Dynamic Matrix-Fracture Transfer Behaviour in Dual-Porosity Models

Imperial Users onl

Centrality dependence of elliptic flow of multi-strange hadrons in Au+Au collisions at sNN\sqrt{s_{NN}} = 200 GeV

We present recent results of the mid-rapidity elliptic flow ($v_2$) for multi-strange hadrons and the $\phi$ meson as a function of centrality in Au + Au collisions at the center of mass energy $\sqrt{s_{NN}}$ = 200 GeV. The transverse momentum dependence of $\phi$ and $\Omega$ $v_2$ is similar to that of pion and proton, indicating that the heavier strange ($s$) quark flows as strongly as the lighter up ($u$) and down ($d$) quarks. These observations constitute a clear piece of evidence for the development of partonic collectivity in heavy-ion collisions at the top RHIC energy. In addition, the mass ordering of $v_2$ breaks between the $\phi$ and proton at low transverse momenta in the 0-30\% centrality bin, possibly due to the effect of late hadronic interactions on the proton $v_2$.Comment: 4 pages, 3 figures, SQM 2015 proceeding

Probe the QCD phase boundary with elliptic flow in relativistic heavy ion collisions at STAR

We present measurement of elliptic flow, $v_2$, for charged and identified particles at midrapidity in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 - 39 GeV. We compare the inclusive charged hadron $v_2$ to those from transport model calculations, such as UrQMD model, AMPT default model and AMPT string-melting model. We discuss the energy dependence of the difference in $v_2$ between particles and anti-particles. The $v_2$ of $\phi$ meson is observed to be systematically lower than other particles in Au+Au collisions at $\sqrt{s_{NN}}$ = 11.5 GeV.Comment: 5 pages, 3 figures, the proceedings of the 7th International Workshop on Critical Point and Onset of Deconfinement (CPOD2011

The Effect of CWS on Adolescent Health

This article will be covering the problem of celebrity worship. Celebrity worship has been in debate over the past few years regarding whether it is a harmful activity or not among adolescents, but with the recent established psychological disorder of Celebrity Worship Syndrome, it can be shown that it has become a serious health issue. One side argues that celebrity worship is harmless, even a helpful practice to pursue. The other side, however, argues that celebrity worship is detrimental to the mental and physical wellbeing of the adolescents. It is important to understand what celebrity worship entails, the different tests in place used to measure it, and the effect practicing celebrity worship can have on an adolescent to full realize how harmful engaging in celebrity worship really is

Theta series and generalized special cycles on Hermitian locally symmetric manifolds

We study generalized special cycles on Hermitian locally symmetric spaces $\Gamma \backslash D$ associated to the groups $G=\mathrm{U}(p,q)$, $\mathrm{Sp}(2n,\mathbb{R})$ and $\mathrm{O}^*(2n)$. These cycles are (covered by) locally symmetric spaces associated to subgroups of $G$ which are of the same type. Using oscillator representation and a construction which essentially comes from the thesis of Greg Anderson, we show that Poincar\'e duals of these generalized special cycles can be viewed as Fourier coefficients of a theta series. This gives new cases of theta lifts from the cohomology of Hermtian locally symmetric manifolds associated to $G$ to vector valued automorphic forms associated to the groups $G'=\mathrm{U}(m,m)$, $\mathrm{O}(m,m)$ or $\mathrm{Sp}(m,m)$ which forms a reductive dual pair with $G$ in the sense of Howe

Testing Cold Dark Matter Models Using Hubble Flow Variations

COBE-normalized flat (matter plus cosmological constant) and open Cold Dark Matter (CDM) models are tested by comparing their expected Hubble flow variations and the observed variations in a Type Ia supernova sample and a Tully Fisher cluster sample. The test provides a probe of the CDM power spectrum on scales of $0.02h$ Mpc^{-1}\la k\la 0.2h Mpc$^{-1}$, free of the bias factor $b$. The results favor a low matter content universe, or a flat matter-dominated universe with a very low Hubble constant and/or a very small spectral index $n_{ps}$, with the best fits having $\Omega_0\sim 0.3$ to 0.4. The test is found to be more discriminative to the open CDM models than to the flat CDM models. For example, the test results are found to be compatible with those from the X-ray cluster abundance measurements at smaller length scales, and consistent with the galaxy and cluster correlation analysis of Peacock and Dodds (1994) at similar length scales, if our universe is flat; but the results are marginally incompatible with the X-ray cluster abundance measurements if our universe is open. The open CDM results are consistent with that of Peacock and Dodds only if the matter density of the universe is less than about 60% of the critical density. The shortcoming of the test is discussed, so are ways to minimize it.Comment: 8 pages, 10 figures, submitted to MNRA

Size-independent Shear Band Formation in Amorphous Nanowires made from Simulated Casting

Molecular dynamics simulations indicate that surfaces strongly influence the strain localization behavior of amorphous nanowires in tension. A sample preparation routine that simulates casting was employed to facilitate the relaxation of the sample surface. Samples as short as 15 nm (7.5 nm in diameter) form dominant shear bands during deformation. The elastic energy release during plastic deformation is sufficient to provide the excess potential energy required for the shear band nucleation at rather small sample sizes. The results show that shear band formation is almost size-independent and is bounded only by its own length scale.Comment: 13 pages, 3 figures, to be appeared in Appl. Phys. Let