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We want to keep him. That is what I know so other reports, I would suggest, are erroneous. In particular, ICCUB researchers are interested in the study of microquasars, as objects which exhibit the characteristic accretion disc and perpendicular jets of relativistic matter of quasars, both thereby being governed by essentially the same physical processes as well as being subject to a timescale which is much more amenable to observations.

They are also interested in the study of gamma-ray binaries, which are able to accelerate particles up to TeV energies. Activitiy Research in High Energy Astrophysics has been focused on observations, theoretical modelling and numerical simulations to understand the physics of astrophysical outflows. Semi-analytical and numerical calculations of the radiation processes taking place in the sources have been developed to enable predictions of observable features in the different scenarios under investigation small and large scales, galactic and extragalactic sources of outflows ,.

Finally, there have been improvements on the knowledge of absorption mechanisms and on wind mixing in gamma-ray binaries through low frequency observations with LOFAR and GMRT. Recently, they have directed an important part of their efforts to the study of ultra-cold atomic gases and Bose-Einstein condensates. Analysis of the values of neutron star radius obtained by performing a global microscopic description of a neutron star, from the core to the crust.

Study of the nuclear symmetry energy and identification of observables which can constrain different aspects of this energy, as its density dependence. The neutron star contains about a Sun's worth of mass packed in a sphere the size of a large city. First results for the magnetic moments of light nuclei from LQCD calculations. Analysis of quantum phenomena which appear when placing bosons in optical lattices. Determination of the complete phase diagram for one-dimensional binary mixtures of bosonic ultracold atomic gases in a harmonic trap.

Study of the properties of three bosons in a onedimensional parabolic trap at zero temperature. The composition of the group reveals this variety of interests, extending to many of the forefront areas of research in Particle Physics. Several members share their activity in phenomenological aspects with their work in more formal parts of theoretical physics and gravitation.

Furthermore, they have an ever growing interest in the cosmological and astrophysical implications of particle physics phenomenology. Activitiy The activity has been influenced to a large extent by the first LHC results. ICCUB members are also sharpening their theoretical tools to take adequate stock of the next three years of running starting in spring These include resumation techniques and jet physics. Several features of heavy ion collisions particularly in the domain of hard probes and the study of properties of QCD under extreme conditions have also received considerable attention during Activity in the study of the behaviour of jets in quark-gluon plasma has been significant, including studies from holographic QCD.

QCD-related research includes work on lattice field theory, specially in connection with b-physics. ICCUB researchers also have relevant activity in the development of parton distribution functions using neural networks. Relevant contributions are also being made in the field of neutrino physics, axion physics and other dark matter candidates as well as dark energy in contact with the cosmology and astrophysics groups.

ICCUB research in this field focuses on the investigation of the dynamics of star-forming regions in our Galaxy and on the study of the first stages of stellar evolution. ICCUB researchers intend to acquire a perspective as wide as possible by pursuing both an observational approach, ranging from the optical to the radio domain, and a theoretical approach, based on state-of-the-art supercomputer simulations of the evolution of star-forming regions.

Activitiy The observational study of fragmentation in high-mass star-forming regions has been continued with high angular resolution observations of the 1. It has been studied the density structure of the two hubs by means of a simultaneous fit of the radial intensity profile. The NH3 synthesized beam is shown in the bottom left corner. Color stars depict the positions of YSOs with colors indicating their evolutionary stage. It was also investigated the interplay between magnetic field, turbulence, gravity and UV radiation feedback.

Both the stellar mass distribution and the star formation rate are in excellent agreement with the observations. This simulation has been used to solve the long-standing luminosity problem, meaning the origin of the characteristic luminosity and the large luminosity spread of protostars.

ICCUB Annual Report by Institut de Ciències del Cosmos - Issuu

ICCUB activities cover a wide spectrum of areas reported in the hep-th and quant-ph archives. Supersymmetric field theories are studied seeking to understand the ultraviolet behavior of theories with extended supersymmetries and deriving exact results. Research in quantum information is quite active too focusing in several topics such as entanglement entropy, tensor networks, quantum error correction, many-body quantum systems, topological order; ultra-cold gases; and quantum simulation. Using supersymmetric localization, matrix integrals and resurgence techniques, various aspects of supersymmetric gauge theories in three and four dimensions have been studied, including quantum phase transitions and vacuum expectation values of Wilson operators.

ICCUB researchers on Astrodynamics are devoting their efforts to addressing some fundamental issues concerning: First, they have continued with their activities related to the end of life disposal of spacecraft at the libration point regions. Second, they worked on the computation of Lagrangian Coherent Structures for the determination of invariant manifolds and long-term stability regions in Celestial Mechanics and Astrodynamics. In third place, in collaboration with CNES, they have continued their research plan about parameter identification of space debris and accurate estimation of collision probabilities.

The group on Image Processing is focused on the use of the wavelet and curvelet transforms to improve the ability of image sensors to detect faint stars and moving objects. Applications to Astronomy and Remote Sensing are developed. The group is studying the effects of the curvelet transform over interferometric images and the effect of deconvolution using wavelets and curveletsbased maximum likelihood estimator in adaptive optics observations. ICCUB researchers are also working on obtaining super-resolution using additive-substitutive wavelets techniques on remotely sensed images.

Activitiy During year the main activities were focused on the application of deconvolution to increase the limiting magnitude of images obtained for space debris detection. Activities of the group were also devoted to the continuation of the study of the deconvolution by multiresolution of images obtained using adaptive optics and the comparison of classical, myopic and blind algorithms.

Studies of image fusion and superresolution also continued. The experimental expertise in this area is the study of the stereo and enantioselective effect of hydrodynamic flows in the formation of supramolecular systems by self-assembly as well as the phase transitions from achiral building blocks to chiral supramolecules.

The substances under research are amphiphilic porphyrins. The general objective of these works is the understanding of unusual chiral polarizations in the spontaneous emergence of chirality during the chemical evolution that eventually lead to living systems. Activitiy The theoretical discussion of experimental results on spontaneous mirror symmetry and their concordance with possible Earth prebiotic scenarios has been reported.

Specific efforts have been made and partially reported in the discussion of chemical scenarios to justify, in the frame of linear thermodynamics of irreversible processes, a bias from the racemic composition in the absence of any external chiral polarization. Engineering models for prediction of peak flux and fluences of solar energetic particle events. Solar flares and coronal mass ejections, the main agents of SEP-acceleration, together with proxies of solar activity, the solar wind plasma and the interplanetary magnetic field, are the background components of the SEP scenario.

The estimate release time has been compared with the results obtained by using a simulation to unfold the interplanetary transport effects. A three-dimensional magnetohydrodynamic code was used to simulate such a shock and the evolution of the downstream-to-upstream ratios of the plasma variables at its front were determined.

The main objective is to elucidate physical mechanisms that control bubble formation, bubble-flow interactions, and heat exchange in the absence of gravity, in view of improving current designs and searching for new strategies for efficient thermal control in microgravity environments. Activitiy In the activity has focused on the optimization and characterization of an innovative design for capillary boiling through controlled localized nucleation. The prototype system has proven to work robustly in a gravity-insensitive way and has been fully characterized within a variety of relevant parameters.

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The device generates regular slug flows that can be used as input for heat-exchange or other devices. Based on the results obtained, a new design has been proposed for controlled capillary boiling on a passive self-sustained closed-loop system. On the theoretical side, an idealized version of the nucleation device has been solved exactly showing interesting scaling properties of fundamental interest. ICCUB is currently participating in the development of the following electronics and instrumentation: The spectrograph input optics also include a slit slicer which reformats each probe field into 3 end-toend slices of a fixed 4.

The spectrograph optics then provide a range of configurations providing the observer with the ability to choose between maximal multiplex advantage and maximal wavelength coverage, with several intermediate options, depending upon the needs of the science program. The ISS has been optimized to minimize the power consumption and to provide the best performance making use of the reduced number of parts available for space applications. The TFRM is a 0. Nearly all kind of image survey programs can benefit from those specifications. Apart from other less time consuming programs, since the beginning of science TFRM operations, ICCUB researchers have been conducting two specific and distinct surveys: In parallel other programs as the search for near earth objects NEO and the observations of high energy sources are carried out regularly.

It has been necessary a thorough analysis of the collisions and possible interferences between the probe arms. The algorithm has been tested with base cases, providing promising results. The total number of. A mean of Regarding the exoplanet survey, during ICCUB researchers continued observing 48 selected fields detecting hundreds of new variable stars and studying the possibility of new exoplanets around them using newly implemented algorithms.

Also, the optical counterparts of four high-energy sources were systematically observed to establish the variations of their light curves and the models to explain them. They maintain the leading role of the Spanish groups in Gaia at the highest technological, scientific and management levels. It also has deputy managers in CU2 and CU3. It was created to handle the distributed computing of the LHCb experiment, and now other communities, such as CTA, have begun to use it. Several patches have been introduced in the Initial Data Treatment system IDT , developed at ICCUB, in order to cope with the real telemetry as well as with the onboard detection levels, changes in the control electronics etc.

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Testing in parallel of new IDT versions still continue. These datasets will be used to prepare the final catalogue and database, containing more than one billion objects. The ICCUB team is developing and coordinating the ongoing processing tasks to fully deploying the new ones associated to the Gaia Archive. This integration ensures that DIRAC will still be a competitive project as the trend in distributed computing evolves. It provides software engineering solutions and high-performance data compression strategies including proprietary implementations.

Besides being resilient to outliers in the data, it offers an optimum compromise between resources consumption and compression ratio. It can be applied to scientific research projects, supercomputing, or companies dealing with Big Data scenarios. SiUB staff and associate members hold more than ten years of experience developping instrumentation at different levels: SiUB is making use of this experience.

The first work package was nearly finished by the end of , leading to a DWT-based pre-processing stage for lossless or lossy FAPEC image compression. Ideas Service SiUB After its creation in , the service has slowly started to operate providing support for local research groups and external laboratories.

The service has also signed collaboration agreements with a couple of companies. See section Electronic and Instrumentation Development for more details. Finally, several collaboration agreements have been signed with Scientifica Internacional S. In both cases, good results open the opportunity of longer term relationships. European Community EC Period: Radial and longitudinal effects Reference: Jordi Torra Roca Agency: High-energy phenomena in stellar objects. Theory and multi-wavelength observations Reference: Pilar Ruiz Lapuente Agency: Theory and multi-wavelength observations.

Physics exploitation and Upgrade. Aplicaciones para Solar Orbiter y herramientas para el tiempo espacial Reference: Canfranc Underground Physics Reference: Gravitation, Strings, and Cosmology Reference: Maximizing the scientific return of future galaxy surveys Reference: Physical Cosmology, PhysCos Reference: Hamamatsu Photonics France S. Advanced electronics for Hamamatsu detectors II Reference: Advanced electronics for Hamamatsu detectors IV Reference: Advanced electronics for Hamamatsu detectors V Reference: Miniaturization of the controller for an endoscopic diagnosis capsule Reference: Ovesco Endoscopy AG Period: Physics Letters B, Vol.

Aaij, R; et al. Nuclear Physics B, Vol. Physical Review Letters, Vol. Observation of Z production in proton-lead collisions at LHCb. Journal of High Energy Physics, Vol.

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Physical Review D, Vol. Article Nuclear Physics A, Vol. European Physical Journal C, Vol. Observation of associated production of a Z boson with a D meson in the forward region. First measurement of the charge asymmetry in beautyquark pair production. Precision luminosity measurements at LHCb. Journal Of Instrumentation, Vol. Observation of charmonium pairs produced exclusively in pp collisions.

Journal of Physics G: Nuclear and Particle Physics, Vol. Characterizing the Galactic warp with Gaia: The tilted ring model with a twist. Symmetry energy of warm nuclear systems. European Physical Journal A, Vol. Astronomy and Astrophysics, Vol. Astrophysical Journal Supplement Series, Vol. Black hole lightning due to particle acceleration at subhorizon scales.

The Astrophysical Journal, Vol. Rapid and multiband variability of the TeV bright active nucleus of the galaxy IC Landscape-inversion phase transition in dipolar colloids: Tuning the structure and dynamics of 2D crystals. Lowest resonance in QCD from low-energy data. Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples.

Analysis of dilepton angular distributions in a parity breaking medium. Mild quasilocal non-Gaussianity as a signature of modified gravity during inflation. Effective equation of state for running vacuum: Spontaneous parity violation under extreme conditions: An effective lagrangian analysis. Chemical potentials and parity breaking: Symmetry, Integrability and Geometry: From the crust to the core of neutron stars on a microscopic basis. Physics of Atomic Nuclei, Vol.

Formation of large-scale magnetic structures associated with the Fermi bubbles. Large N phase transitions in supersymmetric Chern-Simons theory with massive matter. Magnetic moments of light nuclei from lattice quantum chromodynamics. Dynamics of Carroll particles. Classical and Quantum Gravity, Vol. Statistical tests of sterile neutrinos using cosmology and short-baseline data. Bayesian comparison of U 1 lepton flavor models. Design of novel luminescent porphyrins bearing donor— acceptor groups. Journal of Porphyrins and Phthalocyanines, Vol.

Signs of neutrino mass in current cosmological datasets. Morphology and growth of polarized tissues. European Physical Journal E, Vol. Disentangling a dynamical Higgs. Stellar content and elemental abundances in the massive cluster NGC Physical Review C, Vol. Tensor force effects and gigh-momentum components in the nuclear symmetry energy. Holographic collisions in confining theories. Gaia photometry for white dwarfs. Conformal symmetry for relativistic point particles.

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Nuclear Physics A, Vol. Longitudinal coherence in a holographic model of asymmetric collisions. A Be-type star with a black-hole companion. Galaxy and mass assembly GAMA: Universal scaling dependence of QCD energy loss from data-driven studies. Constraints on the Galactic thin disc evolution from Tycho data. Deformations of the canonical commutation relations and metric structures. Spectral geometry with a cut-off: Journal of Geometry and Physics, Vol. Higgs mass in noncommutative geometry. Fortschritte der Physik, Vol. XMM-Newton observations reveal the disappearance of the wind in 4U Dynamical sectors of a relativistic two particle model.

Elastic nucleon-nucleus scattering as a direct probe of correlations beyond the independent-particle model.

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Multiscale confining dynamics from holographic RG flows. Decoupling and non-decoupling dynamics of large D black holes. Instability of rotating black holes: Holographic superconductivity in the large D expansion. Higher-dimensional black hole solutions: General Relativity and Gravitation, Vol. Unitarity and causality constraints in composite Higgs models. On the stability of multiscale models of dynamical symmetry breaking from holography. Detailed calculation of inner-shell impact ionization to use in photon transport codes.

Radiation Physics and Chemistry, Vol. Cross sections of K-shell ionization by electron impact, measured from threshold to keV, for Au and Bi. Journal of Physics B: Atomic, Molecular and Optical Physics, Vol. Exact probes of orientifolds. Exact results for Wilson loops in arbitrary representations. Physical Review A, Vol. Josephson physics of spin-orbit-coupled elongated BoseEinstein condensates.

CP violation with a dynamical Higgs. Advances in High Energy Physics, Vol. Riemann correlator in de Sitter including loop corrections form conformal fields. The Weyl tensor correlator in cosmological spacetimes. Journal of Cosmology and Astroparticle Physics, Vol. Schwinger effect in de Sitter space. Quantum correlations and spatial localization in onedimensional ultracold bosonic mixtures.

New Journal of Physics, Vol. Dark matter and halo bispectrum in redshift space: On the origin of the molecular outflows in IRAS Astrophysical Journal Letters, Vol. On the effect of the ionizing background on the Lyman alpha forest autocorrelation function. Updated fit to three neutrino mixing: Reevaluation of the prospect of observing neutrinos from Galactic sources in the light of recent results in gamma ray and neutrino astronomy. Quantum Hall Phases of two-component bosons. Physical Review B, Vol. Topological phases in small quantum Hall samples.

KROME-a package to embed chemistry in astrophysical simulations. A CO survey in planet-forming disks: Characterizing the gas content in the epoch of planet formation. Correcting EChO data for stellar activity by direct scaling of activity signals. Low depth quantum circuits for Ising models. Annals of Physics, Vol. Simulated annealing for tensor network states. Homothetic motions and Newtonian cosmology.

Fixing a rigorous formalism for the accurate analytic derivation of halo properties. Halo mass definition and multiplicity function. Quantum computation of prime number functions. Quantum Information and Computation, Vol.

Puyol más que un capitán Documental Canal Plus

UNSP L12 The Physics of the B Factories. Topical issue on nuclear symmetry energy. No new cosmological concordance with massive sterile neutrinos. Matrix Bases for Star Products: Cross sections for inner-shell ionization by electron impact. Vertical velocities from proper motions of red clump giants. New production mechanism for keV sterile neutrino Dark Matter by decays of frozen-in scalars.

Radiation hard programmable delay line for LHCb calorimeter upgrade. Journal of Instrumentation, Vol. The incidence of obscuration in active galactic nuclei. Application to the young stars in the Galactic anticenter survey. Dosimetric application of a special pencil ionization chamber in radiotherapy X-ray beams. Physical Review E, Vol.

Subharmonic oscillations of collective molecular motors.