Physics Archives – Page 75 of 144

Neutrino telescopes point towards exotic physics

The IceCube lab at the Amundsen-Scott South Pole Station in Antarctica monitors the world’s largest neutrino telescope, which consists of more than 5000 optical sensors held in a cubic kilometre of the polar ice cap.
Image credit: NSF/S Lidström

It is more than six years since Uppsala University was host to the first Workshop on Exotic Physics with Neutrino Telescopes. Since then, the large neutrino telescopes IceCube and ANTARES have been completed and indirect searches for dark matter, monopoles and other aspects of physics beyond the Standard Model are proceeding at full strength. Indeed, some theoretical models have already been called into question by recent results from these detectors. Meanwhile, searches for dark-matter candidates and indications of physics beyond the Standard Model in experiments at the LHC have set stringent constraints on many models, complementing those derived from the neutrino telescopes. The time was therefore ripe for a second workshop, with the Centre for Particle Physics of Marseilles (CPPM) as host, bringing together 47 experts on 3–6 April.

Dark matter

Review talks on supersymmetric dark-matter candidates and the status of experimental searches opened the first day’s sessions. Supersymmetry – still a well motivated candidate for physics beyond the Standard Model – has been put to the first serious tests at the LHC. The discovery there of a Higgs boson at a mass of 126 GeV can be seen either as just another confirmation of the Standard Model or as a first glimpse of physics beyond it. The lack of evidence so far for supersymmetry from direct searches at the LHC raises the limits of supersymmetric particle masses to the scale of tera-electron-volts and has implications for the dark-matter candidates arising in supersymmetric models. The current preferred mass-range for the lightest, stable neutralino is in the region of hundreds of giga-electron-volts. This is good news for neutrino telescopes, which – by design – are sensitive to high-energy particles. The downside is that the predicted rates from annihilation of neutralinos accumulated in heavy celestial objects are low if the constraints from the Wilkinson Microwave Anisotropy Probe and the LHC are taken into account. Only a handful of minimal supersymmetric Standard Model variants predict rates in cubic-kilometre neutrino telescopes that are of the order of 100 events per year or higher.

DeepCore, the denser array in the centre of IceCube, has opened up the possibility to pursue physics topics otherwise impossible with a detector designed for tera-electron-volt neutrino astrophysics.
Image credit: IceCube collaboration

However, the neutralino in minimal supersymmetry is not the only viable candidate for dark matter. In models with R-parity violation, a long-lived but unstable gravitino with a mass between a few and a few hundred giga-electron-volts could be a component of the dark matter in the halo of galaxies. Neutrinos of any flavour can be produced in gravitino decay and can be detected by neutrino telescopes. A feature of gravitino dark matter is that it would leave no signal in direct-detection experiments because the cross-section for the interaction between a gravitino and normal matter is suppressed by the Planck mass to the fourth power.

Models with extra dimensions of sizes in the range 10^–3–10^–15 m can also provide dark-matter candidates. Extra dimensions can be accommodated (or even required) in supersymmetry, string-theory or M-theory, where they give rise to branons – weakly interacting and massive fluctuations of the field that represents the 3D brane on which the standard world lives. As stable and weakly interacting objects, branons make a good candidate for dark matter, following the usual scenario: relic branons left over after a freeze-out period during the evolution of the universe accumulate gravitationally in the halos of galaxies, where they annihilate into Standard Model particles that can be detected by gamma-ray telescopes, surface arrays or neutrino telescopes.

A summary of current flux limits on relativistic (β > 0.6) monopoles, from the neutrino telecopes ANTARES and IceCube, together with an older limit from the MACRO experiment and the Parker bound.
Image credit: Anna Obertacke, Wuppertal

From the experimental side, the IceCube, ANTARES, Baikal, Baksan and Super-Kamiokande collaborations presented their latest results on the search for dark matter from different potential sources – the Sun, the Galaxy or nearby galaxies. Their search techniques are similar and based on looking for an excess of neutrinos over the known atmospheric-neutrino background from the direction of the sources. DeepCore, the denser array in the centre of IceCube, which was not part of the original design, has proved extremely useful in lowering the energy reach of the detector. It has opened up the possibility of pursuing physics topics that would otherwise be impossible with a detector designed for tera-electron-volt neutrino astrophysics. Using the surrounding strings of IceCube as a veto, starting and contained tracks can be defined, therefore turning IceCube into a 4π detector with an energy threshold of around 10 GeV, with access to the Galactic centre and the whole Southern Sky.

However, none of the experiments report any excess, and upper limits on the neutrino flux and on the cross-section for interactions between weakly interacting massive particles (WIMPs) and nucleons have been calculated over an ample range of WIMP masses, from about 1 GeV (Super-Kamiokande) to 10 TeV (IceCube). An example of the long-term search capability, as well as consistency in data analysis, was presented for the Baksan experiment. Although it has the smallest of the detectors mentioned above, it has gathered data over 24 years, from 1978 to 2009.

Monopoles, nuclearites and more

Monopoles and heavy, highly ionizing particles leave a unique signal in a neutrino telescope: a strong light-yield along the path of the particle, which is much more intense than the usual track-pattern of a minimum-ionizing muon. If the particle is nonrelativistic, then the separation of such a signal from relativistic muons traversing the detector is even easier. However, dedicated online or offline triggers are needed because for a nonrelativistic particle, light is deposited in the detector over a time of up to tens of milliseconds, instead of a few microseconds for a relativistic muon.

The best limit for fast (β > 0.75) monopoles, at a level of about 3 × 10^–18 cm^–2 s^–1, was presented by the IceCube collaboration using data from its 40-string configuration, although the ANTARES limit – at a level of around 7 × 10^–17 cm^–2 s^–1 – remains the best so far, at between 0.65 < β < 0.75. However, the sensitivity of the full IceCube detector could extend to β = 0.60 and reach a level of between 2 × 10^–18 cm^–2 s^–1and 10^–17 cm^–2 s^–1 in a one-year exposure, depending on the assumptions on the monopole spin. Results are expected soon, when the ongoing data analysis is finalized.

The Super-Kamiokande collaboration presented a novel way to search for monopoles using the Sun as the target. The idea is that super-heavy monopoles that have been gravitationally trapped in the Sun will induce proton decay along their orbits. Neutrinos with an energy of tens of mega-electron-volts will then be emitted by the decays of the muons and pions produced as the protons decay. This is a low-energy signal that is well below the threshold of large-scale neutrino telescopes but for which Super-Kamiokande has sensitivity. Indeed, this experiment provides the best limit so far on the flux of super-heavy monopoles in the range 10^–5 < β < 10^–2. At the other end of the kinematic spectrum, radio-Cherenkov detectors such as RICE and ANITA provide the best limits for ultrarelativistic monopoles of intermediate mass, at the level of 10^–19 cm^–2 s^–1.

Another bright signature, although from a different process, is produced by slowly moving heavy nuclearites. These massive stable lumps of up, down and strange quarks could be detected in neutrino telescopes through the blackbody radiation emitted by the overheated matter along their path. From the analysis of 310 days of live time in the years 2007–2008, the ANTARES collaboration reported a flux limit at the level of 10^–17 cm^–2 s^–1 sr^–1 for nuclearite masses larger than 10¹⁴ GeV and β around 10^–3. Indeed, the limit improves previous results from the MACRO experiment by a factor of between three and an order of magnitude, depending on the nuclearite mass.

The atmosphere, acting as a target for ultra-high-energy cosmic rays, can be a useful source for searches of physics beyond the Standard Model

The atmosphere, acting as a target for ultra-high-energy cosmic rays, can be a useful source for searches of physics beyond the Standard Model. The interaction of a cosmic ray of energy around 10¹¹ GeV with a nucleon in the atmosphere takes place at a much higher centre-of-mass energy than is achievable in accelerator laboratories and a wealth of physics can be extracted from such collisions. Supersymmetric particles can be produced in pairs and, except for the lightest, they can be charged. Even if unstable, they can, because of the boost in the interaction, reach the depths of a detector and emit Cherenkov light as they traverse an array. The signature is two minimum-ionizing, parallel, coincident tracks separated by more than 100 m. These types of searches are being carried out by the two large neutrino-telescope collaborations, IceCube and ANTARES.

A schematic of the 0.1 km² ANTARES neutrino telescope deployed in the Mediterranean Sea.
Image credit: F Montanet, CNRS/IN2P3 and UJF for Antares/produced with POV-ray

The same interactions of cosmic rays with the atmosphere can also be used to probe non-standard neutrino interactions arising from the effects of tera-electron-volt gravity and/or extra dimensions. At high energies, neutrino interactions with matter may become stronger and the atmosphere can become opaque to neutrinos with energies of peta-electron-volts. A signature in a neutrino telescope would be an absence of regular neutrinos with ultra-high energies accompanied by an excess of muon bundles at horizontal zenith angles. The same effect would take place with a cosmogenic neutrino flux – that is, the flux of neutrinos produced by the interactions of ultra-high-energy cosmic rays with the cosmic microwave background radiation. In the absence of a discovery so far, this flux can be assumed to be at a level compatible with gamma-ray constraints from the Fermi Gamma-ray Space Telescope. The neutrino-nucleon cross-section will depend on the number of extra dimensions, N_D, and a lack of events over the expected flux can be transformed into a limit on N_D. However, the effect in neutrino telescopes with volumes of a cubic kilometre or so is not big. For values of N_D not excluded by the LHC, fewer than one event a year is estimated for IceCube. Only with the larger radio arrays is the expected number of events of the order of 10 per year.

The recent two peta-electron-volt events announced by the IceCube collaboration have already been used to set stringent limits on the violation of Lorentz invariance. If strict Lorentz invariance does not hold, then neutrino bremsstrahlung of electron–positron pairs (ν → νe⁺e^–) is possible, so extragalactic neutrinos would rapidly lose energy via such a process. This would lead to a depletion of the ultra-high-energy neutrino flux at the Earth. Assuming that the IceCube events are, indeed, extragalactic (that is, they have travelled of the order of megaparsecs from the sources to the Earth) and that the extragalactic high-energy neutrino flux is at most at the level of the current IceCube limit of 2 × 10^–8 cm^–2 s^–1 sr^–1, a limit can be set on Lorentz invariance violation, parameterized by the factor δ, defined as (dE/dp)²-1. Under these assumptions, the bound obtained from the two IceCube events is δ <10^–18, which is orders of magnitude smaller than the current best limit of 10^–13.

Even if conventionally produced, the absolute normalization of the atmospheric lepton spectrum is not well understood

High-energy atmospheric muons and neutrinos present a background to many of the topics discussed in the workshop. Even if conventionally produced, the absolute normalization of the atmospheric lepton spectrum is not well understood – in particular the contribution from prompt charm decays. Calculations of an atmospheric lepton component, which is rarely considered, from the decays of unflavoured mesons (η, η’, ρ, ω, φ), were presented at the workshop. These mesons decay rapidly to μ⁺μ^– pairs and in very-high-energy cosmic-ray interactions the products of the decays can be the dominant muon flux at energies above 10⁶ GeV, forming a background that must be taken into account in exotic searches.

One of the unexpected developments in the field since the first ideas of building neutrino telescopes has been their use in neutrino-oscillation physics. On one hand, the detectors can probe oscillation physics at energies not reachable by the smaller detectors. On the other, an aggressive plan to lower the energy threshold of IceCube and the proposed KM3NeT array to the few-giga-electron-volt region is underway, and IceCube has already produced physics results with its low-energy subarray, DeepCore. Plans to build megatonne water-Cherenkov detectors with a giga-electron-volt energy threshold – PINGU at the South Pole and ORCA in the Mediterranean – were also discussed in the workshop. These detectors consist of about 20–50 strings of optical modules with an inter-string separation of 20 m, to be compared, for example, with the 125 m inter-string separation of IceCube or the 70 m inter-string separation of DeepCore. Such detectors may address the issue of the neutrino mass hierarchy at a relatively low cost and on a short timescale because the technology exists already and the deployment techniques are the same as in IceCube and ANTARES.

Are some atomic nuclei pear shaped?

CCnew1_05_13 — The shape of ²²⁴Ra as deduced from the experiments at ISOLDE.

Most atomic nuclei that exist naturally are not spherical but have the shape of a rugby ball. While state-of-the-art theories are able to predict this behaviour, the same theories have predicted that for some particular combinations of protons and neutrons, nuclei can also assume an asymmetrical shape like a pear, with more mass at one end of the nucleus than the other. Now an international team studying radium isotopes at CERN’s ISOLDE facility has found that some atomic nuclei can indeed take on this unusual shape.

Most nuclear isotopes predicted to have pear shapes have for a long time been out of reach of experimental techniques. In recent years, however, the ISOLDE facility has demonstrated that heavy, radioactive nuclei, produced in high-energy proton collisions with a uranium-carbide target, can be selectively extracted before being accelerated to 8% of the speed of light. The beam of nuclei is directed onto a foil of isotopically pure nickel, cadmium or tin where the relative motion of the heavy accelerated nucleus and the target nucleus creates an electromagnetic impulse that excites the nuclei.

By studying the details of this excitation process it is possible to infer the nuclear shape. This method has now been used successfully to study the shape of the short-lived isotopes ²²⁰Rn and ²²⁴Ra. The data show that while ²²⁴Ra is pear shaped, ²²⁰Rn does not assume the fixed shape of a pear but rather vibrates about this shape.

The findings from the teams at ISOLDE are in contradiction with some nuclear theories and will help others to be refined. The experimental observation of nuclear pear shapes is also important because it can help in experimental searches for atomic electric dipole moments (EDMs). The Standard Model of particle physics predicts that the value of the atomic EDM is so small that it will lie well below the current observational limit. However, many theories that try to refine the model predict values of EDMs that should be measurable. Testing these theories requires improved measurements, the most sensitive being to use exotic atoms whose nuclei are pear shaped.

The new measurements will help to direct the searches for EDMs currently being carried out in North America and in Europe, where new techniques are being developed to exploit the special properties of radon and radium isotopes. The expectation is that the data from the nuclear-physics experiment at ISOLDE can be combined with results from atomic-trapping experiments that measure EDMs to make the most stringent tests of the Standard Model.

ALPHA presents novel investigation of the effect of gravity on antimatter

The ALPHA collaboration at CERN has made the first direct analysis of how antimatter is affected by gravity. The ALPHA experiment was the first to trap atoms of antihydrogen, held in place with a strong magnetic field for up to 1000 s. Although the main goal is not to study gravity, the team realized that the data that they have collected might be sensitive to gravitational effects. Specifically, they searched for the free fall (or rise) of antihydrogen atoms released from the trap, which allowed them to measure limits directly on the ratio of the gravitational to inertial mass of antimatter, F=M_g/M.

Measuring a total of 434 atoms, they found that in the absence of systematic errors, F must be < 75 at a statistical significance level of 5%; the worst-case systematic errors increase this limit to < 110. A similar search places somewhat tighter bounds on a negative F, that is, on antigravity. Refinements of the technique, coupled with larger numbers of cold-trapped antiatoms, should allow future measurements to place tighter bounds on F and approach the interesting region around 1.

Meanwhile, the antimatter programme at CERN is expanding. AEgIS and GBAR, two experiments currently under construction, will focus on measuring how gravity affects antihydrogen.

CMS hunts for low-mass dark matter

Astronomical observations – such as the rotation velocities of galaxies and gravitational lensing – show that more than 80% of the matter in the universe remains invisible. Deciphering the nature of this “dark matter” remains one of the most interesting questions in particle physics and astronomy. The CMS collaboration recently conducted a search for the direct production of dark-matter particles (χ), with especially good sensitivity in the low-mass region that has generated much interest among scientists studying dark matter.

Possible hints of a particle that may be a candidate for dark matter have already begun to appear in the direct-detection experiments; most recently the CDMS-II collaboration reported the observation of three candidate events in its silicon detectors with an estimated background of 0.7 events. This result points to low masses, below 10 GeV/c², as a region that should be particularly interesting to search. This mass region is where the direct-detection experiments start to lose sensitivity because they rely on measuring the recoil energy imparted to a nucleus by collisions with the dark-matter particles. For a low-mass χ, the kinetic energy transferred to the nucleus in the collision is small, and the detection sensitivity drops as a result.

The CMS collaboration has searched for hints of these elusive particles in “monojet” events, where the dark-matter particles escape undetected, yielding only “missing momentum” in the event. A jet of initial-state radiation can accompany the production of the dark-matter particles, so a search is conducted for an excess of these visible companions compared with the expectation from Standard Model processes. The results are then interpreted within the framework of a simple “effective” theory for their production, where the particle mediating the interaction is assumed to have high mass. An important aspect of the search by CMS is that there is no fall in sensitivity for low masses.

CCnew3_05_13 — CMS 90% CL upper limits on the χ–nucleon cross-section as a function of χ mass for spin-independent (left) and spin-dependent scattering (right). Also shown are limits from other experiments, and the 68% and 90% contours for the candidate events from CDMS (arXiv:1304.4279 [hep-ex]).

The monojet search requires at least one jet with more than 110 GeV of energy and has the best sensitivity if there is more than 400 GeV of missing momentum. Events with additional leptons or multiple jets are vetoed. After event selection, 3677 events were found in the recent analysis, with an expectation from Standard Model processes of 3663 ± 196 events. The contribution from electroweak processes dominate this expectation, either from pp → Z+jets with the Z decaying to two neutrinos or from pp → W+jets, where the W decays into a lepton and neutrino, while the lepton escapes detection.

With no significant deviation from the expectation from the Standard Model, CMS has set limits on the production of dark matter, as shown in the figures of the χ–nucleon cross-section versus χ mass. The limits show that CMS has good sensitivity in the low-mass regions of interest, for both spin-dependent and spin-independent interactions.

CP violation observed in the decays of B⁰_s mesons

In March 2012, the LHCb collaboration reported an observation of CP violation in charged B-meson decays, B^± → DK^±. Now, just over a year later, the collaboration has announced a similar observation in the decays in another B meson, in this case the B⁰_s meson composed of a beauty antiquark b bound with a strange quark s. This first observation of CP violation in the decays B⁰_s → K^–π⁺ with a significance of more than 5σ marks the first time that CP violation has been found in the decays of B⁰_s mesons – only the fourth type of meson where this effect has been seen. It is an important milestone for LHCb because the precise study of B⁰_s decays is sensitive to possible physics beyond the Standard Model.

CCnew5_05_13 — Fig. 1. The analysis studied the decays of B⁰ and B⁰_s mesons into K and π mesons. In this event a decay produces a negative K (red track) and a positive π (green track).

The study of CP violation in charmless charged two-body B decays provides stringent tests of the Cabibbo-Kobayashi-Maskawa picture of CP violation in the Standard Model. However, the presence of hadronic contributions means that several measurements from such decays are needed to exploit flavour symmetries and disentangle the different contributions. In 2004, the BaBar and Belle collaborations at SLAC and KEK, respectively, discovered direct CP violation in the decay B⁰ → K⁺π^– and a model-independent test was proposed to check the consistency of the observed size of the effect with the Standard Model. The test consists of comparing CP violation in B⁰ → K⁺π^– with that in B⁰_s → K^–π⁺. The B factories at KEK and SLAC did not have the possibility of accumulating large enough samples of B⁰_s decays and, despite much effort by the CDF collaboration at Fermilab’s Tevatron, CP violation had until now not been seen in B⁰_s → K^–π⁺ with a significance exceeding 5σ.

CCnew6_05_13 — Fig. 2. Invariant mass spectra obtained using the event selection adopted for the best sensitivity on (a, b) ACP (B⁰ → K⁺π^–) and (c, d) ACP (B⁰_s → K^–π⁺). Panels (a) and (c) show the K⁺π^– invariant mass, whereas panels (b) and (d) show the K^–π⁺ invariant mass. The results of the unbinned maximum likelihood fits are overlaid. The main components contributing to the model used in the fit are also shown.

Using a data sample corresponding to an integrated luminosity of 1.0 fb^–1 collected by the experiment in 2011, the LHCb collaboration measured the direct CP-violating asymmetry for B⁰_s → K^–π⁺ decays, ACP (B⁰_s → K^–π⁺) = 0.27 ± 0.04 (stat.) ± 0.01 (syst.), with a significance of more than 5σ. In addition, the collaboration improved the determination of direct CP violation in B⁰ → K⁺π^– decays, ACP (B⁰ → K⁺π^–) = –0.080 ± 0.007 (stat.) ± 0.003 (syst.), which is the most precise measurement of this quantity to date. The four plots in figure 2 show different components of the K⁺π^– invariant mass. The upper plots indicate the well established difference in the decay rates of B⁰ mesons. The enlargements in the lower plots reveal that a difference is also visible around the mass of the B⁰_s meson. The measured values are in good agreement with the Standard Model expectation.

Only the data sample collected in 2011 was used to obtain these results, so LHCb will improve the precision further with the total data set now available, which more than trebled with the excellent performance of the LHC during 2012.

Luminosity-independent measurement of the proton–proton total cross-section at 8 TeV

The TOTEM collaboration has published the first luminosity-independent measurement at the LHC of the total proton–proton cross-section at a centre-of-mass energy of 8 TeV. This follows the collaboration’s published measurement of the same cross-section at 7 TeV, which demonstrated the reliability of the luminosity-independent method by comparing several approaches.

The method requires the simultaneous measurements of the inelastic and elastic rates, as well as the extrapolation of the latter down to a four-momentum transfer squared, |t| = 0. This is achieved with the experimental set-up consisting of two telescopes, T1 and T2, to detect charged particles produced in inelastic proton–proton collisions, and Roman Pot stations to detect elastically scattered protons at very small angles.

The analysis at 8 TeV was performed on two data samples recorded in July 2012 during special fills of the LHC with the magnets set to give the parameter β^* = 90 m. During these fills, the Roman Pots were inserted close to the beam, allowing the detection of around 90% of the nuclear elastic-scattering events. Simultaneously, the inelastic scattering rate was measured by the T1 and T2 telescopes.

By applying the optical theorem, the collaboration determined a total proton–proton cross-section of 101.7 ± 2.9 mb, which is in good agreement with the extrapolation from lower energies. The method also allows the derivation of the luminosity-independent elastic and inelastic cross-sections: σ_el = 27.1 ± 1.4 mb and σ_inel = 74.7±1.7 mb. The two measurements are consistent in terms of detector performance, showing comparable systematic uncertainties, and they are both in good agreement with the extrapolation of the lower-energy measurements.

Chasing new physics with electroweak penguins

Fig. 1. Feynman diagrams for B-meson decay to a K or K^* meson and two muons (b→sμ⁺μ^– at quark level). The diagram on the left dominates and is known as an “electroweak penguin”; the diagram on the right is a “box” diagram. The spectator quark, q, can be of u or d type.

The recent identification of the new particle discovered at the LHC as a Higgs boson with a mass of 125 GeV/c² completes the picture of particles and forces described by the Standard Model. However, it does not mark the end of the story as, unfortunately, the Standard Model is an incomplete description of nature. Puzzles still remain, for example, in explaining the existence of dark matter and the matter–antimatter asymmetry. The answers to these puzzles may lie in the existence of as yet undiscovered particles that would have played a key role in the early, high-energy, phase of the universe and whose existence would help to complete the description of nature in particle physics. The question then is: at what energy scale would these new particles appear?

Particle physics provides no certain knowledge about this scale but the hope is that the new particles might be produced directly in the high-energy proton–proton collisions of the LHC. However, new particles could also be observed indirectly through the effects of their participation as virtual particles in rare decay processes. By studying such processes, experiments can probe mass scales that are much higher than those accessible directly through the energy available at the LHC. This is because quantum mechanics and Heisenberg’s uncertainty principle allow virtual particles to have masses that are not constrained by the energy of the system. Searches based on virtual particles are limited by the precision of the measurements, rather than the energy of the collider.

Rare potential

One promising place to look for contributions from new virtual particles is in the rare transitions of b quarks to s quarks in which a muon pair (dimuon) is produced: b → sμ⁺μ^–. Described by the Feynman diagrams shown in figure 1 (overleaf), these involve what are known as “flavour-changing neutral currents” because the initial quark changes flavour without changing charge. In the Standard Model, transitions of this type are forbidden at the lowest perturbative order – that is, at “tree-level”, where the diagrams have only two vertices. Instead, they are mediated as shown in figure 1 by higher-order diagrams known as “electroweak penguin” and “box” diagrams. For this reason the Standard Model process is rare, which enhances the potential to discover new high-mass particles.

Fig. 2. Invariant mass distributions for several b→sμ⁺μ^– transitions reconstructed at LHCb. Signals from B⁺→K⁺μ⁺μ^– (LHCb collaboration 2013d) B⁰→K^*μ⁺μ^–, B_s→φμ⁺μ^–, B⁰→K^*_s μ⁺μ^–, B⁺→K^*+μ⁺μ^– and Λ_b→Λμ⁺μ^– (LHCb collaboration 2013e) are clearly visible. These plots were obtained with 1fb^-1, a third of LHCb’s total data set. The decay modes in the bottom row contain either a long-lived K^*_s or a Λ, which are challenging to reconstruct.

Studies of flavour-changing neutral currents have paved the way for discoveries in particle physics in the past, specifically in the decays of K mesons, where s quarks change to d quarks. Investigations of mixing between the mass eigenstates of the neutral kaon system and of rare K-meson decays led to the prediction of the existence of a second u-like quark (the charm quark, c), at a time when only three quarks were known (u, d and s). It was 10 years before the existence of the c quark was confirmed directly. Similarly, the observation of CP violation in neutral kaons led to the prediction of the third generation of quarks (b and t). Now, the study of flavour-changing neutral-current processes related to the third generation of quarks – in particular the rare b → sμ⁺μ^– transitions – could soon provide similar evidence for the existence of new particles.

The LHCb detector is characterized by excellent vertex and momentum resolution.

Several b → sμ⁺μ^– transitions have already been observed by the Belle, BaBar and CDF experiments at KEK, SLAC and Fermilab respectively. So far, the results have been limited by the small size of the data sets but with the LHC, a new era of precision has begun. The collider is the world’s largest “factory” for producing particles that contain b quarks: in one year, it produced about 10¹² b hadrons in the LHCb experiment, while running at a centre-of-mass energy of 7 TeV with an instantaneous luminosity in the experiment of 4 × 10³² cm^–2 s^–1. ATLAS and CMS have also recently joined the game, showing their first results on the B⁰ → K^*0 μ⁺μ^– decay at the BEAUTY 2013 conference (ATLAS collaboration 2013 and CMS collaboration 2013).

The LHCb detector is characterized by excellent vertex and momentum resolution (coming from its tracking systems) and impressive particle-identification capabilities (from its two ring-imaging Cherenkov detectors). Combined with the large b-hadron production rate, these features allow LHCb to reconstruct clean signals of rare b-hadron decays (figure 2). These processes have branching fractions below 10^–6 and at most occur once in every 100 million collisions.

The branching fractions of these decays are sensitive to new physics but their interpretation is unfortunately complicated. The b quark has hadronized, so the observations relate to hadronic rather than quark-level processes. A lack of detailed understanding of the hadronic system limits the usefulness of the branching-fraction measurements in the search for new physics.

Angles and asymmetries

Fortunately, the branching fractions of these decays are not the only handles for investigating new particle contributions. It is often much more instructive to look at the angular distribution of the particles coming from the decay. However, such angular analyses are experimentally challenging because they require a detailed understanding of how both the geometry of the detector and the reconstruction of the event bias the angular distribution of the particles.

Fig. 3. Forward–backward asymmetry, A_FB, of the dimuon system as a function of the dimuon invariant-mass-squared (q²) for B⁰→K^*0μ⁺μ^–. The region where A_FB changes sign is also shown. There is remarkable agreement between the experimental result and the predictions of the Standard Model.

The decays B⁰→ K^*0μ⁺μ^– and B_s→ φμ⁺μ^– have been shown to be highly sensitive to a variety of new physics scenarios (LHCb collaboration 2013a and 2013b). These decays are characterized by three angles: θ_K, which describes the K^* or φ decay; θ_l, which describes the dimuon decay; and Φ, the angle between the K^* or φ and the dimuon decay planes.

The angular distribution of the particles depends on the properties of the underlying theory. For instance, two features of the Standard Model drive the angular distribution: the photon exchanged in the penguin diagram of figure 1 is transversely polarized, while the charged-current interaction (the W exchange) is purely left-handed. The angle in the dimuon system also has an intrinsic forward–backward asymmetry that arises from interference between the different diagrams. The forward–backward asymmetry can be studied as a function of the mass of the dimuon system, which can be anywhere between twice the muon’s mass and the difference between the mass of the B and the mass of the K^* or φ.

In the Standard Model, the forward–backward asymmetry has a characteristic behaviour, changing sign at a dimuon mass of around 2 GeV/c². It turns out that this point can be predicted with only a small theoretical uncertainty. Figure 3 shows LHCb’s measurement of the forward–backward asymmetry in the decay B⁰→ K^*0μ⁺μ^– . In addition, the angle Φ can be used to test nature’s left-handedness, through an observable called A_T⁽²⁾.

It is important to emphasize that the room for new physics is still large given the statistical uncertainty of the present measurements.

So far, measurements of both the forward–backward asymmetry and A_T⁽²⁾ show good agreement with the predictions of the Standard Model. While there is no evidence for any disagreement, it is nevertheless important to emphasize that the room for new physics is still large given the statistical uncertainty of the present measurements.

Another way to decrease the theoretical uncertainty associated with the hadronic transitions is to form asymmetries between specific decay modes – for example, CP asymmetries between particle and antiparticle decays. In the Standard Model, the decay B⁰→ K^*0μ⁺μ^– and its CP conjugate are expected to have the same branching fraction to about 1 part in 1000. With the large LHC data samples, LHCb has verified this at the level of 4% (LHCb collaboration 2013e).

Another example concerns so-called isospin asymmetries between decays that differ only in the type of spectator quark (u or d), labelled q in figure 1. The isospin asymmetry between B⁰ and B⁺ decays is defined as:

This is formed using the branching fractions of the B⁰ and B⁺ decays and the ratio τ⁰/τ⁺ of the lifetimes of the B⁰ and the B⁺. In the Standard Model, the spectator quark is expected to play only a limited role in the dynamics of the system, so isospin asymmetries are predicted to be tiny. Experimentally, A_I is measured as a double ratio with respect to the decay channels B⁰→ K^(*)0 J/ψ or B⁺→ K^(*)+ J/ψ, which give the same final states after the J/ψ decays to μ⁺μ^– and are well known from previous measurements.

Fig. 4. The isospin asymmetry A_I, measured by LHCb between the B⁰→K^*0μ⁺μ^– and the B⁺→K^*+μ⁺μ^– decays and between the B⁰→K⁰μ⁺μ^– and the B⁺→K⁺μ⁺μ^– decays, as a function of the dimuon invariant-mass-squared (q²). The Standard Model predicts a small isospin asymmetry for both sets of decays.

Isospin asymmetries have been measured for both B→ K^*μ⁺μ^– and B→ Kμ⁺μ^– by the BaBar, Belle, CDF and LHCb experiments. All of these measurements are in good agreement with each other and favour a value for A_I(B→ K^*μ⁺μ^–) that is close to zero and a negative value for A_I(B→ Kμ⁺μ^–). The LHCb experiment observes a negative isospin asymmetry in this channel at the level of four standard deviations (from zero) as figure 4 shows (LHCb collaboration 2012). This unexpected result is yet to be explained. Indeed, most extensions of the Standard Model do not predict a significant dependence on the charge or flavour of the spectator quark.

Looking to the future

The LHCb experiment has already on tape a data set that is roughly three times larger than that used in its results published so far. Even with only 1 fb^–1 of integrated luminosity currently analysed, LHCb has larger samples than all previous experiments combined in most of the channels shown in figure 2. Furthermore, while the selected current data sets contain hundreds of events, the samples will be of the order of tens of thousands of events once the experiment has been upgraded. With these larger data sets the LHCb collaboration will be able to chase progressively smaller and smaller deviations from the Standard Model. This will allow them to probe ever higher mass scales, far beyond those that can be accessed by searching directly for the production of new particles at the LHC. A new era in precision measurements of flavour-changing neutral currents is now opening.

John Ellis on the origin of penguins

The penguin diagram — The original penguin diagram for b→s decay, where a gluon produces an ss̄ pair. LHCb is investigating electroweak decays where a μ⁺μ^– pair is produced from a photon or a Z boson.

“Mary K [Gaillard], Dimitri [Nanopoulos], and I first got interested in what are now called penguin diagrams while we were studying CP violation in the Standard Model in 1976 … The penguin name came in 1977, as follows.

In the spring of 1977, Mike Chanowitz, Mary K and I wrote a paper on GUTs [grand unified theories] predicting the b quark mass before it was found. When it was found a few weeks later, Mary K, Dimitri, Serge Rudaz and I immediately started working on its phenomenology.

That summer, there was a student at CERN, Melissa Franklin, who is now an experimentalist at Harvard. One evening, she, I and Serge went to a pub, and she and I started a game of darts. We made a bet that if I lost I had to put the word penguin into my next paper. She actually left the darts game before the end, and was replaced by Serge, who beat me. Nevertheless, I felt obligated to carry out the conditions of the bet.

For some time, it was not clear to me how to get the word into this b-quark paper that we were writing at the time … Later … I had a sudden flash that the famous diagrams look like penguins. So we put the name into our paper, and the rest, as they say, is history.”

John Ellis in Mikhail Shifman’s “ITEP Lectures in Particle Physics and Field Theory”, hep-ph/9510397. Reproduced here courtesy of symmetry magazine.

AMS measures antimatter excess in space

CCnew1_04_13 — Perched on the International Space Station around 400 km above the Earth, the Alpha Magnetic Spectrometer (AMS) collects data from primary cosmic rays before they can interact with the atmosphere.
Image credit: NASA.

The international team running the Alpha Magnetic Spectrometer (AMS) has announced the first results in its search for dark matter. They indicate the observation of an excess of positrons in the cosmic-ray flux. The results were presented by Samuel Ting, the spokesperson of AMS, in a seminar at CERN on 3 April, the date of publication in Physical Review Letters.

The AMS results are based on an analysis of some 2.5 × 10¹⁰ events, recorded over a year and a half. Cuts to reject protons, as well as electrons and positrons produced in the interactions of cosmic rays in the Earth’s atmosphere, reduce this to around 6.8 × 10⁶ positron and electron events, including 400,000 positrons with energies between 0.5 GeV and 350 GeV. This represents the largest collection of antimatter particles detected in space.

The data reveal that the fraction of positrons increases from 10 GeV to 250 GeV, with the slope of the increase reducing by an order of magnitude over the range 20–250 GeV. The data also show no significant variation over time, or any preferred incoming direction. These results are consistent with the positrons’ origin in the annihilation of dark-matter particles in space but they are not yet sufficiently conclusive to rule out other explanations.

The AMS detector is operated by a large international collaboration led by Nobel laureate Samuel Ting. The collaboration involves some 600 researchers from China, Denmark, Finland, France, Germany, Italy, Korea, Mexico, the Netherlands, Portugal, Spain, Switzerland, Taiwan and the US. The detector was assembled at CERN, tested at ESA’s ESTEC centre in the Netherlands and launched into space on 16 May 2011 on board NASA’s Space Shuttle Endeavour. Designed to study cosmic rays before they interact with the Earth’s atmosphere, the experiment is installed on the International Space Station. It tracks incoming charged particles such as protons and electrons, as well as antimatter particles such as positrons, mapping the flux of cosmic rays with unprecedented precision.

An excess of antimatter within the cosmic-ray flux was first observed around two decades ago in experiments flown on high-altitude balloons and has since been seen by the PAMELA detector in space and the Large Area Telescope on the Fermi Gamma-ray Space Telescope. The origin of the excess, however, remains unexplained.

One possibility, predicted by theories involving supersymmetry, is that positrons could be produced when two particles of dark matter collide and annihilate. Assuming an isotropic distribution of dark-matter particles, these theories predict the observations made by AMS. However, the measurement by AMS does not yet rule out the alternative explanation that the positrons originate from pulsars distributed around the galactic plane. Moreover, supersymmetry theories also predict a cut-off at higher energies above the mass range of dark-matter particles and this has not yet been observed.

AMS is the first experiment to measure to 1% accuracy in space – a level of precision that should allow it to discover whether the positron observation has an origin in dark matter or in pulsars. The experiment will further refine the measurement’s precision over the coming years and clarify the behaviour of the positron fraction at energies above 250 GeV.

ATRAP makes world’s most precise measurement of antiproton magnetic moment

CCnew2_04_13 — Stephan Ettenauer with the Penning trap apparatus that allows measurements of single antiprotons in the ATRAP experiment.

The Antihydrogen TRAP (ATRAP) experiment at CERN’s Antiproton Decelerator has reported a new measurement of the antiproton’s magnetic moment made with an unprecedented uncertainty of 4.4 parts per million (ppm) – a result that is 680 times more precise than previous measurements. The unusual increase in precision results from the experiment’s ability to trap individual protons and antiprotons, as well as from using a large magnetic gradient to gain sensitivity to the tiny magnetic moment.

By applying its single particle approach to the study of antiprotons, the ATRAP experiment has been able make precise measurements of the charge, mass and magnetic moment of the antiproton. Using a Penning trap, the antiproton is suspended at the centre of an iron ring-electrode that is sandwiched between copper electrodes. Thermal contact with liquid helium keeps the electrodes at 4.2 K, providing a nearly perfect vacuum that eliminates the stray matter atoms that could otherwise annihilate the antiproton. Static and oscillating voltages applied to the electrodes allow the antiproton to be manipulated and its properties to be measured.

The result is part of an attempt to understand the matter–antimatter imbalance of the universe. In particular, a comparison of the antiproton’s magnetic moment with that of the proton, tests the Standard Model and its CPT theorem at high precision. The ATRAP team found that the magnetic moments of the antiproton and proton are “exactly opposite”: equal in strength but opposite in direction with respect to the particle spins and consistent with the prediction of the Standard Model and the CPT theorem to 5 parts per million.

However, the potential for much greater measurement precision puts ATRAP in position to test the Standard Model prediction much more stringently. Combining the single particle methods with new quantum methods that make it possible to observe individual antiproton spin flips should make it feasible to compare an antiproton and a proton to 1 part per billion or better.

Precision measurements of B⁰_s mesons put the squeeze on new physics

The “winter” conferences earlier this year saw the LHCb collaboration present three important results from its increasingly precise search for new physics.

One fascinating area of study is the quantum-mechanical process in which neutral mesons such as the D⁰, B⁰ and B⁰_s can oscillate between their particle and antiparticle states. The B⁰_s mesons oscillate with by far the highest frequency of about 3 × 10¹² times per second, on average about nine times during their lifetime. In an updated study, the collaboration looked at the decays of B⁰_s mesons into D^–_sπ⁺ with D^–_s decays reconstructed in five different channels. While the B⁰_s oscillation frequency Δm_s has been measured before, the oscillations themselves had been previously seen only by folding the decay-time distribution onto itself at the period of the measured oscillation. In this updated analysis the oscillation pattern is spectacularly visible over the full decay-time distribution, as figure 1 shows. The measured value of the oscillation frequency is Δm_s = 17.768 ± 0.023 ± 0.006 ps^–1, which is the most precise in the world (LHCb collaboration 2013a).

CCnew3_04_13 — Fig. 1. The decay-time distribution measured for B⁰_s oscillations.

CP violation can occur in the B⁰_s sector – in the interference between the oscillation and decay of the meson – but it is expected to be a small effect in the Standard Model. Knowledge of such CP-violating parameters is important because they set the scale of the difference between properties of matter and antimatter; they may also reveal effects of physics beyond the Standard Model. LHCb has previously reported on a study of B⁰_s decays into J/ψ φ and J/ψ π⁺π^– final states, but now the analysis has been finalized. One important improvement is in the flavour tagging, which determines whether the initial state was produced as a B⁰_s or anti-B⁰_s meson. This decision was previously based on “opposite-side” tagging, i.e. from measuring the particle/antiparticle nature of the other b-quark produced in conjunction with the B⁰_s. The collaboration has now achieved improved sensitivity by including “same-side” tagging, from the charge of a kaon produced close to the B⁰_s, as a result of the anti-s-quark produced in conjunction with the B⁰_s. This increases the statistical power of the tagging by about 40%. The values of the CP-violating parameter φ_s, together with the difference in width of the heavy and light B⁰_s mass states, ΔΓ_s, are shown in figure 2, which also indicates the small allowed region for these two parameters, corresponding to φ_s = 0.01 ± 0.07 ± 0.01 rad and ΔΓ_s = 0.106 ± 0.011 ± 0.007 ps^–1 (LHCb collaboration 2013b)

CCnew5_04_13 — Two-dimensional profile likelihood in the (ΔΓ_s, φ_s) plane showing the small allowed region for the two parameters.

Last, the collaboration has opened a door for important future measurements with a first study of the time-dependent CP-violating asymmetry in hadronic B⁰_s meson decays into a φφ pair, a process that is mediated by a so-called penguin diagram in the Standard Model. Both φ mesons decay in turn into a K⁺K^– pair. The invariant mass spectrum of the four-kaon final state shows a clean signal of about 880 B⁰_s → φφ decays. A first measurement of the CP-violating phase φ_s for this decay indicates that it lies in the interval of (–2.46, –0.76) rad at 68% confidence level. This is consistent with the small value predicted in the Standard Model, at the level of 16% probability. Although the current precision is limited, this will become a very interesting measurement with the increased statistics from further data taking (LHCb collaboration 2013c)

These results represent the most precise measurements to date, based on data corresponding to the 1 fb^–1 of integrated luminosity that LHCb collected in 2011. They are in agreement with the Standard Model predictions and significantly reduces the parameter region in which the signs of new physics can still hide.

Topics

Reset your password

Registration complete