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MiniBooNE rules out new kind of neutrino

Neutrinos are elementary particles with no electric charge that barely interact with matter. According to the original Standard Model of particle physics, neutrinos come in three types or “flavours” – electron, muon and tau – all of which should have no mass. But in recent years several experiments have given clear evidence that neutrinos can change or “oscillate” from one flavour to another over long distances. This effect has led physicists to conclude that neutrinos do have mass after all, thus forcing them to make subtle modifications to the Standard Model.

However, physicists have long been puzzled by a rogue result obtained by the Liquid Scintillating Neutrino Detector (LSND) at Los Alamos in 1995, which hinted at oscillations between anti-muon neutrinos and anti-electron neutrinos. What was odd was that the large value measured for the “mass difference” – one of the six parameters that govern neutrino oscillations – was inconsistent with previous measurements. If the LSND’s claims were true, the Standard Model would need a major overhaul, possibly requiring the existence of a fourth kind of “sterile” neutrino with unusual interactions.

The MiniBooNE experiment at Fermilab, which began taking data in 2002, was designed to look for the same kind of oscillations seen with the LSND experiment but to do so with a higher degree of accuracy. It involves searching for signs of electron neutrinos in the hoards of muon neutrinos produced 500 m away by an 8-GeV beam of protons from Fermilab’s Booster accelerator. The conclusion: there is no evidence to support LSND’s claims.

David Wark of the Rutherford Appleton Laboratory in the UK told Physics Web that this is good news for the Standard Model: “It means that the picture we have of neutrino oscillations looks secure, and we can proceed without a troubled conscience to the next generation of particle physics experiments such as T2K and NOvA.” The null result also means that sterile neutrinos are unlikely to exist. “They’ve gone from ghosts that clunk in the night to ghosts that make no sound whatsoever,” Wark added.

MiniBooNE must now repeat its experiment using anti-muon neutrinos to comprehensively rule-out the LSND’s results. If this version finds oscillations, which would be unlikely, it would mean a violation of so-called charge-parity-time (CPT) symmetry and consequently Einstein’s special relativity. “The Standard Model is not quite out of the woods yet,” said Wark.

Mild forecast for next solar cycle

The fact that the Sun goes through cycles of activity was first noticed in the mid-19th century when astronomers began charting the number of cool, dark patches or “sunspots” on the solar surface where magnetic activity is intense. However, in the mid-1970s — when the first accurate data of the Sun’s polar magnetic field started being recorded — astronomers found evidence for a possible link between the value of the field at the end of one cycle and the overall strength of the next cycle. If such a link does exist, one could then predict the strength of future cycles based on past data. Indeed, the polar field is so low in the current solar cycle that the next cycle is predicted to be the weakest for 100 years.

Rather than relying on observational data to predict the strength of future cycles, however, two US physicists last year tried to predict the activity of solar cycles by theoretically modelling the Sun’s internal “dynamo action”, which converts the turbulent movement of solar material into magnetic energy. Strangely, the model, which was developed by Mausumi Dikpati and Peter Gilman from the National Center for Atmospheric Research in the US, predicted that the peak activity of the next cycle would be very high — quite at odds with the method using observational trends.

Arnab Rai Choudhuri and colleagues from the Indian Institute of Science in Bangalore and the Chinese Academy of Sciences in Beijing now think that Dikpati and Gilman’s model was flawed because of the way it treated a key element of the dynamo model known as the “Babcock-Leighton mechanism”, which produces a weak “poloidal” field when pairs of sunspots decay. Dikpati and Gilman fed records of past sunspot data into their model to calculate the strength of this mechanism, but Choudhuri’s team say that the production of the poloidal field is inherently random and cannot be calculated in this way. Instead, they have created a model that is “corrected” around the minimum by polar magnetic field data, which they say is more accurate.

Using this model, Choudhuri’s team calculate that the next cycle (known as cycle 24) will be about 35% weaker than cycle 23. If they are correct, this would be good news for satellite communications, because solar flares and coronal mass ejections, which can generate violent magnetic storms in the Earth’s atmosphere, become more common as solar activity increases. But Choudhuri is happy to wait to see if he is right. “We shall have a verdict from the Sun-god himself within the next four to five years whether [Dikpati and Gilman’s] prediction or our prediction comes closer to the truth,” he said in a recent review paper.

Spins turn light off

Many researchers are trying to develop “spintronic” devices that use the spin of the electron as well as its electrical charge to store and process information. Others, meanwhile, are trying to exploit the interaction between light and the collective oscillations of electrons on the surfaces of metals (called plasmons) to create “plasmonic” devices for processing and transmitting data. Now, Abdul Elezzabi and Kenneth Chau at the University of Alberta, along with Mark Johnson at the Naval Research Laboratory in Washington, DC, have created a material that combines spintronics and plasmonics to switch a beam of terahertz light.

When their material is exposed to an external magnetic field, the electrons in the micrometre-sized cobalt particles become spin polarized. If light in the terahertz frequency range is shone on the material, the electromagnetic field associated with the light drives some spin-polarized electrons from the cobalt into the partial gold coating (see figure). This leads to an electrical resistance between the gold and cobalt called anisotropic magnetoresistance (AMR).

With the magnetic field turned off, there is no AMR and much of the light is transmitted through the material via plasmons. However, as the field is turned on, the increased resistance brought on by AMR impedes the flow of plasmons and the light transmission drops by over 70% in some samples.

Elezzabi told Physics Web that the team has observed this switching effect in other magnetic materials and is currently trying to find materials that enhance the effect. He said that in principle the effect is not restricted to terahertz light – which is sandwiched between the ultraviolet and microwave bands – but it would be difficult to achieve at higher (microwave) frequencies because the light’s electric field oscillates so rapidly that spin-polarized electrons would not accumulate in the gold coating.

Elezzabi also said that the group are in the process of filing a patent related to several devices based on the effect.

Buffer boosts optical integration

Current optical communications systems exploit silicon-based integrated circuits for processing electronic signals, and separate devices for processing optical signals. For optical switches and modulators to be created on a silicon substrate, a material with a strong electro-optical effect (where the refractive index changes under an applied voltage) must be formed on the substrate.

One suitable material is the ferroelectric material lead zirconate titanate (PZT). But it has so far been difficult to propagate light successfully through PZT, due to disruption of its crystal structure caused when a single-crystal film is formed on top of the silicon substrate.

Now a team of engineers from the Tokyo Institute of Technology and Fujitsu laboratories have overcome this problem by fabricating a three-layer buffer between the PZT optical layer and the silicon base. The buffer minimizes disruption to the film’s atomic alignment, as well as preventing any reaction between the optical layer and the silicon substrate.

The buffer zone comprises strontium ruthenium oxide, ceria, and yttrium-stabilized zirconia layers, over which a single-crystal film of PZT is formed.

Using the standard wavelength of infrared light used in optical communications, 1550 nm, the PZT propagation loss was reduced to less than 1 decibel per centimetre. This is claimed to be only 10% of the losses usually seen in PZT.

This work brings closer the ultimate goal of processing both electrical and optical signals on a shared substrate, removing one of the major barriers to any substantial integration and opening up the prospect of ultra-compact optical communications systems.

The new technology was supported by the Japanese government, and will be presented at the 24th Meeting on Ferroelectric Materials and Their Applications (FMA-24) and at the International Symposium on the Application of Ferroelectrics (ISAF 2007) to be held in Nara, Japan, from 27 May 2007.

Relativity trick slashes computing times

“There’s no such thing as a free lunch” is the usual response Vay receives when he tells his particle-physicist colleagues how to speed-up computer simulations a thousand times over by making a simple mathematical transformation. And it’s hardly surprising: many physicists use relativity theory routinely, and think they already know how to simplify calculations by considering relativistic interactions from the perspective of an observer in a convenient “reference frame” where many tricky factors cancel-out.

Although such reference frames help the human brain to get to grips with the interactions, Vay says they do no favours for computer programs. In a particle accelerator, for example, a centimetre-wide pulse can cover distances of many kilometres – and this huge difference in length scales makes computer simulations very time consuming. Instead, he says that if the reference frame itself is moving relativistically compared to the interaction, the difference in scales becomes much less significant.

“The first time I noticed it my reaction was to think that I had made a mistake in my calculations,” Vay told Physics Web. “After I checked them, I assumed that it was probably known already and I used it without reporting it formally. Only last year I realized it was largely unknown.”

Vay’s method of choosing reference frames works because of a familiar effect of relativity known as length contraction. If an observer is in a reference frame that is moving fast compared to an object – and the closer to the speed of light the better – the length of that object appears to be shorter. Vay realized, however, that not only do individual lengths reduce, but also the difference between them. This means that simulations run from the perspective of a relativistic reference frame are much less complex, and therefore take much less time to compute.

Vay has tried his method on several examples of relativistic interactions including a free-electron laser, a laser-plasma accelerator, and a particle beam colliding with an electron cloud. For the particle beam example, the simulation in a typical reference frame took over a week to run, whereas in Vay’s relativistic, “ideal” reference frame it took just half an hour.

Groups at the University of California in Los Angeles and Tech-X Corporation in the US are already exploring Vay’s time-saving method for simulating relativistic experiments. Nevertheless, the question remains of why such a simple consequence of relativity has never surfaced. “Computer simulations didn’t exist when relativity was invented,” said Vay. “It’s plausible that the effect was identified early on by the founders of relativity, but didn’t lead them to any interesting applications.”

Electron tunnelling seen in real time

A laser pulse consists of a small number of electric-field oscillations that can pull the outer electrons of atoms away from their binding nuclei. At the peaks of these oscillations, the pull can be so great that the outer electrons are given a chance to escape (or tunnel) from the atom, even though they don’t have enough energy to overcome the attractive pull of the nucleus. But this process occurs so quickly that current instruments can only see the final ionized atom, and not any intermediate states.

Ferenc Krausz and colleagues from the Max-Planck Institut für Quantenoptik have now found a way around instrument limitations by probing atoms with two pulses of different-wavelength light that are carefully-timed to take snapshots of the tunnelling process.

The technique involves probing atoms that have very tightly bound electrons – in this case those of neon – which do not readily ionize with a laser pulse alone. The atoms must first be prepared by an exciting pulse, which sends some of the electrons to outer regions of the atom where tunnelling can be induced by an ionizing pulse.

This two-stage process is where the advantage lies: if the exciting pulse has a much shorter wavelength than the ionizing laser pulse, it can be switched on at many points in the ionizing pulse’s cycle, and only at these points will electrons be in a position to tunnel. Then, by noting when in the ionizing laser’s cycle the electrons tunnel, a picture of how the electrons leave the atom can gradually be reconstructed.

In practice the two pulses must be synchronized to within several billion-billionths of a second to achieve any sort of accuracy. To get over this hurdle, Krausz and his team used the same infrared laser to make both pulses. First, they shone the laser though a gas jet to produce a pulse of extreme (very short wavelength) ultraviolet light. This pulse then travelled to the sample of neon atoms with the original laser pulse delayed behind. Finally, using mirrors to carefully alter the delay, the physicists could chart the tunnelling of the electrons with a resolution of less than one femtosecond (10-15 s).

According to 40-year-old quantum theory, the probability of an electron tunnelling through the potential barrier should increase stepwise with every successive peak of the ionizing pulse. Now Krausz and his team are the first to be able to confirm this is exactly the case (see figure: “Tunnelling”).

The light-induced tunnelling technique may now be used to provide further observations of electron movement, giving scientists unprecedented insights in areas such as microelectronics and biological imaging. “There may be issues with transient [short-lived] states that we’ve never been able to capture,” Jonathan Marangos, an expert in sub-femtosecond technology, told Physics Web. “This technique will enable us to do that.”

Angling for the best knot

Determining exactly where a knot breaks in a material is not easy. First, the shape of the knot changes as it is tightened. Second, it is difficult to watch how the broken strands recoil, which takes place very quickly. Third, most knots unravel after breaking, making it hard to reconstruct a broken knot.

Hiroki Uehara and colleagues at Gumna University have now found a simple solution to these knotty problems. They first stretched a knot to nearly its breaking point and then daubed ink onto the exposed portions of the knot – leaving the internal portions of the knot unstained. After the ink had dried, they continued to pull until the knot broke. By comparing the ink patterns on the strand before and after breaking they were able to determine exactly where the knot failed.

The researchers focused on simple “torus” knots, which can be characterized in terms of how many times the strand crosses over itself in the knot (see figure). When the knots were made in the PVDF (poly(vinylidene fluoride)) material, Uehara and colleagues were surprised to find that knots with the lowest crossing numbers were significantly stronger than knots with higher numbers – which is exactly the opposite of what is observed with traditional, nylon fishing line.

By examining the broken strands using optical and electron microscopes, the physicists discovered that torus knots with low crossing numbers broke due to the bending of the strand at one edge of the knot. However, torus knots with high crossing numbers broke deep inside the knot as a result of the twisting of the strand.

Uehara told Physics Web that the results suggest that nylon is more flexible and resistant to damage by twisting than PVDF, but that more experimental work is needed to understand the processes involved.

Preliminary tests on a different type of knot in PVDF (called a “twist knot”) suggest that strength increases with crossing number in that knot – the opposite of what was seen for PVDF torus knots. Uehara believes that this occurs because there is actually much less twisting in a twist knot.

Physicists take a crack at rocks

Humans have been cracking rocks for at least one million years – first to make tools and then to quarry and shape building materials. While both stone-age toolmakers and modern-day mechanical engineers have developed a practical understanding of the cracking process, a microscopic theory of cracking has remained elusive. The problem is that most rocks are made of grains that come in many different shapes and are arranged in many different ways. This makes it very difficult to predict when and where a crack will begin and how it will propagate.

Despite these structural variations, Jörn Davidsen of the University of Calgary and colleagues at the GeoForschungsZentrum Potsdam have found that a collection of different rock samples (two sandstones, two granites and a basalt) appear to crack in a very similar manner.

The rocks were fractured by subjecting them to external pressure and detecting the sounds emitted during microcracking events. Microcracks are tiny ruptures that occur in the rock before it shatters.

The team then analysed the sounds to determine the magnitude of the microcracks and the “waiting times” between successive events. Waiting times are important because they reveal how successive microcracks lead to the large-scale structural failure of a material.

Davidsen and colleagues then took the waiting times for each sample and divided them by the average waiting time for that sample. Amazingly, the probability distribution of these normalized waiting times could be described by the same mathematical formula known as a gamma function — which gives a high probability for short waiting times, with the probability dropping rapidly for longer waiting times.

The waiting times shared the same probability distribution despite the fact that the average waiting times of the rocks differed by a factor of almost 100 from sample to sample. The team also showed that normalized waiting times associated with sounds emitted after an earthquake are described by the same distribution – suggesting that the cracking of rock on a massive scale is associated with earthquakes.

Davidsen told Physics Web that the universal nature of the probability distribution suggests that the precise microscopic details of the material may not play a significant role in the cracking process after all. This could mean that a successful model of rock cracking could be developed without having to worry about the rocks at a microscopic level. The researchers are now busy trying to develop a model of cracking that can reproduce the observed universality.

A triangle that matters

When is a triangle not a triangle? Believe it or not, this peculiar riddle encapsulates much of the latest research in particle physics. The triangle in question is the “unitarity triangle”, an abstract diagram representing the interactions between different types of quarks – the fundamental constituents of neutrons and protons. A vital part of the Standard Model of particle physics, the unitarity triangle provides clues about the subtle difference between matter and antimatter, helping to reveal why the universe did not vanish into nothingness immediately after the Big Bang.

By rights, an equal amount of matter and antimatter should have been created in the Big Bang. But the universe we see today consists entirely of matter, implying that there must be some difference between the behaviour of particles and of their corresponding antiparticles. The Standard Model incorporates such a difference via a phenomenon called charge–parity (CP) violation – a broken symmetry of nature that was discovered experimentally in the 1960s. It is this phenomenon that links the unitarity triangle to the real world, since the extent of CP violation – and hence the degree to which matter and antimatter differ – is proportional to the area of the triangle.

However, the amount of CP violation predicted by the Standard Model can only account for about a billionth of the matter–antimatter imbalance we see in the universe. In fact, this is just one of several problems with the Standard Model; others being that it does not explain gravity or the identity of “dark matter”. Hence, physicists believe that, despite its many successful predictions, the Standard Model will eventually be overthrown by a more general theory. One way to test such theories is by measuring the properties of the unitarity triangle: according to the Standard Model, it is perfectly triangular; but if new particles exist, then the triangle will be “broken”.

Since the discovery of CP violation, various experiments have measured its effects on particles called neutral kaons, but such measurements do not relate directly to the properties of the unitarity triangle. However, in the last few years researchers at huge particle physics experiments called BaBar and Belle in the US and Japan, respectively, have made precise measurements of the angles and the lengths of the sides of the unitarity triangle by studying the behaviour of different particles called B-mesons. The results so far show that the diagram is very close to triangular. But there is still room for uncertainty, and refining our knowledge of the unitarity triangle with future experiments is a crucial way to finally take physics beyond the Standard Model.

Violating symmetry

In the Standard Model, all matter is made up of quarks and leptons, each of which comes in six different types or “flavours”. Both quark and lepton flavours fall into three generations of two particles each: for quarks these are up and down, charm and strange, and top and bottom; while the lepton generations each contain a charged lepton – electron, muon and tau – and a correspondingly named neutrino. Each quark and lepton also has an antimatter partner. All atoms are constructed from just the particles of the first generation – up and down quarks (which combine to form protons and neutrons) and electrons. One of the fundamental questions in particle physics is why there should be two, and only two, additional generations with similar properties but greater mass.

To complicate this picture of the subatomic world, the flavour of a quark can change as a result of the weak interaction. For example, nuclear beta decay – in which a neutron decays into a proton, an electron and an electron antineutrino – is the result of a down quark in the neutron converting to an up quark by emitting a “W-boson”, one of the particles that carry the weak interaction. Because W-bosons have a charge of ±1 (in units of the electron’s charge), such conversions can occur only between “up-type” quarks (up, charm, top), which have a charge of +2/3 and “down-type” quarks (down, strange, bottom), which have a charge of –1/3.

The probability of each of the nine possible quark flavour changes is described using a 3×3 matrix called the Cabibbo–Kobayashi–Maskawa (CKM) mixing matrix. The rows of the matrix correspond to the uptype quarks, the columns to the down-type quarks and the square of each element of the matrix gives the probability of that particular flavour change occurring (see below). Meanwhile, the weak interactions of antiquarks are governed by the complex conjugate of the CKM matrix – the matrix formed by keeping the real part of each element the same but reversing the sign of the imaginary part. Therefore, if the CKM matrix contained no imaginary elements, quarks and antiquarks would have exactly the same weak interactions.

However, experiments show that this is not the case due to CP violation. The letters C and P represent symmetry operations: C, for charge conjugation, means exchanging every particle in a system with its antiparticle; and P, for parity, means reversing all three spatial coordinates. Until the 1960s physicists thought that if both the C and P operations were carried out on a system simultaneously, the new system would behave in exactly the same way as the original. However, in 1964 Jim Cronin and Val Fitch at Princeton University observed that the decays of particles called long-lived neutral kaons, consisting of down and strange quarks and antiquarks, did not respect CP symmetry. This discovery, which earned Cronin and Fitch the Nobel prize, was a shock, and it took 10 years before Makoto Kobayashi and Toshihide Maskawa of Kyoto University in Japan proposed a solution in the form of the CKM matrix.

At the time of Cronin and Fitch’s discovery only quarks from the first two generations were known, which only allows for a 2×2 mixing matrix with real-number elements – following the 1963 proposal of Nicola Cabibbo. Kobayashi and Maskawa’s idea was to introduce a third generation of quarks, leading to a 3×3 matrix that contains complex numbers and therefore accommodates CP violation. Predicting the existence of two new quarks was a radical step, but the gamble paid off in 1977 when the bottom quark was discovered at Fermilab in the US. Indeed, the CKM matrix was a well-established part of the Standard Model even before the discovery of the top quark (the up-type version of the bottom quark), also at Fermilab, in 1995.

The nine elements of the CKM matrix are not all independent. For example, since an up quark must convert into one of the three down-type quarks, so the three associated probabilities must sum to one. In fact, the CKM matrix can be expressed in terms of just four independent parameters: three real “mixing angles” and one imaginary “phase” that leads to CP violation. The unitarity triangle is simply a way of representing these numbers in a diagram, first proposed by James Bjorken and Cecilia Jarlskog in 1988, where the angles (labelled α, β and γ) and the lengths of the sides (Ru and Rt) correspond to certain combinations of elements of the CKM matrix (see figure 5). The height of the triangle depends on the imaginary phase, so it is precisely because the CKM matrix includes complex numbers that the unitarity triangle is a triangle, not a 1D line.

Although Kobayashi and Maskawa had successfully predicted the third generation of quarks, to confirm that this was indeed the correct explanation of CP violation researchers had to show that the unitarity triangle really is triangular by determining its angles and sides. This can be done by measuring carefully chosen decays of particles in which the changes of quark flavour that occur, and hence the elements of the CKM matrix involved, correspond to one of the parameters of the triangle.

Critically for these experimental measurements, CP violation is expected to be much larger for particles containing bottom quarks than it is for the kaons in which it was first observed. That is, particles containing bottom quarks can behave very differently to those containing bottom antiquarks. This can be seen, for example, in the different rates at which B-mesons and antimesons (combinations of a bottom quark or antiquark with an up or down quark or antiquark) decay to give certain products. By studying these “CP asymmetries” in the B-meson system, researchers can therefore pin down the properties of the unitarity triangle.

A production line for bottom quarks

Only a tiny fraction of B-mesons undergo the interesting decays for which large CP asymmetries are predicted. In order to constrain the unitarity triangle, we therefore need to produce huge numbers of B-mesons, which calls for a particle collider known as a “B-factory”. In these machines, electrons and positrons are smashed into each other with just the right energy to create a particle called the Y(4S), which consists of a bottom quark and antiquark, and which decays almost immediately into a B-meson and antimeson. Crucially, the electron and positron beams in these colliders do not have the same energy, so that conservation of momentum ensures that the B-mesons produced are moving. This allows researchers to determine the time the particles take to decay, and hence their decay rate, from the distance that they travel before they do so. Two such asymmetric machines were completed in 1999 at the Stanford Linear Accelerator Center (SLAC) in California and KEK in Japan.

The primary objective of these B-factories was to measure the angle β of the unitarity triangle, so the target rate of electron–positron collisions was set by the estimated number of B-mesons needed to measure this parameter accurately. Serendipitously, at the time those estimates were made, the top quark was expected to be much lighter than it was subsequently found to be. This miscalculation, together with competition between SLAC and KEK, pushed the machines to achieve extremely high collision rates. Over a billion B-meson pairs have now been produced by the two B-factories, and their accompanying particle detectors – BaBar at SLAC and Belle at KEK – have reaped the benefits of the extra data.

The specific process that allows β to be measured is the asymmetry in the decay rates of B0-mesons (a bottom antiquark and a down quark) and B0-antimesons (a bottom quark and a down antiquark) to two other mesons, Ks (the short-lived neutral kaon) and J/ψ (a charm quark and antiquark). This asymmetry arises because a B0-meson can decay to a J/ψ and a Ks either directly or after first “oscillating” into a B0 – and vice versa for a B0. Oscillation is a phenomenon whereby a neutral B-meson can transform into its antimeson by momentarily creating a particle–antiparticle pair of “virtual” top quarks – the uncertainty principle allows the much heavier top quarks to be created but only for a very short time. Due to quantum-mechanical interference between the direct and oscillating decay routes, B0-mesons on average live slightly longer before decaying to J/ψ and Ks than do B0. Because of the particular elements of the CKM matrix that correspond to the flavour changes in the oscillation and direct decay, the size of this asymmetry is proportional to sin2β.

To observe this asymmetry, researchers first need to identify large numbers of decays resulting in J/ψ Ks, which is made more difficult by the fact that this particular decay only occurs once in every 2000 decays (see figure 2). We then need to know whether it was the B0 or the B0 from the initial collision that decayed to the J/ψ and Ks. This is done by looking at how the other meson produced in the electron–positron collision decayed to determine whether it was a B0 or a B0 – an operation known as “flavour tagging”. Finally, to determine how long the B-mesons lived, we must measure the position at which they decayed. It was these requirements to be able to tag flavour and measure decay positions accurately that drove the design of the BaBar and Belle detectors (see below).

The BaBar and Belle teams published their first results on the B0 → J/ψ Ks decay in 2001. As predicted by the Standard Model, they saw a large asymmetry in the decay rates of the B0 and B0 – enabling researchers to determine the angle β of the unitarity triangle. The teams have continued to refine these measurements, and the current world average is β = 21.2° ± 1.0°. The fact that the angle is non-zero means that CP violation definitely occurs in the B-meson system, and the amount agrees with previous studies of the much smaller CP-violation effects in the kaon system.

In order to define a triangle, however, it is necessary to measure at least two angles. It was initially thought that sin2α could be measured in much the same way as sin2β but using B0 → π+π– decays instead of B0 → J/ψ Ks. Since pions consist of up and down quarks and antiquarks, different elements of the CKM matrix are involved compared with the latter decay, and hence a different angle can be measured. However, unlike the B0 → J/ψ Ks decay, the asymmetry in the B0 → π+π– decay is not simply proportional to sin2α, so further calculation is necessary to extract the angle correctly.

Similarly, while it has been known for some time that the third angle, γ, can be obtained by measuring CP asymmetries in B → DK decays (where D is a meson containing charm quarks), it is hard to obtain precise constraints on the parameter because only about one in a million B-mesons decay to the relevant states. Nevertheless, impressive progress has been made in measuring both α and γ, thanks to close co-operation between theorists and experimentalists to devise new analysis techniques. The current world average values are α = 92° ± 7° and γ = 82° ± 20°. Within error, the three angles do indeed sum to 180°, but reducing their uncertainties remains of paramount importance to test for signs of “new physics”.

Sizing up the sides

What about the sides of the unitarity triangle? By definition the bottom side has a length of one, but the other two sides must be measured experimentally to test whether their lengths are consistent with the angles. This is known as “overconstraining” the triangle. If the Standard Model is correct, all the measurements will be consistent with a single triangle, while any deviation would indicate new physics at work. While the measurements of the angles rely on CP asymmetries between B-mesons and antimesons, the sides can be determined just from the rates of appropriate decays. This may sound less challenging, but considerable complications arise for measuring both sides.

The left-hand side of the triangle depends on the element of the CKM matrix that relates up and bottom quarks, Vub. There are two strategies to try to measure its value: the first, known as “inclusive”, requires the rate for B-mesons to decay into any particle containing an up quark (plus a lepton and a neutrino) to be measured; the second, “exclusive”, technique requires just the rate for one particular such decay. In both cases, some theoretical input is necessary in order to extrapolate the measurements into values of Vub, which is now measured as |Vub| = (4.09 ± 0.26) × 10–3. This gives the length of the left-hand side of the triangle as Ru = 0.381 ± 0.014.

The measurement of the other side of the unitarity triangle presents yet another complication. The crucial input to determine this side is the CKM element Vtd, which governs the rate of transitions from a top quark to a down quark. Yet the energies in the B-factories are far too low to produce the extremely massive top quarks. Furthermore, the small numbers of top quarks that have been produced at higher-energy colliders decay predominantly to bottom quarks. This makes it almost impossible to observe their much rarer decays to lighter quarks in any existing or proposed experiment.

However, all is not lost. As mentioned earlier, virtual top quarks are created in the oscillation of B-mesons, and it turns out that the rate of B0–B0 oscillations, which is described by the parameter Δmd, is governed by Vtd. It is extremely challenging for theorists to calculate the constants that relate Vtd to Δmd, but by considering the rate of oscillations of another neutral meson called the B0s (a bottom antiquark and a strange quark), given by Δms, progress has been made. In particular, a technique called lattice quantum chromodynamics has recently enabled the constants relating the ratio |Vtd|/|Vts| to Δmd/Δms to be obtained. Since the values of Δmd and |Vts| are known, the only missing piece of information is then Δms.

Measuring Δms is difficult because the B0s–B0s oscillations are very fast. However, last year the CDF experiment at Fermilab was able to make a remarkably precise measurement of Δms of about 2.75 THz (see Physics World July 2006 pp32–34, print version only). This allowed the length of the final side of the triangle to be measured as Rt = 0.904 ± 0.028. By overlaying all the measurements of the angles and sides on a single diagram, we are now able to examine whether they are consistent with a single triangle (see figure 3). So far, everything matches up with a triangle with a height of 0.344 ± 0.016.

The hunt for new physics

The precise measurements of the unitarity triangle are a triumph for the B-factories and the Standard Model, but they have nevertheless left many physicists downhearted. The reason is that despite the successes of the Standard Model, it has long been known that it cannot be the full story. As well as not being able to account for most of the matter–antimatter asymmetry in the universe, it does not explain the dark matter and dark energy thought by cosmologists to make up most of the universe, nor does it include gravity. It is fervently hoped that results from the Large Hadron Collider (LHC), starting up later this year at CERN, will provide evi dence of physics beyond the Standard Model. Yet physicists are impatient, and measurements of bottom quarks could provide clues before then – for example, if more precise measurements showed that the angles and sides of the unitarity triangle did not exactly match up.

One inconsistency in the triangle might be revealed by comparing the value of β determined from B0 → J/ψ Ks decays with measurements of the same parameter in different decays, such as those in which a bottom quark converts to a strange quark. These decays occur via virtual-particle “loops” in which the bottom quark decays into a virtual W-boson and an up-type quark, which then recombine to form a strange quark. If heavier, as-yet unknown particles exist, they could also be produced fleetingly in these loops, leading to measurable effects in rates of these decays. Recent measurements from BaBar and Belle suggest that there may indeed be new particles appearing in the loops that mediate such decays. At present, the experimental uncertainties are too large for us to be certain, but this is a tantalizing hint that theories beyond the Standard Model, such as supersymmetry, may be in action in the real world.

As the B-factories continue to refine their measurements, the LHC draws nearer to switching on. While about a million B-mesons per day are produced at BaBar and Belle, the LHC will produce many more than this number every second. In particular, the LHCb experiment, one of four detectors positioned around the LHC collider, will allow much more precise measurements of parameters such as γ via dedicated studies of the wealth of particles containing bottom quarks (see Physics World October 2006 pp37–39; print version only). However, because each proton–proton collision at the LHC will produce hundreds of particles, in stark contrast to the electron–positron collisions at the B-factories that produce only a B-meson and antimeson, it will be challenging to identify the decays of interest.

As well as producing more particles containing bottom quarks, a crucial advantage of the LHC is that it can produce a wider variety of these particles, in particular the B0s-meson, which is not produced by the B-factories. This will allow a more precise measurement of Δms and, more importantly, the first study of CP violation in B0s-mesons. For example, the LHCb will study the decay B0s → J/ψ Φ, which is analogous to the B0 → J/ψ Ks decay measured at the B-factories. Unlike the B0 decay, the CP asymmetry in this decay is predicted by the Standard Model to be rather small. Hence, if a significant amount of CP violation is observed, it will provide a clear sign of new physics.

It might seem that the observation of new physics would mean the end of the story for B physics and the unitarity triangle. But in fact, such a discovery would require much work to be done to determine the detailed properties of the new particles, and establish whether their CP-violation effects can make up the shortfall in our understanding of the matter dominance in the universe. For this, researchers are proposing a “Super Flavour Factory” – an electron–positron collider similar to the existing B-factories but with a rate of collisions at least 100 times greater. Such an experiment would allow us to precisely constrain the unitarity triangle – even though by then it may no longer actually be a triangle – as well as study for the first time processes that are particularly sensitive to the properties of new physics, such as decays of the tau lepton.

So, when is a triangle not a triangle? As far as we can tell from the impressive results obtained by the researchers at BaBar and Belle, not yet! But we know that there must be CP violation beyond that explained by the Standard Model, and we hope that new particles that may account for this will soon be observed at the LHC. This suggests that more precise studies will reveal a chink in the triangle, opening a rich new field of research to pin down the properties of the new physics.

Box: The CKM matrix and the unitarity triangle

The Standard Model of particle physics contains six “flavours” of quark – up (u), down (d), charm (c), strange (s), top (t) and bottom (b) – that are divided into three generations of “up-type” quarks (u, c and t) with a charge of +2/3 and “down-type” quarks (d,s and b) with a charge of –1/3. Quarks can change flavour from an up-type to a down-type or vice versa via the weak interaction. The probability for each of these flavour changes occurring is described by a 3×3 matrix with complex-number elements called the Cabibbo–Kobayashi–Maskawa (CKM) matrix, VCKM. For example, the square of the element Vud gives the probability for an up quark to convert to a down quark. The corresponding probabilities for antiquark conversions are given by the complex conjugate of this matrix, V*CKM. The fact that these two matrices are not identical (because they contain complex numbers) explains the phenomenon of CP violation, whereby quarks and antiquarks behave slightly differently.

Since the weak interactions have to conserve probability – that is an up-type quark must convert to one of the three down-type quarks but nothing else – the CKM matrix must be “unitary”. Mathematically, a unitary matrix has the property that when it is multiplied by its Hermitian conjugate, V†CKM (the transpose of its complex conjugate), the result is the unit matrix. This relationship leads to a number of equations relating the CKM matrix elements. Some represent the conservation of probability directly – i.e. the squares of the elements in each row or column must sum to give one – but there are others where three complex numbers sum to zero, such as: V*ubVud + V*cbVcd + V*tbVtd = 0

The latter relationships can be represented graphically on an “Argand diagram”, which has axes that correspond to real and imaginary numbers. On such a diagram, a complex number is represented by a line, and so the sum of several complex numbers can be represented by starting one line where the previous one ends, much like adding up vectors. In the unitarity equations of the CKM matrix, three complex numbers sum to zero, so the three lines join up to form a triangle known as a “unitarity triangle”. There are six unitarity triangles in all – one for each pair of columns or rows in the CKM matrix – and the height of each triangle corresponds to the amount of CP violation in the transitions of the quarks involved.

Most of the triangles are very elongated, corresponding to very small CP-violation effects. However, the triangle describing the transitions of bottom and down quarks is predicted to have sides that are approximately the same length as each other. Due to the importance of this triangle, it is usually known as the unitarity triangle. The unitarity triangle is conventionally drawn with the length of one side rescaled to unit length and rotated to lie along the real axis. The lengths of the other two sides and the three angles correspond to combinations of the elements of the CKM matrix and must be determined experimentally.

Box: BaBar and Belle

A million B-mesons per day are produced in electron–positron collisions at SLAC in the US and KEK in Japan. The decay products of the B-mesons are examined by huge particle detectors comprising many subsystems – BaBar (figure 6) at SLAC and Belle (figure 7) at KEK.

To determine the positions at which the B-mesons decay requires precise measurements of the paths of the decay products, which is achieved with silicon detectors located as close as possible to the collision point. It is also important to determine the type of particles produced in the decays. Both experiments use innovative particle-identification techniques that take advantage of the “Cerenkov radiation” produced when a charged particle passes through a material at a speed greater than the speed of light in that material. The angle at which this light is emitted depends on the mass of the particle allowing, for example, pions to be distinguished from kaons.

At a Glance: Unitarity triangle

  • The unitarity triangle is an abstract diagram representing how the six known quarks can transform into one another via the weak force
  • It is a vital component of the Standard Model of particle physics because it explains the subtle difference between matter and antimatter known as CP violation
  • The Standard Model predicts that the diagram is perfectly triangular, while more general proposed theories such as supersymmetry suggest that it is not
  • Researchers at particle colliders known as B-factories in the US and Japan have recently made precise measurements of the angles and sides of the unitarity triangle
  • Although these measurements are consistent with the diagram being triangular, particle physicists continue to hunt for deviations that could reveal new physics
  • Future machines, such as the Large Hadron Collider and a proposed Super Flavour Factory, will allow even more precise measurements of the triangle to test for physics beyond the Standard Model

More about: Unitarity triangle

P Harrison 2003 “Nature’s flawed mirror” Physics World July pp27–31
T Nakadaira 2004 “B-factories score direct hit on CP violation” Physics World October pp21–22
The Heavy Flavour Averaging Group
The CKMFitter collaboration
The UTFit collaboration

Blog life: Shtetl Optimized

Blogger: Scott Aaronson
URL: scottaaronson.com/blog
First post: October 2005

Who is the blog written by?

Scott Aaronson is a postdoc at the Institute for Quantum Computation at the University of Waterloo, Ontario, Canada. His research interests are computational complexity, quantum computing and the foundations of quantum mechanics. The strange title of the blog comes from a conversation among graduate students about who they would have been had they lived 700 years ago. “I would’ve been the chief rabbi of my shtetl,” said Aaronson. “All day long I’d debate questions like how much restitution you’d have to pay if your ox gored your neighbour’s sheep. And for this, I’d get an arranged marriage with the most beautiful girl in town.”

What topics does it cover?

While Aaronson writes mainly about quantum computing, other posts are divided into intriguing categories including “Adventures in meatspace”, “The fate of humanity” and “Rage against doofosity”.

Who is it aimed at?

Aaronson recently posted a non-mathematical explanation of Peter Shor’s algorithm for finding the prime factors of a large number using a quantum computer. This was described by Shor himself as “the best job of explaining quantum computing to the man on the street that I’ve seen”. But some posts are more technical. A list of the “ten most annoying problems in quantum computing” starts with: “Given an n-qubit pure state, is there always a way to apply Hadamard gates to some subset of the qubits so as to make all 2n computational basis states have non-zero amplitudes?”

Why should I read it?

Aaronson’s trenchant comments on the Canadian company D-Wave’s claims to have demonstrated “the world’s first commercial quantum computer” made an amusing counterpoint to the media hype. He describes the firm’s 16-bit quantum computer as “about as useful for industrial optimization problems as a roast-beef sandwich”.

How often is it updated?

Daily, with the occasional longer gap between posts.

Can you give me a sample quote?

“From this day forward, my allegiances in the String Wars will be open for sale to the highest bidder. Like a cynical arms merchant, I will offer my computational-complexity and humor services to both sides, and publicly espouse the views of whichever side seems more interested in buying them at the moment. Fly me to an exotic enough location, put me up in a swank enough hotel, and the number of spacetime dimensions can be anything you want it to be: 4, 10, 11, or even 172.9 + 3πi.”

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