The available data on nuclear fusion cross sections important to energy generation in the
Sun and other hydrogen-burning stars and to solar neutrino production are summarized and …

In this article we review the current state of the field of solar neutrinos, including flavor
oscillations, nonstandard effects, solar models, cross section measurements, and the broad …

In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

The paper describes a multilevel, multichannel R-matrix code, azure, for applications in
nuclear astrophysics. The code allows simultaneous analysis and extrapolation of low …

We report on a new measurement of the 14N (p, γ) 15O capture cross section at Ep= 140 to
400 keV using the 400 kV LUNA accelerator facility at the Laboratori Nazionali del Gran …

The astrophysical S (E) factor of 14 N (p, γ) 15 O has been measured for effective center-of-
mass energies between E eff= 119 and 367 keV at the LUNA facility using TiN solid targets …

Nuclear astrophysics strives for a comprehensive picture of the nuclear reactions
responsible for synthesizing chemical elements and for powering the stellar evolution …

In stars with temperatures above 20× 106 K, hydrogen burning is dominated by the CNO
cycle. Its rate is determined by the slowest process, the 14N (p, γ) 15O reaction. Deep …

The synthesis of nuclei in diverse cosmic scenarios is reviewed, with a summary of the basic
concepts involved before a discussion of the current status in each case is made. We review …

Abstract The 14 N (p, γ) 15 O reaction, which controls energy production in the CNO cycle,
has contributions from both resonance and direct captures to the ground and excited states …