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View article: GRB 250702B: discovery of a gamma-ray burst from a black hole falling into a star
GRB 250702B: discovery of a gamma-ray burst from a black hole falling into a star Open
Gamma-ray bursts are the most luminous electromagnetic events in the Universe. Their prompt gamma-ray emission has typical durations between a fraction of a second and several minutes. A rare subset of these events have durations in excess…
View article: GRB 250702B: Discovery of a Gamma-Ray Burst from a Black Hole Falling into a Star
GRB 250702B: Discovery of a Gamma-Ray Burst from a Black Hole Falling into a Star Open
Gamma-ray bursts are the most luminous electromagnetic events in the universe. Their prompt gamma-ray emission has typical durations between a fraction of a second and several minutes. A rare subset of these events have durations in excess…
View article: First Measurement of a Weak <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>r</mml:mi></mml:math>-Process Reaction on a Radioactive Nucleus
First Measurement of a Weak -Process Reaction on a Radioactive Nucleus Open
This Letter reports on the first cross-section measurements for the ^{94}Sr(α,n)^{97}Zr and ^{86}Kr(α,n)^{89}Sr reactions. In particular, our measurement of ^{94}Sr(α,n)^{97}Zr is the first weak r-process reaction cross section obtained us…
View article: <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mmultiscripts><mml:mi>Ne</mml:mi><mml:mprescripts/><mml:none/><mml:mn>21</mml:mn></mml:mmultiscripts></mml:math> energy levels approaching the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>α</mml:mi></mml:math>-particle threshold
energy levels approaching the -particle threshold Open
Nuclei around Ne20 exhibit an interplay of different excitations caused by different aspects of nuclear structure, including single-particle and multiparticle configurations and collective rotations. One-nucleon transfer reactions selectiv…
View article: Measurement of the <sup>86</sup>Kr(α,n)<sup>89</sup>Sr cross section at energies relevant for the weak r-process
Measurement of the <sup>86</sup>Kr(α,n)<sup>89</sup>Sr cross section at energies relevant for the weak r-process Open
The r-process has been shown to be robust in reproducing the abundance distributions of heavy elements, such as europium, seen in ultra-metal poor stars. In contrast, observations of elements 26 < Z < 47 display overabundances relative to …
View article: Evolution of Accreting Neutron Star Common Envelopes and Their Nucleosynthesis Possible P-nuclide Production
Evolution of Accreting Neutron Star Common Envelopes and Their Nucleosynthesis Possible P-nuclide Production Open
In a binary system, a short lived phase called a common envelope can occur in which both stars share the envelope of the primary. During this phase, there is the opportunity for nucleosynthesis to occur at high temperatures and densities i…
View article: The impact of 17O + α reaction rate uncertainties on the s-process in rotating massive stars
The impact of 17O + α reaction rate uncertainties on the s-process in rotating massive stars Open
Massive stars are crucial to galactic chemical evolution for elements heavier than iron. Their contribution at early times in the evolution of the Universe, however, is unclear due to poorly constrained nuclear reaction rates. The competin…
View article: New Experimental <sup>23</sup>Na(α, p)<sup>26</sup>Mg Reaction Rate for Massive Star and Type Ia Supernova Models
New Experimental <sup>23</sup>Na(α, p)<sup>26</sup>Mg Reaction Rate for Massive Star and Type Ia Supernova Models Open
The 23 Na( α , p ) 26 Mg reaction has been identified as having a significant impact on the nucleosynthesis of several nuclei between Ne and Ti in Type Ia supernovae, and of 23 Na and 26 Al in massive stars. The reaction has been subjected…
View article: The MUGAST-AGATA-VAMOS campaign : set-up and performance
The MUGAST-AGATA-VAMOS campaign : set-up and performance Open
The MUGAST-AGATA-VAMOS set-up at GANIL combines the MUGAST highly-segmented silicon array with the state-of-the-art AGATA array and the large acceptance VAMOS spectrometer. The mechanical and electronics integration copes with the constrai…
View article: From nuclei to neutron stars: simple binding energy computer modelling in the classroom (part 1)
From nuclei to neutron stars: simple binding energy computer modelling in the classroom (part 1) Open
We present a simple activity based on the liquid-drop model which allows secondary school students to explore the uses of mathematical models and gain an intuitive understanding of the concept of binding energy, and in particular the signi…
View article: An implantation Diamond detector as a beam monitor for an intense radioactive ion beam
An implantation Diamond detector as a beam monitor for an intense radioactive ion beam Open
We present the characterization of a Diamond detector and its response as a beam rate monitor with full stopping of radioactive ion beams of high intensity. The detector has been implemented in the VAMOS focal plane at GANIL and utilised i…
View article: Single-particle structure in neutron-rich Sr isotopes approaching the N = 60 shape transition
Single-particle structure in neutron-rich Sr isotopes approaching the N = 60 shape transition Open
Background: Neutron-rich nuclei around neutron number N = 60 show a dramatic shape transition from spherical ground states to prolate deformation in 98Sr and heavier nuclei. Purpose: The purpose of this study is to investigate the single-p…
View article: Single-Particle Structure of Neutron-Rich Sr Isotopes Via d( 94,95,96 Sr, p) Reactions
Single-Particle Structure of Neutron-Rich Sr Isotopes Via d( 94,95,96 Sr, p) Reactions Open
The region around neutron number N = 60 in the neutron-rich Sr and Zr nuclei is one of the most dramatic examples of a ground state shape transition from (near) spherical below N = 60 to strongly deformed shapes in the heavier isotopes. Th…
View article: Nucleosynthetic yields from neutron stars accreting in binary common envelopes
Nucleosynthetic yields from neutron stars accreting in binary common envelopes Open
Massive-star binaries can undergo a phase where one of the two stars expands during its advanced evolutionary stage as a giant and envelops its companion, ejecting the hydrogen envelope and tightening its orbit. Such a common envelope phas…
View article: Isospin-symmetry breaking corrections for the description of triplet energy differences
Isospin-symmetry breaking corrections for the description of triplet energy differences Open
The charge-independence breaking of the nuclear interaction is analyzed by means of energy differences
\namong analog states in T=1 isobaric multiplets. Data on triplet energy differences in the sd, pf, and pf5/2g shells, i.e., 18<A<66, ar…
View article: Rotational excitation of the Hoyle state in <sup>12</sup>C
Rotational excitation of the Hoyle state in <sup>12</sup>C Open
International audience
View article: A new statistical method for the structure of the inner crust of neutron stars
A new statistical method for the structure of the inner crust of neutron stars Open
We investigated the structure of the low density regions of the inner crust\nof neutron stars using the Hartree-Fock-Bogoliubov (HFB) model to predict the\nproton content $Z$ of the nuclear clusters and, together with the lattice\nspacing,…
View article: Search for highly excited states in <sup>28</sup>Si
Search for highly excited states in <sup>28</sup>Si Open
CITATION: Montanari, D., et al. 2017. Search for highly excited states in ²⁸Si. Journal of Physics: Conference Series, 863(1):012051, doi:10.1088/1742-6596/863/1/012051.
View article: CAKE: the coincidence array for K600 experiments
CAKE: the coincidence array for K600 experiments Open
The combination of a magnetic spectrometer and ancillary detectors such as silicon detectors is a powerful tool for the study of nuclear reactions and nuclear structure. This paper discusses the recently commissioned silicon array called t…
View article: Isospin Symmetry at High Spin Studied via Nucleon Knockout from Isomeric States
Isospin Symmetry at High Spin Studied via Nucleon Knockout from Isomeric States Open
One-neutron knockout reactions have been performed on a beam of radioactive ^{53}Co in a high-spin isomeric state. The analysis is shown to yield a highly selective population of high-spin states in an exotic nucleus with a significant cro…
View article: Shell evolution approaching the N= 20 island of inversion: Structure of 26Na
Shell evolution approaching the N= 20 island of inversion: Structure of 26Na Open
The levels in 26Na with single particle character have been observed for the first time using the d(25Na, pγ ) reaction at 5 MeV/nucleon. The measured excitation energies and the deduced spectroscopic factors are in good overall agreement …
View article: A Study Of 23Na And 12C
A Study Of 23Na And 12C Open
Progress report for first part of Ph.D. studies. Describes my work on the DAQ for Aarhus 5MV accelerator. A newly developed analysis and simulation library for small scale DSSD experiments. Futhermore, an experimental study of 23Na(a,p) an…
View article: Study of the<sup>26</sup>Al(n,p)<sup>26</sup>Mg and<sup>26</sup>Al(n,α)<sup>23</sup>Na reactions using the<sup>27</sup>Al(p,p')<sup>27</sup>Al inelastic scattering reaction
Study of the<sup>26</sup>Al(n,p)<sup>26</sup>Mg and<sup>26</sup>Al(n,α)<sup>23</sup>Na reactions using the<sup>27</sup>Al(p,p')<sup>27</sup>Al inelastic scattering reaction Open
26Al was the first cosmic radioactivity ever detected in the galaxy as well as one
\nof the first extinct radioactivity observed in refractory phases of meteorites. Its nucleosynthesis
\nin massive stars is still uncertain mainly due to th…