Scaling in few-body nuclear physics

The nuclear matter calculations with realistic nucleon-nucleon potentials present a general scaling between the nucleon-nucleus binding energy, the corresponding saturation density, and the triton binding energy. The Thomas-Efimov three-body effect implies in correlations among low-energy few-body and many-body observables. It is also well known that, by varying the short-range repulsion, keeping the two-nucleon information (deuteron and scattering) fixed, the four-nucleon and three-nucleon binding energies lie on a very narrow band known as a Tjon line. By looking for a universal scaling function connecting the proper scales of the few-body system with those of the many-body system, we suggest that the general nucleus-nucleon scaling mechanism is a manifestation of a universal few-body effect.

Renormalization in few-body nuclear physics

Renormalized fixed-point Hamiltonians are formulated for systems described by interactions that originally contain point-like singularities (as the Dirac-delta and/or its derivatives). They express the renormalization group invariance of quantum mechanics. The present approach for the renormalization scheme relies on a subtracted T-matrix equation.

Experimental nuclear physics.

Includes bibliographies.

Radioactivity and nuclear physics.

Includes bibliographical references.

Metrical geometry, contact transformations and nuclear physics.

Cover title.

Elements of nuclear physics /

"To incorporate recent findings ... since the Italan text [Il nucleo atomico] was written, essential modifications have been introduced in the present edition."--Pref.

Principles of nuclear physics

Mode of access: Internet.

Conference on biological applications of nuclear physics. July 12-27, 1948.

Includes bibliographies.

Atomic and nuclear physics /

Includes bibliographies.

Applied nuclear physics

Includes bibliographies.

Radioactivity and nuclear physics,

Bibliographical foot-notes. "References": p. 291-294.

The role of nuclear physics in supernovae and the evolution of neutron stars, Neutrino Opacities, Equation of State, Transport Coefficients, and Dark Matter Production

Thesis (Ph.D.)--University of Washington, 2016-08