Quantum manipulation power for quantum information processing gets a boost (Vol. 49, No. 1)

Improving the efficiency of quantum heat engines involves reducing the number of photons in a cavity, ultimately impacting quantum manipulation power.
Traditionally, heat engines produce heat from the exchange between high-temperature and low-temperature baths. Now, imagine a heat engine that operates at quantum scale, and a system made up of an atom interacting with light (photons) confined in a reflective cavity of sub-atomic dimensions. This setup can either be at a high or low temperature, emulating the two baths found in conventional heat engines. Controlling the parameters influencing how such quantum heat engine models work could dramatically increase our power to manipulate the quantum states of the coupled atom-cavity, and accelerate our ability to process quantum information. In order for this to work, we have to find new ways of improving the efficiency of quantum heat engines. In a study published recently, the authors show methods for controlling the output power and efficiency of a quantum thermal engine based on the two-atom cavity.
K.W. Sun, R. Li and G.-F. Zhang, A quantum heat engine based on the Tavis-Cummings model, Eur. Phys. J. D 71, 230 (2017)
[Abstract]
Quasi-effective medium theory for multilayered magneto-dielectric structures (Vol. 45 No.2)

Maxwell–Garnett theory is the most widely used effective medium theory for the determination of the permittivity/permeability of nano-composite materials. However, it places a serious restriction on the physical dimensions of the constituents, that is, the feature sizes must be smaller than the incident wavelength. Thus, its applicability is limited to the quasi-static regime. An alternative theory has now been proposed by the authors which uses mode-dependent quasi-effective impedances to allow exact calculations of the far field scattering/extinction of complex multi-shell structures regardless of the object physical dimensions.
To demonstrate the physical insights that are to be gained based on this quasi-effective medium theory the authors have studied two practical examples: (i) they consider the problem of surface plasmon hybridization in concentric multi-shell particles, and (ii) they have applied the theory to design an object-independent cloak which consists of an arbitrary shaped object enclosed by a set of concentric shells. The most significant advantages of this new theory are its simplicity, ease of implementation and the important insights the theory provides into the optical properties of complex systems.
D. A. Genov and P. C. Mundru, "Quasi-effective medium theory for multi-layered magneto-dielectric structures", J. Opt. 16, 015101 (2014)
[Abstract]
Rare events in “noisy” networks (Vol. 49, No. 3)

Bringing diseases to extinction and mitigating the effects of human-caused environmental changes which accelerate the rate of species extinction are issues of worldwide importance. Both phenomena are typically rare events, relying on the interplay between network topology, nonlinear dynamics, and random fluctuations from the environment and interactions. However, the prediction of such rare events in general stochastic networks was an unsolved problem, despite extensive work in network dynamics. Here we solve the problem of predicting rare events as large fluctuations from metastable states with a general theory that combines mean-field approximations, large-deviation techniques and network topology. A benefit of our approach is its flexibility in describing the effects of multiple sources of different continuous and discrete noise. Using our theory, we demonstrate that networks with both internal interaction noise and external parameter noise exhibit a cross-over where the familiar exponential scaling of rare-event times with the number of nodes in the network is lost, and parametric noise dominates.
J. Hindes and I. B. Schwartz, Rare events in networks with internal and external noise, EPL 120, 56004 (2017)
[Abstract]
Reading between the lines of highly turbulent plasmas (Vol. 48, No. 3)

Study shows how to identify highly turbulent plasma signatures in the broadening of the shapes of lines emitted by ions and atoms within.
Plasma, the ionised state of matter found in stars, is still not fully understood, largely due to its instability. Astrophysicists have long-since sought to develop models that can account for the turbulent motions inside plasma, based on observing line shapes emitted by atoms and ions in the plasma. Turbulences are typically detected through the observation of broadened lines due to the Doppler effect, similar to the principle behind radar. In a new study published recently, the authors develop an iterative simulation model that accurately predicts, for the first time, the changes to the line shape in the presence of strong plasma turbulence. Ultimately, the authors aim to provide a system for assessing plasma turbulence that is valid for both a stellar atmosphere and the ITER tokamak designed to generate fusion energy.
R. Stamm, I. Hannachi, M. Meireni, H. Capes, L. Godbert-Mouret, M. Koubiti, J. Rosato, Y. Marandet, M. Dimitrijević and Z. Simić, Line shapes in turbulent plasmas, Eur. Phys. J. D 71, 68 (2017)
[Abstract]
Refraction index of shock compressed water at megabar pressure (Vol. 47 No. 1)

Compressing water at megabar pressure through laser-driven shocks induces phase changes and may finally produce a metallic fluid. Such phase is particularly relevant for planetology since water is one of the main constituents of the mantles of giant planets like Uranus and Neptune, and its metallization has been recognized as a possible source of the magnetic field of such planets. In this work we study the transition of water by looking at its optical properties. Increasing pressure water changes from transparent to opaque (absorbing) and finally reflecting. We provide the first quantitative measurement of water refractive index in the megabar range, a measurement, which can give information on how the material is approaching gap closure (metallization). We also performed measurements on water precompressed at 10 kbar, allowing getting off-Hugoniot states at high pressure but low temperature. Refraction index for transparent and opaque water was measured using a VISAR system. At high compression a sharp increase of the real and imaginary part of the refraction index was observed. Experiments were performed at the LULI and RAL laboratories.
D. Batani, K. Jakubowska, A. Benuzzi-Mounaix, C. Cavazzoni, C. Danson, T. Hall, M. Kimpel, D. Neely, J. Pasley, M. Rabec Le Gloahec and B.Telaro, Refraction index of shock compressed water in the megabar pressure range, EPL 112, 36001 (2015)
[Abstract]
Relativity Matters: Two opposing views of the magnetic force reconciled (Vol. 49, No. 2)

How magnetic force acts on charged subatomic particles near the speed of light
Current textbooks often refer to the Lorentz-Maxwell force governed by the electric charge. But they rarely refer to the extension of that theory required to explain the magnetic force on a point particle. For elementary particles, such as muons or neutrinos, the magnetic force applied to such charges is unique and immutable. However, unlike the electric charge, the magnetic force strength is not quantised. For the magnetic force to act on them, the magnetic field has to be inhomogeneous. Hence this force is more difficult to understand in the context of particles whose speed is near the speed of light. Moreover, our understanding of how a point-particle carrying a charge moves in presence of an inhomogeneous magnetic field relied until now on two theories that were believed to differ. The first stems from William Gilbert's study of elementary magnetism in 16th century, while the second relies on André-Marie Ampère electric currents. In a new study just published, the authors succeeded in resolving this ambiguity between Amperian and Gilbertian forms of magnetic force. Their solution makes it possible to characterise the interaction of particles whose speed is close to the speed of light in the presence of inhomogeneous electromagnetic fields.
J. Rafelski, M. Formanek, and A. Steinmetz, Relativistic Dynamics of Point Magnetic Moment, Eur. Phys. J. C 78, 6 (2018)
[Abstract]
Removing complexity layers from the universe’s creation (Vol. 44 No. 5)

Understanding complexity in the early universe may require combining simpler models to interpret cosmological observations. The authors publish results pertaining to theoretical predictions of cosmological systems’ dynamics.
They found that the combination of Einstein’s special relativity and quantum-mechanical dynamics is mathematically identical to a complex dynamical system akin to two interlocked processes with different energy scales. To model it, the authors consider a quantum mechanical dynamics in a background polycrystalline space where particles exhibit a Brownian motion. The observed relativistic dynamics then comes solely from a particular grain distribution in this space. In cosmology, such distribution might stem from early universe’s formation.
This new interpretation focuses on the interaction of a quantum particle with gravity. The non-existence of the relativistic dynamics leads to a natural mechanism for the formation of particles-antiparticles asymmetry. When coupled with cosmology, the authors’ approach predicts that a charge asymmetry should have been produced at ultra-minute fractions of seconds after the Big Bang, in agreement with constraints born out of recent cosmological observations.
P. Jizba and F. Scardigli, ‘Special relativity induced by granular space’, Eur. Phys. J. C 73, 2491 (2013)
[Abstract]
Renormalisation group for 3-body interactions in 1D (Vol. 42, No. 6)

One important message emerging from developments of effective field theories and effective Hamiltonians for nuclear physics is that many-body forces are inevitable whenever degrees of freedom are eliminated. At the same time, first-principles calculations have shown that two-body forces alone are not able to give an accurate account of the energies of light nuclei and the saturation of nuclear matter. Three- (possibly more-) body forces are thus essential in low-energy nuclear physics. The construction of effective interactions through elimination of degrees of freedom can be done either by imposing a cut-off on the Hilbert space or by applying a transformation putting the Hamiltonian into a simpler form, such as a diagonal matrix.
The Similarity Renormalization Group follows the latter route by means of a continuous set of transformations. It has proved to be a powerful tool in low-energy nuclear physics, when applied mainly in the context of expansions using harmonic-oscillator basis states. The present paper provides the first application of this method to three-body interactions in a momentum-space basis. Although the models studied are simple ones (bosons in 1D), the structure of the evolution equations has the full complexity of any set of three-body equations. The results show the expected decoupling of high- from low-momentum states for both two- and three-body interactions, which means that only low-momentum matrix elements of the evolved potentials are needed to describe low-energy states. This work paves the way for applications to few-nucleon scattering processes and nuclear matter, starting from realistic nuclear forces in three dimensions.
The Similarity Renormalization Group for Three-Body Interactions in One Dimension
O. Åkerlund , E.J. Lindgren, J. Bergsten, B. Grevholm, P. Lerner, R. Linscott, C. Forssén, L. Platter, EPJ A, 47, 1 (2011)
[Abstract]
Replica techniques can predict learning curves (Vol. 44 No. 1)

We show that statistical physics approaches, in particular the replica method, can be used to accurately predict the learning curve of a Gaussian process (GP) inferring a function from noisy data, for a wide range of discrete input spaces. The learning curve quantifies performance as average mean square error versus number of training examples.
GPs are a popular Bayesian inference technique. A GP prior is placed over a function space, and combined with the likelihood of the observed data given a function. Bayes’ theorem then gives a posterior distribution over functions. For a likelihood describing Gaussian noise corrupting the observed function values, this is again a GP, which can be used to make predictions about the function. GPs are “non-parametric”: they effectively represent functions with infinitely many parameters. This makes analysis of their learning curves non-trivial, and much has been achieved for GPs learning functions whose inputs are real-valued. However, predictions are generally only qualitatively correct, with exact solutions only for special cases. We show for the case where inputs are discrete, specifically vertices on a random graph, that replica techniques can be used to predict learning curves exactly in the limit of large graphs.
The starting point is to represent the average error as the derivative of a partition function. We rewrite this so that only neighbouring vertices are directly coupled. From here one can apply the replica method to find the required quenched average over the randomness in the data set. The results apply to random graph ensembles constrained by any fixed degree distribution, and can be generalised to more complicated ensembles.
M. J. Urry and P. Sollich, ‘Replica theory for learning curves for Gaussian processes on random graphs’, J. Phys. A: Math. Theor. 45, 425005 (2012)
[Abstract]
Repulsive Casimir forces at quantum criticality (Vol. 47 No. 3)
Casimir forces act between macroscopic objects immersed in a fluctuating entity, which may be the quantum vacuum or material medium in a state hosting sizable fluctuations. These forces were first discussed in 1948 as an observable manifestation of the quantum nature of the vacuum, lying at the heart of quantum electrodynamics. At a somewhat later stage it was realized that a material medium brought to the vicinity of a critical state induces analogous interactions once some macroscopic bodies become immersed therein.
In most of the known cases the Casimir force is attractive in situations where the bodies in question are identical. This however turns out not to be a general rule.
In our theoretical work we addressed a system of bosonic particles in the vicinity of a quantum critical state, where both thermal and quantum fluctuations are strong. As our exact analysis indicates, the sign of the Casimir force between two bodies immersed in such a medium may be changed by varying the ratio between their separation D and the thermal de Broglie length λ. In the thermal regime D>>λ the force in question is attractive, however, by varying the system setup so that D<<λ one crosses over to a regime admitting repulsive Casimir interactions.
P. Jakubczyk, M. Napiórkowski and T. Sęk, Repulsive Casimir forces at quantum criticality, EPL 113, 30006 (2016)
[Abstract]
Resolving tension on the surface of polymer mixes (Vol. 49, No. 1)

Credit iker-urteaga via Unsplash
A new study finds a simple formula to explain what happens on the surface of melted mixes of short- and long-strand polymers.
Better than playing with Legos, throwing polymer chains of different lengths into a mix can yield surprising results. In a new study published recently, physicists focus on how a mixture of chemically identical chains into a melt produces unique effects on their surface. That’s because of the way short and long polymer chains interact with each other. In these kinds of melts, polymer chain ends have, over time, a preference for the surface. Now, the authors have studied the effects of enriching long-chain polymer melts with short-chain polymers. They performed numerical simulations to explain the decreased tension on the surface of the melt, due to short chains segregating at the surface over time as disorder grows in the melt. They found an elegant formula to calculate the surface tension of such melts, connected to the relative weight of their components.
P. Mahmoudi and M.W. Matsen, Entropic segregation of short polymers to the surface of a polydisperse melt, Eur. Phys. J. E 40, 85 (2017)
[Abstract]
Revealing the microscopic origin of φ0 Josephson junctions (Vol. 46 No. 5-6)

A spontaneous dissipationless current (supercurrent) can flow in a superconducting ring even in the absence of a magnetic flux, if the ring is interrupted by a so-called φ0 junction. In the present work the authors present a full microscopic theory that explains the appearance of the anomalous φ0 phase in junctions with an intrinsic spin-orbit coupling (SOC) and a spin-splitting field like the exchange field in ferromagnets. The SOC generates the spin precession of moving particles, and, in addition, it causes a spin-dependent deflection of electron trajectories. The latter can be interpreted in terms of an effective spin- dependent SU(2) magnetic field that in normal systems is the origin of the intrinsic spin Hall effect and the existence of spin currents in the equilibrium state. A finite φ0 in a Josepson junction is directly related to the appearance of an equilibrium spin current with a spin projection parallel to the exchange field. These findings are the first steps towards spin-orbitronics with superconductors by making a natural connection between charge-spin conversion in dissipative and superconducting structures.
F. S. Bergeret and I. V. Tokatly, Theory of diffusive φ0 Josephson junctions in the presence of spin-orbit coupling, EPL, 110, 57005 (2015)
[Abstract]
Revisiting quantum effects in MEMS (Vol. 45 No. 1)

Credit: United States Government Work
Micro- and nano-electromechanical devices, referred to as MEMS and NEMS, are ubiquitous. They are found in car airbags and smart phones. The trouble is that, as their size decreases, forces typically experienced at the quantum level start to matter in these nanodevices. The authors have studied the mechanical and electrical stability of MEMS and NEMS, depending on the plate thickness and the nature of the material used. They show that previous works overestimated the operating conditions of the devices by not taking into account this Casimir/van der Waals effect. In addition, they demonstrate that the stability of these devices under the Casimir force changes depending on the nature and thickness of the metal coatings used. It also depends on the variation of concentration of the free charges in the silicon used, which changes with doping levels.
R. Esquivel-Sirvent and R. Perez-Pascual, “Geometry and charge carrier induced stability in Casimir actuated nanodevices”, Eur. Phys. J. B, 86, 467 (2013)
[Abstract]
Robustness of states at topological insulator interfaces (Vol. 48, No. 5-6)

Topological phases of matter are characterized by invariant numbers. In two-dimensional time-reversal symmetric electronic systems, a Z2 valued (0 or 1) invariant distinguishes trivial insulators from non-trivial ones. Interfaces between trivial and non-trivial topological insulators are known to host conductive channels protected against disorder. The protection of these states originates from the necessity of a gap closure in order to change topology. However, if the two regions are of the same topological phase, there is no such requirement.
Using a multi-orbital model, it is shown in this study that conductive states can also emerge at the interface between two non-trivial topological insulators characterized by opposite spin Chern numbers, another invariant. In general, these states are sensitive to disorder. However, it is possible under some conditions to reduce the effect of disorder, or even to cancel it. These conditions are clarified. Since analogues of topological insulators can be presently made with polaritons, ultracold atomic gases, phononic or photonic materials, these conclusions should motivate experimental studies in many directions.
A. Tadjine and Ch. Delerue, Robustness of states at the interface between topological insulators of opposite spin Chern number, EPL 118, 67003 (2017)
[Abstract]
Rodeo in liquid crystal (Vol. 46 No. 3)

Scientists have achieved an unprecedented level of control over defects in liquid crystals that can be engineered for applications in liquid matter photonics.
Sitting with a joystick in the comfort of their chairs, scientists can play “rodeo” on a screen magnifying what is happening under their microscope. They use very strong laser tweezers to locally melt the liquid crystal into a phase where the molecules are oriented in all directions, encircling one part of the fibre. They subsequently switch-off the laser light, resulting in molecules reverting back from being oriented in all directions to being parallel to each other, creating several pairs of defects—akin to localised disruptions of the crystal’s ordering field —forming a ring. The defect ring is used as a non-material "rope" to entangle and strongly bind a microsphere and long fibre of micrometric diameter. The results of this work have been published recently by the authors. They believe that their findings could ultimately open the door to controlling the flow of light using light of a specific frequency in the Gigahertz range in liquid crystal photonic microdevices.
M. Nikkhou, M. Škarabot and I. Muševič,, Topological binding and elastic interactions of microspheres and fibres in a nematic liquid crystal, Eur. Phys. J. E, 38, 23 (2015)
[Abstract]
Subcategories
- Highlights
- Vol. 41 No. 6 - Highlights
- Vol. 42 No. 3 - Highlights
- Vol. 41 No. 5 - Highlights
- Vol. 42 No. 1 - Highlights
- Vol. 42 No. 2 - Highlights
- Vol. 42 No. 4 - Highlights
- Vol. 42 No. 5 - Highlights
- Vol. 43 No.2 - Highlights
- Vol. 42 No. 6 - Highlights
- Vol. 43 No.1 - Highlights
- Vol. 43 No.3 - Highlights
- Vol. 43 No.4 - Highlights
- Vol. 43 No.5 - Highlights
- Vol. 43 No.6 - Highlights
- Vol. 44 No.1 - Highlights
- Vol. 44 No.2 - Highlights
- Vol. 44 No.3 - Highlights
- Vol. 44 No.4 - Highlights
- Vol. 44 No.5 - Highlights
- Vol. 45 No.1 - Highlights
- Vol. 45 No.2 - Highlights
- Vol. 45 No.3 - Highlights
- Vol. 45 No.4 - Highlights
- Vol. 45 No.5-6 - Highlights
- Vol. 46 No.1 - Highlights
- Vol. 46 No.2 - Highlights
- Vol. 46 No.3 - Highlights
- Vol. 46 No.4 - Highlights
- Vol. 46 No.5-6 - Highlights
- Vol. 47 No.1 - Highlights
- Vol. 47 No.2 - Highlights
- Vol. 47 No.3 - Highlights
- Vol. 47 No.5-6 - Highlights
- Vol. 48 No. 1 - Highlights
- Vol. 48 No. 2 - Highlights
- Vol. 48 No. 3 - Highlights
- Vol. 48 No.4 - Highlights
- Vol. 48 No.5-6 - Highlights
- Vol. 49 No.1 - Highlights
- Vol. 49 No.2 - Highlights
- Vol. 49 No.3 - Highlights
- Vol. 49 No. 4 - Highlights
- Vol. 49 No. 5-6 - Highlights
- Vol. 50 No. 1 - Highlights
- Vol. 50 No. 2 - Highlights
- Vol. 50 No. 3 - Highlights
- Vol. 50 No. 4 - Highlights
- Vol. 50 No. 5-6 - Highlights
- Vol. 51 No. 1 - Highlights
- Vol. 51 No. 2 - Highlights
- Vol. 51 No. 3 - Highlights
- Vol. 51 No. 4 - Highlights
- Vol. 51 No. 5 - Highlights
- Vol. 52 No. 1 - Highlights