The problem of energy losses suffered by energetic ions moving in condensed matter with velocities smaller than the Fermi velocity is studied from different viewpoints. For protons, comparison between linear dielectric theory results and those obtained by means of a scattering approach is made. Within...
Studies on the interaction of light with matter 对于光与物质相互作用的研究,它是人类不断前进的产物之一。自然科学的研究一直以来都是人类进步的铺路石。通过对光和物质相互作用的研究,我们可以更好地理解各种自然现象,生产出更加智能化的产品和强效的技术。本文将分为三个部分,对光与物质相互作用的研究进行探讨...
Interaction of short and intense light pulses with matter: visible versus VUV S. Guizard et al., "Interaction of short and intense light pulses with matter: visible versus VUV," Proc. SPIE 6586, 65860F (2007)... S Guizard,G Geoffroy,J Gaudin,... - Conference on Damage to Vuv 被引...
High-Intensity X-Rays - Interaction with Matter: Processes in Plasmas, Clusters, Molecules, and Solids Filling the need for a book bridging the effect of matter on X-ray radiation and the interaction of x-rays with plasmas, this monograph provides comprehens... SP Hauriege - Wiley 被引量:...
INTERACTION OF LASER RADIATION WITH MATTER. LASER PLASMA: Formation of a long-lived plasma bubble as a result of irradiation of a metal target by a pulsed ... LASER PLASMA: Formation of a long-lived plasma bubble as a result of irradiation of a metal target by a pulsed XeCl laser AN Pa...
Interaction of ions and ion clusters with a disordered electron gas: Collective and single-particle excitations - art. no. 046415 Interaction of ions and ion clusters with a disordered electron gas: Collective and single-particle excitations - art. no. 046415... NHDAM Hh. - 《Physical Review...
摘要: Gravitational wave generation by a strong shock wave in the interaction of high power laser with matter is analyzed in linear approximation of gravitational theory. The analytical formulas and estimat关键词: General Relativity and Quantum Cosmology ...
This chapter provides a physical background to the following ones. It describes the particle and wave properties of light and the diffraction, polarization, refraction, reflection, and absorption of light and statistics of photon emission and absorption.
The large absorption of the 21-centimetre transition of hydrogen around redshift 20 is explained by radiation from the first stars, combined with excess cooling of the cosmic gas caused by baryon–dark matter scattering. As the first stars heated hydroge