نتایج جستجو برای: spherical shell

تعداد نتایج: 97671  

Journal: :Physical review letters 2002
S P Regan J A Delettrez F J Marshall J M Soures V A Smalyuk B Yaakobi R Epstein V Yu Glebov P A Jaanimagi D D Meyerhofer P B Radha T C Sangster W Seka S Skupsky C Stoeckl R P J Town D A Haynes I E Golovkin C F Hooper J A Frenje C K Li R D Petrasso F H Séguin

The Rayleigh-Taylor instability in its highly nonlinear, turbulent stage causes atomic-scale mixing of the shell material with the fuel in the compressed core of inertial-confinement fusion targets. The density of shell material mixed into the outer core of direct-drive plastic-shell spherical-target implosions on the 60-beam, OMEGA laser system is estimated to be 3.4(+/-1.2) g/cm(3) from time-...

Journal: :Physical review letters 2013
D T Yordanov D L Balabanski J Bieroń M L Bissell K Blaum I Budinčević S Fritzsche N Frömmgen G Georgiev Ch Geppert M Hammen M Kowalska K Kreim A Krieger R Neugart W Nörtershäuser J Papuga S Schmidt

The neutron-rich isotopes of cadmium up to the N=82 shell closure have been investigated by high-resolution laser spectroscopy. Deep-uv excitation at 214.5 nm and radioactive-beam bunching provided the required experimental sensitivity. Long-lived isomers are observed in (127)Cd and (129)Cd for the first time. One essential feature of the spherical shell model is unambiguously confirmed by a li...

2008
Charles D. Dermer

An analysis of the interaction between a spherical relativistic blast -wave shell and a stationary cloud with a spherical cap geometry is performed assuming that the cloud width ∆cl ≪ x, where x is the distance of the cloud from the GRB explosion center. The interaction is divided into three phases: (1) a collision phase with both forward and reverse shocks; (2) a penetration phase when either ...

2003
R. Mansouri M. Borhani

We consider a spherical thick 3-brane immersed in a five-dimensional bulk spacetime. We demonstrate how the thick brane equation of motion expanded in powers of the thickness of the brane can be obtained from the expected junction conditions on the boundaries of thick brane with the two embedding spacetimes. It is shown that the finite thickness leads to a faster collapse of the spherical shell...

2003
ZHAN Peng

We report a feasible approach to the preparation of monodispersed metal-shell composite microspheres based on a combination of surface reaction and surface seeding techniques. The method was implemented for coating polystyrene (PS) spheres with silver shell having a variable thickness by controlling the amount of reagents in the reaction procedure. These composite spherical particles in dimensi...

2006
Ram Brustein Martin B. Einhorn Amos Yarom

We consider a collapsing relativistic spherical shell for a free quantum field. Once the center of the wavefunction of the shell passes a certain radius rs, the degrees of freedom inside rs are traced over. We show that an observer outside this region will determine that the evolution of the system is nonunitary. We argue that this phenomenon is generic to entangled systems, and discuss a possi...

Journal: :Chemical communications 2006
Masih Darbandi Thomas Nann

A new one-pot synthetic method for preparing core/shell YF3@SiO2 nanoparticles with different morphologies, from spherical to elongated structures ("pearl necklace"), is described; absorbance and photoluminescence spectroscopy reveals intrinsic but no extrinsic defects in the YF3.

Journal: :Math. Comput. 2005
Qiang Du Lili Ju

In this paper the numerical approximations of the GinzburgLandau model for a superconducting hollow spheres are constructed using a gauge invariant discretization on spherical centroidal Voronoi tessellations. A reduced model equation is used on the surface of the sphere which is valid in the thin spherical shell limit. We present the numerical algorithms and their theoretical convergence as we...

Journal: :The Journal of chemical physics 2007
Felicia Tam Allen L Chen Janardan Kundu Hui Wang Naomi J Halas

The plasmon response of a spherical metallic shell becomes significantly more complex as its size is increased beyond the quasistatic limit. With increasing size and decreasing aspect ratio (r1/r2), higher order multipolar modes contribute in a more dominant manner, and two distinct core-shell geometries exist that provide the same dipole plasmon resonance, with differing relative multipolar co...

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