... first 1 / 2 + state in ' Be from electron scattering and astrophysical implications ... resonance parameters of the first 1 / 2 + state in ' Be have been derived in ... 9Be , electron scattering PACS : 25.30.Dh , 26.20.Fj , 26.30.Hj ...

... state ( J = 3 , г ( 2.03 ± 0.15 ) MeV ) and first excited state ( J = 1/2 , Ex = ( 10.21 ± 0.28 ) MeV , г = ( 1.49 ... 9Be are calculated on a multichannel three - body model in which the internal structure of the a particle is ...

... astrophysical 12N ( p , γ ) 130 reaction rate from the 2H ( 12N , 13O ) n reaction and its astrophysical implications . Phys . Rev. C 87 : 015803 . doi : 10.1103 / PhysRevC.87.015803 Herndl , H. , Hofinger , R. , Jank , J. , Oberhummer ...

Originally published in 1982, this collection of essays provides an integrated overview of the application of nuclear science to astronomy.

... state of spin ( 1,2,3 ) + exists near 1.12 MeV in 24 Al . PHYSICS RESEARCH ( CONT . ) ENERGY RESEARCH ABSTRACTS The ... resonance , it is concluded that the results imply that <BR> / sub n / ≈ 1.3 <BR> / sub p / , or alternatively ...

... first application of the seminal theoretical work done by Hill and Van Vleck ... state . These formulas , as well as the previ- ously derived lower - order ... parameters to fit 655 term values for the A2Π ( v = 0 , 1 , 2 , 3 ) ...

Presents the physics of stars in relation to modern topics such as neutrino oscillations, supernovae, black holes, and gravitational waves.

This book contains chapters on some of the crucial and trending research topics in nuclear structure, including the nuclei lying on the extremes of spin, isospin and mass.

... ( 1/2 ) p . 64-76 Using the experimental free - scattering phase shifts as ... first by means of a naive model and then within a coupled- channel calculation in which the Hilbert space is enlarged in order to include the A resonance ...