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The power of robotics

My son Alex should have spent more time this spring on his homework. Instead, he spent it building a robot.

Let me explain. Alex, 14, is a member of the SciBorgs — the Bronx High School of Science robotics team. He and two dozen other team members took part in an annual competition sponsored by the US charity FIRST (For Inspiration and Recognition of Science and Technology). Each January, FIRST challenges high-school teams to build, in six weeks, a robot able to compete with other robots in performing complex tasks like climbing stairs and stacking pyramids. This year the competition attracted over 42 000 high-school students in 1684 teams, mainly from the US but also 10 other countries, including five teams from Israel, 10 from Canada and three from the UK.

FIRST was founded two decades ago by the award-winning inventor Dean Kamen, whose innovations range from the insulin pump to the two-wheeled, gyroscopically balanced Segway personal transporter. Kamen and his colleagues were worried about declining student interest in hands-on technology education, and the trend for programmes that teach students not with hands-on experience but with computer screens. Real creativity requires extensive experience with materials and tools, the absence of which threatens not only engin­eering education, but any kind of experimental science and technology.

“To think conceptually, you first need experience in the physical world,” Michael Dubno, chair of FIRST in New York, told me at one competition. “You have to understand the materials viscerally — what makes them work, what makes them break — before you can program them. Experience in the physical world leads to deeper theoretical understanding. Schools nowadays think they can leave out the physical step — that it’s just vocational. You can’t.”

The most effective way to engage students, FIRST’s founders decided, was to stage events that were both competitive and collaborative, in an atmosphere that had all the hoopla of high-school sports. Every year, it presents a fresh challenge. “In school, it goes like this: ‘Teach, practise, test. Repeat.’ In FIRST, it’s the opposite: ‘Here’s a problem with no obvious solution. Solve it!’[It is obvious which] one actually turns on your brain,” explains Dubno.

Lunar lunacy

The challenge this year — the 40th anniversary of the Apollo 11 Moon landing — was called “Lunacy”. Teams had to design and build a robot to move around a low-friction playing field made of a polymer material called Regolith to simulate driving on the lunar surface. The robot had to collect balls, or “Moon rocks”, and deposit them in trailers. Alex and the other SciBorgs — and members of their all-girl sibling team the Iron (Fe26) Maidens — stayed after school until late at night, and worked on weekends, to feverishly complete their robot.

The SciBorgs’ regional final took place in March at New York City’s Javits Convention Center. Shortly after they arrived, an inspector told the team that its last-minute tinkering had put the robot 5 kg over the weight limit. Alex and others scrambled to remove support bars and cut holes in structural elements. Desperate, they also removed the compressor that powered the actuators of the shooting mechanism, hoping to rely on tanks of compressed air. But during the practice round, the actuators ran out of air. The team quickly reinstalled the compressor, sacrificing air tanks and more support bars.

A total of 66 teams took turns squaring off on a playing field roughly 16.5 m by 11 m in size. Each match was a competition between two alliances of three robots each. NASA was even present, providing welding machines and other equipment to aid robot-builders who needed to make repairs. “For the kids, the robot makes the connection between the textbook and the real world,” NASA support engineer Robert Thate told me. “You see the light bulbs go off.”

Thousands of cheering spectators filled stands around the field, many dressed in costumes and school colours. I decided to drop in on Systemetric, the sole UK team at this regional heat. (Foreign teams attend a regional event of their choice.) Its members were from Hills Road Sixth Form College in Cambridge, which has regularly taken part in FIRST competitions since 2002. (It was also part of the winning alliance in 2004, although it could not afford to attend the championship that year.)

Systemetric was easy to locate in the crow­ded stands; its members were all dressed in the red, white and blue of the Union Jack. As their physics teacher, David Massey, ex­plained, some 24 team members had made the trip, thanks to their sponsors Microsoft Research paying the $6000 entry fee and chip manufacturer ARM helping to pay for the students’ flights.

“It’s a shame there’s nothing like this in the UK,” Massey said. “It teaches the kids several things they can’t otherwise learn. This is the first time they build a large piece of machinery, for instance. It’s the first time they interact with adult mentors. It’s the first time they work in large teams. And it also gives them the chance to learn how to panic — how to go through a crisis without giving up. Where else can they learn that?”

The critical point

A few teams complained to me that the short timescale forced them to build the first thing that came to their minds, without having time to systematically review design possibilities. When I repeated this to Kamen, he laughed.

“You never have enough time or money,” he said. “You never know what’s going to happen when you turn on the prototype, or what your competitors are doing. In six weeks the kids have to conceive, design, prototype, build, bust, rebuild and ship. FIRST provides a microcosm in which they can do this is an exciting and supportive climate.”

Alex’s team did not win in New York, but a victory at the Hartford regional heat sent them to the finals in Atlanta, where they came 14th out of 88 teams in their division. He and his team mates were disappointed that they had not been placed higher, but they have already started to build a chassis for next year’s robot. The homework will get done somehow.

The unique universe

Three decades ago, talk of other universes was not seen by most physicists to be part of science. Most research in theoretical physics and cosmology concerned observable features in our universe and most papers and seminars referred to experimental results. However, since then there has been a gradual shift, during which it first became acceptable to work on theories that described not only our universe, but other possible universes, universes with less or more dimensions, or universes with different kinds of particles and forces. In the last few years, we have moved further away from theories of our one universe, as these other worlds went from being logically possible to hypothetically actual. It is now common to hear about the multiverse — a quantum cosmology that takes for granted that the visible universe that we see around us is just one of a vast or infinite number of universes.

The multiverse assumption often comes hand in hand with a metaphysical assumption regarding the nature of time. It has been argued by many experts in quantum cosmology that time is not a fundamental concept, but an approximate and emergent one. If this is correct, then we experience time in a timeless universe for reasons similar to why we, who live in a quantum universe, experience one that obeys classical physics: we are composed of very large numbers of fundamental particles and emergent statistical regular­ities determine much of what we experience.

Furthermore, the combination of the multiverse assumption and the timeless assumption effectively gives us a static meta-universe. Even if our own universe evolves in time, at a deeper level it is part of a timeless, eternal, ensemble of universes.

There are good reasons for these conclusions, and like many others in the field of quantum cosmology I have explored them. However, in the last few years I have come to believe that these conclusions are profoundly mistaken. In collaboration with the Brazilian philosopher Roberto Mangabeira Unger, we have been trying to understand the source of the problems and develop an alternative notion of time and law on the cosmological scale. Our reasons for doing so are based partly on concerns about whether these theories are testable by doable observations, partly on the current results of attempts to realize the timeless ap­proach and partly on philosophical considerations.

The problem with the timeless multiverse

In a timeless world in which our universe is just one of many equally real universes, the laws of physics must be very different from those that most physicists can ever have conceived. This is because the laws of physics are no longer determinable by what we observe in our own universe, for they must apply to all of the vast en­semble of universes. A fundamental law then no longer proscribes what happens in our universe; instead it gives probability distributions for properties of the ensemble of universes.

To understand why, it is helpful to distinguish between the notion of a fundamental law and an effective law. A fundamental law is posited to hold “meta-universally” from first principles and must be unique. String theory, for instance, is an attempt at discovering such fundamental laws of nature. Effective laws, at the other extreme, govern experiments at scales that we observe directly within one universe, down to the small scales probed by the Large Hadron Collider and up to the scales probed by observations of the cosmic microwave background. We can only observe the effective laws, but we hope that it should be possible to derive them from fundamental laws — otherwise the latter has no connection with what we observe. The question is whether that indirect connection provides enough ground for experimentally testing the fundamental laws so that they are relevant for our scientific understanding of the world.

Unfortunately, it appears that if string theory, or a similar theory, is true, then the fundamental theory does not in fact predict what the effective laws of nature are. Instead, it gives rise to a vast landscape of possible effective laws — a concept I introduced in my book Life of the Cosmos (the word landscape was meant to be evocative of fitness landscapes in biology). We then must have hypotheses for how the single ef­fective laws that describe our universe are chosen from the vast list of possibilities allowed by the fundamental theory. This is one of the major motivations for specu­lation about multiverses.

Several ideas have been suggested for how to select the effective laws that apply to our universe from the larger set of possibilities. One possibility, which has been much studied, is that the ensemble of universes is populated by laws by an effectively random process. An example is eternal inflation. In this scenario the process that produces the ensemble occurs at energy scales so high that they swamp any processes we have experimental access to. The result is that a universe like ours, populated by structures that depend on physics at much lower energy scales, is very atypical in the ensemble of universes. One then has to depend on the anthropic principle to pick out the very few universes hospitable to life, which are very rare in the actual ensemble. Not surprisingly, given that the characteristics of the ensemble can be postulated at will and are not subject to experimental tests, the result is that we cannot make precise and unambiguous predictions about anything observable in our own universe.

An alternative approach, which does lead to at least a few falsifiable predictions, is cosmological natural selection, which I introduced in 1992. This is based on a cosmological scenario that is constructed to be analogous to population biology. Universes are born from “bounces” deep inside black holes, which replace their singularities, where time had been hypothesized to end, with new expanding universes. This leads to a prediction that a typical universe is one where the parameters are tuned to maximize the production of black holes. There is in fact evidence that this is true of the laws that govern our universe. Most importantly, in this theory our universe is supposed to be typical of the ensemble, which leads to several genuinely testable predictions, all of which have held up since they were first published, such as the prediction that the upper mass limit of stable neutron stars is about 1.6 solar masses.

The contrast between these two kinds of multiverse theories leads to a question: why is the theory based on natural selection predictive — but not the one based on random production of universes? This helps us understand why the reality of time is necessary to explain how the laws of physics are chosen.

It is apparent that a scenario in which a population of universes evolves, rather than just being a random timeless distribution, requires a notion of time that is real at a level above individual universes. But to understand why the timeless picture fails, we have to go deeper to the foundations of quantum theory. For example, without time, and without the assumption that what exists is the single universe that we observe, it is hard to make sense of statements about probability relevant to what we observe in our universe. Since quantum mechanics is a probabilistic theory, we then run into trouble by trying to extend it to a realm where probability appears to make no sense. A number of authors have attempted to address this question, by proposing ad hoc measures for deducing predictions from ensembles of multiverses. At least up to the present time, none of these appears to be justified by anything other than the need to reproduce what we observe.

A related issue is the recovery of classical space and time, which general relativity describes, as part of an effective theory. These must be emergent aspects of a fundamental quantum theory, much like the classical notions of a particle being at a definite place and travelling on definite trajectories is emergent from quantum mechanics. This is non-trivial because the notions of quantum space—time, which arise in quantum the­ories of gravity, are very different.

So far, approaches to quantum gravity that assume that both space and time are emergent fail to reproduce the space—time that we know. On the other hand, two approaches that assume that time is fundamental and non-emergent succeed, at least to some extent, in describing how space—time may emerge. The most developed of these is causal dynamical triangulations, which has impressive results indicating the emergence of classical space—time. A more recent attempt, quantum graphity, also has preliminary indications for the emergence of space given the existence of time. Furthermore, fundamental time is also needed to make sense of probability and describe the evolution of effective laws, which ties to the earlier issue.

These results were the first evidence that led me to consider the idea that there might have to be a fundamental global notion of time in any fully consistent approach to quantum gravity that can recover general relativity in the approximation in which the universe is large. This hypothesis is strengthened by recent results in unimodular gravity, which several authors have argued solves the long-standing problem of the cosmological constant — something that is necessary for a large classical space—time to emerge. What is remarkable, as pointed out by the physicists Rafael Sorkin of the Perimeter Institute for Theoretical Physics, William Unruh of the University of British Columbia, Van­couver, and others, is that this approach des­cribes evolution in a global time related to the space—time volume of the past.

What is a cosmological law?

To understand the difference between the two paradigms of emergent time versus fundamental time we need to appreciate how much of our usual notion of physical law has evolved historically from our experience of laboratory observations. In the laboratory we do not, by definition, study the whole universe. We study a small subsystem of the universe that, to some reasonable approximation, can be regarded as isolated (apart from the measuring instruments that we use to observe it). When we do this, we explore the possibility that we can prepare that closed system over and over again, at different times and in different places, with the same elements and different configurations. We abstract physical laws from what is common in a large set of experiments, and study what becomes different when the initial conditions are different. This allows us to make a clean distinction between laws and initial conditions. The laws are held to be invariant, at least over scales of time and space larger than the scales pertaining to our experiments.

This situation is almost the same for most astronomical observations. We cannot prepare stars and galaxies in any state that we want, but we can observe vast numbers of them and we can treat them as approximately isolated. Hence, in astronomy we also have a justification for distinguishing between laws and initial conditions.

The separation of scientific explanation into law and initial conditions leads to one of the most universal and powerful notions in physics — the notion of configuration space. This is the space of all possible configurations, or states, of the system. In classical and quantum physics we assume that this space exists a priori and outside of time, and that it can be studied independently of the laws of motion. These laws then specify the rules for how the point that describes the initial conditions in configuration space evolves in time. We call this the Newtonian schema for explanation.

The Newtonian schema is the basis for the claim that time is not fundamental in cosmology. From this point of view, time is seen merely as a parameter on a trajectory in configuration space, and not as an intrinsic part of the physical law. The present moment, the time we experience, has no place in this description. The philosopher who does not believe in the flow of time points to the trajectory in the configuration space and says that the only thing that is real is that the whole history of the universe exists timelessly — what in general relativity is called the “block universe” picture. Many physicists and philosophers have fallen for the temptation of believing in the “block universe” picture. To them, our experience of the flow of time is just an illusion.

This argument is faulty for two reasons. First, it does not prove that time is not fundamental. When we observe motion, we record a series of measurements of a system’s position. These can be graphed on the configuration space, resulting in a curve that represents the record of the motion. This graph is timeless, because it is a representation of a record of a past motion, which is, of course, no longer changing. The correspondence is between a mathematical object, which is static, and a series of records of observations, which is also static. The fact that we can make this correspondence be­tween a mathematical object and a record of past mo­tion does not imply that the actual motion that the observations sampled is timeless. Nor does it imply that behind the real evolution in time of the real world there exists a complete correspondence to a timeless mathematical object. To posit this further relation is a pure metaphysical fantasy, which is not implied by anything in the science (see “The fourth principle: mathematics and Platonism” below).

New principles

The second failure of the argument for time not being fundamental is that it is far from clear that the Newtonian schema applies on the scale of the universe as a whole. Almost all work in classical and quantum cosmology assumes that it does. But given the difficulties that these subjects encounter, I think it more likely that the answer is no.

One reason for suspecting that the Newtonian schema does not apply to cosmology is that the experimental context that gives meaning to the separation of causes into laws and initial conditions is completely missing. There is no possibility of preparing the universe in different initial configurations, and there is no way to determine by observation the full initial conditions. Any observer, within the universe, can only see a fraction of any initial-value surface. Thus, the notion of initial conditions is simply not realizable in cosmology. If there is just one universe, there is no reason for a separation into laws and initial conditions, as we want a law to explain just the one history of the one universe.

The same is true for the configuration space of the cosmos. The universe happens once, so what is the meaning of all the states that exist in state space but are never realized in the history of the universe? The notion of the “quantum state of the universe” is a fiction, divorced from anything that could be prepared or measured in practice. These considerations suggest that the notions of configuration space and state space correspond to measurements and preparations that can be operationally realized only in the case of a small subsystem of the universe. These concepts — or at least their operational basis — fail us when we try to extend them to the whole universe.

The issue of time also looks different from this perspective. Time in the Newtonian schema is a parameter used to label points on a trajectory describing the system evolving in configuration space. When the system is small and isolated, this time parameter refers to the reading of a clock on the wall of the observer’s laboratory, which is not a property of the system. When we try to apply this notion to the universe as a whole, the time parameter must disappear. Some have attempted to argue that this means that time itself does not exist at a cosmological scale, but that is the wrong conclusion. What disappears is not time, but the clock outside of the system — which would be an absurd object since the system is the whole universe.

Indeed, it may be that sticking to the Newtonian schema, when it has no operational significance, leads us to take the multiverse scenario seriously. If our scientific methodology only makes sense when applied to subsystems of a vaster universe, then it is tempting to react to the problems that arise when we try to extend it uncritically to that whole universe by positing that our universe is in fact a subsystem of an even vaster multiverse. We get to do physics as we have been trained to, but this is a trap because to do this we must employ structures that have no operational significance. Better, in our view, to regard the Newtonian schema as inapplicable to cosmology, and to look for another notion of law that can make sense when applied to our entire, but single, universe.

But once we state that the distinction between laws and initial conditions has no counterpart in the cosmological context, this renders moot several puzzles that the extension of the Newtonian paradigm to cosmology has brought about. What is the initial quantum state of the universe? How do we interpret it? How do we define probabilities in quantum cosmology? How do we do physics when time has disappeared?

The physical law in a single, time-bound universe

By discarding the Newtonian schema for cosmology and dispensing with the notion of the multiverse, we also no longer have any reason to suspect that time is an illusion. This led Unger and me to consider the implications of a natural philosophy based on a different set of principles.

1. There is only one universe. There are no others, nor is there anything isomorphic to it.
This logically implies that there are no other universes, nor copies of our universe, whether within or without. The first is impossible as no subsystem can model precisely the larger system it is a part of, while the second is impossible because the one universe is by definition all there is. This principle also rules out the notion of a mathematical object isomorphic in every respect to the history of the entire universe, a notion that is more metaphysical than scientific.

2. All that is real is real in a moment, which is a succession of moments. Anything that is true is true of the present moment.
This says that not only is time real, but also that everything else that is real is situated in time. Nothing exists timelessly.

3. Everything that is real in a moment is a process of change leading to the next or future moments. Anything that is true is then a feature of a process in this process causing or implying future moments.
The third principle incorporates the notion that time is an aspect of causal relations. A reason for asserting it is that anything that just existed in a moment, without causing or implying an aspect of the state at a future moment, would be gone in the next moment. Things that persist must be thought of as processes leading to newly changed processes. An atom in a moment is a process leading to a different or a changed atom in the next moment.

This alternative metaphysical framework has im­plications for the nature of physical law. Since nothing is true or real outside of time, there is no possibility of speaking of eternal laws. Laws are regularities that we discover hold for very long stretches of time, but there is no reason for laws to be true timelessly — indeed, there is no way to make sense of that notion. This opens the door to the possibility that laws evolve in time, which is an idea that has been on the table ever since the great American logician Charles Sanders Peirce wrote in 1891 that “To suppose universal laws of nature capable of being apprehended by the mind and yet having no reason for their special forms, but standing inexplicable and irrational, is hardly a justifiable position. Uniformities are precisely the sort of facts that need to be accounted for. Law is par excellence the thing that wants a reason. Now the only possible way of accounting for the laws of nature, and for uniformity in general, is to suppose them results of evolution.”

From this point of view, the notion of transcending our time-bound experiences in order to discover truths that hold timelessly is an unrealizable fantasy. When science succeeds, we do nothing of the sort; what we physicists really do is discover laws that hold in the universe we experience within time. This, I would claim, should be enough; anything beyond that is more a religious urge for transcendence than science.

So, what is physics without a clean separation into laws and initial conditions, and hence, without the notion that there is a space of configurations that exists timelessly? We do not know the full answer to this, but we have a few observations.

First, by discarding the Newtonian schema for cosmology we have much less reason to consider our universe one of many other actual universes. Indeed, we may also be able to dispense with the notion of a vast number of other possible universes, that somehow are never realized. We can imagine instead a notion of law that applies only to the single universe that really exists. We also no longer have any reason to suspect that time is an illusion because, as outlined above, the main arguments from physics for time being emergent and not fundamental come from the misapplication of the Newtonian schema to the universe as a whole.

As we attempt to realize those principles, we seek a notion of law that cannot be applied to an imagined universe within a multiverse, and which cannot be imagined to hang around timelessly waiting for a universe to begin that it can then govern. Given that the universe only happens once, we must try to imagine a new kind of law that applies only that one time. Such a law need not — and should not — have any sense in which it exists outside of time. Nor could it be conceived of as apart from the universe it describes. It might indeed be a law that evolves in time; that is, a law where the distinction between a one-time narration of the history of the one universe and the statement of principles governing that history weakens.

If the timeless multiverse paradigm now ascendant is correct, then we are approaching the end of a process that will eliminate the reality of time and replace it with a shadowy kind of “existence” within an eternal frozen world consisting of vast numbers of possibilities. If, on the other hand, the principles that Unger and I propose are closer to the truth, then we are at the beginning of a new adventure in science where we have to reconceive the notion of law to apply to a single universe that happens just once. In either case we will end up conceiving our universe in very different and less familiar terms than before.

But did we really imagine that completing the revolution started by Einstein would be possible without having to discard some of our comfortable beliefs in favour of disturbing and almost inconceivable new ideas? At this level we do science not for ourselves, but for the fu­ture generations that will live comfortably in conceptual worlds that we can at best only point roughly towards. Press)

At a Glance: Against the timeless multiverse

• Many cosmologists today believe that we live in a timeless multiverse — a universe where ours is just one of an ensemble of universes, and where time does not exist • The timeless multiverse, however, presents a lot of problems. Our laws of physics are no longer determinable from experiment and it is unclear what the connection is between fundamental and effective laws • Furthermore, theories that do not posit time to be a fundamental property fail to reproduce the space—time that we are familiar with • Many of these puzzles can be avoided if we adopt a different set of principles that postulates that there is only one universe and that time is a fundamental property of nature. This scenario also opens the way to the possibility that the laws of physics evolve in time.

The fourth principle: mathematics and Platonism


Believers in eternal truth often point to mathematics as a model of a realm with timeless truths. What is called the Platonic view of mathematics holds that mathematical objects (the things that the theorems of mathematics are about, such as numbers, spheres, planes, curves and so on) exist in a separate timeless realm of reality. Mathematicians explore this realm with their minds and discover truths that exist outside of time, in the same way that we discover the laws of physics by experiment. But mathematics is not only self-consistent, it also plays a central role in formulating laws of fundamental physics, which the physics Nobel laureate Eugene Wigner once referred to as the “unreasonable success of mathematics in physics”.

One way to explain this success within the dominant metaphysical paradigm of the timeless multiverse is to suppose that physical reality is mathematical, i.e. we are creatures within the timeless Platonic realm. The cosmologist Max Tegmark calls this the mathematical universe hypothesis. A slightly less provocative approach is to posit that since the laws of physics can be represented mathematically, not only is their essential truth outside of time, but there is in the Platonic realm a mathematical object, a solution to the equations of the final theory, that is “isomorphic” in every respect to the history of the universe. That is, any truth about the universe can be mapped into a theorem about the corresponding mathematical object.

If nothing exists or is true outside of time, then this is all wrong. However, if mathematics is not the description of a different timeless realm of reality, what is it? What are the theorems of mathematics about if numbers, formulas and curves do not exist outside of our world? This leads Unger and me to a new view on mathematics that can be summarized in a fourth principle.

4. Mathematics is derived from experience as a generalization of observed regularities when time and particularity are removed.
Consider a game, for example chess. It was invented at a particular time, before which there is no reason to speak of any truths of chess. But once the game was invented, a long list of facts became demonstrable. These are provable from the rules, and can rightly be called the theorems of chess. These facts are objective, in that any two minds that reason logically from the same rules will reach the same conclusions about whether a conjectured theorem is true or not.

Now a Platonist would say that chess always existed timelessly in an infinite space of mathematically describable games. We do not achieve anything by believing that, except an emotion of doing something elevated. Moreover, it is clear that a lot is lost; for example, we have to explain how it is that we finite beings embedded in time can gain knowledge about this timeless realm. We find it much simpler to think that at the moment the game was invented a large set of facts become objectively demonstrable, as a consequence of the invention of the game. We have no need to think of them as eternally existing truths, which are suddenly discoverable, instead we can say they are objective facts that are evoked into existence by the invention of the game of chess. Our view is that the bulk of mathematics can be treated the same way, even if the subjects of mathematics such as numbers and geometry are inspired by our most fundamental observations of nature. Mathematics is no less objective, useful or true for being evoked by and dependent on discoveries of living minds in the process of exploring the single, time-bound universe.

More about: Against the timeless multiverse

R Bousso, B Freivogel and I-S Yang 2008 Boltzmann babies in the proper time measure Phys. Rev. D 77 103514
R Loll 2008 The emergence of spacetime or quantum gravity on your desktop Class. Quantum Grav. 25 114006
F Markopoulou 2008 Space does not exist, so time can
www.fqxi.org/community/essay/winners/2008.1
L Smolin 2000 The present moment in quantum cosmology: challenges to the arguments for the elimination of time
Time and the Instant (ed) R Durie (Manchester, Clinamen Press)
L Smolin 2006 The status of cosmological natural selection arXiv:hep-th/0612185
R M Unger 2007 The Self Awakened: Pragmatism Unbound (Harvard University

Web life: Phun

So what is the site about?

Phun is a free, downloadable physics-simulation programme that bills itself as a “2D physics sandbox”. The programme’s limitless virtual space allows users to construct simple (and not-so-simple) machines out of levers, gears, motors and as many different shapes as they care to draw, then set them in motion. The results can be educational, bizarre or downright hilarious, depending on what you choose to do, but thanks to a sophisticated simulation engine, they will always be physically realistic — unless you decide to turn off friction and gravity.

Okay, so what can you do with it?
The possibilities are almost endless, but the programme provides a few sample “phunlets” to get you started. With the trebuchet, for example, you can try swapping the central hinge for a motor, changing the counterweight’s mass (or filling it with water) and reducing friction on the sling. Clicking on most objects brings up a list of physical properties, including mass, area, moment of inertia, motor speed and kinetic energy. The “tracer” feature makes it easier to follow the paths of moving objects — useful if you accidentally fill your trebuchet projectile with helium — and the “hand” tool allows you to pick up your creations and fling them about (try it with the “ragdoll” phunlet). But this is the tip of the iceberg: the site’s designers have deliberately left it “open for creativity and exploration”, and the best way to find out more is simply to play with it for an hour or two.

Who created it, and who is it aimed at?
Phun began life as Emil Ernerfeldt’s MSc project at Sweden’s Umeå University. His supervisor, Kenneth Bodin, wanted a programme to use as a teaching tool at the Umevatoriet, a local science centre. However, the project quickly grew beyond its original scope, and now both Ernerfeldt and Bodin work for Algoryx, an interactive physics-software company Bodin founded in 2007 with colleagues from Umeå. Since then, Algoryx has developed a commercial version of Phun called Algodoo, which offers some nifty extra features like light beams and graphing tools. Lecture material, tutorials and a dedicated website for educators and learners are also in the works, Bodin told Physics World. With their bright, colourful interfaces and easy-to-understand controls, both Algodoo and its free cousin Phun were clearly designed with young people in mind, but those who left school years ago will still find plenty of interest.

Anything in particular I should look out for?
Phun has spawned a thriving online community of users who post tips on the main Phun site and videos of their creations on YouTube. If you want more Phun than catapults or cars can offer, these videos are full of ideas, and some are little short of amazing. Two videos by Probber show off an elaborate water-based Heath Robinson contraption, while in JDKmedeng’s “Mars Mission”, a four-stage rocket transports a rover vehicle onto a simulated red planet (where the force of gravity is, of course, reduced). For sheer silliness, it is hard to beat “Duckotron”, which stars a singing mechanical duck and an accident-prone human. However, it is Phunico’s multi-geared sushi-making machine that really takes the prize. The timing of each stage of the process (rice, nori wrap, salmon eggs) is astonishingly fine, and the explanation at the end makes it clear just how much work went into this particular bit of Phun.

Is scientific fraud committed by only a few 'bad apples'?

By Michael Banks

Everyone hears the big stories of fraud in science. Indeed, a feature in last month’s Physics World (May 2009 pp24–29) documented the rise and fall of Jan Hendrik Schön who published a number of papers in prestigious journals such as Nature and Science that have since been shown to include fabricated data.

But how common are the smaller cases of misconduct? It is not easy to get accurate data about how common misconduct is within the research community. One could, for example, look at the number of paper retractions in journals, but these only include cases that have been discovered, and possibly not all retractions are based on fraudulent work.

So who better to ask than the researchers themselves if they have ever fabricated of falsified data? Well, Daniele Fanelli from the University of Edinburgh in the UK has analysed over 20 surveys in which scientists were asked a number of questions about scientific misconduct including if they had ever made up data points or distorted their results.

Fanelli found that, on average, 2% of scientists admitted to fabricating, falsifying or have modified data at least once during their careers. While over a third of researchers said they have published papers with “questionable research practises” such as not including data in a publication that may counter their conclusions or dropping data points from analysis because they were deemed “inaccurate”.

Fanelli also analysed surveys that asked researchers about the practises of their colleagues. He found that 14% said they knew someone who had fabricated data, while a massive 72% said they knew someone who has published papers with “questionable research practises”.

As Fanelli points out, it is sometimes difficult to interpret what researchers may term as misconduct, “the fuzzy boundary between removing noise from results and biasing them towards a desired outcome might be unknowingly crossed by many researchers”.

Sweden wins race to host next-generation neutron source

Sweden will host Europe’s next-generation neutron facility that, once built, will be the most powerful source of neutrons in the world. The €1.48bn European Spallation Source (ESS) will cater for thousands of researchers every year in fields from condensed-matter physics to biology.

At a meeting of research ministers in Brussels last night to decide the site for the ESS, nine countries including France, Germany and Italy supported Lund’s bid. Only one country supported another candidate bid. The other bids to host the ESS were from Bilbao, Spain and Debrecen in Hungary.

The ESS will generate intense beams of neutrons by a process called “spallation”. The Lund design will accelerate protons to energies of 1.3 GeV, with a beam power of 5 MW, before smashing them into 1200 litres of liquid mercury. Neutrons will be driven out from the mercury nuclei, before being cooled and guided to a maximum of 44 experimental stations.

The ESS will specialize in long wavelength, or “cold”, neutrons that suit experiments on large-scale structures such as biological molecules. The Lund bid has been promised 50% of the total costs – including funds for 22 instruments – from not just the Swedish government but Denmark and Norway too. The rest will come from other governments such as the UK and Germany, which will be able to claim beam time in proportion to the amount of funding they provide.

“We have an excellent infrastructure in Lund with nearby science parks and technology companies, and everyone speaks English,” says Colin Carlile, director for ESS Scandinavia. The bid was also boosted by the Swedish government’s decision in October last year to build a 3 GeV X-ray synchrotron facility – MAXIV – that would be the brightest in the world once constructed, next to the ESS.

The ESS is expected to have running costs of about €100m per year and the first neutrons are expected 10 years from now with all the instruments to be completed five years after that.

“The ESS will be more powerful than the Spallation Neutron Source in Oak Ridge in the US,” says Peter Tindemans, chair of the ESS Initiative, which represents the various consortia bidding to host the facility. “It will be the first long-pulse source in the world, making it different from all existing neutron facilities.”

New method to seek life-supporting exoplanets

 

Scientists in the US have come up with a new method to search for oceans on “exoplanets” — planets outside our Solar System. The method, which involves studying how colours shift with an exoplanet’s rotation, could help in the quest for discovering extraterrestrial life.

There are several methods already used to spot water on exoplanets. One is spectroscopy, which can reveal the characteristic absorption wavelengths of water molecules and which has already been used successfully on giant planets. Others involve searching for the appearance of clouds or the glint of light shining off a reflective surface, although this latter technique has so far only been used for other liquids, such as methane on Saturn’s moon Titan.

Now Nick Cowan at the University of Washington in Seattle and others, including those on NASA’s EPOXI mission team, have designed a complementary method that should boost the chances of finding exoplanets with oceans — and, therefore, with life. “Since water is thought to be a prerequisite for life, we have effectively proposed another test for habitability,” Cowan told physicsworld.com.

Earth as an exoplanet

The researchers developed their method using data from Deep Impact, a NASA space probe that was launched in January 2005 to study the composition of a comet orbiting the Sun. Since Deep Impact completed this primary mission a few months later, it has been progressing on an extended mission called EPOXI to study another comet as well as distant exoplanets. During this extended mission, Cowan and colleagues have used the “high resolution imager” telescope on Deep Impact to examine Earth from a distance of a few tens of millions of miles, as though our planet were an exoplanet.

The overall colour of Earth is grey with some blue due to Rayleigh scattering of sunlight off the atmosphere. However, the researchers found that where the sky is clear — that is, with no clouds — the average colour changes with the Earth’s rotation: when the continents are in view, the colour shifts towards the red end of the spectrum; when the sea is in view, the colour shifts further into the blue. Such changes of colour should be able to reveal oceans on real exoplanets.

“The upshot [over the other methods] is that we don’t need very much spectral resolution — a few different filters would suffice — but we need pretty short exposures so that we can track time-variability,” says Cowan.

Bigger telescopes

However, Cowan adds that to see oceans on real Earth-sized exoplanets, which would be at least several light years away, astrophysicists would need a much larger telescope. This could come in the form of the proposed successor to the Hubble Space Telescope, called the Advanced Technology Large-Aperture Space Telescope, or ‘ATLAST‘, although it would need a device known as a coronagraph to block out the light from an exoplanet’s host star.

Still, it might be possible to see oceans on giant, “super Earth” planets when NASA’s forthcoming New Worlds observatory goes into orbit, perhaps by 2017. New Worlds will combine a large, 4 m diameter telescope with a very large coronagraph specifically for the detection of exoplanets.

Andreas Quirrenbach, an astronomer at the University of Heidelberg in Germany who is member of the US Exoplanet Task Force, thinks it might be a “matter of taste” whether this method would give proof of extra-solar oceans. “I myself would demand a higher standard, i.e. a spectrum, and I believe most astronomers would feel the same way,” he says.

But Quirrenbach adds that the method could serve either to give clues where watery planets exist, so that they can be followed up with spectroscopy, or simply complement spectroscopy to give more information. Over time, he says, the method could “develop into a tool to carry out a census of ocean-bearing planets around many stars, once we have convinced ourselves that the method is reliable by checking a fair number of cases spectroscopy.”

The research will appear in the August Edition of The Astrophysical Journal

Particle physics – it matters, say UK policy makers

A new report, Particle Physics – It Matters, was released today after collaboration between the UK Institute of Physics (IOP) and the UK Science and Technology Facilities Council (STFC). CERN physicist and TV presenter Brian Cox was alongside STFC Director of Science Programmes, John Womersley, at the IOP headquarters in London to present the report to the UK media.

One of the key messages in the report is the imperative to continue investing public money in fundamental research, like the Large Hadron Collider at CERN, despite the deepening recession. “Getting ourselves out of this mess will require a scientifically trained workforce,” said Womersley.

With the UK being a leading investor in the experiments at CERN the report places a strong emphasis on the economic return of this facility. For every £1 CERN pays to an industrial contractor, it generates £3 of utility, claims the report.

Both presenters were eager to point out the wide benefits of applications that have sprung incidentally from particle physics, such as the World Wide Web and the charge couple devices (CCDs) found in digital cameras. Looking to the future, Cox also described emerging spin-offs like grid computing and the idea of converting nuclear waste into less harmful material using high energy proton accelerators.

Womersley was similarly optimistic about the continued emergence of new technologies from particle physics, but he also talked about the need for scientists and policy makers to develop a common language to aid the decision-making process over science funding. He rejected the allegation that the Government have been short-sighted over previous policy decisions. “The political importance assigned to climate change, which is certainly an issue beyond the horizon of the next budget, shows that the Government are not immune to long-term thinking.”

On this issue, Cox emphasized the economic and political incentives for investing larger amounts of money in UK science, perhaps even “doubling” current investment. “Investing in fundamental science is perhaps the cheapest way of becoming a global leader in anything,” he said.

Particle Physics – It Matters can now be downloaded from the Institute of Physics website.

What’s your view of astronomers?

By Michael Banks

This month was undoubtedly a good time to be an astronomer. The European Space Agency launched the Herschel and Planck satellites that will map the geometry of the universe and study the formation of the earliest galaxies.

While NASA astronauts upgraded and repaired the Hubble Space Telescope to extend the mission’s life until 2014 and giving it increased resolving power to image galaxies in even more detail.

One would think that these missions, in conjunction with the International Year of Astronomy, would help astronomy grow in the public’s imagination. So this year is perhaps a good time as any to take stock and improve how astronomers are perceived by the public.

Michael West, an astronomer at the European Southern Observatory (ESO), has documented some examples of how astronomers in the past have been revered, reviled and also ridiculed as well as offering some ideas about how astronomers can improve their public image.

But why do astronomers care about their image? Well, according to West most developed countries spending on astronomy “is usually equivalent to the cost of one or two cups of coffee per resident” so during times of economic difficulty astronomy could be a tempting subject to cut.

Indeed, astronomers in the UK might concur with West as the UK recently cancelled funding for the Clover telescope, which would have searched for the signatures of gravitational waves in the Comic Microwave Background.

So as astronomy is funded by the taxpayer and also needs the support of politicians to get funding, West points out that the image of astronomy matters greatly.

West documents a number of examples when astronomers had enjoyed favourable public opinion or even elite status including a time as far back as 840 AD when an imperial edict issued by the Tang dynasty said that Chinese astronomers “are on no account to mix with civil servants and common people.”

More recently, West points to a poll in the New York Times in 2005 where the public voted the fifth most prestigious occupation as being an astronomer or physicist.

But perceptions have not always been so rosy. According to West, the recent debacle when the International Astronomical Union stripped Pluto of its planet status was a “public relations disaster” causing the public to express their outrage about the decision.

West points to a review of the fiasco by astronomers David Jewitt at the University of Hawaii Institute for Astronomy and Jane Luu at the Massachusetts Institute of Technology. They conclude that the public perception of astronomers has been damaged as a result and that “millions of people now think of astronomers as having too much time on their hands and are unable to articulate the most basic definitions.”

So what are his solutions? Not surprisingly, West says that astronomers must learn to communicate with the public and points to a programme run at ESO that gives astronomers media training and helps them become better science communicators.

West also says that astronomers should join the social networking bandwagon and use websites such as Twitter and Facebook as well as writing blogs to communicate their results to the public.

Indeed, the astronomer Edward Bigelow noted in a letter to the magazine Popular Astronomy that “the greatest present need of astronomy, is not more big telescopes and big observatories, but a more favourable public opinion.” That was not in 2009, but 1916. Almost 100 years later, West sees these sentiments just as relevant today.

Obama nominates new NASA boss

The Obama administration has nominated former astronaut Charles F Bolden as NASA’s next administrator. If, as expected, the Senate approves his nomination, Bolden will take over from associate administrator Chris Scolese, who has been in charge of NASA since previous boss Michael Griffin resigned in January. Meanwhile, Lori Garver, president of the consulting firm Capital Space, is set to become deputy administrator.

Bolden, a retired general in the US Marine Corps, took part in four shuttle missions. He served as NASA’s assistant deputy administrator from 1992 to 1994. Bolden was also an official adviser for the current maintenance flight to the Hubble Space Telescope, having piloted the space-shuttle flight that put the observatory into orbit in 1990.

“I believe he is a competent and enthusiastic administrator, and NASA needs both of those characteristics,” Gene McCall, a senior scientist at Los Alamos National Laboratory told physicsworld.com. “Bolden knows NASA well, particularly the manned space programme, but he is less familiar with the scientific programmes.”

Once in office, Bolden will have to manage the transition from the space-shuttle programme to its replacement, the Constellation programme, and to strike a balance between manned and unmanned missions. He will also have to manage relationships with powerful members of Congress who have interests in the agency.

The Obama administration has also started a review into NASA’s human spaceflight programme, which is being headed by Norman Augustine, former chief executive of the technology firm Lockheed Martin. He will report his findings in August to Bolden, who will decide whether or not to accept the recommendations.

“The plan at the time of the inauguration was to name a NASA administrator and have them immediately order the review,” says John Logsdon, a space-policy expert at the National Air and Space Museum in Washington, DC. “When the nomination process dragged on, the White House decided it could not wait any longer to start the review.”

How your research makes the headlines

science news.jpg
Churnalism

By James Dacey

I wrote last week about Ben Goldacre, the impassioned medical doctor cum journalist who is waging war against the crackpots and media institutions who churn out sensational headlines based on Bad Science.

For a lighter take on the science news cycle check out this comic by Jorge Cham, originally posted on his website phdcomics.com.

Like all good observational humour it is devilishly witty whilst capturing the essence of an everyday activity. With a liberal sprinkling of hyperbole!

Some of the keener researchers out there may be familiar with Cham from his talks on the conference circuit.

Cham began producing comics about life in academia whilst studying for his PhD in mechanical engineering at Stanford.

Since realising where his talents and passion lie he has been working full time on his comic strip Piled Higher and Deeper.

And yes I do see the irony in posting a blog about “churnalism” based on the content of someone else’s website…

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