Skip to main content

Hubble sees mystery object

There are four possible explanations for the object: a highly obscured galaxy, an old elliptical galaxy at redshift 3 or 4, a galaxy at redshift 12, or an intergalactic carbon star. However, there are problems with all of these interpretations. “It would be very strange to have found a highly obscured galaxy with colours this extreme in one very small area such as the Hubble Deep Field image,” says Dickinson. And if the object is an old elliptical galaxy, he says, the stars inside some galaxies must have formed near the beginning of the Universe. Similarly, if the object is a highly reddened carbon star, it must be well outside our galaxy.

According to Dickinson the evidence is pointing towards a normal galaxy at extreme red shift. Earlier measurements at the Kitt Peak Observatory gave a “tentative” redshift of 12.5, but Dickinson has yet to confirm these findings. “While it may or may not be correct, these estimates are usually highly accurate,” says Meg Urry from STScI.

The result has big implications for cosmology. If the object is confirmed as a galaxy, then it suggests that large-scale cosmological structures collapsed into galaxies billions of years earlier than astronomers previously believed. The galaxy would also be three times brighter than equivalent modern-day galaxies. A final answer will require new observations, but these will take some time. “Because the object is so faint, it will be very tough to nail down,” says Dickinson. “I think there’s a healthy ‘wait and see’ attitude to see how it pans out. Unfortunately this may require a long wait, although a final answer should appear when the Next Generation Space Telescope is launched in 2007.”

New evidence for superconducting stripes

The neutron scattering experiments were carried out by Herb Mook from the Oak Ridge National Laboratory and colleagues, while the ion channelling experiments were performed by Rajeshwar Sharma from the University of Maryland and co-workers. Mook and co-workers showed that certain magnetic fluctuations in YBCO are one-dimensional – as would be expected if the stripe model was correct – whereas previous results had found evidence for two-dimensional fluctuations. The apparent discrepancy is due to the use of twinned and detwinned crystal samples.

The stripe models also predict various phase transitions as a function of temperature. Using MeV helium ion channelling – an ultrafast probe with sub-picometre resolution – Sharma and co-workers observed fluctuations in the YBCO lattice that were consistent with the prediction of the stripe models.

Snooker moves to the atomic scale

Scanning tunnelling microscopes (STMs) rely on an ultrafine ‘tip’ to push atoms over a surface. The atoms are pushed either by the tip itself, or by an electric field. The new technique relies on the current that tunnels from the tip to the atom. As the tip approaches the bromine atom, the atom moves closer to the surface. At a critical point, the atom is repelled, breaks contact with the surface, and jumps away from the tip along the easiest available direction. This is at right angles to the direction that the tip is moving in — just like the ‘cut’ shot in snooker. Pethica and colleagues solved the thermal judder problem by including a ‘dither’ – a rapid, small amplitude oscillation – perpendicular to the direction that the tip was moving in. This stops the tip from missing the atom and also prevents ‘miscues’.

Astronomers look to ‘virtual’ observatories

The first virtual observatory to receive significant funding will be a European project called ASTROVIRTEL, which is based at the ESO headquarters in Garching, Germany. European astronomers will be able to apply for grants from the European Commission to analyse the archive, which will include data from the Very Large Telescope (VLT), the New Technology Telescope (NTT), the Infrared Space Observatory (ISO) and Hubble.

In the US the Space Telescope Science Institute (STScI) in Baltimore has pioneered easy-to-use software for accessing the Hubble archive, and is also the centre for all NASA’s near-infrared, optical and ultraviolet observations. This means that it now holds the largest archive of observational data in the world. The institute also provides research grants for academics interested in archival research. “It has been extremely successful,” says Melissa McGrath from STScI. “Even if the telescope comes down in 2010, the HST data archive is going to be a fantastic resource for many years to come.”

The success of the project has led to a new initiative called the National Virtual Observatory that will merge the largest archives — such as those from the 2-micron Survey at Caltech, the Sloan Digital Sky Survey, the new Palmer Sky Survey and Hubble — into a single digital resource. The archive will also be open to amateur astronomers. “The potential for amateur astronomers to carry out serious research will increase with these archives,” says McGrath. “I hope they just jump in and publish.”

High-speed switching at low voltages

Converting electrical signals into optical pulses is one of the speed ‘bottlenecks’ in current telecommunications systems. To reach high data speeds, a series of electro-optic devices called modulators, all operating at different wavelengths, are used. The most common modulators are based on a lithium niobate compound, but they require high voltages (5 V) to work. The devices also have limited gain and high noise levels.

The new polymer modulators only require 1 volt to work, which reduces energy consumption and heating in the device. Although lithium niobate modulators currently only operate at 2.5 GHz, a new technique based on so-called Bragg gratings is expected to reduce the voltage needed to operate them, and also increase the transmission rate to 100 GHz. However, the fact that the modulators still generate heat and cannot be integrated directly onto silicon chips could leave a gap in the market for the new polymer devices.

Universities receive third funding boost

The JIF scheme is designed to bring facilities at UK universities to the forefront of international research. Nearly £600m has been awarded to 109 projects in 28 different institutions since the UK Government and the Wellcome Trust – the world’s largest biomedical research charity -first funded the scheme. The size of the third round awards varies between £500 000 and £19 m.

Edinburgh University’s Materials and Micro-Analysis Centre will determine the chemical composition, texture and structure of synthetic and natural materials. The centre will spend part of the money buying a high-resolution ion microprobe.

The money for the nanotechnology facility at Birmingham will go towards improving the clean room and new equipment for removing and depositing material. “It will be a unique piece of equipment in the UK, if not Europe,” says Phil Prewett from Birmingham University. Meanwhile, the upgrades to the atmospheric observatories for the Reading University-led consortium will monitor clouds and water vapours, as well as aerosol particles and pollution drifting towards the UK from north-west Europe. “It’s a substantial upgrade to a research area that has had negligible resources,” says Keith Browning from Reading University.

The University of Ulster will construct a state-of-the-art building with extensive computer modelling systems for its fire safety engineering research facility. “For the first time we will be able to simulate fires by computer and have actual ‘controlled’ fires in the same area. It represents a major advance in the study of fires, particularly predicating how they start in the first place, how people react to them and the best way of evacuating buildings,” says Jim Shields, director of fire research at the university.

Comet Hyakutake makes a mark on Ulysses

Ulysses was launched to make continuous measurements of the solar wind, a steady stream of ionized particles that flows outwards from the star. In 1998 Pete Riley and colleagues from Los Alamos National Laboratory published a paper describing a dramatic drop in the number of protons registered by Ulysses. They suggested that a comet could have caused the signal.

Recently two groups independently discovered that Comet Hyakutake was probably the source of the signal. Geraint Jones of Imperial College in London and colleagues used the magnetometer to calculate the size of the comet’s tail. “The fast, polar solar wind preserved the structure of the tail over an exceptional distance,” says Jones, “otherwise it would have been extremely hard to recognize it.” Jones noticed that Comet Hyakutake had crossed between the Sun and Ulysses on the 23 April 1996, which was 8 days before the instruments went haywire on 1 May. The size of the tail, together with its magnetic field, speed and the position of the spacecraft, pointed to Hyakutake as the source.

Meanwhile, a team led by George Gloeckler from the University of Maryland noticed that the SWICS detector on Ulysses had picked up the same patterns of carbon, nitrogen and oxygen ions detected in Halley’s comet. After hearing about the magnetic field results from Jones, they concluded that the ions were from Hyakutake. “We were greatly surprised to find cometary material so far away from the nucleus,” he says, “and the discovery of otherwise invisible comets may [now] be possible.”

However, Jones does not intend to spend too much time looking for comets. “The chances are really small that a comet’s tail will pass in front of Ulysses,” he says, “but we may well be surprised again.”

Quantum computers think big

The Innsbruck model relies on ions stored in an array of microtraps. Because the microtraps can be fabricated in a solid state device, thousands of traps can be put into an array. The internal quantum state of the ions acts as the qubit. A different ion, called the head ion, moves above the array to read the information stored by the trapped ions. A laser beam directed at the head ion causes it to move, which leads to an interaction with one of the ions in the array.

According to Cirac and Zoller, the method combines the scalability associated with the solid-state approach to quantum computing with the control found in quantum optical systems, such as photons and ions in traps.

Collaborating with the enemy?

About a year ago I was asked to speak at a local women’s studies conference on mathematics, science and technology. I didn’t flatter myself at having been chosen, because nearly every local woman who was even vaguely involved with science or mathematics at a professional level had been invited to speak. Nevertheless, I had for some time been investigating female astronomers from the 17th, 18th and 19th centuries, so I volunteered to discuss my research.

What I had done was to read the diaries and correspondence of many female astronomers from the scientific revolution and to examine the written work of the people closest to them. The result of my research was a short paper entitled “Innovators or interpreters: the historic role of women in science.” From this anecdotal data, I concluded that, historically at least, successful women scientists tended to collaborate with a male partner or partners, usually a close relative. The astronomer Caroline Herschel (1750-1848), for example, worked with her brothers William and John.

I also found that, because women were not admitted to university or to any of the scientific societies, this relationship with male scientists tended to be of the utmost importance to them. The female partner in the collaboration was entirely dependent on the male for access to libraries and to current scientific thought. She would also rely on the male colleague to help her to disseminate her work.

Finally, social dictates of the period created an atmosphere outside the collaboration that was challenging, to say the least. Society in general frowned on women in science, and other non-scientific women were especially cutting. A woman who embarked on such a career did so at the peril of being considered unladylike, immodest or worse.

The problem is that the work of the female partner in such collaborations has often been more closely identified with the male colleague than with the woman, with the result that the women’s role in the partnership has been eclipsed. Worse, the female scientists themselves consistently downplayed their own accomplishments.

I therefore concluded that the male/female collaboration of the period was the saving grace for women in the sciences. It also forced modern women to be far too modest about their scientific achievements – something that is all too common, even now, as we enter the new millennium.

The feminist backlash

I didn’t think that my conclusions were particularly astonishing. So when the first wave of feminist reaction hit me, I was completely taken by surprise by the number and tone of e-mails from my female colleagues. Why wasn’t I more supportive of female physicists? Why did I assume that women only succeeded if they collaborated with men? What about mentoring younger women scientists: isn’t that working? And why did I cast women as their own worst enemies?

The real, unasked questions were even more insidious. Don’t you know who the real enemy was? Don’t you know who the real enemy is? Although I know what I am expected to say as a feminist – namely that men are entirely responsible for women’s lack of recognition and success in science – I am afraid that I just cannot agree.

Many efforts have been launched, in the US and elsewhere, to increase the number of women studying science at university. Others aim to raise the level of awareness of women’s accomplishments in physics. Some, like the effort by the University of California at Los Angeles to showcase 20th-century women in physics, are quite well done and thought-provoking. Its Women in Physics Web site reminds us that, while the number of women who are active in physics is still small, that percentage is increasing, and that women are doing important work in the field. Teachers can use the site to find women who have been overlooked (even in modern textbooks) and then present them and their achievements in the classroom.

However, these well-meaning attempts are often frustrated by the reality of the numbers game. No-one disputes the fact that far more men work in physics, mathematics and engineering than women. All of the department-shuffling in the world cannot alter the fact that, in spite of the best recruitment efforts in my own department – and in countless other physics and astronomy departments around the world – there is often only one female member of staff. The reason is not, as my sisters in science argue, because men are the natural enemy of women. There are simply not enough women with the right skills, especially in mathematical proficiency, who are interested in entering the field.

Into the classroom

Seven years ago I undertook a study in the US with Pamela Lanaro, an education specialist from the Northern California Education Foundation, who was convinced that the problem began at an early age. It is well known that up to the age of 12 or 13, girls and boys do equally well in maths and science, whether or not they study in single-sex or mixed classes. In fact, girls even appear to have a slight edge over boys.

According to the prevailing wisdom at the time of our study in 1993, it was believed that girls were somehow socialized to defer to boys, with the tacit encouragement of teachers, who favoured boys over girls. At middle-school level, when pupils are aged between 10 and 14, so the argument went, the impact on girls finally catalyses and girls give up. To test this belief we developed several exercises that were designed to demonstrate various abstract concepts in physics. We then tested how well the boys and girls in a mixed middle-school science class understood these concepts when they studied together, and compared the results with another group that had been split into boys-only and girls-only classes.

We expected to see a significant improvement in the performance of the segregated girls’ class, and just a moderate difference in the performance of the other mixed and the boys-only class. What we saw instead was surprising. The performance of the integrated class improved (girls and boys alike), as did the boys’ class. However, the segregated girls’ class did not show any marked improvement at all. From my anecdotal observations I knew why. The girls – unlike the boys alone or the boy-girl partnerships – were constantly trying to find consensus. It did not matter to the girls if the answer was right or wrong; the important thing was that everyone agreed on the conclusion. They were afraid to argue with one another.

We were stunned. Most other studies at that time had shown that girls tended to do better in single-sex classes. The only major difference between our study and the others was that we had been working with a slightly younger group of girls and in a relatively large class. When Lanaro’s subsequent studies produced similar data, we were left asking ourselves if sociological or biological factors affected girls’ leap to abstraction. There is evidence that the answer is: “a little of both”. Whereas boys at that age are making strides to stand out – in keeping with the biological and evolutionary imperative – girls are doing just the opposite and for the same reasons. For women there is safety in numbers, and bucking that trend, in nature, is courting disaster.

Timing may also have played a major role for the girls in our study. Our 12- and 13-year-old seventh graders were all within a year or so of the onset of puberty, and the biological and emotional changes that take place at that time are well documented. Unfortunately for girls, the onset of puberty coincides with the cognitive stage of human development at which abstract reasoning becomes possible. Boys, on the other hand, get a couple of years of blissful ignorance before puberty rears its ugly head, which may give them the “edge” that we see in late middle school and high school. It may be that many girls cannot cope with these overwhelming biological, sociological and intellectual challenges simultaneously.

Understanding the problem is one thing; knowing what to do to correct it is another. We recommended that children should begin to receive algebraic concepts in concrete form and be taught mathematical modelling at much earlier ages, suggestions that are currently being considered for inclusion in the curriculum for fifth-year pupils in California. It will be several years before we know if the jump-start programme increases the number of women entering mathematics and science, but we have some hopes in that regard.

Collaborate and succeed

The truly interesting thing from our study, I found, wasn’t in the test group at all. It was in the control group where boys and girls studied together, and it shed light on the dynamic nature of male-female collaborations. The girls in our control group, each of whom was made to partner a boy, improved their performance at more or less the same rate as the boys. When I went back to look at the performances of each of the partnerships, I saw, for the most part, little discrepancy between them. For some reason, each person in the partnership challenged the other – and both benefited.

I see this as being positive. Perhaps I am a little biased, because I am in a long-term male-female collaboration with my research partner and co-author David Madore. For the past two-and-a-half years we have been studying various apparent anomalies and symmetries in special relativity (see xxx.lanl.gov/abs/astro-ph/0001123). During that time, as with any close partnership, there have been times when we wanted to kill each other and occasions when we pushed each other so far away from accepted thought that we ultimately had to retreat, but we never, ever settled for the mediocrity of consensus.

Physics isn’t a search for consensus; it is a search for truth. When the truth sometimes contradicts the long-held consensus – as both my recent work with Madore and my earlier work with Lanaro show – the researchers have to challenge each other not to fall back into the comfortable. Similarly, while Newton’s work provided the fundamentals for all known physics, by the middle of the 19th century it was apparent that Newtonian mechanics was not the last word. Newton, however, was comfortable; Maxwell was not, which meant that the essential truth of the Maxwell equations was systematically overlooked for almost 50 years. Working on the edge of known truth is not a comfortable place to be. To work through it, and arrive at whatever new truth is there, a dynamic collaboration is necessary.

Whatever the gender make-up of the partnership, the important thing is for all members within it to challenge one another actively and constructively. Women may have an added burden. Although our evolutionary background encourages us to concede, to agree and to create consensus, our duty as physicists is to challenge known thought and to arrive at new and unimagined truth. We also have a higher duty, as humans speaking for humanity, not to hide behind our feminine modesty but to tell the world what that new truth is.

The key to this is collaboration. We must create collaborations that will challenge not only our own abilities and sensibilities, but also those of the scientific community and the world at large.

Do you have any comments on this forum? Why not email Physics World at pwld@iop.org

Dark-matter dispute intensifies

The controversy surrounding evidence for the discovery of “dark matter” particles has heated up following two conflicting talks given at a conference at the end of February. The papers were presented at the 4th International Symposium on Sources and Detection of Dark Matter/Energy in the Universe held in Marina del Ray, California. (Most of the transparencies from the conference are available on the Web.)

For almost 70 years astronomers have known that dust, gas and other ordinary matter cannot account for almost 90% of the mass of many galaxies. The galaxies must contain other “dark” matter to explain the orbital motions of stars around their centres. Many astrophysicists, cosmologists and particle physicists have conjectured that this seemingly empty space could be populated by a dense body of massive, but very weakly interacting, particles called WIMPs. Such particles would then provide the gravitational fields needed to keep the stars moving as observed.

Since the results of the first experimental efforts to detect these particles were published in 1987, literally dozens of experiments have been performed around the world. Two of the most sensitive experiments to date are the DAMA experiment at the Gran Sasso laboratory in Italy, and the CDMS experiment at Stanford University in the US. The DAMA collaboration – which includes physicists from the University of Rome Tor Vergata, the University of Rome La Sapienza and the Chinese Academy in Beijing – has been searching for WIMPs for several years using a large array of sodium-iodide detectors located 1400 m below ground. The CDMS experiment uses cryogenic detectors and is located just 10 m underground. The collaboration includes researchers from several centres in the US and Russia.

Assuming that they do exist, a WIMP will occasionally strike a nucleus in the detector material head-on and cause an elastic recoil. The recoil energy depends on the mass and velocity of the WIMP, together with the mass of the target nucleus. This energy can be measured in several ways, depending on the detector used. A scintillation photon may be emitted, electric charge may be liberated, or a phonon could cause a slight rise in temperature in the cryogenic material.

The challenge for dark-matter experiments is to discern the small effects produced by the rare WIMP interactions from the vast number of background events. This background includes cosmic rays and radioactive particles released from the detector and its surroundings. As a result, great care is taken to shield the detectors from comic radiation and to ensure that any radioactive impurities in the detector or shielding material are removed (see “The search for dark matter” by Nigel Smith and Neil Spooner Physics World January 2000).

Claims and counterclaims

For several years, the Italian group has claimed that it is has found evidence for WIMP interactions as the Earth and the Sun move through a sea of cold dark-matter particles in the halo of the Milky Way. The relative velocity with which the Earth moves through the dark-matter halo changes because of the way the planet rotates around the Sun. This means that the WIMP signal in June should be higher than that in December. The DAMA detectors have been used to search for this annual modulation in the signal.

The Italian group has accumulated thousands of hours worth of data using a 100 kg array of sodium-iodide detectors to measure scintillations of light. After several years of operation, the researchers see evidence for a seasonally dependent signal that is consistent with the position and velocity of the Earth throughout the year (see figure). This experiment is extremely difficult and requires complex data analysis to uncover the very subtle evidence of such a modulation. Researchers who have doubted the results in the past have suggested that a more mundane process – such as the ambient temperature – could give rise to the same effects.

In the conference session devoted to the experimental search for dark matter, which I chaired, Pierreluigi Belli of the DAMA collaboration presented a paper entitled “Searching for the WIMP annual modulation signature at Gran Sasso: results and perspectives”. During his 30-minute talk, Belli discussed the experimental details in great depth. He paid particular attention to the constant checks that were carried out to monitor the quality and control the stability of the experiment. The conclusion was that the DAMA experiment demonstrates definite evidence for the existence of a signal consistent with that expected from WIMPs with a mass between 44 and 62 GeV c-2.

The question-and-answer session that followed Belli’s report lasted almost 25 minutes. There were many questions concerning the experiment – particularly about the analysis of the data – and Belli addressed each one in detail. While the entire audience may not have been completely satisfied with some of his responses, Belli left no question unanswered.

The next talk by Richard Gaitskell of the CDMS collaboration, “Recent results on direct searches”, was intended to demonstrate that the experimental evidence presented by the Italian group was, in fact, not real. The CDMS experiment is based on an entirely new type of detector technology that uses germanium and silicon crystals cooled to low temperatures. The detectors simultaneously measure the ionization and heat produced by nuclear recoils. The technology has clearly demonstrated that it is capable of separating events caused by a WIMP displacing a nucleus in the crystal from background events caused by gamma rays and X-rays from natural radioactivity in the surrounding materials.

The CDMS experiment would have definitely refuted the DAMA results if it were not for 13 events in which the germanium nuclei recoiled after being struck by some massive particle. Gaitskell presented details of a number of experiments and calculations designed to show that all 13 of these events were most probably caused by background neutrons produced from cosmic rays entering their laboratory. From their analyses, the CDMS researchers concluded that almost all of these events were definitely from neutrons, and should not be attributed to scattering events from dark-matter WIMPs. (The transparencies from the talk and a paper that has been submitted to Physical Review Letters are available on the Web at cdms.berkeley.edu).

Nevertheless, the discussion that arose during the question session that followed centred on the ability of the collaboration to guarantee that these were, in fact, neutron events. Doubting Thomases of the neutron-identification schemes maintained that one could not conclude that these were definitely neutrons. Furthermore, if these events do not originate from neutrons, the results of the CDMS collaboration are, in fact, exactly as one would expect if the DAMA results are correct. At present, many in the field believe that a stalemate exists. Of course, a large number of people at the conference took one side or the other.

Breaking the deadlock

In the next year or two, both collaborations plan significant upgrades and improvements to their detectors. The DAMA collaboration is planning to increase the mass of its sodium-iodide detector to 250 kg, which will make the experiment far more sensitive to the annual-modulation signal. Meanwhile, the CDMS collaboration plans to move its detector to the Soudan Underground Laboratory, which is located approximately 700 m underground in an abandoned iron mine in Ely, Minnesota. Previous experiments by other groups at the Soudan lab have shown that the background from neutrons will essentially be eliminated. We should therefore learn for certain whether the 13 events observed in the shallow underground laboratory at Stanford are due to neutrons or not.

The increased sensitivity of the two experiments – together with a number of other experiments – will allow physicists to search for dark matter in greater detail. The experiments will either discover WIMPs or rule out particles in a large mass range and with a wide range of interaction properties.

The discovery of cold dark-matter particles would be one of the most important in the history of physics. It would clarify many questions concerning the birth, evolution and final destiny of our universe. A definitive confirmed discovery would certainly merit a Nobel prize and a distinguished place in history for those who provided the intellectual leadership.

Copyright © 2026 by IOP Publishing Ltd and individual contributors