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Neutrino prediction proved wrong

Researchers have been worried about the discrepancy between the experimental data and simulations at Super-Kamiokande for some time. According to the simulations, the experiment was detecting too few muon neutrino events or too many electron neutrinos. Boezio and others decided to tackle the discrepancy by making measurements in the atmosphere.

Atmospheric neutrinos are created by so-called secondary cosmic rays in the Earth’s atmosphere. These are created when galactic cosmic rays – called primaries – collide with nuclei in the atmosphere. Approximately 85% of the primary cosmic rays are protons and 12% are alpha particles. The rest are electrons or the nuclei of heavier atoms. As they enter the Earth’s magnetic field, the primary cosmic rays are accelerated to kinetic energies over 1 GeV. Both the primary and secondary cosmic rays create muons, which decay into neutrinos. Between a quarter and a third of the muon’s momentum is transferred to the neutrino. Boezio and his colleagues therefore measured the number of muons in the Earth’s atmosphere and compared their results with the number and energy of the neutrinos detected by Super-Kamiokande. Their results were closer to the experimental number of neutrinos measured by Super-Kamiokande than the result of the simulations. It seems as if the simulations have been overestimating the number of muon neutrinos that should be detected by Super-Kamiokande by 36%.

Gemini telescope passes first hurdle

Gemini-North is situated on top of Mauna Kea, an extinct volcano some 4200 meters above sea level. Mauna Kea is a popular location for telescopes because of its high altitude and clear skies. The 8-meter Gemini telescopes are the latest in a new generation of large telescopes that already includes the two 10-metre Keck telescopes in Hawaii, the 8-metre Subaru telescope, also in Hawaii, and the Very Large Telescope, a set of four 8-metre telescopes in Chile. Two of the four telescopes in the VLT have been completed.

The Gemini telescopes will allow astronomers to view the faintest and most distant objects in sky at near infrared wavelengths, where stars are not obscured by vast interstellar dust clouds. “Astronomy is about origins,” says Malcolm Longair of Cambridge University, a member of the governing board of Gemini. “We want to study the origins of the universe, the origins and galaxies, stars and planets and even the origins of life itself.”

Observing time on the telescopes will be split between the Gemini partners according to their financial contribution to the project. The breakdown will be: US 47.6%, UK 23.8%, Canada 14.3%, Australia 4.8%, Chile 4.8%, Argentina 2.4%, Brazil 2.4%. Over the next five months, Gemini scientists will calibrate and test the instruments on the telescope, and will announce in November which instruments are available for the start of observations in January 2000. Gemini managers will use a procedure called Q-mode observing to ensure that the instrument best suited for observations at a particular time is used. For example, if weather conditions change so that they are more favourable for observations in the near-infrared as opposed to the visible, the telescope will switch to near-infrared instruments.

In common with other large telescopes and radio telescopes, Gemini will have to live with interference from satellites in low-Earth orbits. These satellites interfere with the lasers used by Gemini to operate its “active optics” system, which allows it to make corrections for the effects of atmospheric turbulence on observations. “It’s a growing problem,” says Gemini project director, Matt Mountain.

AMS hints at cosmic-ray mystery

The experiment also found that changes in the strength of the Earth’s magnetic field with latitude do not alter the number of low-energy protons hitting the Earth’s atmosphere. However the experiment failed to detect any anti-helium atoms among the three million ordinary helium atoms that it detected. The two main goals of the experiment are to detect anti-matter left over form the big bang (as opposed to anti-matter created by high-energy cosmic rays crashing into particles in space), and to detect “dark matter” particles. As much as 99% of the universe is thought to be made up of dark matter but it is difficult to detect because it does not emit radiation (hence the name dark).

The AMS project is a collaboration between 37 research institutions in China, Finland, France, Germany, Italy, Portugal, Romania, Russia, Spain, Switzerland, Taiwan, Korea and the United States.

Defects work for laser

The photonic crystal was made by using an ion beam to drill a 2D hexagonal array of holes in a layer of indium gallium arsenide phosphide (InGaAsP). The regular spacing of the holes means that only certain wavelengths of light can propagate in the crystal. The holes were 515 nm apart and had a radius of about 180 nm. The crystal was prepared such that one of the holes was “missing” – this defect provided the laser cavity for the device. Photons are trapped in the defect, which is only 0.03 cubic micrometers in size. When cooled to 143 Kelvin, the device emitted pulses of laser radiation with a wavelength of 1.5 microns.

Has man caused climate change?

The Earth’s average global temperature has increased by 0.6 Kelvin in the past 100 years. There are believed to be four main processes that can effect the Earth’s climate. Two of these, small aerosol particles from volcanic eruptions and changes in solar luminosity, occur naturally. The other two, sulphate aerosols and greenhouse gases such as carbon dioxide, are due to increasing industrialization, in particular the burning of forests and fossil fuels.

Lockwood and colleagues found that the total magnetic flux leaving the Sun has risen by a factor of 1.4 since 1964, and has probably increased by a factor of 2.3 since 1901. Their results could provide support for the theory that changes in the solar wind – a stream of charged particles emitted by the Sun – could contribute to climate change. The solar wind and the Sun’s magnetic field are intimately linked. According to the theory charged particles in the solar wind would deflect high-energy cosmic rays that would otherwise have ionized the Earth’s lower atmosphere, leading to the formation of clouds. Since cloud cover determines the amount of solar radiation reflected by the Earth back into space, a more powerful solar wind implies less cloud cover which, in turn, suggests that the Earth would warm up.

However, the paper by Tett and colleagues suggests that natural effects alone cannot account for the pattern of temperature change observed over the past 50 years. They used the HadCM2 computer model to predict the Earth’s global temperature during five overlapping 50-year periods (1906-56, 1916-1966, .), and then compared the results with observations. The program models both the oceans and the atmosphere, and also allows for changes in greenhouse emissions, surface albedo (i.e. reflectivity), volcanic aerosols and solar irradiance. They ran the programme with a number of different solar models, including one that matched the effects highlighted by Lockwood. The results were similar for all cases: it is not possible to distinguish between the contributions of human activity and natural variations to global warming in the first half of the century, but after 1946 increases in the concentration of man-made greenhouse gases and sulphate aerosols was the dominant effect.

Neutrino lab sees “first light”

The observatory is a joint project between Canada, the US and the UK, and was officially opened last year. It is the first detector that is capable of distinguishing between the three different types of neutrino – electron, muon and tau neutrinos. Neutrinos are generated by nuclear reactions deep inside the sun, by cosmic ray interactions in the atmosphere, or by violent astrophysical events such as supernovae explosions.

“Detecting any neutrino is no mean feat, and SNO is attempting to do it in a way that no one has ever tried before, ” says David Wark, a team member from Oxford University. “We have spent more than a decade trying to reach the lowest levels of radioactive contamination ever seen while building a complex detector the size of an apartment block in the dreadful conditions at the bottom of a very deep mine. Some of my friends doubted my sanity, and frankly I was starting to agree with them.”

Neutrinos travel at the speed of light and only interact with matter via the weak force, which makes them extremely difficult to detect. Neutrino detectors must be placed hundreds of metres below ground to isolate them from cosmic rays, and must be made from ultrapure materials to prevent natural radioactivity mimicking neutrino interactions. When a neutrino interacts with the heavy water at SNO, a faint flash of Cerenkov radiation is emitted and recorded by the photomultiplier tubes. When 30 detectors see at least one photon each at the same time, the observatory registers it as an event. Only 10-20 solar neutrino events are expected per day.

Astronomers hope to use the Sudbury detector to confirm the evidence for neutrino mass obtained at the Super-Kamiokande detector in Japan last year. An accurate measurement of the mass could help solve the ‘solar neutrino problem’ – the fact that existing experiments detect less than half the solar-neutrino flux predicted by theory. The Super-Kamiokande results suggest that electron neutrinos are oscillating into muon neutrinos, which cannot be detected by existing neutrino observatories. As Sudbury can detect muon neutrinos, it should record a higher flux of solar neutrinos than Super-Kamiokande.

Feynman’s spirit lives on in computing

Richard Feynman, both as a man and as a scientist, excited varied reactions: you either loved him or you hated him. As a man, he was either narrow-minded and sexist, or else charming and completely fair in the most unselfconscious way. As a scientist, he was either “a magician” – the most impressive kind of genius – or else he was “not in the first rank of physicists”. This book will not offer much guidance among this range of opinions, since it is mostly about computation, rather than Feynman. However, the snapshots of – and reactions to – that fascinating personality come as a welcome, refreshing stream running through the technical essays that form the bulk of the text.

Feynman is rightly remembered chiefly for his work on quantum electrodynamics, for which he shared the 1965 Nobel Prize for Physics, and for his three-volume Lectures on Physics. The fact that he worked on the basic principles of computation in his later years has often been regarded as a relatively minor afterthought, but it is becoming more and more clear that Feynman was better at picking his subjects than that implies. After all, it is more important in science to recognize the interest of something significant but not fully understood, than it is to fully understand something insignificant. In the study of computation and its limits, which are set by the underlying laws of nature, we have an example of the former. Although Feynman did valuable work in the early exploration of this subject, his most important contribution was to generate interest in it.

This book is a loosely connected collection of technical articles, lectures and anecdotes selected by Anthony Hey, head of computing at Southampton University. It takes us from stimulating contributions by Feynman himself – such as his famous 1959 lecture “There’s Plenty of Room at the Bottom”, which foresaw nanotechnology, and the clear and focused “Simulating Physics With Computers” lecture from 1981 – to 16 papers, by 16 authors, of varying degrees of precision and readability that cover some of the questions thrown up by the subject. These range from fundamental physics, such as the nature of information, to practical issues such as progress in metal-oxide-silicon technology, with room for exploratory ideas and open questions.

Hey has gathered the papers together under five loose headings – “Feynman’s Course on Computation”, “Reducing the Size”, “Quantum Limits”, “Parallel Computation” and “Fundamentals” – but a weakness is that the collection is not very coherent. It is neither a guide nor an introduction to the subject, nor even a “volume 2” to the earlier Feynman Lectures on Computation (Perseus, 1996), which contained transcripts of a lecture course that Feynman gave in the early 1980s. This book instead provides a tour round some of the issues. The standard varies considerably from author to author, but the introductory overview is well written and succeeds in binding the book together. Indeed, it is a pleasure to find historical notes and scientific analysis next door to one another – a welcome reminder that science is a human endeavour.

After the gentle introduction, we plunge straight into a technical paper by John Hopfield. This is an update of his 1982 paper on neural networks, and is an important contribution – but hard work for the reader. I feel it would have benefited from some illustrative examples of what has been learned since 1982. In contrast, the paper by Gerry Sussman and Jack Wisdom, showing (from specialized computer hardware) that the motion of Pluto is chaotic, stands alone very well. It is not only readable and self-contained but also technically precise and impressive – although again I would have enjoyed a few more descriptive comments. It is left to Marvin Minsky to state the implication that there is sufficient instability in the solar system to throw the Earth out into space one day (unless it is first swallowed up by the Sun swelling to red-giant proportions).

Several of the authors mention Feynman’s championing of real understanding in science. Carver Mead, for example, uses the following apt Feynman quotation: “The real glory of science is that we can find a way of thinking such that the law is evident.” Mead contributes two technical chapters. The first discusses a new approach for combining electromagnetism and quantum mechanics that avoids Maxwell’s equations and starts instead from experimental observations on a loop of superconducting wire. Although his approach is interesting, I am not convinced that it would be the most insightful route to take. “Nowhere in natural phenomena, ” proposes Mead about superconductors, “do the basic laws of physics manifest themselves with more crystalline clarity.” Give me a Young’s slit electron interference pattern any day.

The section on “Reducing the Size” opens with Feynman’s “There’s Plenty of Room at the Bottom” lecture, which is a pleasure to see made available for a wide readership, and which sets a standard for all scientific after-dinner speakers. Feynman’s speech was visionary, and Mead carefully surveys what has happened in practice since then (i.e. metal-oxide-silicon technology), and where things are heading. There is also a chapter by the late Rolf Landauer entitled “Information is Inevitably Physical”, in which he gives opinions and historical notes that help to draw attention to several overlooked contributions.

Quantum computers appear in the section entitled “Quantum Limits”, and the subject is well introduced by Feynman himself, as well as by Charles Bennett and Richard Hughes. Bennett is lively as well as precise. “Quantum computing, ” he says, “is like controlled fusion” – in other words, it promises much, but may take many years to achieve. He also argues that quantum information and communication, not quantum computing, is the “wild west, or Internet” of quantum information science. Hughes, meanwhile, gives a clear and steady discussion of both the theory and practice of quantum computing. However, I found the chapter by Paul Benioff much less useful. It aims to say something about “quantum robots”, which are quantum machines with on-board quantum computers, operating in a quantum environment. But his treatment amounts to writing down sums over quantum states and time-steps, with little insight into what is going on.

Several of the chapters discuss cellular automaton computers. These are the type of updated array computations made widely known by Martin Gardner’s article in Scientific American on John Conway’s “Game of Life”. The chapter by Norman Margolus is excellent, clarifying what can and cannot be done, explaining what are the interesting questions, and incorporating good illustrations. The chapter would allow a beginner to understand what is going on and get to more advanced concepts, such as invertible rules and partitioning. It is also thorough and carefully referenced.

In separate chapters, Minsky and Tommaso Toffoli tackle the idea that the natural world might be like a grand cellular automaton. They try to see if reasonable assumptions about microscopic computing cells distributed throughout space could give rise to laws of physics as we know them, including things like quantum dynamics and relativity. However, I do not know why Hey has assigned these two chapters to different sections of the book, as I feel they should both have been in the section on “Fundamentals”. Toffoli makes a better stab at the task, which renders Minsky’s chapter less interesting by comparison. But one is left with the feeling that the theory is not going to work out with the elegance we look for, and that nature will in fact surprise us with something else that we have not thought of. Wojciech Zurek then follows with a good discussion of Maxwell’s demon and “algorithmic entropy”.

Two chapters seem rather empty to me. These are Geoffrey Fox on “Internetics”, which presents experience of large-scale computing dressed in the muddling language of management structures, and John Wheeler on “Information, Physics, Quantum: the Search for Links”, which seems profound but actually is a fine example of the tale of The Emperor’s New Clothes.

One thing that emerged from the book was a rather lovely glimpse or sketch of the quality of the final period of Feynman’s life. This was not well covered in James Gleick’s biography Genius: Richard Feynman and Modern Physics, but sometimes the heart of a person emerges with greater clarity as they approach death. The chapter by Daniel Hillis, “Richard Feynman and the Connection Machine”, is a wonderful essay, beautifully written: mathematics, history and friendship brought together in Feynman-esque clarity with all the poise and care of a poem.

Element 118 discovered at Berkeley

The new elements were made by bombarding a lead-208 target with an intense beam of high- energy krypton-86 ions over an 11-day period. The krypton ions were accelerated by the 88-inch cyclotron at the Lawrence Berkeley National Laboratory in California. Three atoms of element 118 were detected, all containing 118 protons and 175 neutrons. The atoms decayed to element 116 in less than a millisecond by emitting an alpha particle, and continued to decay by alpha- particle emission all the way down to element 106. “The observation of a chain of six high-energy alpha decays within about one second unambiguously signalled the production and decay of element 118, ” said Ken Gregorich, who led the research team.

The lead-krypton scheme for producing element 118 was suggested by Robert Smolanczuk from the Soltan Institute for Nuclear Studies in Poland earlier this year. Before Smolanczuk’s calculations it was thought that the “cold fusion” technique would not be able to create elements above element 112.

Bill Richardson, head of the US Department of Energy, which runs the Berkeley laboratory, used the discovery to highlight the importance of openness at US national labs. “Scientific excellence does not recognize national boundaries, ” he said. “We will damage our ability to perform world-class science if we cut off our laboratories from the rest of the world.” Security at the labs has been increased following the recent revelations about the leaking of nuclear secrets from Los Alamos to China, and restrictions have been placed on non-US nationals working at the labs. Four of the team that discovered element 118 were born in Germany.

Cosmology bestsellers


1. The Elegant Universe: Superstrings, Hidden Dimensions, and the Quest for the Ultimate Theory by Brian Greene

A fascinating and thought-provoking journey through the mysteries of space, time, and matter. Today physicists and mathematicians throughout the world are feverishly working on one of the most ambitious theories ever proposed: superstring theory. String theory proclaims that all of the happenings in the universe are reflections of microscopically tiny vibrating loops of energy, a billionth of a billionth the size of an atom. Brian Greene, one of the world’s leading string theorists, relates the scientific story and the human struggle behind twentieth-century physics’ search for a theory of everything. The Elegant Universe makes some of the most sophisticated concepts ever contemplated viscerally accessible and thoroughly entertaining. Read a news story on the book.

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2. Unweaving the Rainbow: Science, Delusion, and the Appetite for Wonder by Richard Dawkins

Did Newton “unweave the rainbow” by reducing it to its prismatic colours, as Keats contended? Did he, in other words, diminish beauty? Far from it, says Dawkins.
With the prose that has made his books worldwide bestsellers, Dawkins addresses the most important and compelling topics in modern science, from astronomy and genetics to language and virtual reality. Richard Dawkins has written a tribute to science “not because it is useful (though it is), but because it is uplifting, in the same way as the best poetry is uplifting.”

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3. The Whole Shebang : A State-Of-The-Universe(s) Report by Timothy Ferris

Timothy Ferris provides a clear, elegantly written overview of current research and a forecast of where cosmological theory is likely to go in the twenty-first century. He explores the questions that have occurred to even casual readers: What does it mean to say that the universe is “expanding, ” or that space is “curved”? — and sheds light on the possibility that our universe is only one among many universes, each with its own physical laws and prospects for the emergence of life. Read a review.

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4. The Inflationary Universe : The Quest for a New Theory of Cosmic Origins by Alan Guth and Alan Lightman

Alan Guth is one of the inventors of inflationary theory. In this book he describes how he, with a number of colleagues, wrestled with attempts to match the standard ‘big bang’ model of cosmology with astronomical observations gathered in the latter part of the 20th Century. The result is a theory of “inflation” which postulates that the universe underwent an incomprehensibly large expansion in the first fraction of a microsecond of its existence. As a first-person account, it is along side The First Three Minutes as a standard book that every scientist interested in astronomy should read.

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5. The Life of the Cosmos by Lee Smolin

Cosmologist Lee Smolin offers a startling new theory of the universe that is radically different from anything proposed before. He argues that the laws of nature may be subject themselves to natural selection. Read a review.

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6. Mere Creation; Science, Faith & Intelligent Design by William A. Dembski (Editor)

Nineteen experts trained in mathematics, mechanical engineering, philosophy, astrophysics, ecology, evolutionary biology, and other disciplines challenge the reigning ideology of materialistic naturalism on both scientific and philosophical grounds, as they press their case for a radical rethinking of established evolutionary assumptions.

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7. Probability 1 : Why There Must Be Intelligent Life in the Universe by Amir D. Aczel

Carl Sagan believed it–now the bestselling author of Fermat’s Last Theorem tries to prove it. Basing his book on the discoveries being made by the Hubble telescope, data emerging from Mars, and knowledge about life at the extremes, Aczel pulls together everything science has discovered, and mixes in probability theory to argue the case for the existence of intelligent life beyond this planet.

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8. Stephen Hawking’s Universe : The Cosmos Explained by David Filkin and Stephen Hawking

Stephen Hawking’s Universe is a journalistic rewrite of A Brief History of Time. It reveals step-by-step how we can all share his understanding of the cosmos, and our own place within it. Many readers will consider it an easier read than Hawking’s famous bestseller.

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9. The Little Book of the Big Bang : A Cosmic Primer by Craig J. Hogan

The Little Book of the Big Bang explains what modern cosmology is all about: What happened at the beginning, how matter formed, how structure formed, what may happen to the universe in the future – and most important, how we know all this. Although aimed at the layman, personal reviews at Amazon seemed mixed on how effective the book is at explaining some of the standard astronomical concepts.

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10. Before the Beginning : Our Universe and Others by Martin J. Rees

In this engaging and carefully reasoned account of our universe and its place within a grander scheme, one of the UK’s most eminent astronomers draws together recent advances in astrophysics and up-to-the-minute research to cast a piercing light on man’s place in the cosmos. Highly readable and recommended.

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Fractals determine date of paintings

The physicists scanned a series of Pollock’s artworks into a computer and masked each painting with a series of grids. They then counted the number of squares that contained part of the painted pattern (N) – using the well-know ‘box-counting’ method of fractal geometry – and reduced the size of the squares (L). The largest square was the size of the painting while the smallest was 1mm. The fractal behaviour of the painting could then be pinpointed by plotting a log graph between the two values N and L. They discovered that Pollock’s paintings consist of two distinct fractal patterns. One was determined by the paint dripping on the canvas and gradually becomes finer over time. The other pattern was shaped by his motions around the canvas.

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