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17:00
$S$ matrices of elastic $\alpha$-$^{12}$C scattering at low energies in cluster effective field theory
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Shung-Ichi ANDO
(Sunmoon University)
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17:05
Analytic expression of triple-$\alpha$ reaction rates by a non-adiabatic three-body model
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Masahiko KATSUMA
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17:10
A new Multi-Channel and Monte Carlo R-Matrix analysis for the estimate of $\rm ^{17}$O destruction rate in stars
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Andreas BEST
(University of Naples "Federico II")
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17:15
Understanding the S- and C-type Giant Stars in the Milky Way
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Yoshiya MORI
(Monash University)
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17:20
Astrophysical S factor of $^{15}\mathrm{N}(p, \gamma)^{16}\mathrm{O}$ in the cluster effective field theory
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Sangyeong SON
(Kyungpook National University)
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17:25
The first direct measurement of the $65\,keV$ resonance strength of the $^{17}\mathrm{O}(p,\gamma)^{18}\mathrm{F}$ reaction at LUNA
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Riccardo Maria GESUÈ
(Gran Sasso Science Institute)
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17:30
First study of the $^{139}$Ba(n,γ)$^{140}$Ba reaction to constrain the conditions for the astrophysical i process
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Dennis MUECHER
(University of Cologne)
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17:35
Constraining neutron-capture cross section for the i-process for the 151−153Nd(n,γ)152−154Nd reaction via the β Oslo
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Hannah BERG
(Michigan State University)
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17:40
Experimental integral cross-sections of photonuclear reactions on proton-rich $^{113}In$ and $^{114}Sn$ nuclei for cosmic nucleosynthesis modelling
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Anastasiia CHEKHOVSKA
(Institute of Solid State Physics, University of Latvia)
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17:50
Impact of the excited- and bound-state $\beta$-decays of $^{63}$Ni on weak $\textit{s}$-process nucleosynthesis [1]
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Xinxu WANG
(Beihang University, China)
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17:55
Neutron capture and total cross-section measurements on 94,95,96Mo at n_TOF and GELINA
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Riccardo MUCCIOLA
(University and INFN Torino)
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18:00
Estimation of fission from proton-induced uranium-238 using the Langevin method
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Chang-hoon SONG
(Pusan National University)
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18:05
Measurement of the 159Tb(n, γ) cross section at the CSNS Back-n facility
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Suyalatu ZHANG
(Inner Mongolia Minzu University)
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18:10
Production of solar abundances for nuclei beyond Sr: do we need better nuclear physics input?
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Sara PALMERINI
(University of Perugia and INFN Perugia, Italy)
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18:15
Measurement of the 27Al(p,alpha)24Mg fusion reaction at astrophysical energies via the Trojan Horse Method.
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Sara PALMERINI
(University of Perugia and INFN Perugia, Italy)
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18:20
The impact of systematic and statistical nuclear uncertainties on the i-process nucleosynthesis
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Sébastien MARTINET
(Université Libre de Bruxelles)
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18:25
Massive star models with the updated 12C+12C reaction rate
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Gwangeon SEONG
(UNIST)
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18:30
The COREA experiment: measurement of 12C(α,𝛄)16O reactions with an active-target TPC
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Shin Hyung KIM
(Korea University)