Skip to main content

Physicist shares Japan Prize

The prize was awarded in the category “Generation and Design of New Materials Creating Novel Functions.” Ironically, when Esaki first submitted his paper describing the use of thin-film growth techniques to engineer new semiconductor materials, it was rejected by Physical Review Letters because it was “too speculative” and involved “no new physics.” Esaki was working for IBM at the time and later published a shortened version of the paper in the IBM Journal of Research and Development .

Superlattices crystals are composed of layered thin films that exploit quantum effects to generate unusual electrical and optical properties now used in a wide variety of semiconductor products. Almost half of the world’s semiconductor physicists now work in this area.

Esaki was born in Osaka in 1925 and received both his BSc and PhD from the University of Tokyo. He received the Nobel prize for his PhD work on what is now known as the Esaki tunnel diode.

Sensenbrenner criticises Shuttle-Mir missions

The missions were established “for all the wrong reasons” and gave the impression that scientific co-operation is a form of foreign aid, Sensenbrenner told the Indian Science Congress Association in a recent speech. He said that the Shuttle-Mir mission, worth $400 million, was compensation to Russia for the cancellation of a rocket technology deal with India in 1994. “I disagree with the President Clinton’s chief scientific advisor, Jack Gibbons, who offers ‘no apologies’ for the fact that US-Russian co- operation is part of overall US foreign policy, not just space policy” he said.

Sensenbrenner was also concerned about international agreements in general, noting that over 90 percent of NASA’s space projects now have international components. He seemed more optimistic when discussing the recent agreement between the US and CERN, the European particle physics laboratory, hailing it as a classic example of how US scientific interests are best served. “The lessons learned during the negotiation of the LHC [at CERN] agreement should be applied to any scientific negotiations that the US undertakes.” Sensenbrenner hopes a similar contract will be undertaken with negotiations for the International Thermonuclear Experimental Reactor (ITER).

Physicists honoured at the Savoy

The awards were presented by Brian Manley, president of the Institute. Speaking before the presentations, Manley stressed the importance of education to the UK and outlined his hopes for the Institute’s 16- to 19-year old curriculum initiative. Manley also called for increased investment in science education and basic research in the physical sciences.

The guest speaker, Peter Williams, chairman of Oxford Instruments, also stressed the importance of education and the need for science to capture the hearts, minds and imaginations of the young. Williams also took issue with recent suggestions that the 21st century would be the century of biology, or the Internet, saying that every area of science, engineering and technology would play a central role in the next century.

The Institute of Physics Awards 1998
President’s Medal: Lord Dainton

Premier awards
Glazebrook Medal & Prize: Cyril Hilsum
Guthrie Medal & Prize: Derek Charles Robinson
Paul Dirac Medal & Prize: David Deutsch

Principle awards
Max Born Medal & Prize: Gerhard Abstreiter
Harrie Massey Medal & Prize: Donald Blair Melrose
Holweck Medal & Prize: William Gelletly

Senior awards
Charles Vernon Boys Medal & Prize: Shaun Neil Fisher
Bragg Medal & Prize: Maurice George Ebison
Duddell Medal & Prize: Meirion Francis Lewis
Kelvin Medal & Prize: Lesley Scott Dent Glasser
Maxwell Medal & Prize: Andrew James Fisher
Paterson Medal & Prize: Neil Loxley
Rutherford Medal & Prize: Anthony Michael Hillas

Science budget fails to match inflation in the UK

In a now common procedure, the actual figures were released in a written answer to a question from a MP, thus avoiding any debate about the figures. The figure for the next financial year will be £1, 338.326 million, an increase of 0.6% on last year but 2% below the official inflation rate.

However, the figures for the two research councils which support most of the physicists in UK universities have fallen slightly. The budget of the Engineering and Physical Sciences Research Council (EPSRC) is down by 0.87%, while that of the Particle Physics and Astronomy Research Council (PPARC) will fall by 0.3%.

The lobby group Save British Science Society was not impressed: “this is not what we expect from a government whose Prime Minister has committed it to correcting the effects of past under-funding” it said in a press release.

Science Budget allocations

£ million
1997-98 1998-99
BBSRC 183.300 185.739
ESRC 64.896 65.990
EPSRC 386.373 382.982
MRC 289.070 290.208
NERC 165.116 171.771
PPARC 191.850 191.268
International Subscription Reserve 8.800 3.028
CCLRC 1.450 1.462
Pensions 11.530 12.298
Royal Society 22.271 22.621
Royal Academy 3.370 3.436
OST Initiatives 2.302 2.376
Joint Research Equipment Initiative — 4.147
LINK/Foresight — 1.000
Total 1, 330.327 1, 338.326

Light gets in your eyes

To do this Levy adapted a technique used by solar astronomers in which a black disk is placed in the focal plane of the telescope. The size of the disk is chosen so that it exactly matches the Sun’s image in the focal plane, allowing astronomers to observe the delicate structure of the corona. Levy hit upon the idea of splitting a mirror or visor into an array of optical components. He then placed a layer of a photosensitive material, such as indium tin oxide, in the focal plane of each component. As light intensity increases, the layer becomes optically thick. However, only those segments being illuminated by light from bright objects get dark, and the rest of the image can pass through the array. Such a device could have applications in rear-view mirrors, or cars, or in binoculars.

A lucid account of the universe

A more detailed review by Bernard Pagel of the Nordic Institute for Theoretical Physics (NORDITA) appears in the January 1998 issue of Physics World

Some 30 years ago, the hot big-bang paradigm was dramatically confirmed by the discovery of the microwave background radiation and its precise black-body nature. Since then, cosmology has advanced at a rapid and accelerating pace. It has also developed widening contacts with related sciences, notably particle physics.

The Whole Shebang by Timothy Ferris is enlivened by imaginative chapter titles, literary quotations, personal anecdotes, and interviews with many of the leading protagonists in the field. Without any mathematics in the main text, the author explains difficult concepts with remarkable lucidity and conciseness, while the end-notes and glossary are invaluable mines of information.

There are, however, a few technical inaccuracies in the book. For example, Ferris ascribes the time-dependence of the Hubble “constant” to deceleration, and gives an uncharacteristically inadequate explanation for the Sunyayev-Zeldovich effect. He also suggests that all carbon survives when it acts as a catalyst in the carbon-nitrogen-oxygen cycle of hydrogen-burning in stars, and says that a single photon going through a double slit makes a complete interference pattern.

These criticisms do not, however, seriously detract from the overall picture. This is an outstandingly learned, well written, lively and thought-provoking book – and a great read.

Superficial images

Reviewed by Matin Durrani

Felice Frankel, the renowned landscape photographer, was hosing her driveway one Sunday afternoon when she decided to search for one of the more interesting puddles. After dropping some oil onto the water, she waited half an hour until the diffraction colours caught her eye, and then captured a stunning image of the oil slick on camera.

It is just one of 58 intriguing images of the surface of objects taken by Frankel, who is also an artist-in-residence at the Massachusetts Institute of Technology. Her pictures range from ferrofluids, liquid crystals, microelectrodes and optical waveguides, to unfamiliar views of everyday objects like soap bubbles, gemstones, “tears” of wine and drops of water. Interesting notes at the end of the book explain the photographic techniques that Frankel used, while the accompanying text by George Whitesides, a chemistry professor at Harvard University, clearly and lucidly explains the science behind the surfaces.

Weighty history misses mark

Reviewed by John Maddox

If war is too important to be left to the generals, then surely the research community should be on its guard against leaving the history of discovery to the historians of science who have recently captured their eponymous field. That must surely be the reasonable person’s first reading of this well intentioned but shapeless book. The second reading may be a little more sympathetic: there is some good stuff buried in these 939 pages, but it has to be winkled for – not easy with a object that weighs more than 2.2 kg, the upper limit of the Maddox kitchen scales.

The declared intention gives the game away. The editors say in their introduction that “what is science?” is the first question that “anyone has in mind” when opening a book entitled Science in the 20th Century. (It isn’t, of course: people who buy this type of book believe they know what science is, although they may be surprised and even disillusioned by what they read in what they buy.) The editors begin their next paragraph by saying “The current definition which scientists give is one answer…”, but then add that they “cannot but give particular weight to it”, saying that it would be “unwise to reject…out of hand” the opinions of “epistemologists, historians, sociologists, engineers, professional popularizers, politicians…or the ‘man in the street'”. (Why engineers are in such dubious company is not explained.) In fact, the 48 chapters that follow give far less than “particular weight” to the opinions of the practitioners, but indulge the sociologists ad lib.

By now, of course, the whole world knows that there has recently been a revolution in the history of science. Academic practitioners of the trade have rejected the idea that their job is to sing the praises of great men and women and celebrate their intellectual achievements. Instead, the “social context” is what matters now. From there it is only a short step to the view that the content of science is moulded by the prevailing social context, and that it has no greater force than any other “point of view”.

The more polite components of this message are spelled out by Michael Aaron Dennis from the Department of Science and Technology Studies at Cornell University in his introductory chapter entitled “The Historiography of Science”. This turns out to be an account of the revolution in the history of science before and after the Second World War. Like others, Dennis places the seeds of revolution in the second international congress of the history of science held in London in 1931, and in particular in a paper on Newton read at the congress by Boris Hessen, one of a substantial Soviet delegation.

Nobody denies the interest and importance of that occasion. Hessen’s paper made two points at great length – namely that Newton would have formulated the principle of energy conservation if only the steam engine had already been invented, and that Newton’s Principia was not so much a work of genius as a response to the military needs of the time. Nothing in what follows in this review should be taken to suggest that these are improper lines of inquiry. Indeed, they are of great interest. However, the question is whether those who follow these inquiries prove their case as often as they would like the rest of us to believe. And, in any case, can contextual studies of that kind validly be passed off as the history of science?

Dennis is especially revealing in his discussion of the history of science in the US during and immediately after the Second World War, culminating in the publication of Science: The Endless Frontier – the influential argument by Vannevar Bush in favour of US government support for basic research. Like a real historian, Dennis uncovers the origins of this document, in which the physicist- historian Bernard Cohen and the historian George Sarton had an important hand.

Dennis tells how James Conant (in his role as president of Harvard) sought to make the history of science a “servant of science” when he was planning his undergraduate course “NatSci-4”, which introduced non-scientists to science. A dedicated band of Harvard acolytes set about preparing case histories of discovery that were, in Dennis’ opinion, a pedagogical failure. People like the physicist Gerald Holton come poorly out of the episode; the hero is Thomas Kuhn, who was following the course, saw through the sham and later (when at Yale) wrote The Structure of Scientific Revolutions. That too, says Dennis, was when historians of science saw that the history of science is a discipline in its own right, and not dependent on the sciences.

With marching orders like these, it is not surprising that the contributions that follow are a disparate collection, hardly likely to give any kind of reader a connected account of science in the 20th century. The chapters are divided into two main sections, one labelled “Science and the Social Fabric”, and the second called “Research Dynamics”. The second is the more interesting, but often suffers from the fact that the contributors feel they need to give sociological considerations their due. Moreover, some contributors write of the disciplinary history of their subjects – for example, which institutions sprang up, where and when – rather than writing about the intellectual content.

Thus Harmke Kamminga from the Wellcome Unit for the History of Medicine at Cambridge University, writing on “Biochemistry, Molecules and Macromolecules”, marvels that biochemistry had such diverse beginnings (animal metabolism, nutrition, chemical pathology and so on) and at its continuing “permeability” to influences from other fields of science (genetics, for example, now). Historians, he says, are hard-pressed to define biochemistry and will not be able to do so until there has been a detailed and comparative analysis of the “stated intentions of those who self-consciously promoted and practised the new biochemistry…” and of “changes of major objectives over time”. Really?

That difficulty is also said to be relevant to understanding why biochemistry sprang into life in the first decade of this century. Curiously, Kamminga does not mention Emil Fischer. His work on carbohydrates, proteins and even nucleic acids is likely to have set competitive juices flowing in all kinds of university departments outside Germany. (Fischer does, however, rate a mention in Mary Joe Nye’s chapter entitled “Atomic and Molecular Science 1900-1960”.)

For my money, one of the best chapters is the one on high-energy physics by Sam Schweber from the physics department at Brandeis University. At the outset, he takes a self-denying ordinance, saying that “big science” inevitably has political connotations because of the costs, and that he will therefore ignore them. But quite what people other than those in the field will make of ideas such as “symmetry breaking”, which is not fully explained, is anybody’s guess. Michael Mahoney of Princeton University also gives an excellent account of the search for theories of computation, which has the virtue of emphasizing the link with Chomsky’s theories of language.

On the other side of the coin are the more general articles such as “From Eugenics to Genetic Manipulation” by Daniel Kevles of the Division of Humanities and Social Sciences at California Institute of Technology. It is true that the term “eugenics” was invented by Francis Galton in Britain in 1883, but is it constructive – let alone fair – to describe everything that has happened since then in applied human genetics (including the pre-natal diagnosis of fetuses with Down’s syndrome) as part of the waxing and waning of Galton’s naïve ambition? And what exactly does it mean to conclude, as Kevles does, that “…the flow of history compels us to think and act anew – not about eugenics, but about the control of human genetic information by geneticists, the media, insurers, employers and government”?

This monumental volume is thus a disappointment, to say the least. (“Monumental” is not a cheap reviewer’s joke: the sheer bulk of the printed pages detached one of the covers in my copy. The weight arises from the publishers’ decision – no doubt in response to a demand for the facility to place illustrations anywhere in the text – to print it on heavily coated paper, which also means that the text must be read in uniform light.) I can think of no category of reader who would read through cover to cover and have the feeling that he or she then knew something in the large about science in the 20th century that they did no know before. Nor would a newcomer to science have a sense of what were the great landmarks of the century almost past – such as relativity, quantum mechanics, Hubble’s law and the structure of DNA. The aftertaste is more likely to be the sense of having read an extra-large issue of a journal such as Social Studies in Science.

With that said, the book does serve both by declaration and example to make the ambitions of the new historians explicit. In my opinion, studies of the social, political and ethical connotations of science are interesting, important and entirely legitimate. Moreover, in open societies, there is no way in which they can be suppressed. But there is also a need for an “internal” history of science, to use the language of this book. In other words, we need an account of the remarkable developments of the past 100 years that reflects the recurring difficulty of solving problems that have not been formulated at earlier times – and of the endless false starts that arise as a consequence. That is what the research community could do for itself. It could also do more to demand that its independent academic colleagues in the history of science submit their publications to the rigorous peer-review that is commonplace in science proper.

Fermion first for quantum interference

Bosons (for example, photons) cause constructive interference patterns. This means that the probability that both particles are detected in the same direction is enhanced by the intereference.

On the other hand fermions (such as electrons), are predicted to cause destructive interference patterns. This suggests that, compared to classical physics, the probability of finding the particles moving in the same direction after a collision should decrease. Such quantum interference is responsible for the Pauli exclusion principle, which states that two electrons can never occupy the same state.

Yamamoto and colleagues at Stanford and NTT Basic Research Laboratories in Japan have designed an experiment to observe this behaviour. The apparatus depended on a mesoscopic electron beam splitter etched onto a gallium arsenide electron gas system. To reduce current noise, the apparatus was cooled to 1.6 Kelvin. According to their calculations, the fermion collision noise level should be 52% that of the classical collision noise level if no quantum effects occur. However, the researchers measured a suppression of collision noise level which averages to 56% of the classical value, thus indicating the presence of quantum interference.

Perrin’s hypothesis reborn

In a unimolecular reaction a molecule breaks into two smaller molecules (or atoms) in a manner that appears to be independent of the chemical composition of its surrounding. The number of molecules falls exponentially with time. Perrin’s radiation hypothesis is based on two conjectures: the reacting substance has to absorb radiation at the frequency required for activation and, secondly, the radiation density had to be high enough to supply the energy for activation. Langmuir discredited the theory by pointing out that the activation energies for such reactions are in the ultraviolet frequency range and that the molecules involved are known not to absorb energy in this region.

Seventy years later researchers realized that there may be some situations in which the radiation model might work. Large molecules can absorb energy in the infrared region and the radiation density is also high enough for activation to occur. However, a lack of experimental data in the low-pressure regime caused the theory to be rejected again.

Robert Dunbar of Case Western Reserve University in the US and Terrance McMahon of the University of Waterloo in Canada have now carried out a series of experiments on alcohol compounds using a FT-ICR (Fourier transform ion cyclotron resonance) ion trap (Science 279 194-197, 1998). This apparatus is ideal for studying the low pressure reactions of molecules in a collision-free environment. The researchers noticed some striking observations: an unusual pressure dependent behaviour of the breakdown rates; and amplification of the breakdown rate when hydrogen was replaced by deuterium.

Theoretical modelling indicates that a radiation hypothesis is the only feasible explanation for the reactions observed in the experiments. The authors conclude that “the ambient blackbody radiation activation mechanism represents a major addition to the field of chemical kinetics, with particularly promising applications to cluster ions and large biomolecule ions.”

Copyright © 2026 by IOP Publishing Ltd and individual contributors