Fluid dynamical prediction of changed v1-flow at energies available at the CERN Large Hadron Collider

Substantial collective flow is observed in collisions between lead nuclei at Large Hadron Collider (LHC) as evidenced by the azimuthal correlations in the transverse momentum distributions of the produced particles. Our calculations indicate that the global v1-flow, which at RHIC peaked at negative rapidities (named third flow component or antiflow), now at LHC is going to turn toward forward rapidities (to the same side and direction as the projectile residue). Potentially this can provide a sensitive barometer to estimate the pressure and transport properties of the quark-gluon plasma. Our calculations also take into account the initial state center-of-mass rapidity fluctuations, and demonstrate that these are crucial for v1 simulations. In order to better study the transverse momentum flow dependence we suggest a new"symmetrized" vS1(pt) function, and we also propose a new method to disentangle global v1 flow from the contribution generated by the random fluctuations in the initial state. This will enhance the possibilities of studying the collective Global v1 flow both at the STAR Beam Energy Scan program and at LHC.

Ein digitales Kulturobjekt. Der Fall der »Restaurierung« des Ecce homo von Borja

Im August 2012 brachte der Heimatverein von Borja, in Spanien, auf seinem Blog seine »tiefe Betroffenheit« über einen, wie es hieß, »unbeschreiblichen Vorgang« zum Ausdruck: Ein Wandgemälde in der Iglesia del Santuario de la Misericordia war in einer Form restauriert worden, die das ursprüngliche Motiv - den Schmerzensmann - fast unkenntlich machte. Die Affäre ging in kürzester Zeit durch die internationale Presse und durch das Internet. Sie schlug dabei unerwartet hohe Wellen, mit denen sich Hohn und Spott über den in fast allen Kommentaren als »misslungen« bezeichneten Restaurierungsakt ergoss. Im Web 2.0 hingegen gab das dergestalt »restaurierte« Antlitz des Ecce homo Anlass zu einer Vielzahl von Neuinterpretationen, es avancierte zu einem regelrechten Internet-Phänomen, das in der vorliegenden Studie in Hinblick auf den Umgang mit und die Aneignung von Bildern im digitalen Zeitalter untersucht werden soll.

Homo musicus et politicus

Toimitettua

Disseny d'una instal·lació de calefacció i ACS per una vivenda a partir d'energies renovables

En el present document es pretén desenvolupar els càlculs i especificacions necessàries, així com les característiques tècniques per poder dur a terme el disseny de la instal·lació de calefacció i ACS pel sistema de plaques solars tèrmiques i pel sistema geotèrmic. Es realitzarà un estudi previ per tenir un coneixement arquitectònic de la vivenda i així poder realitzar els càlculs de la demanda energètica. Es farà una descripció de les diferents alternatives de sistemes d'energia renovables que existeixen i es valoraran en funció de les necessitats del projecte per a trobar la més idònia. Una vegada triades les dues opcions, es procedirà a descriure de forma descriptiva i tècnicament, els sistemes escollits i dissenyar les instal·lacions pel seu bon funcionament. Per últim es farà un estudi econòmic de l'amortització dels dos sistemes escollits, per poder valorar si son econòmicament viables.

Viabilitat de les energies renovables a la comarca de la Segarra

El present projecte té la finalitat de fer un estudi sobre les diferents tipologies d'energies renovables i les possibilitats de la seva implantació a la comarca de la Segarra.

Microscopic-macroscopic approach for binding energies with the Wigner-Kirkwood method. II. Deformed nuclei

The binding energies of deformed even-even nuclei have been analyzed within the framework of a recently proposed microscopic-macroscopic model. We have used the semiclassical Wigner-Kirkwood ̄h expansion up to fourth order, instead of the usual Strutinsky averaging scheme, to compute the shell corrections in a deformed Woods-Saxon potential including the spin-orbit contribution. For a large set of 561 even-even nuclei with Z 8 and N 8, we find an rms deviation from the experiment of 610 keV in binding energies, comparable to the one found for the same set of nuclei using the finite range droplet model of Moller and Nix (656 keV). As applications of our model, we explore its predictive power near the proton and neutron drip lines as well as in the superheavy mass region. Next, we systematically explore the fourth-order Wigner-Kirkwood corrections to the smooth part of the energy. It is found that the ratio of the fourth-order to the second-order corrections behaves in a very regular manner as a function of the asymmetry parameter I=(N−Z)/A. This allows us to absorb the fourth-order corrections into the second-order contributions to the binding energy, which enables us us to simplify and speed up the calculation of deformed nuclei.

Caracteristicas diferenciales entre el fragmento de craneo de Homo sp.de Venta Micena (Orce, Granada) y los equidos

Se ha realizado un detallado estudio diferencial entre la morfología del fragmento craneal de Orce y varios équidos jóvenes, puesto que en anteriores trabajos ya se ha separado del resto de los mamiferos. El resultado obtenido ha sido la perfecta diferenciación anatómica entre todos los caracteres analizados, por lo que se concluye que dicho fragmento craneal de Orce no puede incluirse dentro de la variabilidad de los équidos.

Giant monopole energies from a constrained relativistic mean-field approach

Background:Average energies of nuclear collective modes may be efficiently and accurately computed using a nonrelativistic constrained approach without reliance on a random phase approximation (RPA). Purpose: To extend the constrained approach to the relativistic domain and to establish its impact on the calibration of energy density functionals. Methods: Relativistic RPA calculations of the giant monopole resonance (GMR) are compared against the predictions of the corresponding constrained approach using two accurately calibrated energy density functionals. Results: We find excellent agreement at the 2% level or better between the predictions of the relativistic RPA and the corresponding constrained approach for magic (or semimagic) nuclei ranging from 16 O to 208 Pb. Conclusions: An efficient and accurate method is proposed for incorporating nuclear collective excitations into the calibration of future energy density functionals.

Microscopic-macroscopic approach for binding energies with the Wigner-Kirkwood method

The semiclassical Wigner-Kirkwood ̄h expansion method is used to calculate shell corrections for spherical and deformed nuclei. The expansion is carried out up to fourth order in ̄h. A systematic study of Wigner-Kirkwood averaged energies is presented as a function of the deformation degrees of freedom. The shell corrections, along with the pairing energies obtained by using the Lipkin-Nogami scheme, are used in the microscopic-macroscopic approach to calculate binding energies. The macroscopic part is obtained from a liquid drop formula with six adjustable parameters. Considering a set of 367 spherical nuclei, the liquid drop parameters are adjusted to reproduce the experimental binding energies, which yields a root mean square (rms) deviation of 630 keV. It is shown that the proposed approach is indeed promising for the prediction of nuclear masses.

Fluid dynamical prediction of changed v1-flow at energies available at the CERN Large Hadron Collider

Substantial collective flow is observed in collisions between lead nuclei at Large Hadron Collider (LHC) as evidenced by the azimuthal correlations in the transverse momentum distributions of the produced particles. Our calculations indicate that the global v1-flow, which at RHIC peaked at negative rapidities (named third flow component or antiflow), now at LHC is going to turn toward forward rapidities (to the same side and direction as the projectile residue). Potentially this can provide a sensitive barometer to estimate the pressure and transport properties of the quark-gluon plasma. Our calculations also take into account the initial state center-of-mass rapidity fluctuations, and demonstrate that these are crucial for v1 simulations. In order to better study the transverse momentum flow dependence we suggest a new"symmetrized" vS1(pt) function, and we also propose a new method to disentangle global v1 flow from the contribution generated by the random fluctuations in the initial state. This will enhance the possibilities of studying the collective Global v1 flow both at the STAR Beam Energy Scan program and at LHC.