Results 51 to 60 of about 6,422,375 (242)

Hydrogen Detection Near Surfaces and Shallow Interfaces with Resonant Nuclear Reaction Analysis

open access: yes, 2014
This review introduces hydrogen depth profiling by nuclear reaction analysis (NRA) via the resonant 1H(15N,αγ)12C reaction as a versatile method for the highly depth-resolved observation of hydrogen (H) at solid surfaces and interfaces.
M. Wilde, K. Fukutani
semanticscholar   +1 more source

Identification of programmed cell death in situ via specific labeling of nuclear DNA fragmentation

open access: yesJournal of Cell Biology, 1992
Programmed cell death (PCD) plays a key role in developmental biology and in maintenance of the steady state in continuously renewing tissues. Currently, its existence is inferred mainly from gel electrophoresis of a pooled DNA extract as PCD was shown ...
Yael Gavrieli   +2 more
semanticscholar   +1 more source

Unitary correlation in nuclear reaction theory: Separation of nuclear reactions and spectroscopic factors [PDF]

open access: yes, 2010
Future exact many-body theory will allow us to calculate nuclear reactions based on the adopted $\mathit{NN}$ and many-body nuclear potentials. But $\mathit{NN}$ potentials are not observable and there are an infinite number of the phase-equivalent ...
A. Mukhamedzhanov, A. Kadyrov
semanticscholar   +1 more source

Recent Developments in the Experimental Nuclear Reaction Data Library EXFOR

open access: yes, 2014
The International Network of Nuclear Reaction Data Centres (NRDC) provides nuclear reaction data services to users through collection and compilation of experimental nuclear reaction data in the EXFOR database.
V. Semkova   +3 more
semanticscholar   +1 more source

Nuclear structure, nuclear reaction

open access: yes, 1982
In this thesis, particle- particle angular correlations for reactions in non-zero degree geometry and with non-zero spin nuclei are performed and found to be a valuable tool for spin determination, (d-α) angular correlations in the reaction process 14N(6Li,d)18F* (α)14N are measured for three high excited states in 18F with a 6Li beam of 36MeV.
Etchegoyen, M   +1 more
openaire   +2 more sources

Nuclear Reactions in Stars [PDF]

open access: yesAnnual Review of Nuclear and Particle Science, 1986
For nearly seventy years (essentially since nuclear physics began as discipline) we have suspected that stellar energy generation, stellar evolution, and the synthesis of the elements and isotopes are all intimately related to the occurrence of nuclear reactions in stars.
openaire   +3 more sources

Introduction to Nuclear-Reaction Theory [PDF]

open access: yes, 2019
These notes summarise the lectures I gave during the summer school "International Scientific Meeting on Nuclear Physics" at La R bida in Spain in June 2018. They offer an introduction to nuclear-reaction theory, starting with the basics in quantum scattering theory followed by the main models used to describe breakup reactions: the Continuum ...
Pierre Capel, Pierre Capel
openaire   +3 more sources

Nuclear reaction rates in a plasma [PDF]

open access: yesReviews of Modern Physics, 1997
The problem of determining the effects of the surrounding plasma on nuclear reaction rates in stars is formulated ab initio, using the techniques of quantum statistical mechanics. We derive a result that expresses the complete effects of Coulomb barrier penetration and of the influence of the surrounding plasma in terms of matrix elements of well ...
R. F. Sawyer, Lowell S. Brown
openaire   +3 more sources

Scattering cross section for various potential systems

open access: yesNuclear Engineering and Technology, 2017
We discuss the problems of scattering in this framework, and show that the applied method is very useful in the investigation of the effect of the resonance in the observed scattering cross sections.
Myagmarjav Odsuren   +3 more
doaj   +1 more source

Improved predictions of nuclear reaction rates with the TALYS reaction code for astrophysical applications [PDF]

open access: yes, 2008
Nuclear reaction rates of astrophysical applications are traditionally determined on the basis of Hauser-Feshbach reaction codes. These codes adopt a number of approximations that have never been tested, such as a simplified width fluctuation correction,
S. Goriely, S. Hilaire, A. Koning
semanticscholar   +1 more source

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