Short Description of research interest and expertise
 

Theoretical Nuclear Physics:
structure of light nuclei on the driplines and reactions with Halo nuclei using few-body models (2 and 3 body).

Nuclear Reactions and Astrophysics:
direct capture reactions involving halo nuclei; breakup processes and transfer reactions for extracting spectroscopic factor, asymptotic normalisation coefficients and astrophysical S-factors.

1. Few-body system methods (2 and 3 - body) for application to light nuclei, in particular halo nuclei, including excitation of the bodies: the Pauli-projection method, methods for solving the  coupled equations in the Schr\"{o}dinger and  Faddeev formalism (the Hypershperical method,the Sturmian method).
2. Methods for direct capture calculations and reactions of Astrophysical interest: the low energy methods for calculating cross sections and S-factors, application of the two and three body models for capture reactions.
3. Analytic method for calculating electromagnetic excitations into the continuum.
4. Fresco coupled channels for calculating elastic, transfer reactions and breakup processes: including bound states and states in the continuum (Continuum Discretised Coupled Channels).