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Viewing: Blog Posts Tagged with: antimatter, Most Recent at Top [Help]
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1. The way of the abstract

The realm of theoretical physics is teeming with abstract and beautiful concepts, and the process of bringing them into existence, and then explaining them, demands profound creativity according to Giovanni Vignale, author of The Beautiful Invisible: Creativity, imagination, and theoretical physics. In the excerpt below Vignale discusses the beginnings of theoretical physics and the abstract.

Physics, most of us would agree, is the basic science of nature. Its purpose is to discover the laws of the natural world. Do such laws exist? Well, the success of physics at identifying some of them proves, in retrospect, that they do exist. Or, at least, it proves that there are Laws of Physics, which we can safely assume to be Laws of Nature.

Granted, it may be difficult to discern this lofty purpose when all one hears in an introductory course is about flying projectiles and swinging pendulums, strings under tension and beams in equilibrium. But at the beginning of the enterprise there were some truly fundamental questions such as: the nature of matter, the character of the forces that bind it together, the origin of order, the fate of the universe. For centuries humankind had been puzzling over these questions, coming up with metaphysical and fantastic answers. And it stumbled, and it stumbled, until one day—and here I quote the great Austrian writer and ironist, Robert Musil:

. . . it did what every sensible child does after trying to walk too soon; it sat down on the ground, contacting the earth with a most dependable if not very noble part of its anatomy, in short, that part on which one sits. The amazing thing is that the earth showed itself uncommonly receptive, and ever since that moment of contact has allowed men to entice inventions, conveniences, and discoveries out of it in quantities bordering on the miraculous.

This was the beginning of physics and, actually, of all science: an orgy of matter-of-factness after centuries of theology. Careful and systematic observation of reality, coupled with quantitative analysis of data and an egregious indifference to theories that could not be tested by experiment became the hallmark of every serious investigation into the nature of things.

But even as they were busy observing and experimenting, the pioneers of physics did not fail to notice a peculiar feature of their discipline. Namely, they realized that the laws of nature were best expressed in an abstract mathematical language—a language of triangles and circles and limits—which, at first sight, stood almost at odds with the touted matter-of-factness of experimental science. As time went by, it became clear that mathematics was much more than a computational tool: it had a life of its own. Things could be discovered by mathematics. John Adams and, independently, Urbain Le Ferrier, using Newton’s theory of gravity, computed the orbit of Uranus and found that it deviated from the observed one. Rather than giving up, they did another calculation showing that the orbit of Uranus could be explained if there were another planet pulling on Uranus according to Newton’s law of gravity. Such a planet had never been seen, but Adams and Le Ferrier told the astronomers where to look for it. And, lo and behold, the planet—Neptune—was there, waiting to be discovered. That was in 1846.

Even this great achievement pales in comparison with things that happened later. In the 1860s, James Clerk Maxwell trusted mathematics—and not just the results of a calculation, but the abstract structure of a set of equations—to predict the existence of electromagnetic waves. And electromagnetic waves (of which visible light is an example) were controllably produced in the lab shortly afterwards.

In the 1870s Ludwig

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2. Hunting the Neutrino

By Frank Close

Ray Davis was the first person to look into the heart of a star. He did so by capturing neutrinos, ghostly particles that are produced in the centre of the Sun and stream out across space. As you read this, billions of them are hurtling through your eyeballs at almost the speed of light, unseen.

Neutrinos are as near to nothing as anything we know, and so elusive that they are almost invisible. When Davis began looking for solar neutrinos in 1960, many thought that he was attempting the impossible. It nearly turned out to be: 40 years would pass before he was proved right, leading to his Nobel Prize for physics in 2002, aged 87.

In June 2006, I was invited by The Guardian newspaper to write his obituary. An obituary necessarily focuses on the one person, but the saga of the solar neutrinos touched the lives of several others, scientists who devoted their entire careers chasing the elusive quarry, only to miss out on the Nobel Prize by virtue of irony, chance, or, tragically, by having already died.

Of them all, the most tragic perhaps is the genius Bruno Pontecorvo.

Pontecorvo was a remarkable scientist and a communist, working at Harwell after the war. When his Harwell colleague Klaus Fuchs was exposed as an atom spy in 1950, Pontecorvo immediately fled to the USSR. This single act probably killed his chances of Nobel Prizes.

In the following years, Pontecorvo developed a number of ideas that could have won him one or more Nobels. But his papers were published in Russian, and were unknown in the West until their English translations appeared up to two years later. By this time others in the USA had come up with the same ideas, later winning the Nobel Prize themselves.

Amongst his ideas, one involved an experiment which Soviet facilities could not perform. But most ironic were Pontecorvo’s insights about neutrinos.

Ray Davis had detected solar neutrinos – but not enough of them. For years, many of us involved in this area of research thought Davis’ experiment must have been at fault. But Pontecorvo had another theory which indicated that like chameleons, neutrinos changed their form en route across space from the Sun to Earth. And he was right. It took many years to prove it, but by 2000 the whole saga was completed. Davis duly won his Nobel Prize, but so many years had elapsed that Pontecorvo by then was dead.

So although my piece for The Guardian began as the life story of Ray Davis, Pontecorvo was there behind the scenes to such an extent that it became his story also. It is also the story of John Bahcall, Davis’ lifelong collaborator, who, to the surprise of many, was not included in the Nobel award.

The lives of these three great scientists were testimony to what science is all about: as Edison put it, genius is 1% inspiration and 99% perspiration.

A final sobering thought to put our human endeavors in context: those neutrinos that passed through you when you started reading this article are by now well on their way to Mars.

Frank Close OBE is Professor of Physics at Oxford Univeristy and a Fellow of Exeter College.  He is formerly Head of the Theoretical Physics Division at the Rutherford Appleton Laboratory, and Head of Communications and Public Education at CERN. He has written several books including The Void, Antimatter, 0 Comments on Hunting the Neutrino as of 1/1/1900

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3. Antimatter and ‘Angels and Demons’: A fiction thought to be fact

Frank Close, OBE is Professor of Physics at Oxford University and a Fellow of Exeter College. He was formerly vice president of the British Association for the Advancement of Science (now the British Science Association), Head of the Theoretical Physics Division at the Rutherford Appleton Laboratory, and Head of Communications and Public Education at CERN. His most recent book examines one of the oddest discoveries in physics - antimatter.

In the post below, Frank Close reveals the fallacies concerning antimatter in the Dan Brown novel (and now major cinema release) Angels and Demons. He has previously written for OUPblog on CERN’s Large Hadron Collider.


Many people have never heard of CERN. Of those that have, most know it as the birthplace of the World Wide Web; fewer knew its main purpose, which is as the European Centre for experiments in particle physics. However, with the appearance of Angels and Demons CERN is about to become famous as a laboratory in Geneva that makes antimatter. These two statements about CERN are correct; much else in Dan Brown’s novel, which inspired the movie and has led to much of the popular received wisdom about antimatter, is not.

The movie is of course fiction, but the book on which it is based teases readers with a preface headlined “FACT”. This includes “Antimatter creates no pollution or radiation… is highly unstable and ignites when it comes in contact with absolutely anything… a single gram of antimatter contains the energy of a 20 kiloton nuclear bomb”. CERN is credited as having created “the first particles of antimatter” and the curtain metaphorically rises to the question whether this “highly volatile substance will save the world, or… be used to create the most deadly weapon ever made”.

These “facts” are at best misleading and even wrong, but many, including some in the US military, believe them to be true.

Antiparticles have been made for 80 years; a few atoms of antihydrogen have been made at CERN during the last decade; antimatter, in the sense of anti-atoms organised into amounts large enough to see, let alone contain, is still in the realms of fantasy and likely to remain so.

In Angels and Demons the experimental production of antimatter being equated with The Creation is so central to the plot that a scientist tells the Pope the “good news”, even though it is decades old. Whatever led to our universe, it was not akin to the creation of matter at CERN, in either the fictional or the real world. It is not “something from nothing… practically proof that Genesis is a scientific possibility”. This is at best cod theology and non-science.

The Big Bang is the creation of all energy, all matter, and all of the known universe, together with its space and time. We cannot recreate that singular event, but we can examine what happened afterwards, within what became our present universe.

Energy, lots of it, is what turned into matter and antimatter. Energy is not nothing; it is measurable and when you use some the power company will charge you for it. When you create antimatter together with its matter counterpart, you have to put in the same amount of energy as would be released were they to annihilate one another; you do not get matter from nothing. Now reverse the process, such that antimatter meets matter and is turned back into radiant energy. That certainly is not nothing, as Angels and Demons recognises since the resulting blast is what is going to destroy the Vatican.

It is at this point that some in the US military seem to have adopted this fictional work as its practical guide to antimatter, and to have ignored its many contradictions. The preface of Angels and Demons described antimatter as the ideal source of energy which “creates no pollution or radiation and a droplet could power New York for a day”. Antimatter may not emit radiation so long as it stays away from matter, but in that case it offers nothing to bomb makers or power companies. In order to exploit this “volatile” substance, you need to annihilate it with matter, at which it releases its trapped energy as radiation such as gamma rays.

The statement that there are “No byproducts, no radiation, no pollution” is ironic given that it occurs within a few paragraphs of a warning to beware of the gamma rays. The US Air Force were enthused so much that in promoting their interest in antimatter for weapons they announced “No Nuclear Residue”. The media trumpeted that “a positron bomb could be a step toward one of the military’s dreams from the early Cold War: a so-called `clean’ superbomb” San Francisco Chronicle 4 October 2004, uncanny examples of fiction, written in 2000, presented as if fact in 2004.

As a major milestone in antimatter science CERN is indeed marvellous, but trifling compared with what would be needed to make antimatter in industrial quantities. Even were it possible, the belief that antimatter technology could “save the planet” is specious. As we first have to make the antimatter ourselves, we would waste more energy in making it than we could ever get back, so antimatter is not a panacea for “saving the planet”. Thankfully, neither will it become “the most deadly weapon”.

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4. Antimatter: An Excerpt

Antimatter is much loved by science fiction writers. Yet it is real: there are looking-glass particles that are counterparts of protons, electrons, and other familiar particles of matter. Below is an excerpt from Frank Close’s new book Antimatter, which explains that to even begin to understand antimatter you have to first look at the material world, including ourselves. Frank Close previously wrote for OUPblog on CERN’s Large Hadron Collider.

If you were to see a lump of antimatter, you wouldn’t know it; to all outward appearances it looks no different to ordinary stuff. So perfectly disguised that it is seemingly one of the family, its ability to destroy whatever it touches would make it the perfect ‘enemy within’. So, what is antimatter? Saying that it is the opposite of matter is easy on the ear, but what actually is ‘opposite’ about it? Knowing that the briefest contact with antimatter would commit whatever it touched to oblivion is awe-inspiring, but what gives antimatter this power?

To begin to understand antimatter, we need first to take a voyage into ordinary matter, such as ourselves. Our personal characteristics are coded in our DNA, miniature helical spirals made of complex molecules. These molecules in turn are made of atoms, which are the smallest pieces of an element—such as carbon or hydrogen or iron—that can exist and still retain the characteristics of that element.

Hydrogen atoms are the lightest of all and tend to float up to the top of the atmosphere and escape. For this reason hydrogen is relatively rare on earth, whereas in the universe at large it is the commonest element of all. Most of the hydrogen was made soon after the Big Bang and is nearly fourteen billion years old.

Vast balls of hydrogen burst into light as stars, such as our sun. It is in the stars that the full variety of elements is fashioned. Nearly all of the atoms of oxygen that you breathe, and of the carbon in your skin or the ink on this page, were made in stars about five billion years ago when the earth was first forming. So we are all stardust or, if you are less romantic, nuclear waste, for stars are nuclear furnaces with hydrogen as their primary fuel, starlight their energy output and assorted elements their ‘ash’ or waste products.

To give some idea of how small atoms are, look at the dot at the end of this sentence; it contains some 100 billion atoms of carbon, a number far larger than all humans who have ever lived. To see any of those individual atoms with the naked eye you would need to magnify the dot to be 100 metres across.

Elemental carbon atoms can bind in different forms, such as diamond, graphite, and carbon black—soot, charcoal, and coal. Antimatter also consists of molecules and atoms. Atoms of anticarbon would make antidiamond as beautiful and hard as the diamond we know. Antisoot would be as black as soot, and the full stops in an antibook the same as those you see here. They too would need enlarging to 100 metres size for their anticarbon atoms to be seen. Were we able to do that, we would find that these smallest grains of anticarbon are indistinguishable from those of carbon. So even at the basic level of atoms, matter and antimatter look the same: the source of their contrast is buried deeper still.

Atoms are very small, but they are not the smallest things. It is upon entering them and encountering the basic seeds from which they are made that the profound duality between matter and antimatter is disclosed.

Each atom contains a labyrinth of inner structure. At the centre is a dense compact nucleus, which accounts for all but a trifle of the atom’s mass. While enlargement of our ink-dot to 100 metres is sufficient to see an atom, you would need to enlarge it to 10,000 kilometres, as big as the earth from pole to pole, if you wanted to see the atomic nucleus. The same is true for antidots and antiatoms. It is only when they are seen in such fine detail that the subtle choice of matter or antimatter begins to show.

When the profound entangling of space and time that comes with Einstein’s theory of relativity is married with the will-o’-the-wisp ephemeral world of uncertainty that rules within atoms, an astonishing implication emerges: it is impossible for nature to work with only the basic seeds of matter that we know. To every variety of subatomic particle, nature is forced also to admit a negative image, a mirror opposite, each of which follows the same strict laws as do conventional particles. As the familiar particles build atoms and matter, so can these contrary versions make structures that at first sight appear to be the same as normal matter, but are fundamentally dissimilar.

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5. Big Answers With A Big Bang

Frank Close, OBE, is Professor of Physics at Oxford University and a Fellow of Exeter College. He was formerly vice president of the British Association for the Advancement of Science, Head of the Theoretical Physics Division at the Rutherford Appleton Laboratory, and Head of Communications and Public Education at CERN. He received the Institute of Physics’ Kelvin Medal in 1996, awarded for outstanding contributions to the public understanding of physics. He is the author of The Void, Very Short Introduction to Particle Physics, The Particle Odyssey and many more.  Also, look for Antimatter in January, Close’s newest book.

We asked Close to explain the importance of the Large Hadron Collider to us.  He kindly sent us the post below and the following analogy, comparing the journey for answers about the origin of the universe to sewing a tapestry:  “The quest is like sewing a tapestry, but one where the picture is only revealed as you do so. First you have to make a needle, then feed it with thread and then finally start sewing. It took 20 years to design and build the needle. Last Wednesday we started to put thread through the needle’s eye. It will take some time before we have enough thread, tightly enough wrapped and in sufficient colors to start sewing. That will be later this year or next spring. If we are lucky there may be some parts of the picture where the image quickly comes clear; other parts of the picture may take a lot of time and careful work before the images can be discerned.”

Keep reading to find out the answers this tapestry may hold.

Only nature knows what happened in the long-ago dawn of the Big Bang; but soon humans will too. The visions of the new world will hopefully be tomorrow’s stories. If you want a machine to show how the universe was in the moments of creation, you don’t find it in the scientific instrument catalogs: you have to build it yourself. And so scientists and engineers around the world pooled their knowledge to build the Large Hadron Collider (LHC).

Immediately there were problems. Beyond the ability of a single continent, this became a truly global endeavor; unparalleled in ambition, in political and financial challenges. At its conception, the state of the art in cryogenics, magnets, information technology, and a whole range of technologies was far short of what would be required for the LHC to work. The whole enterprise relied on the belief that bright ideas would emerge to solve problems, any one of which could have proved a show-stopper. There were many who feared that particle physics had bitten off more than it could chew; that the LHC was over-ambitious; that this would be the end of physics.

Now we are almost there. Wednesday, Sept 10 when the current was turned on, and for the first time a beam of protons circulated through the vacuum tubes colder than outer space, was just the start. The next step will be to send two beams, in opposite directions – well, that’s been done but not yet intensely enough to smash into one another and produce data. That is still for the future. At first, and for some months, they are likely to be too diffuse and low energy to produce anything of great use to science. Only later when high energy intense beams collide, and the debris from those mini-bangs pour through the gargantuan detectors, which in turn speed signals to the waiting computers, will the moment we’ve waited for have arrived. A year or two accumulating data and the first answers to the big questions will begin to emerge.

The seeds of matter were created in the aftermath of the Big Bang: quarks, which clustered together making protons and neutrons as the newborn universe cooled, and the electron, which today is found in the outer reaches of atoms. We and everything hereabouts are made of atoms. In the sun and stars intense heat rips atoms apart into their constituents, electrons, protons and neutrons.

By colliding beams of particles, such as electrons or protons, head-on, it is possible to simulate the high-energy hot conditions of the stars and the early universe. At CERN (European Council for Nuclear Research) in the 1980s a machine called LEP (Large Electron Positron collider) collided electrons and their antimatter analogues, positrons, fast enough that they mutually annihilated and created for brief moments in a region smaller than an atom, the conditions that occurred within a billionth of a second of the Big Bang. Trying to reach time zero is like finding the end of the rainbow, and the LHC will take us ten to a hundred times further than ever before. At the LHC the beams of protons will pack a bigger punch and their collisions will show how the universe was at its infancy and perhaps give us some insight to how the universe evolved.

Within a billionth of a second after the Big Bang, the material particles from which we are made, and the disparate forces that act on them, had become encoded into the fabric of the universe. However, the events that led our universe to win the lottery of life were decided earlier than this. Some of them we believe occurred in the epoch that is now within our reach. That is what the LHC promises to reveal.

As the 21st century begins, physics can explain almost all of the fundamental phenomena revealed in the search for our origins, yet there are niggling loose ends. We see hints of a unified theory vaguely in the shadows, but what it is and how the structures that led to the particles and forces that molded us are still perceived only vaguely.

Why are there three spatial dimensions; could there be more? Cosmology suggests that “normal matter” is but one percent of the whole, and that we are but flotsam on a sea of “dark matter”. What that dark sea consists of, how it was formed, why there is any matter at all rather than a hellish ferment of radiation, are unknown.

Why is there structure and solidity to matter when our theories would be happier if everything flitted around at the speed of light? Theorists believe that all structure and ultimately the solidity of matter are the result of a field of force that today permeates the universe known as the Higgs field. This can be made to reveal itself if the conditions are right. For example, as an electromagnetic field can be stimulated to send out electromagnetic waves, so can the Higgs field create waves. However to create these waves requires huge energy. The LHC has been designed to achieve these conditions. As an electromagnetic wave comes in quantum bundles, particles known as photons, so the Higgs waves will come in the form of particles known as Higgs bosons.

There is also the question: why there is anything at all? In the beginning there was nothing: “there was darkness on the face of the void”. Then came a burst of energy: “let there be light and there was light”, though from where it came no-one knows. What we do know is what happened next: this energy coagulated into matter and its mysterious opposite, antimatter, in perfect balance. Anti-matter destroys anything it touches in a pyrotechnic flash. So how did the early universe manage to survive self-annihilation between the newly born matter and antimatter? Something as yet unknown must have occurred in those first moments to upset the balance. For several years we have glimpsed a subtle asymmetry between arcane forms of matter and antimatter made from “strange” and “bottom” quarks and antiquarks. One of the goals of the LHC will be to produce large numbers of particles of bottom matter and their antimatter counterparts in the hope of finding the source of the asymmetry between matter and antimatter.

Ultimately however, this is a voyage of discovery into a world that once existed but was lost in the sands of time, 13.6 billion years ago. Like some astonishing Jurassic Park, the LHC will show once more what that epoch was like. We have ideas of what is to be found, and there are certainly questions, such as those above, whose answers we crave. But in focusing on them like this we are getting ahead of ourselves. We are at the stage of witnessing remarkable engineering, and it is those we should be applauding; as for discoveries in fundamental science – watch this space.

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