Abstract
We present a model, leading to a generalised master equation, from which both angular distributions and spectra of preequilibrium nucleons can be successfully calculated. Implications and limitations of this model are discussed.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Paper version not known
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
