Energy dependence of the isomeric cross section ratio inthe 58Ni(n,p)58Com,greactions

Sensitivity of the fusion cross section to the density dependence of the symmetry energy

P.-G. Reinhard, ∗ A.S. Umar, † P. D. Stevenson, ‡ J. Piekarewicz, § V.E. Oberacker, ¶ and J.A. Maruhn ∗∗ Institut für Theoretische Physik, Universität Erlangen, D-91054 Erlangen, Germany Department of Physics and Astronomy, Vanderbilt University, Nashville, TN 37235, USA Department of Physics, University of Surrey, Guildford, Surrey, GU2 7XH, United Kingdom Department of Physics, Florida State ...

Target dependence of the triply differential cross section for low energy (e, 2e) processes

Cross sections for the formation of Zn ,g and Zn ,g in neutron induced reactions near their thresholds: Effect of reaction channel on the isomeric cross-section ratio

Excitation functions were measured for the reactions Ge(n ,a) Zn , Ga(n ,p)Zn , Zn(n ,2n)Zn , Ge(n ,a)Zn , and Ga(n ,p)Zn ,g over the neutron energy range of 6.3–12.4 MeV. Quasimonoenergetic neutrons in this energy range were produced via the H(d ,n)He reaction using a deuterium gas target at the Jülich variable energy compact cyclotron. Use was made of the activation technique in combination w...

Chirality dependence of the absorption cross section of carbon nanotubes.

The variation of the optical absorption of carbon nanotubes with their geometry has been a long-standing question at the heart of both metrological and applicative issues, in particular because optical spectroscopy is one of the primary tools for the assessment of the chiral species abundance of samples. Here, we tackle the chirality dependence of the optical absorption with an original method ...

Factorization scheme dependence of the NLO inclusive jet cross section

We study the factorization scheme dependence of the next-to-leading order inclusive one jet cross section dσ/dET . The scheme is varied parametrically along the direction that transforms the MS scheme to the DIS scheme: we introduce a parameter λ such that λ = 0 is MS and λ = 1 is DIS. The factorization scale μ is also varied. We observe a change of ±9% in the cross section for ET = 50 GeV when...