Abstract. A modified two-centre atomic orbital expansion is employed in a study of charge transfer in Li3++H collisions at 'Li impact energies E = 1.4-140 keV. Cross sections are calculated for transitions into individual Li2 * orbitals as well as into all bound orbitals. The calculated total transfer cross sections are in excellent agreement with existing experimental data but differ significantly from those of other model descriptions. In recent years, considerable attention has been directed towards an understanding of inelastic processes in collisions of highly charged light projectiles with hydrogen. A particularly intricate problem is that of describing charge transfer in the intermedi-ate- and low-velocity regions where molecula...
The detailed features of the interaction forces within the LiH2+ triatomic system are calculated usi...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...
Abstract. A modified two-centre atomic-orbital expansion is used in an investigation of electron tra...
We calculate the cross section for the charge exchange process in Li 2+(1s) + H(1s) collisions, usin...
We calculate the cross section for the charge exchange process in Li 2+(1s) + H(1s) collisions, usin...
The electron capture processes in Li2 + + H collisions have been investigated by using...
The charge transfer process in collisions of excited (n = 2, 3) hydrogen atoms with He+ and in colli...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The two-center wave-packet convergent close-coupling method has been applied to model the processes ...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
A survey of theoretical studies of charge transfer involving collisions of multiply-charged ions wit...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The detailed features of the interaction forces within the LiH2+ triatomic system are calculated usi...
The detailed features of the interaction forces within the LiH2+ triatomic system are calculated usi...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...
Abstract. A modified two-centre atomic-orbital expansion is used in an investigation of electron tra...
We calculate the cross section for the charge exchange process in Li 2+(1s) + H(1s) collisions, usin...
We calculate the cross section for the charge exchange process in Li 2+(1s) + H(1s) collisions, usin...
The electron capture processes in Li2 + + H collisions have been investigated by using...
The charge transfer process in collisions of excited (n = 2, 3) hydrogen atoms with He+ and in colli...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The two-center wave-packet convergent close-coupling method has been applied to model the processes ...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
A survey of theoretical studies of charge transfer involving collisions of multiply-charged ions wit...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The detailed features of the interaction forces within the LiH2 + triatomic system are calculated u...
The detailed features of the interaction forces within the LiH2+ triatomic system are calculated usi...
The detailed features of the interaction forces within the LiH2+ triatomic system are calculated usi...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...
Low-energy inelastic collisions with neutral hydrogen atoms are important processes in stellar atmos...