Study of $^{113}$In($α,α$) elastic scattering to determine $α$-optical potential relevant for astrophysical $γ$-process

Fuente: arXiv
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Autori principali: Basak, Dipali, Bar, Tanmoy, Sahoo, Lalit Kumar, Saha, Sukhendu, Rana, T. K., Manna, S., Bhattacharya, C., Kundu, Samir, Sahoo, J. K., Meena, J. K., Saha, A. K., Mondal, Ashok Kumar, Basu, Chinmay
Natura: Preprint
Pubblicazione: 2024
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author Basak, Dipali
Bar, Tanmoy
Sahoo, Lalit Kumar
Saha, Sukhendu
Rana, T. K.
Manna, S.
Bhattacharya, C.
Kundu, Samir
Sahoo, J. K.
Meena, J. K.
Saha, A. K.
Mondal, Ashok Kumar
Basu, Chinmay
author_facet Basak, Dipali
Bar, Tanmoy
Sahoo, Lalit Kumar
Saha, Sukhendu
Rana, T. K.
Manna, S.
Bhattacharya, C.
Kundu, Samir
Sahoo, J. K.
Meena, J. K.
Saha, A. K.
Mondal, Ashok Kumar
Basu, Chinmay
contents The $α$-optical potential is one of the key input parameters used to measure the reaction rate of the ($γ,α$)-process using the Hauser-Feshbach(HF) statistical model and the principle of detailed balance. $α$-elastic scattering experiment on $^{113}$In $p$-nucleus was carried out in the energy range E$_{lab}$=26$-$32 MeV. The vacuum evaporation technique was used to prepare the $^{113}$In target~($\sim$86 $μ$g/cm$^2$). An energy-dependent local optical potential parameters set was obtained by analysing the experimental elastic scattering angular distribution data. The local potential parameters are extrapolated for lower energies and are used to measure the $^{113}$In($α,γ$) reaction cross-section.
format Preprint
id arxiv_https___arxiv_org_abs_2401_07554
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Study of $^{113}$In($α,α$) elastic scattering to determine $α$-optical potential relevant for astrophysical $γ$-process
Basak, Dipali
Bar, Tanmoy
Sahoo, Lalit Kumar
Saha, Sukhendu
Rana, T. K.
Manna, S.
Bhattacharya, C.
Kundu, Samir
Sahoo, J. K.
Meena, J. K.
Saha, A. K.
Mondal, Ashok Kumar
Basu, Chinmay
Nuclear Experiment
Solar and Stellar Astrophysics
The $α$-optical potential is one of the key input parameters used to measure the reaction rate of the ($γ,α$)-process using the Hauser-Feshbach(HF) statistical model and the principle of detailed balance. $α$-elastic scattering experiment on $^{113}$In $p$-nucleus was carried out in the energy range E$_{lab}$=26$-$32 MeV. The vacuum evaporation technique was used to prepare the $^{113}$In target~($\sim$86 $μ$g/cm$^2$). An energy-dependent local optical potential parameters set was obtained by analysing the experimental elastic scattering angular distribution data. The local potential parameters are extrapolated for lower energies and are used to measure the $^{113}$In($α,γ$) reaction cross-section.
title Study of $^{113}$In($α,α$) elastic scattering to determine $α$-optical potential relevant for astrophysical $γ$-process
topic Nuclear Experiment
Solar and Stellar Astrophysics
url https://arxiv.org/abs/2401.07554