2022
DOI: 10.1016/j.ppnp.2021.103903
|View full text |Cite|
|
Sign up to set email alerts
|

Photonuclear reactions—From basic research to applications

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
25
0

Year Published

2022
2022
2023
2023

Publication Types

Select...
4
3
1

Relationship

1
7

Authors

Journals

citations
Cited by 88 publications
(31 citation statements)
references
References 500 publications
0
25
0
Order By: Relevance
“…For details of the NRF formalism and methodology see Ref. [1]. Above the particle threshold, states in the continuum are excited.…”
Section: Nuclear Structure Studies At Extremely High Nuclear Temperat...mentioning
confidence: 99%
See 2 more Smart Citations
“…For details of the NRF formalism and methodology see Ref. [1]. Above the particle threshold, states in the continuum are excited.…”
Section: Nuclear Structure Studies At Extremely High Nuclear Temperat...mentioning
confidence: 99%
“…The experimental techniques, the observables and the quantities, which are deduced in these experiments, were reviewed in Ref. [1]. The expected increase of the of the spectral density of the γ beams at ELI-NP with about two orders of magnitude will bring the experimental techniques to a new level of sensitivity.…”
Section: Studies Of Photonuclear Reactions At Eli-npmentioning
confidence: 99%
See 1 more Smart Citation
“…Nuclear Resonance Fluorescence (NRF) measurements [2,3,4] provide insight into several nuclear observables related to the transition strengths. In NRF the measured quantity is related both to the excitation and the de-excitation process of the nucleus.…”
Section: Introductionmentioning
confidence: 99%
“…Such a competition between photo-proton σ(γ, p) and photo-neutron σ(γ, n) cross sections impacts a variety of nuclear and astrophysics phenomena -namely, bremsstrahlung [3,4], nuclear polarizability [5], threenucleon forces [6], collective properties [7], isospin asymmetry and symmetry energy in neutron stars [8][9][10][11], neon and silicon burning at the end of stellar evolution [12] and the nucleosynthesis of p-nuclei [13,14], which are shielded from the rapid-neutron capture by stable isobars. A recent review article by Zilges and co-workers discusses in detail various applications of photonuclear physics [15], e.g. finding new routes for production of medical radioisotopes or nuclear-waste transmutation.…”
mentioning
confidence: 99%