Page 705«..1020..704705706707..710720..»

A Six Year Search for Purely Theoretical Axions is Going Deep … – The Debrief

Physicists embarking on a hunt for proof of theoretical particles known as axions are preparing to go into a deep underground laboratory for the next six years.

Part of the DarkQuantum effort, which recently received a 12.9 million grant from the European Research Council to conduct the search, the research team hopes to find evidence that dark matter is actually made up of previously undetectable axions.

If successful, the discovery would solve the longstanding mystery around dark matter and dark energy that has haunted physicists for decades, an accomplishment the researchers involved believe could rival the discovery of the elusive Higgs boson in 2010.

Deep under the mountains spanning the border between Spain and France, the Canfranc Underground Laboratory is the perfect place to search for axions. Thats because the natural rock layers above the lab help protect the ultra-sensitive equipment the team will employ to hunt for the elusive particle from cosmic radiation and other forms of electromagnetic interference.

Previous efforts to find axions have explicitly failed because of the difficulty separating the signal from the noise. In fact, the equipment and methods used by previous research teams have often been the cause of such noise, something The Debrief previously reported on, making the actual sensors and equipment just as important as the deep underground laboratory itself. For the researchers from Aalto University and the University of Zaragosa who will undertake the hunt, a well-shielded location is critical for their new sensors to work.

Our high-frequency sensor will be 10-100 times more sensitive than previous iterations, and it will be able to scan on the scale of a few microelectron volts, explained Sorin Paraoanu, Aalto University Senior Lecturer, Docent, and the team leader on the research effort. Paranou also says that their specially designed sensor will take advantage of brand new techniques in quantum physics by using superconducting qubits, which are the same qubits used in quantum computers.

However, the researcher says their superconducting qubits will serve in a different role as detectors on this sensor, called a haloscope, allowing the team to probe the depths of the galactic halo for signs of axions.

The theory suggests that, in an ultra-cold environment, we can introduce a magnetic field that will cause any axions present to decay into photons, the professor explains. If we detect any photons in the cavity, then we can conclude that axions are present in the system and that they do indeed exist.

While many possible explanations have been proposed for what makes up dark matter, something physicists know exists because of its gravitational effects but have never been able to observe directly, none have yet been proven. Nonetheless, the researchers on the team think that if dark matter is indeed made up of these theoretical axions, their ultra-sensitive equipment, novel quantum methodology, and the remote location of their deep underground laboratory should be just enough to find them.

The nature of dark matter is one of the biggest mysteries in modern science, explains University of Zaragoza Professor Igor Garcia Irastorza, who heads the DarkQuantum consortium. If dark matter is made of axions, we have a real chance of detecting it with this project.

The team says the six-year hunt will be divided into two distinct phases. The first four years, or the scaling up phase, will include building, fine-tuning, and ultimately transporting the haloscopes to the underground lab. The final two years, the experimental phase, will involve using the sensors to gather data.

We are peering into a deep, dark pit, said Paraoanu of the potential significance of their work. If it exists, the axion goes beyond the standard model of elementary particles,

Such an observation would be comparable in significance to the Higgs boson discovery in the early 2010s, the researcher adds. But at least with the Higgs boson, they knew where to start looking!

Christopher Plain is a Science Fiction and Fantasy novelist and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him directly at christopher@thedebrief.org.

Read the rest here:

A Six Year Search for Purely Theoretical Axions is Going Deep ... - The Debrief

Read More..

Matthew Perry reflected on Julia Roberts romance, ‘flirty faxes’ before death: ‘I was not enough’ – New York Post

Celebrities

By Stephanie Webber

Published Nov. 3, 2023, 11:30 a.m. ET

Matthew Perry was on cloud nine when his romance with Julia Roberts kicked off in the mid-90s and it all began via fax.

Somewhere in the world, there is a stack of faxes about two feet long a two-foot-long courtship, filled with poems and flights of fancy and two huge stars falling for each other and connecting in a beautiful, romantic way, Perry recalled in his 2022 memoir, Friends, Lovers, and the Big Terrible Thing.

Perry reflected on their relationship nearly one year before his tragic death at age 54 on Saturday. In his autobiography, he revealed that the two initially met when Friends co-creator Marta Kauffman urged him to woo her because the actress was interested in appearing on the NBC sitcom.

Turned out Julia had been offered the post-Super Bowl episode in my season two and she would only do the show if she could be in my storyline, he wrote.

I thought long and hard about what to say on the card. I wanted it to sound professional, star to star. (Well, star to much bigger star.) But I wanted something a tad flirty in there, too, to match what she had said, he went on. Im still proud of what I settled on.

He added: I sent her three dozen red roses and the card read: The only thing more exciting than the prospect of you doing the show is that I finally have an excuse to send you flowers.

Her reaction, however, was a bit puzzling.

Her reply was that if I adequately explained quantum physics to her, shed agree to be on the show. Wow. First of all, Im in an exchange with the woman for whom lipstick was invented, and now I have to hit the books, he gushed.

After he completed the task sprinkled in with some metaphorical notes the Oscar winner accepted the invitation.

Not only did Julia agree to do the show, but she also sent me a gift: bagels lots and lots of bagels. Sure, why not? It was Julia f king Roberts, Perry noted. At the time, I was walking on air. I was the center of it all and nothing could touch me. The white-hot flame was mine I kept passing my hand through it, but it didnt burn yet; it was the inert center.

The budding romance began with a three-month-long courtship by daily faxes, which turned romantic. Then they would move on to phone calls that lasted for more than five hours.

It wasnt uncommon for me to read these faxes three, four, sometimes five times, grinning at that paper like some kind of moron. It was like she was placed on this planet to make the world smile, and now, in particular, me. I was grinning like some fifteen-year-old on his first date, Perry wrote in his memoir. It was clear we were in deep smit.

Then on a Thursday, Roberts called and said shed be at his house that Saturday.

How did she even know where I lived? he asked himself. Sure enough, at 2 p.m. that Saturday, there was a knock on my door. Deep breaths, Matty. When I opened it, there she was, there was a smiling Julia Roberts on the other side.

Perry said that he felt like the king of the world alongside the My Best Friends Wedding star. However, his personal battles with drug and alcohol addiction held him back from continuing their relationship.

Dating Julia Roberts had been too much for me, he admitted. I had been constantly certain that she was going to break up with me. Why would she not? I was not enough; I could never be enough; I was broken, bent, unlovable. So instead of facing the inevitable agony of losing her, I broke up with the beautiful and brilliant Julia Roberts.

Perry, who died on Roberts 56th birthday, later gushed about watching his ex win the Academy Award for Erin Brockovich in 2001.

I was incredibly happy for her, he wrote. As for me, I was just grateful to have made it one more day.

Load more...

https://nypost.com/2023/11/03/entertainment/matthew-perry-was-not-enough-for-ex-julia-roberts-before-death/?utm_source=url_sitebuttons&utm_medium=site%20buttons&utm_campaign=site%20buttons

View original post here:

Matthew Perry reflected on Julia Roberts romance, 'flirty faxes' before death: 'I was not enough' - New York Post

Read More..

Dr. Brown: Tracking electrons: The Nobel Prize in physics – Niagara Now

In 2018, Canadian physicist Donna Strickland received the Nobel Prize for physics, alongside French scientist Grard Mourou, her doctoral supervisor.

Her contribution was related to successfully increasing the power of brief pulses of laser light without destroying the laser in the process.

To do so, she stretched the wavelength of the laser beam and increased its amplitude (energy) before shortening the beam to its original wavelength.

In a sentence, it all sounds so easy, but as with most scientific and engineering ventures, the devil was in getting the details right.

Almost a hundred years earlier, Werner Heisenberg was awarded a Nobel for his uncertainty principle as a fundamental property in quantum mechanics.

He showed it was impossible to determine both the position and momentum of an electron at the same time because the energy of any illuminating beam designed to determine those properties would destroy the electron.

Since 1927, Heisenbergs uncertainty principle has been widely accepted as one of the core properties of quantum mechanics.

His theorem was at the heart of last years Nobel in physics. It was awarded to John Clauser, Alain Aspect and Anton Zeilinger for their work that proved entangled particles, such as electrons, remain entangled, whatever the distance between them.

This marked the triumph of quantum mechanics over Albert Einsteins challenge to this field of study: more than five decades prior, Einstein made his strongest claim that uncertainty and other weird properties of quantum mechanics made no sense, even if the practical applications of quantum mechanics worked brilliantly.

This years Nobel might well challenge Heisenbergs uncertainty principle, for if single electrons can be tracked in atoms and molecules, what was uncertain might prove to be certain.

But thats not why this years laureates launched their studies.

Their goal was to develop illuminating beams with wavelengths short enough to identify and understand the behaviour of electrons, and hence the bonding properties, which bind atoms together to form molecules.

Until their studies, that goal seemed impossible.

The 2023 Nobel in physics was awarded to Anne LHuillier, Pierre Agostini and Ferenc Krausz for creating ultra-short wavelength light beams, brief enough to illuminate electrons in atoms and molecules.

Success came first with LHuilliers discovery in 1983 that an infrared laser light illuminating a noble gas, excited electrons in the gas, generating short wavelengths, which corresponded to harmonic frequencies of the laser lights fundamental frequency.

The trick was to combine those harmonic frequencies in such a way that wavelengths as short as several hundred attoseconds in length were created short enough to study electrons.

That goal was reached independently by Pierre Agostini and Ferenc Krausz, with similar results.

(One attosecond is a millionth of a trillionth of a second in duration the number of them in one second is the same as the number of seconds since the universe began staggering and numbing numbers.)

Summing up the reasons for this prize, the Nobel committee stated that LHuillier, Agostini and Krausz demonstrated a way to create extremely short pulses of light that can be used to measure the rapid processes in which electrons move or change energy.

LHuillier discovered a new effect from laser lights interaction with atoms in a gas. Agostini and Krausz demonstrated that this effect can be used to create shorter pulses of light than previously were thought possible, the committee concluded.

The committee was less forthcoming about what practical results might come from these discoveries, except to measure the tightness of bonds in molecules.

Beyond the official comments on the achievements of the laureates is the potential to study, what for almost a century, was considered uncertain by Heisenberg.

That, for me, is the big but unstated story with this prize.

Will frame-by-frame resolution at the subatomic level ever reach a level at which two or more properties of electrons can be studied?

If that happens in the future and the tools are getting better and better perhaps what was uncertain may become certain with much better tools for observing electrons in real-time.

The seventh annual review of the Nobel Prizes began Nov. 1 with the physics prize. Chemistry, medicine, economics, peace and literature will follow.

Sign up with Debbie Krause (dkrause@notlpl.org) at the Niagara-on-the-Lake Public Library.

Dr. William Brown is a professor of neurology at McMaster University and co-founder of the InfoHealth series at the Niagara-on-the-Lake Public Library.

See original here:

Dr. Brown: Tracking electrons: The Nobel Prize in physics - Niagara Now

Read More..

Laurier researcher Shohini Ghose documents the untold legacies of … – Wilfrid Laurier University

When Shohini Ghose was growing up, the only woman in science she knew of was Uhura, the fictional communications officer on Star Trek. Only as an adult did she learn that a woman from her home region of Bengal, India, Bibha Chowdhuri, had made massive contributions to modern physics.

Bibha was involved in discovering two fundamental particles in nature, the neutrino and the pion, says Ghose, a professor of Physics and Computer Science at Wilfrid Laurier University. Shes Bengali, Im Bengali, and yet I never heard her name. We didnt celebrate those stories.

Ghose is hoping to change that with the release of her new book, Her Space, Her Time: How Trailblazing Women Scientists Decoded the Hidden Universe. It chronicles the inspiring stories of women physicists and astronomers, like Chowdhuri, who made indelible scientific contributions, yet have remained unsung in history.

Ghose, founder of the Laurier Centre for Women in Science and a Natural Sciences and Engineering Council of Canada Chair for Women in Science and Engineering, shares the inspiration for her research and why she hopes readers of her new book are left feeling hope, inspiration and outrage.

Science is my inspiration. The universe is full of wonder and excitement, and I feel the same feelings when I read about these women who followed their goals and passions no matter what challenges they faced. In physics and astronomy classrooms, I didnt have many other women or people from my own background to turn to. It could be quite lonely and I felt like I didnt belong, to the point that I almost quit. With this book, I want to change the idea that women are not part of the scientific story. Its empowering to feel connected to women of that caliber.

When I began teaching astronomy many years ago, I wanted to incorporate human stories into my lectures that the students could connect to. It grew from there. At the Laurier Centre for Women in Science, we spend a lot of time thinking about these issues. Whenever Im studying a particular area of science, Ive learned that there is probably more to the story than I know of. I now make a point to find out about the hidden women who were likely involved in each discovery.

Someone who is close to my heart is Cecilia Payne-Gaposchkin, an astronomer and astrophysicist who was based at Harvard University during the 1920s. In her PhD thesis, she was one of the first people to use a new theory at the time, the theory of quantum physics. She used the mathematics of that theory to understand the composition of all stars and show that they were made of hydrogen and helium, which we take for granted today. This was a transformational discovery, yet she went unrecognized for many years. She didnt have an official role at Harvard until much later, when she was finally made a faculty member. Then she became the first woman to ever chair a department at Harvard.

Cecilia is a role model because of her arc of discovery and resilience. No matter how little recognition she got, she kept doing amazing research and eventually left an incredible legacy. And she did it using quantum physics, which is my field, so shes very special to me.

Yes. Often, the men they worked with got awards for their work. A male scientist used the same techniques as Bibha Chowdhuri to confirm her discoveries and won the Nobel Prize. Another woman, Lisa Meitner, was nominated for the Nobel Prize 48 times and never won. She is basically the one who discovered nuclear fission, which led to nuclear energy, the atom bomb, nuclear physics, and so on. She never won, yet she kept going. How do you continue in the face of such obvious resistance? These women were so resilient. Its amazing, and its also infuriating. I hope readers feel outrage for what these women had to deal with just to do what they love.

In addition to their legacies of cutting-edge science, these women addressed challenges and biases that they faced to break glass ceilings. They were rule breakers. They earned leadership positions. They set up awards for young women to be recognized in their fields. They started women in physics committees, which we have everywhere today. These women used their voices to support other women, which is how change happens.

Originally posted here:

Laurier researcher Shohini Ghose documents the untold legacies of ... - Wilfrid Laurier University

Read More..

Enhancing Cosmic Microwave Background Precision: The Role of … – AZoQuantum

A recent study published in the journal Physical Review D, designated as an Editors Suggestion, has indicated that forthcoming missions will achieve enhanced precision in detecting deviations from parity symmetry within the cosmic microwave background polarization.

Cosmic Microwave Background (CMB) polarized light subjected to gravitational lensing effects, in addition to cosmic birefringence. On the far left, the white lines show the polarization pattern of the CMB light generated in the early universe. These rotate due to cosmic birefringence, resulting in the currently observed CMB depicted by the black lines on the right side of the image. However, the path of light is bent by the gravitational distortion of space-time created by the large-scale structure in the middle, and so the white lines showing the polarization pattern on the right side of the image show what is observed. Image Credit: Naokawa and Namikawa

This improvement results from the diligent efforts of a pair of researchers who have factored in the gravitational lensing effect.

Cosmology endeavors to tackle profound inquiries regarding the universe's scope, origin, and inception, presenting empirical support for theoretical models based on fundamental physics. The widely accepted Standard Model of Cosmology, while notable, remains incapable of addressing fundamental enigmas such as dark matter and dark energy.

In 2020, the scientific community unveiled a fascinating phenomenon called cosmic birefringence, deduced from data on the polarization ofcosmic microwave background (CMB).

Polarization characterizes the oscillation of light waves perpendicular to their direction of propagation. Ordinarily, the polarization plane remains constant, but under particular conditions, it may undergo rotation.

A re-evaluation of CMB data has proposed that the polarization plane of CMB light might have experienced a slight rotation from its origin in the early universe to the present, a transgression of parity symmetry recognized as cosmic birefringence.

The intricate nature of cosmic birefringence defies conventional physical laws, suggesting that hitherto undiscovered physics, like axionlike particles (ALPs), may underlie this phenomenon.

The discovery of cosmic birefringence holds the potential to unveil the enigmatic properties of dark matter and dark energy, thus prompting an emphasis on refining CMB observations in future missions.

To accomplish this, enhancing the precision of current theoretical calculations is pivotal. Yet, existing calculations have fallen short due to their omission of gravitational lensing.

In response, a recent study conducted by a research duo led by Fumihiro Naokawa, a Doctoral Student from The University of Tokyo's Department of Physics and Research Center for Early Universe, and Toshiya Namikawa, Project Assistant Professor from the Center for Data-Driven Discovery and Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU).

The study has unveiled a theoretical framework for cosmic birefringence that incorporates gravitational lensing effects. Additionally, they have developed a numerical code that integrates gravitational lensing effects, which will be indispensable for future analyses.

Naokawa and Namikawa initially formulated an analytical equation delineating how gravitational lensing alters the cosmic birefringence signal.

Leveraging this equation, they integrated a novel program into an existing code to calculate gravitational lensing corrections, ultimately examining the disparities in signals with and without gravitational lensing adjustments.

Their findings reveal that disregarding gravitational lensing results in an observable cosmic birefringence signal that does not align satisfactorily with theoretical predictions, potentially rejecting the veracious theory.

Furthermore, the researchers simulated forthcoming observational data, highlighting the significance of gravitational lensing in the quest for ALPs. Their results disclosed that the omission of gravitational lensing yields significant systematic biases in the model parameters of ALPs deduced from observed data, diminishing the fidelity of the ALPs model.

The gravitational lensing correction tool introduced in this study is already in use in contemporary observational investigations. Naokawa and Namikawa are committed to its continued application in the analysis of data from future missions.

Naokawa, F & Namikawa, T (2023) Gravitational lensing effect on cosmic birefringence. Physical Review D. doi.org/10.1103/PhysRevD.108.063525.

Source: https://www.ipmu.jp/en

Visit link:

Enhancing Cosmic Microwave Background Precision: The Role of ... - AZoQuantum

Read More..

Strathmore’s Guffogg, world renown artist, to be featured in Venice in … – Porterville Recorder

Shane Guffogg, a world renown artist, who was raised in Lindsay and Strathmore, will have his art featured at the historic Scala Contarini del Bovolo in Venice, Italy.

Beginning in April, 2024, Guffogg will present a new series of 21 paintings titled At the Still Point of the Turning World. This unprecedented series of works represents Guffogg's ongoing dialogue with T.S. Eliot, and with the famous poem Four Quartets, which inspired him to create large-scale paintings that explore the intersection of time and space, consciousness and transcendence, with the concept of movement, escape and migration.

The dialogue between the artist's abstract paintings and the poet who won the Nobel Prize for Literature in 1948 tells of the human race and its living in constant movement, tension, in constant passage and breaking of the diaphragm between now and elsewhere.

The exhibition was born from the artist's study and deep immersion in the writings of Eliot. Guffogg connects with the writer's thoughts, which are deeply rooted in ancient Christian ideologies and Eastern Sacred Texts, giving rise to an exhibition that places our transitory nature at the center of its message of humanity throughout history. This transience mutability, as well as the drive and tendency of the single individual to mutate and subvert the "status quo," in search of an "other place," space and solution to the dimension of exteriority and extraneousness not only geographical and geopolitical, but social, temporal and contextual.

The theme of the exhibition also has strong autobiographical roots in the artist's life and family history. Guffogg's father immigrated to the United States in 1957 from northern England, where he had worked as a coal miner since the age of 15. His motivation for the search for an "Elsewhere" was mainly economic, driven by the pursuit of the "American dream," which in England, as in Italy, in Europe and beyond, was the alternative for millions of individuals to social and economic depression post World War II and pre Economic Boom.

Guffogg moved to Los Angeles in the late 1980s from the Central Valley for similar reasons: it's important to underline how, before the contemporary "information age" reached almost every corner of the globe, there was an urgent need to gravitate towards places where innovative ideas were developing and progressive thought was welcomed and art and culture were esteemed rather than ridiculed.

Guffogg's artistic research revolves around the capturing of fleeting moments of thought, presence. Impulses, and movements.

The painted lines that make up the works in the first room of the exhibition symbolize movement influenced by the newfound chaos prevalent in our 24-hour news cycle, he said. Through these nine paintings, my goal is to establish order using color and symmetry that transcends both Eastern and Western thought, addressing the core of our common humanity: the desire to be part of something bigger than ourselves while maintaining our individual identity and purpose.

The paintings in the second room also draw inspiration from T.S. Eliot's four Quartets. In contrast to the ethereal themes of the first room, these twelve paintings explore the physical realm, blending Western painting techniques with Eastern calligraphy.

The nine paintings in the first room are intended for contemplation, bypassing the need for intellectual analysis of how or why they exist. The second room represents the flip side of the same coin, designed to be confrontational and physically engaging.

Guffogg's artistic process is deeply philosophical and views each brushstroke as a thought that evokes sensory memories essential for the creation of a visual language. In this way, his paintings are like words that can be read and interpreted, but also exist in a realm beyond language. By exploring the Eastern and Western ideological influences within Eliot's poem, Guffogg found a rich source of inspiration that allowed him to create a hypnotic rhythm of creation, pulsating between past, present and future.

From the beginning of his career, Guffogg has been influenced by the art and ideologies of ancient cultures and civilizations. Another part is quantum physics, and the vibration of the invisible and intuitive musical score of nature. These paintings absorb his psyche through the physical process of painting.

For the exhibition at the Contarini del Bovolo, Guffogg is inspired by three verses from the first section of Burnt Norton; Reach into the silence, Only Through Time is Time Conquered, and Neither Flesh nor Fleshless. Eliot wrote the first section in 1936 before the Second World War, with a consideration of the element of air, staged in early summer. It begins with Eliot inviting the reader into a rose garden to experience the timeless beauty and essence of all knowledge.

Guffogg's Reach into the Silence will be the first works the public sees when they enter the exhibition. When a guest arrives at Palazzo Contarini del Bovolo, he will enter through a 15th-century staircase 28 meters high. Due to its curvilinear shape the staircase is called bovolo, that's, spiral. This staircase has two sides; Gothic and Renaissance, and is one of the most fascinating elements in the history of Venice architecture.

The exhibition will be divided into two rooms, each characterized by a different passage from Eliot's poetry. The first room features eight paintings titled, Reach into the Silence. These eight paintings measure 6 x 5 feet each (182.8 x 152.4 cm). These works use a neutral palette inspired by the Bovolo building and surrounding area, intertwining Venetian reds, grays, subtle lavender accents, blues, greens and nude tones. The visual effects of countless thin lines, each representing months of the artist's presence as he paints, are condensed into a single moment, a shimmering, unexpressed silence that invites the viewer to contemplate the abstract nature of time and space. At the end of the room there will be a horizontal painting titled, Only Through Time, Time is Conquered, which draws on the colors of the rich history of Venice and the painting by Tintoretto, a sketch for the commission of Paradise at the Doge's Palace, a work that's part of the collection of IPAV and permanently exhibited in the rooms of Palazzo Contarini.

This final painting, measuring 7 x 9 feet (213.6 x 274.3 cm) will also allow viewers to experience the movement of the artist's hand in creating the work. The viewer will have a QR code to scan and then, once pointed at the painting, the AR will be activated showing the inversion of the application of colors and lines, until the painting is in the initial phase, which will then dissolve visually revealing Tintoretto.

The second room will host the series Neither Flesh nor Fleshless, which takes up another passage from Eliot's poetry. This series includes 12 paintings consisting of two paintings measuring 60 x 48 inches (152.4 x 121.9 cm), six paintings 40 x 36 inches (101.6 x 91.4 cm), and four paintings 30 x 24 inches ( 76.2 x 60.9 cm). All the paintings are oil on canvas and the paintings in the second room use chiaroscuro and calligraphic movements to create a bridge between past and present. These works are figurative yet rooted in abstraction, inviting viewers to contemplate the interplay between the physical and the ephemeral.

The titles will be printed as signage on the walls, but the signage will also activate another AR component that will display the title of each painting in Italian and English, in the context of the poem so the viewer can see where the titles were taken from. While these two rooms are not intended to make an overt political statement, they represent a chance for viewers to contemplate their place in the world. In an age of constant information overload, Guffogg believes art has an essential role to play in guiding people towards self-awareness. Using augmented reality, Guffogg is expanding the possibilities of what art can be, inviting viewers to see and think beyond the 24/7 information age.

Ultimately, his vision for this exhibition is one that allows viewers to contemplate what it means to live in the 21st century, acknowledging the past while existing in the present moment.

Guffogg, who also attended Porterville College, earned a bachelor's from the California Institute of the Arts in 1985.

The rest is here:

Strathmore's Guffogg, world renown artist, to be featured in Venice in ... - Porterville Recorder

Read More..

How Many Atoms Does It Take to Trace the History of the Universe? – Columbia University

Is the book for non-scientistsas well as scientists?

To be my endemically curmudgeonly self, Im not sure I can accept thepremise of the question. Every 5-year-old is a scientistthey insistently ask questions about, and do experiments on, the natural world. Somehow, our educational system and the larger culture convince people by the time they get to college that humankind is divided into two subspecies: scientists and non-scientists. Ive been working for decades to try and demolish this notion, albeit with limited success.

Temporarily suspending my objection to the question, the book is written for non-scientists. It assumes no prior knowledge whatsoever about atoms. The book does use numbers (e.g., it takes 15 milliontrillion atoms to make a poppy seed), but gives helpful analogies to visualize such numbers (e.g., if those atoms were marbles, theyd fill a warehouse 25 stories tall and the size of New York State).

Read my books (and others like them)! Professional journal articles are indeed filled with jargon and require specialized knowledgethey are designed as an efficient way for scientists dedicated to one field to talk to their colleagues in that same field; such articles are not even very accessible to scientists from other fields.

But this is not the only way scientists communicate. They give public talks, write articles and books for a general audience, produce You Tube videos, and work with science museums. Science is a crowning intellectual achievement of humankind, and, in a technology-saturated world, it is essential that its methods, as well as its results, be shared widely.

Uncharacteristically, I have had time to read several books lately. The first was Big Rock Candy Mountain by Wallace Stegner, who is my favorite American author (and hugely under-appreciated in my humble opinion). He has, simultaneously, both piercing insight into, and generous empathy for, the human condition. The second book was Michael Ondaatjes The Cats Table, a wonderful, semi-autobiographical tale of a 10-year-old boy alone on a ship from Sri Lanka to prep school in Englandtranscendent writing.

Then there was A Gentleman in Moscow by Amor Towles which, after the first few pages, I thought was too arch, but which evolved into a charming tale populated by a marvelous collection of characters. In oneday, two different people on two different airplanes noticed what I was reading and said great book. I also found it highly unusual that Towles says on the book jacket flap that the success of his first novel (Rules of Civilitynext on my list) allowed him the luxury of retiring from investment bankingperhaps the first time in literary history that career switch has happened.

I also read The Primacy of Doubt by Tim Palmerheavy-going, but with some interesting speculations connecting chaos theory with climateforecasting, quantum mechanics, geopolitical instability, pandemics, and human consciousness.

In addition to Rules of Civility, next on my stack is Philip Kitchers On John Stuart Mill, one of the first in a series put out by Columbia University Press on the Core Curriculum. I have this fantasy that one day before I retire from Columbia (or perhaps after I retire), I will teach Contemporary Civilization, and I figure Philip is a good first tutor for me.

A course called Frontiers of Astrophysics, which is designed to introduce our undergraduates from CC, SEAS, GS, and Barnard to the hot topics in our discipline. We showcase a lot of the research being done here at Columbia to illustrate the kind of work in which they might participate. I will also give lectures in Frontiers of Science, which, I am pleased to say, will celebrate its 20th anniversary as part of the Core this year.

Ive just started my next book, Somewhere Under the Rainbow (with apologies to Music Professor Walter Frisch, whose book on Over the Rainbow I also read this summer, come to think of it). Its an exploration of the sea of electromagnetic radiation in which we are all immersed, and for which we have detectors (our eyes) that can sense just one out of the 60 octaves the universe sends us. From warming yesterdays pizza, to using your cell phone, to finding Mayan cities hidden in the jungle, to medical imaging, to the astonishing applications in biology, geology, physics, and, of course, the symphony of waves the universe sends us, it is all just light of different wavelengths. I plan to lift the narrow veil our eyes impose.

Scientifically, with my colleague Frits Paerels, Im still pursuing a problem I was working on when I got to Columba 46 years agotrying to understand the densest matter in the universe: the cores of neutron stars. If we could just measure both the mass and the diameter of one star, wed have a very interesting constraint on both the structure of the atomic nucleus and the first microsecond of the Big Bang. Were tantalizingly close, but Im not sure well succeedas usual, we need more data!

Excerpt from:

How Many Atoms Does It Take to Trace the History of the Universe? - Columbia University

Read More..

A review of liquid crystal spatial light modulators devices and applications – Phys.org

This article has been reviewed according to ScienceX's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility:

close

Technology to control and harness light has existed for centuries, often as static solutions that must be custom-designed. It is only in the past couple of decades that the digital era of micro-electronics and computing has seen fast rewritable technology meant for displays find its way into the mainstream of optics.

In a new review published in Opto-Electronic Science, the authors showcase the recent advances in replacing the traditional static optical toolkit with a modern digital toolkit for "light on demand." The result has been the introduction of digitally controlled light to nearly all major optical laboratories worldwide, opening new paths for the creation, control, detection, and harnessing of exotic forms of structured light. The advanced toolkit promises novel applications from classical to quantum, ushering in a new chapter in on-demand structured light.

The authors of this article reviewed recent progress in using a modern digital toolkit for on-demand forms of sculptured light, offering new insights and perspectives on this nascent topic. The core technology that has advanced this field is the liquid crystal spatial light modulator (SLM), allowing high resolution tailoring of light in amplitude, phase, polarization, or even more exotic degrees of freedom such as path, orbital angular momentum, and even spatiotemporal control. These simple yet highly effective devices are made up of millions of pixels that can be modulated in phase, for spatial control of light in an in-principle lossless manner.

In the review, the authors show how such SLMs can be exploited for a myriad of tasks, from creating all forms of structured light to fast and efficient detectors. They have fueled advances in optical communication, microscopy, imaging and have even become indispensable in modern quantum optics laboratories.

It has brought the highly technical and difficult field of diffractive optics and digital holography very much into the mainstream, for anyone to access with relatively cheap solutions. For instance, diffractive optical elements as computer generated holograms could finally be exploited for what they are: just "pictures" to be displayed. SLMs have made this giant leap possible, overcoming the cost and complexity of prior solutions.

Most importantly, the "pictures" are rewritable, for on-demand real-time solutions for real-world applications. For instance, holographic optical tweezers allow light-matter interactions to be controlled with just a change to a picture (computer generated hologram), refreshing in real-time for trapping, tweezing and manipulating objects in 3D. This has seen direct application in physics, chemistry, medicine and biology, diverse fields of impact.

The authors unpack the mechanics of how SLMs work, provide novel insights and perspectives based on their long track record in the topic, revealing how this new field is rapidly accelerating along with the nascent topic of structured light. They suggest what the future may hold when present challenges are transformed into exciting applications.

More information: Yiqian Yang et al, A review of liquid crystal spatial light modulators: devices and applications, Opto-Electronic Science (2023). DOI: 10.29026/oes.2023.230026

Provided by Compuscript Ltd

See more here:

A review of liquid crystal spatial light modulators devices and applications - Phys.org

Read More..

October Altcoin Gainers – These Five Altcoins Paved the Way – BeInCrypto

October was a bullish month for the cryptocurrency market, filled with altcoin gainers. Bitcoin (BTC) and several other cryptocurrencies reached new yearly highs.

As Halloween ushers an end to October, BeInCrypto looks at 5 altcoins that made October frighteningly profitable. The five October altcoin gainers are:

The POLYX price has increased quickly since October 13. The upward movement has been parabolic, leading to an all-time high price of $0.43 on October 30.

The increase caused a breakout from the $0.29 horizontal resistance area, which had been in place since April.

The all-time high was close to the 1.61 external Fib level of the most recent decrease. Once the price is at an all-time high, the Fib level often acts as the area for the top.

If POLYX breaks out above it, it can increase by 75% to the 2.61 external Fib level at $0.66.

Despite this bullish prediction, failure to close above the $0.44 resistance can lead to a 25% drop to the $0.29 horizontal area, which is expected to provide support.

The TRB price has increased alongside a parabolic ascending support line since the beginning of September. The upward movement led to a new yearly high of $125 yesterday.

Currently, TRB trades slightly above the 0.618 Fib retracement level of the entire previous decrease at $105. Whether the price moves above it or gets rejected can determine if the future trend is bullish or bearish.

A successful close above this area can lead to a 50% increase to the next resistance at $165.

On the other hand, a rejection and breakdown from the parabolic ascending support line will mean the upward movement is complete. In that case, a 40% drop to the closest support at $66 will be likely.

The SOL price has increased alongside an ascending support trendline since the beginning of the year. More recently, it bounced above the line in September (green icon), accelerating its rate of increase.

The next month, SOL broke out from the $28 horizontal area. This was a crucial area since it had been in place since November 2022.

Today, SOL reached a new yearly high of $37. If the price continues upwards, it can increase by another 46% and reach the next resistance at $47.

Despite this bullish SOL price prediction, failure to sustain the increase can cause a 25% drop to the $28 area, validating it as support.

The INJ price increased by 50% last week, breaking out from the $9 horizontal resistance area. The price reached a new yearly high of $14.50 today. This was the highest price since November 2021.

Currently, INJ trades inside the $13.50 horizontal resistance area. This is the final resistance before the all-time high region.

So, if INJ breaks out, it can double in price and reach the all-time high of $27.

Despite this bullish prediction, a rejection from the $13.50 horizontal resistance area can trigger a 35% drop to validate the $9 support area again.

The MINA price has increased swiftly since its $0.36 low on October 11. On October 24 alone, the price increased by 110%, leading to a high of $0.98.

However, the upward movement could not be sustained. Rather, MINA created a long upper wick (red icon) and fell below the $0.88 horizontal resistance area.

Now, MINA trades just above the $0.58 horizontal support area. Whether it bounces or breaks down can determine the future trends direction.

A bounce can lead to a 40% increase to the next resistance at $0.88. On the other hand, a breakdown can cause a 40% drop to $0.37.

For BeInCryptos latest crypto market analysis,click here.

In line with the Trust Project guidelines, this price analysis article is for informational purposes only and should not be considered financial or investment advice. BeInCrypto is committed to accurate, unbiased reporting, but market conditions are subject to change without notice. Always conduct your own research and consult with a professional before making any financial decisions.

Read more here:
October Altcoin Gainers - These Five Altcoins Paved the Way - BeInCrypto

Read More..

Ripple rally to $0.66 likely with bullish developments in the altcoin – FXStreet

Ripple price sustained above the $0.59 level, on Friday, close to its $0.62 local top. On-chain indicators reveal a rising demand for XRP tokens among market participants. Rising trade volume and daily active addresses are indicative of brewing interest among traders.

The altcoin yielded 10.70% gains over the past month. The altcoin has been in a consistent uptrend for the past three days. The US Federal Reserves interest rate decision failed to sway the bullish outlook of retail traders and XRP price continued posting gains.

Also read: Ripple makes comeback to $0.60 after XRP held by retail traders notes a significant increase

Whale transaction count (>$100,000) vs XRP price

XRP trade volume, daily active addresses vs XRP price

Payment remittance firm Ripple announced that the Dubai Financial Services Authority (DFSA) has approved the digital asset XRP for use within the Dubai International Financial Centre (DIFC).

Virtual asset firms within the DIFC will now be able to incorporate XRP into their virtual asset services. XRP is the first virtual asset to be approved by the regime. Bitcoin, Ethereum, and Litecoin rank in the list of assets previously approved under the DFSAs virtual assets regime.

The legal and regulatory clarity is likely to benefit XRP. The asset will be used by institutions located in the DIFC for value exchange, boosting its utility.

XRP price is $0.5980 on Binance at the time of writing. As seen in the price chart below, there is a Fair Value Gap between $0.6682 and $0.6758. The lower level, $0.6682, is expected to act as a resistance for the altcoin as the XRP price rally continues.

The bullish developments in XRP are likely to support the assets uptrend. A successful break past $0.6682 will send XRP to the upper boundary of the FVG, at $0.6758. The move from $0.5980 (current price) to $0.6682 (FVG) marks a 12% gain from the current price.

XRP/USDT one-day price chart on Binance

On the downside, the 10-day Exponential Moving Average (EMA) at $0.5769, could act as a support.

Ripple is a payments company that specializes in cross-border remittance. The company does this by leveraging blockchain technology. RippleNet is a network used for payments transfer created by Ripple Labs Inc. and is open to financial institutions worldwide. The company also leverages the XRP token.

XRP is the native token of the decentralized blockchain XRPLedger. The token is used by Ripple Labs to facilitate transactions on the XRPLedger, helping financial institutions transfer value in a borderless manner. XRP therefore facilitates trustless and instant payments on the XRPLedger chain, helping financial firms save on the cost of transacting worldwide.

XRPLedger is based on a distributed ledger technology and the blockchain using XRP to power transactions. The ledger is different from other blockchains as it has a built-in inflammatory protocol that helps fight spam and distributed denial-of-service (DDOS) attacks. The XRPL is maintained by a peer-to-peer network known as the global XRP Ledger community.

XRP uses the interledger standard. This is a blockchain protocol that aids payments across different networks. For instance, XRPs blockchain can connect the ledgers of two or more banks. This effectively removes intermediaries and the need for centralization in the system. XRP acts as the native token of the XRPLedger blockchain engineered by Jed McCaleb, Arthur Britto and David Schwartz.

Follow this link:
Ripple rally to $0.66 likely with bullish developments in the altcoin - FXStreet

Read More..