output
19922026
most citedThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

3.1k citations

Showing 2006 · nucl-thShow all

10 papers · 2 filters

nucl-th2006★ 3 cited

Working Group Summary: Chiral Dynamics in Few-Nucleon Systems

H. -W. Hammer, N. Kalantar-Nayestanaki, D. R. Phillips

We summarize the findings of our Working Group, which discussed progress in the understanding of Chiral Dynamics in the A=2, 3, and 4 systems over the last three years. We also ide…

nucl-th2006

Effective Range Corrections in Few-Body Systems with large Scattering Length

L. Platter

The effective field theory with contact interactions alone is a powerful tool to compute low-energy observables for three-body systems with large scattering length. Recent calculat…

nucl-th2006★ 3 cited

Three-Body Elastic and Inelastic Scattering at Intermediate Energies

H. Liu, Ch. Elster, W. Gloeckle

The Faddeev equation for three-body scattering at arbitrary energies is formulated in momentum space and directly solved in terms of momentum vectors without employing a partial wa…

nucl-th2006★ 207 cited

Universal Properties of the Four-Body System with Large Scattering Length

H. -W. Hammer, L. Platter

Few-body systems with large scattering length have universal properties that do not depend on the details of their interactions at short distances. We study the universal bound sta…

nucl-th2006★ 44 cited

Nucleosynthesis in neutron-rich ejecta from quark-novae

Prashanth Jaikumar, Bradley S. Meyer, Kaori Otsuki +1

We explore heavy-element nucleosynthesis by rapid neutron capture (r-process) in the decompressing ejecta from the surface of a neutron star. The decompression is triggered by a vi…

nucl-th2006★ 37 cited

Breaking of nucleon Cooper pairs at finite temperature in 93-98Mo

K. Kaneko, M. Hasegawa, U. Agvaanluvsan +9

The S shape of the canonical heat capacity is known as a signature of the pairing transition and along an isotopic chain it is significantly more pronounced for nuclei with an even…