By Jean-Patrick Connerade, Andrey Solov'yov
This ebook offers a “snapshot” of the newest and important advances within the box of cluster physics. it's a entire overview in accordance with contributions by means of the individuals of the 2d foreign Symposium on Atomic Cluster Collisions (Isacc 2007) held in July 19–23, 2007 at Gsi, Darmstadt, Germany. the aim of the Symposium is to advertise the expansion and exhange of medical info at the constitution and homes of nuclear, atomic, molecular, organic and complicated cluster platforms studied through photonic, digital, heavy particle and atomic collisions. specific recognition is dedicated to dynamic phenomena, many-body results happening in cluster platforms of a unique nature - those comprise difficulties of fusion and fission, fragmentation, collective electron excitations, section transitions, and so forth. either the experimental and theoretical elements of cluster physics, uniquely put among nuclear physics at the one hand and atomic, molecular and sturdy kingdom physics at the different, are mentioned.
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Extra info for Latest advances in atomic cluster collisions: structure and dynamics from the nuclear to the biological scale
Exit channel along the quasi-ﬁssion valley (see Fig. 6). However, at non-zero excitation energy there is a chance for the nuclear system to overcome the multi-dimensional inner potential barriers and ﬁnd itself in the region of the CN conﬁguration. Within the Langevin calculations, a great number of events should be tested to ﬁnd this low probability. For the studied reaction, for example, only several fusion events have been found among more than 105 total tested events [see dark region 4 in Fig.
Furthermore, the screening eﬀect shifts the proton drip-line to more proton-rich nuclei, and the stability line with respect to β decay is shifted to more neutron-rich nuclei. Implications for the creation and survival of very heavy nuclear systems are discussed. Keywords: Superheavy nuclei; supernova explosions; electron gas. 1. Introduction The properties of nuclei in astrophysical environments have enjoyed continuous interest for over more than 30 years. , Refs. 2–7. In this contribution, we focus on the physics of nuclei embedded in a dense electron gas8 at zero temperature.