would be "spaghettified" by intense tidal forces caused by the difference in the gravitational pull on their upper and lower body. This would kill them before they hit the event horizon, at least for smaller black holes, in which the Schwarzschild radius is close to the gravitational singularity.

This concept was initially referred to as a "frozen star" due to the apparent freezing of light at the event horizon. It wouldn't receive its more familiar and snappier name until 1967, when Princeton University physicist John Wheeler coined the term "black hole" during a lecture.

Oppenheimer and colleagues may have taken a different path than Schwarzschild, but still, the two teams of physicists arrived at the same destination: the concept of a stellar body so massive that its gravity traps light and causes infinite redshift. Schwarzschild had the theory, but Oppenheimer and colleagues were the first scientists who truly understood the physical birth of a black hole.

Three years later, Oppenheimer would travel to Los Alamos, cementing his place in history and in the perception of the public. But many, scientists especially, remember him as the father of black holes.

"Oppenheimer made very significant contributions to black hole physics and physics as a whole," Calmet concluded. "While the general public may associate his name with the bomb and the Manhattan Project, his contributions to physics and astrophysics are well appreciated by the scientific community.

"He was one of the leading physicists during his lifetime and was extremely influential, and his seminal work is still relevant today."

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Was Oppenheimer, the father of the atomic bomb, also the father of ... - Space.com

Geometric and physical interpretation of the action principle … – Nature.com

As we want to characterize the evolution of states over time, the appropriate setting is phase space extended with the time variable12,13. That is, the space charted by position q, momentum p and time t as can be seen in Fig.1. In the same way that we write (x^i = [ x, y, z ]) for the three dimensions of space, we write

$$begin{aligned} xi ^a = [ q, p, t] end{aligned}$$

(1)

for the three dimensions of the extended phase space.

Evolutions in the extended phase space and the divergence-free displacement field.

Under the assumption that

$$begin{aligned}&the,,system ,,undergoes ,,deterministic ,,and ,,reversible \&evolution end{aligned}$$

(DR)

we can define a displacement vector field

$$begin{aligned} begin{aligned} vec {S}&= left[ frac{dq}{dt},frac{dp}{dt},frac{dt}{dt} right] \&= S^a e_a = frac{dxi ^a}{dt} e_a. end{aligned} end{aligned}$$

(2)

that describes how states move in time. [Where possible, we will be writing the same expression in both vector calculus and component notations.] In dynamical system literature, this is referred to as the vector field of the dynamical system. The time component of the displacement vector field is constrained, as we have

$$begin{aligned} S^t=frac{dt}{dt}=1. end{aligned}$$

(3)

If assumption (DR) is valid, we expect the flow of states through a closed surface to be zero: as many states flow in as flow out of the region. Alternatively, if we assign a probability, or probability density, to each trajectory, the assumption requires that probability not to change, so integrating the probability over a closed surface must yield zero. However we see it, assumption (DR) means the field is divergence-free. [Given that this is a three-dimensional space, we can use the standard tools of vector calculus.] That is,

$$begin{aligned} nabla cdot vec {S} = partial _a S^a = 0. end{aligned}$$

(4)

Since the displacement field is divergence-free, it admits a vector potential. We have

$$begin{aligned} begin{aligned} vec {theta }&= [theta _q, theta _p, theta _t] = theta _a e^a \ vec {S}&= - nabla times vec {theta } = - epsilon ^{abc} partial _b theta _c , e_a. \ end{aligned} end{aligned}$$

(5)

The minus sign is introduced to match conventions. Mathematically, this is analogous to what is done for a magnetic field or for an incompressible fluid.

Because the displacement field must satisfy (3), without loss of generality we can set

$$begin{aligned} begin{aligned} vec {theta }&= [p, 0, -H(q,p,t)] \&= p e^q - H(q,p,t) e^t, end{aligned} end{aligned}$$

(6)

where H is a suitable function of q, p and t. The potential (vec {theta }) is closely related to the canonical one-form of symplectic geometry and the contact form of contact geometry. By applying definition (2) and expanding (5) with (6), we have

$$begin{aligned} left[ frac{dq}{dt},frac{dp}{dt},frac{dt}{dt} right] = - nabla times vec {theta } = left[ frac{partial H}{partial p},-frac{partial H}{partial q}, 1 right] , end{aligned}$$

(7)

which yields Hamiltons equations. Note that the argument works in reverse: any Hamiltonian system with one degree of freedom yields a divergence-free displacement field, and therefore satisfies (DR).

As shown in (a), the variation of the action is the flow of the displacement field (vec {S}) through the surface (Sigma) that sits between the path (gamma) and its variation (gamma '). In (b) we see that the flow is zero if the path is an actual evolution of the system, since the displacement field will be parallel to the path (gamma) and therefore tangent to the surface (Sigma).

We now turn to constructing the principle of stationary action. As illustrated in Fig.2a, take a path (gamma) with endpoints A and B, not necessarily a solution of the equations of motion. Then take a variation (gamma ') of that path and identify a surface (Sigma) between them. We can ask: what is the flow of the displacement field (vec {S}) through (Sigma)? Because (vec {S}) is divergence-free, the flow through (Sigma) will depend only on the contour, therefore the question is well posed. Using Stokes theorem, we find

$$begin{aligned} begin{aligned} - iint _{Sigma } vec {S} cdot dvec {Sigma }&= iint _{Sigma } left( nabla times vec {theta } right) cdot dvec {Sigma } \&= oint _{partial Sigma = gamma cup gamma '} vec {theta } cdot dvec {gamma } \&= int _{gamma } vec {theta } cdot dvec {gamma } - int _{gamma '} vec {theta } cdot dvec {gamma }' \&= delta int _{gamma } vec {theta } cdot dvec {gamma }. end{aligned} end{aligned}$$

(8)

Now suppose (gamma) is a solution of the equation of motion, as in Fig.2b. Then (gamma) is a field line and the flow is tangent to (Sigma) no matter what (gamma ') we picked. The converse is true: if we look for those paths for which the flow through (Sigma) is zero no matter what (gamma '), (gamma) must be everywhere tangent to (vec {S}) so we find a solution to the equation of motion. The solutions, then, are those paths and only those paths for which

$$begin{aligned} 0 =delta int _{gamma } vec {theta } cdot dvec {gamma } = - iint _{Sigma } vec {S} cdot dvec {Sigma } end{aligned}$$

(9)

We call this the principle of stationary action in Hamiltonian form.

The last step is to express the principle exclusively in terms of kinematic variables: position, time and velocity. This can be done if we assume that

$$begin{aligned} the,, kinematics ,,of ,,the ,,system ,,is ,,enough ,,to ,,reconstruct ,,its ,,dynamics. end{aligned}$$

(KE)

This means that by looking at just the trajectory in space q(t), we are able to reconstruct the state at each moment in time. Therefore we must be able to write (p=p(q,dot{q})), and therefore we can also write

$$begin{aligned} begin{aligned} delta int _{gamma } vec {theta } cdot dvec {gamma }&= delta int ^{t_2}_{t_1} vec {theta } cdot frac{dvec {gamma }}{dt} dt \&= delta int ^{t_2}_{t_1} left( p frac{dq}{dt} - H right) dt \&= delta int ^{t_2}_{t_1}L(q, dot{q}, t) dt = 0. end{aligned} end{aligned}$$

(10)

We find that a system for which (DR) and (KE) are valid can be characterized in terms of the principle of stationary action with a suitable Lagrangian. The converse is also true: if the principle of stationary action allows for a unique solution, then the conjugate momentum and the Hamiltonian are well defined and the system satisfies both (DR) and (KE).

We have thus demystified the principle of stationary action, and turned it into a geometric property: requiring the principle of stationary action is equivalent to requiring that the solutions are the field lines of a divergence-free field in phase space. We also have a clear physical meaning: the principle of stationary action is equivalent to assuming determinism/reversibility (DR) and kinematic equivalence (KE). However, we do feel that the principle expresses these requirements in a very roundabout way.

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Geometric and physical interpretation of the action principle ... - Nature.com

A new type of quantum bit in semiconductor nanostructures – Science Daily

Researchers have created a quantum superposition state in a semiconductor nanostructure that might serve as a basis for quantum computing. The trick: two optical laser pulses that act as a single terahertz laser pulse.

A German-Chinese research team has successfully created a quantum bit in a semiconductor nanostructure. Using a special energy transition, the researchers created a superposition state in a quantum dot -- a tiny area of the semiconductor -- in which an electron hole simultaneously possessed two different energy levels. Such superposition states are fundamental for quantum computing. However, excitation of the state would require a large-scale free-electron laser that can emit light in the terahertz range. Additionally, this wavelength is too long to focus the beam on the tiny quantum dot. The German-Chinese team has now achieved the excitation with two finely tuned short-wavelength optical laser pulses.

The team headed by Feng Liu from Zhejiang University in Hangzhou, together with a group led by Dr. Arne Ludwig from Ruhr University Bochum and other researchers from China and the UK, report their findings in the journal "Nature Nanotechnology," published online on 24 July 2023.

Lasers trigger the radiative Auger process

The team made use of the so-called radiative Auger transition. In this process, an electron recombines with a hole, releasing its energy partly in the form of a single photon and partly by transferring the energy to another electron. The same process can also be observed with electron holes -- in other words, missing electrons. In 2021, a research team succeeded for the first time in specifically stimulating the radiative Auger transition in a semiconductor.

In the current project, the researchers showed that the radiative Auger process can be coherently driven: they used two different laser beams with intensities in a specific ratio to each other. With the first laser, they excited an electron-hole pair in the quantum dot to create a quasiparticle consisting of two holes and an electron. With a second laser, they triggered the radiative Auger process to elevate one hole to a series of higher energy states.

Two states simultaneously

The team used finely tuned laser pulses to create a superposition between the hole ground state and the higher energy state. The hole thus existed in both states simultaneously. Such superpositions are the basis for quantum bits, which, unlike conventional bits, exist not only in the states "0" and "1," but also in superpositions of both.

Hans-Georg Babin produced the high-purity semiconductor samples for the experiment at Ruhr University Bochum under the supervision of Dr. Arne Ludwig at the Chair for Applied Solid State Physics headed by Professor Andreas Wieck. In the process, the researchers increased the ensemble homogeneity of the quantum dots and ensured the high purity of the structures produced. These measures facilitated the performance of the experiments by the Chinese partners working with Jun-Yong Yan and Feng Liu.

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A new type of quantum bit in semiconductor nanostructures - Science Daily

Life in a Foreign University | How pursuing PhD at ISTA in Austria benefitted this IIT-Kanpur student – The Indian Express

(Thisletter is part of a seriesby The Indian Express where we bring to you the experiences of students at different foreign universities. From scholarships and loans to food and cultural experiences students tell us how life is different in those countries and things they are learning other than academics)

Similar to most students, I was also applying to the US for higher studies after completing my degree programme in India. I graduated from the Indian Institute of Technology, Kanpur with a dual degree (MS + BS) in Physics and was looking for options for pursuing a PhD. It was then that someone suggested that Anton Zeilinger, a well-known physicist and now a Nobel laureate, has a group at the University of Vienna and I should consider applying in Austria.

I researched some more about the university and decided to take admission to the Institute of Science and Technology Austria (ISTA) after much deliberation. I did not apply to the University of Vienna as at times you dont get to work with such renowned physicists directly. Instead, its their students with whom you have to work. Anton Zeilinger was part of a group called CoQuS Complex Quantum Systems and ISTA and the University of Vienna were a part of it.

CoQus was an initiative of the Austrian government for research on quantum physics. Initially, it was more exclusive with only a few professors but now it has transformed into VCQ Vienna Centre for Quantum Sciences. VCQ is a bigger collaboration of many research groups from University of Vienna, Technical University of Vienna and ISTA. It promotes sharing and discussion of ideas, viewpoints by organising summer schools, colloquiums and conferences.

I was also drawn towards ISTA as Johannes Fink was a part of the programme. I was following Mr Fink and his work in the field of quantum optics and quantum computing.

My application process for ISTA

After sending in my application, I emailed Johannes Fink explaining my interest in the field of quantum physics, especially in the topics he was researching. After reading my email, Mr Fink conducted a Skype interview with me. Thankfully, he liked me and said that he will make sure that my application gets through.

The application process is quite standard. I had to submit my transcripts, rsum, letters of recommendation, and statement of purpose. Once that is done, ISTA calls you for an interview. They select a bunch of 100 to 150 students for interviews from all the applications received. Its a three day event which is hosted by ISTA where they take care of flight tickets to hotel bookings.

They organise everything, show you around the campus, around the town, you can talk to the students present on the campus, talk to the professors and experience everything by yourself. For me particularly, it showed how rich the institute is which ensures that your funding will be secured and research will be well-funded.

Once you are selected, you get a letter of invitation which has to be shown at the embassy so that you can get a visa.

Other than ISTA, I had offers from the University of Rochester, USA and Heriot-Watt University, Scotland. I did not choose the US because I felt the university wasnt that great and for the other university I was a bit uncertain about the funding.

ISTA literally holds your hand

After I decided to join ISTA and accepted their offer, they sent me the logistics details. Over here, they really take care of you. In fact, for the first year, they literally hand-held us. For those in the first years, the accommodation is provided on the campus and it is fully furnished so all you have to do is take the key.For the on-campus accommodation, the international students are given a priority over local students from Austria or neighboring countries.

Once youre in your second year, they ask you to find your accommodation the reason being that the apartments have to be emptied out for the next batch of students. After one year, we developed basic communication skills in German to communicate with the locals and find a place for ourselves. During the initial years, my work was more experimental, so I used to live near the campus. Once it became more theoretical, I shifted to the city of Vienna.

One unique aspect of ISTA is that it is a mix of US and European systems, i.e., when you apply for a PhD you dont need a masters degree.

My life in Austria

I came to Austria in September 2018 and have been living here since then. I completed my PhD in June this year (2023) and currently, I am a post Doctoral student at the institute. My research topic is quantum communication. ISTA allows you to be a post Doctoral student for one year after completing your PhD. In this, you get an increment in your salary and a different contract.

The research is well-funded. Unlike in India where you have to go through a whole process for getting lab equipment, here you can ask for it and you will get it. Even the stipend provided by ISTA is good enough for one person to sustain themselves, enjoy their lives and save money as well.

Vienna is very beautiful and my life here is always bustling with activity. The decision to come here has been one of the best decisions so far. Over the years, I have made a lot of friends here. There is something new to do every evening be it playing volleyball, dancing or indulging in fitness activities. I keep myself free every weekend as my friends and I are always up for some random activity. Last weekend, we went cycling, after that we plucked apricots and later in the day I baked an apricot cake for everyone.

I really enjoy my life here and I would hate to move out of Vienna. There are a lot of Physics related jobs, work-life balance and a good standard of living. Over here, there is great social security, medical and other expenses are covered by the government. Its one of the most livable places in the world and with time I have learned the language as well. There is no reason for me to move out of here. I will soon be applying for permanent residency. In some ways, I am more European than Indian now.

I have travelled a lot across Europe Italy, Switzerland, Serbia, Hungary, Slovenia, Czechia, Denmark and outside Europe, I have been to the US and China. I last visited India in December 2022.

Biggest learning from my experience so far

If you have a choice between solving a problem yourself and getting help from an expert, swallow your pride and get help. Its the most efficient way. Use the saved time elsewhere. Instead of researching a topic, I just find someone with whom I can talk and get a much better idea about what to do in 10-15 mins. It saves a lot of time and prevents me from going down the wrong rabbit hole. And its not limited to research, I use it everywhere, for example, when hunting for a job.

When you are applying for higher studies abroad, its a lot more about probability than you think. Have an open mind, apply to a lot of places and try to reach a person instead of a website portal. It will be a lot more helpful. Once you are in a different place, try to adapt to their culture and be more accepting towards people.

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Life in a Foreign University | How pursuing PhD at ISTA in Austria benefitted this IIT-Kanpur student - The Indian Express

The Interplay between Semiconductors and Quantum Mechanics – EnergyPortal.eu

Exploring the Intricate Interplay between Semiconductors and Quantum Mechanics

The fascinating world of semiconductors is one that is deeply intertwined with the principles of quantum mechanics. This intricate interplay has been the cornerstone of technological advancements in the 21st century, propelling innovations in various fields such as computing, telecommunications, and energy.

Semiconductors, materials that have a conductivity level somewhere between that of conductors and insulators, are the backbone of modern electronics. They are the heart of our computers, smartphones, and many other devices that we use daily. The unique properties of semiconductors, such as their ability to control electrical current, are derived from the principles of quantum mechanics.

Quantum mechanics, a branch of physics that deals with phenomena on a very small scale, such as atoms and subatomic particles, provides the theoretical framework that explains the behavior of semiconductors. In the quantum realm, particles can exist in multiple states at once, a phenomenon known as superposition. Additionally, particles can also be entangled, meaning the state of one particle can instantaneously affect the state of another, regardless of the distance between them.

These quantum phenomena are harnessed in semiconductors through the manipulation of electrons, the subatomic particles that carry electric charge. In a semiconductor, the energy levels that electrons can occupy are grouped into bands. The lower energy band is called the valence band, and the higher energy band is called the conduction band. The gap between these two bands, known as the bandgap, is a crucial property of a semiconductor.

By applying energy to a semiconductor, electrons can be excited from the valence band to the conduction band, leaving behind a hole in the valence band. The movement of these electrons and holes under an electric field constitutes an electric current. The size of the bandgap determines the amount of energy required to move an electron from the valence band to the conduction band, which in turn determines the electrical properties of the semiconductor.

Moreover, quantum mechanics also allows for the creation of quantum wells in semiconductors. A quantum well is a potential well with discrete energy levels. This is achieved by sandwiching a layer of a semiconductor with a small bandgap between two layers of a semiconductor with a larger bandgap. The discrete energy levels in the quantum well lead to a variety of useful properties, such as the emission of light at specific wavelengths, which is utilized in devices like lasers and light-emitting diodes (LEDs).

The interplay between semiconductors and quantum mechanics is not just theoretical; it has practical implications that are shaping our future. For instance, the principles of quantum mechanics are being used to develop quantum computers, which promise to solve complex problems much more efficiently than classical computers. Semiconductors play a crucial role in these quantum computers, as they are used to create qubits, the quantum equivalent of bits in classical computers.

In conclusion, the interplay between semiconductors and quantum mechanics is a fascinating field that is driving technological advancements. By harnessing the principles of quantum mechanics, semiconductors are enabling the development of devices and technologies that are transforming our world. As our understanding of quantum mechanics continues to deepen, we can expect to see even more exciting developments in the realm of semiconductors.

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The Interplay between Semiconductors and Quantum Mechanics - EnergyPortal.eu