A. S. Iljinov
A01=A.S. Iljinov
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Angular Momentum
antinucleon annihilation
Asymmetric Fission
Author_A.S. Iljinov
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Average Multiplicity
Cascade Evaporation
Category1=Non-Fiction
Category=PHM
Charge Exchange Reaction
Collision Term
COP=United Kingdom
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E. Ya. Paryev
Eikonal Approximation
Energy Momentum Conservation Law
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Fission Barrier
Fission Barrier Height
Fission Fragments
hadron interactions
hadron-induced nuclear reactions
Heavy Mesons
Incident Particle
Inclusive Spectra
intranuclear cascade
kinetic equations
Language_English
Liouville Equation
Liouville Von Neumann Equation
Liquid Drop Model
M. V. Kazarnovsky
Mass Energy Distribution
Medium Weight Nuclei
multifragmentation physics
Neutron Halo
nuclear decay processes
PA=Temporarily unavailable
Phase Density
Pre-equilibrium Emission
Price_€100 and above
PS=Active
Saddle Point
Shell Correction
Shell Effects
softlaunch
Product details
- ISBN 9781315894706
- Weight: 870g
- Dimensions: 156 x 234mm
- Publication Date: 29 Nov 2017
- Publisher: Taylor & Francis Ltd
- Publication City/Country: GB
- Product Form: Hardback
- Language: English
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Intermediate-Energy Nuclear Physics is devoted to discussing the interaction between hadrons with nuclei, which leads to the emission of particles during an intranuclear cascade and subsequent decay of a highly excited residual nucleus. Experimental data and the methods and results of the calculation of probabilities of various processes initiated by intermediate-energy hadrons in nuclei are set forth and discussed. The potential for obtaining information on the structure and properties of nuclei by comparing experimental data with theoretical results is analyzed. New issues, such as analytic methods for the solution of kinetic equations describing the cascade, nuclear absorption of hadrons from bound states of hadronic atoms, interaction of antinucleons with nuclei, multifragmentation of highly excited residual nuclei, and polarization phenomena, are discussed in detail.
The book also demonstrates hadron-nucleus interactions that bridge the gap between low-energy and heavy ions physics. It is an interesting reference for nuclear physicists and other researchers interested in the analysis of problems associated with the evolution of the early (hot) universe, neutron stars and supernovas, after-burning of radioactive waste in nuclear energy installations, and electronuclear energy breeding.
