Shock shells in Coulomb explosions of nanoclusters.
نویسندگان
چکیده
We predict that Coulomb explosion of a nanoscale cluster, which is ionized by high-intensity laser radiation and has a naturally occurring spatial density profile, will invariably produce shock waves. In most typical situations, two shocks, a leading and a trailing one, form a shock shell that eventually encompasses the entire cluster. Being the first example of shock waves on the nanometer scale, this phenomenon promises interesting effects and applications, including high-rate nuclear reactions inside each individual cluster.
منابع مشابه
A pr 2 00 6 Controlled Shock Shells and Intracluster Fusion Reactions in the Explosion of Large Clusters
The ion phase-space dynamics in the Coulomb explosion of very large (∼ 10 − 10 atoms) deuterium clusters can be tailored using two consecutive laser pulses with different intensities and an appropriate time delay. For suitable sets of laser parameters (intensities and delay), large-scale shock shells form during the explosion, thus highly increasing the probability of fusion reactions within th...
متن کاملNanoscale modification of silicon surfaces via Coulomb explosion
Coulomb explosions on silicon surfaces are studied using large-scale molecular-dynamics simulations. Processes under investigation begin by embedding a region consisting of 265–365 singly charged Si ions on a Si @111# surface. The repulsive electrostatic energy, initially stored in the charged region, leads to a local state with ultrahigh pressure and stress. During the relaxation process, part...
متن کاملTHE NATURE OF Lyα BLOBS: SUPERNOVA-DOMINATED PRIMORDIAL GALAXIES
We consider a forming galaxy undergoing multitudinous supernova (SN) explosions, as a possible model of Lyα blobs (LABs). For this purpose, an ultra–high resolution hydrodynamic simulation is performed using 1024 grid points, where SN remnants are resolved with sufficient accuracy. It is found that multiple SN explosions produce kpc–size expanding hot bubbles, which drive cool, dense shells by ...
متن کاملar X iv : a st ro - p h / 01 02 16 4 v 1 9 F eb 2 00 1 Bubbles in galactic haloes
We briefly discuss a possible interconnection of vertical HI structures observed in the Milky Way Galaxy with large scale blow-outs caused by the explosions of multiple clustered SNe. We argue that the observed OB associations can produce only about 60 such events, or approximately one chimney per 3 kpc within the solar circle. We also discuss the overall properties of HI shells in nearby face-...
متن کاملCharge storage in Co nanoclusters embedded in SiO2 by scanning force microscopy
Scanning force microscopy was used to study localized charge deposition and subsequent transport in Co nanoclusters embedded in SiO2 deposited on an n-type Si substrate. Co nanoclusters were charged by applying a bias voltage pulse between tip and sample, and electrostatic force microscopy was used to image charged areas, to determine quantitatively the amount of stored charge, and to character...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
عنوان ژورنال:
- Physical review letters
دوره 91 14 شماره
صفحات -
تاریخ انتشار 2003