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G. J. Hanna

Publications and source records attributed to G. J. Hanna.

2 recordsLinked to original sources

Energetics and structural properties of three-dimensional bosonic clusters near threshold

We treat three-dimensional bosonic clusters wih up to N=40 atoms, interacting additively through two-body Van der Waals potentials, in the near-threshold regime. Our study inludes super-borromean systems with N atoms for which all subsystems are unbound. We determine the energetics and structural properties as the expectation value of the interparticle distance as a function of the coupling strength. It has been shown that the coupling strength g*(N), for which the N-body systems becomes unbound, is bounded by the coupling constant g*(N-1) for which the next smaller system with N-1 atoms becomes unbound, i.e., g*(N) >= (N-1)/Ng*(N-1). By fitting our numerically determined ground state energies to a simple functional form with three fitting parameters, we determine the relationship between g*(N) and g*(N-1). Our trimer and tetramer energies fall on the so-called Tjon line, which has been studied in nuclear physics. We confirm the existence of generalized Tjon lines for larger clusters. Signatures of the universal behavior of weakly-bound three-dimensional clusters can possibly be observed in ultracold Bose gases.

cond-mat.other↗

Formation of atomic tritium clusters and condensates

We present an extensive study of the static and dynamic properties of systems of spin-polarized tritium atoms. In particular, we calculate the two-body |F,m_F>=|0,0> s-wave scattering length and show that it can be manipulated via a Feshbach resonance at a field strength of about 870G. Such a resonance might be exploited to make and control a Bose-Einstein condensate of tritium in the |0,0> state. It is further shown that the quartet tritium trimer is the only bound hydrogen isotope and that its single vibrational bound state is a Borromean state. The ground state properties of larger spin-polarized tritium clusters are also presented and compared with those of helium clusters.

physics.atom-ph↗