Charmed Hadrons from Coalescence plus Fragmentation in relativistic nucleus-nucleus collisions at RHIC and LHC

In a coalescence plus fragmentation approach we calculate the heavy baryon/meson ratio and the $p_T$ spectra of charmed hadrons $D^{0}$, $D_{s}$ and $\Lambda_{c}^{+}$ in a wide range of transverse momentum from low $p_T$ up to about 10 GeV and discuss their ratios from RHIC to LHC energies without any change of the coalescence parameters. We have included the contribution from decays of heavy hadron resonances and also the one due to fragmentation of heavy quarks which do not undergo the coalescence process. The coalescence process is tuned to have all charm quarks hadronizing in the $p_T\rightarrow 0$ limit and at finite $p_T$ charm quarks not undergoing coalescence are hadronized by independent fragmentation. The $p_T$ dependence of the baryon/meson ratios are found to be sensitive to the masses of coalescing quarks, in particular the $\Lambda_{c}/D^{0}$ can reach values of about $\rm 1\div 1.5$ at $p_T \approx \, 3$ \mbox{GeV}, or larger, similarly to the light baryon/meson ratio like $p/\pi$ and $\Lambda/K$, however a marked difference is a quite weak $p_T$ dependence with respect to the light case, such that a larger value at intermediate $p_T$ implies a relatively large value also for the integrated yields. A comparison with other coalescence model and with the prediction of thermal model is discussed.Comment: 13 pages, 9 figures. Fig. 5 updated and some minor changes in the tex

Impact of off-shell dynamics on the transport properties and the dynamical evolution of Charm Quarks at RHIC and LHC temperatures

We evaluate drag and diffusion transport coefficients comparing a quasi-particle approximation with on-shell constituents of the QGP medium and a dynamical quasi-particles model with off-shell bulk medium at finite temperature T. We study the effects of the width $\gamma$ of the particles of the bulk medium on the charm quark transport properties exploring the range where $\gamma < M_{q,g}$. We find that off-shell effects are in general quite moderate and can induce a reduction of the drag coefficient at low momenta that disappear already at moderate momenta, $p \gtrsim 2-3\, \rm GeV$. We also observe a moderate reduction of the breaking of the Fluctuation-Dissipation theorem (FDT) at finite momenta. Moreover, we have performed a first study of the dynamical evolution of HQ elastic energy loss in a bulk medium at fixed temperature extending the Boltzmann (BM) collision integral to include off-shell dynamics. A comparison among the Langevin dynamics, the BM collisional integral with on-shell and the BM extension to off-shell dynamics shows that the evolution of charm energy when off-shell effects are included remain quite similar to the case of the on-shell BM collision integral.Comment: 13 pages, 14 figure

Crack formation and damage evolution during consolidation in TBM driven tunnel linings in fine-grained soils

The paper deals with the numerical modelling of crack formation in segmental tunnel linings. A series of numerical analyses was conducted using the finite difference code FLAC2D. The primary aims of the analyses were to back-analyse the damage pattern observed in a TBM driven hydraulic tunnel excavated in clayey soils and to evaluate the safety level of the excavation assessing the stress and strain state of the lining. The excavation of the tunnel and the lining installation were simulated in plane-strain undrained conditions, adopting the stress reduction method. To take into consideration the peculiar interaction mechanism, identified as the cause the damages, the stress release was differentiated based on the orientation along the tunnel wall. Two distinct modelling strategies were used to model the tunnel lining: at first, simple beam elements were used, then, small continuum elements and cable elements were employed to represent the concrete and the steel bars respectively. The implemented algorithm allowed to simulate explicitly the formation of the cracks and their progressive development. Finally, consolidation analyses were carried out to assess the evolution of the damage and the long-term stress and strain level of the lining. The numerical analyses allowed to reproduce the observed damage pattern and to reliably evaluate the stress and strain state in the damaged lining. Furthermore, the long-term analyses showed that the consolidation process has a beneficial effect as the equalization of the pore pressures causes a reduction of the load eccentricity on the lining, thus progressively increasing the level of safety over time. The investigation of the causes of the reported damage and its numerical modelling allowed to remark the importance of proper tail void grouting when excavating under high cover depths in squeezing soils

Cosmography of f(R) - brane cosmology

Cosmography is a useful tool to constrain cosmological models, in particular dark energy models. In the case of modified theories of gravity, where the equations of motion are generally quite complicated, cosmography can contribute to select realistic models without imposing arbitrary choices a priori. Indeed, its reliability is based on the assumptions that the universe is homogeneous and isotropic on large scale and luminosity distance can be "tracked" by the derivative series of the scale factor a(t). We apply this approach to induced gravity brane-world models where an f(R)-term is present in the brane effective action. The virtue of the model is to self-accelerate the normal and healthy DGP branch once the f(R)-term deviates from the Hilbert-Einstein action. We show that the model, coming from a fundamental theory, is consistent with the LCDM scenario at low redshift. We finally estimate the cosmographic parameters fitting the Union2 Type Ia Supernovae (SNeIa) dataset and the distance priors from Baryon Acoustic Oscillations (BAO) and then provide constraints on the present day values of f(R) and its second and third derivatives.Comment: 9 pages, 3 figures, to appear in Phys. Rev.