{"title":"Half-life measurement of short-lived nuclide 146Eu","authors":"Changxin Guo, Yunju Li, Shengquan Yan, Minghao Zhu, Youbao Wang, Yuqiang Zhang, Jinlong Ma, Wei Nan, Tao Tian, Jianglin Hou, Jiayinhao Li","doi":"10.1016/j.nuclphysa.2025.123113","DOIUrl":"10.1016/j.nuclphysa.2025.123113","url":null,"abstract":"<div><div><sup>146</sup>Sm is an important nuclide for both geochronological and astrophysical applications, its precise half-life value is essential for accurate geological applications. Nevertheless, significant discrepancies exist in the measured half-life values of <sup>146</sup>Sm. A new experimental method has been proposed by merely measuring the total amount of <sup>146</sup>Eu and the decay of <sup>146</sup>Sm, corresponding <em>α</em> and <em>γ</em> spectrometers have been developed for the measurement. The preliminary experiment has been carried out in HI-13 tandem accelerator of China Institute of Atomic Energy. Based on <em>α</em> and <em>γ</em> measurements, the half-life of <sup>147</sup>Eu has been double checked and the results agree well with existing values, which gives a verification for the reliability of our half-life measurement systems. The half-life of <sup>146</sup>Eu has been updated to <span><math><mn>4.21</mn><mo>±</mo><mn>0.05</mn></math></span> days, which is 9% lower than the value reported in the database. Based on our analysis, this difference has a significant impact on the determination of the number of <sup>146</sup>Eu atoms, and consequently has an equivalent impact on the measurement of <sup>146</sup>Sm half-life.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123113"},"PeriodicalIF":1.7,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143860488","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-16DOI: 10.1016/j.nuclphysa.2025.123110
J. Koros , A. Simon , J.T. Harke , R.O. Hughes , P. Adsley , B.H. Isselhardt , B. Longfellow , M. Matney , C.S. Reingold
{"title":"Constraining (n,γ) cross sections via surrogate measurements with hyperion","authors":"J. Koros , A. Simon , J.T. Harke , R.O. Hughes , P. Adsley , B.H. Isselhardt , B. Longfellow , M. Matney , C.S. Reingold","doi":"10.1016/j.nuclphysa.2025.123110","DOIUrl":"10.1016/j.nuclphysa.2025.123110","url":null,"abstract":"<div><div>Indirect measurement techniques, such as the surrogate method, are necessary to constrain cross sections and reaction rates that are inaccessible for direct measurement. The surrogate method uses an alternate reaction channel to populate a nucleus of interest, and combines resulting experimental data with theory to constrain the desired (n,<em>γ</em>) cross section. Individual <em>γ</em>-decay probabilities are experimentally extracted using <em>γ</em>-ray spectroscopy. This project utilizes surrogate analysis of <sup>64,70</sup>Zn(p,d) and <sup>64,70</sup>Zn(p,t) reactions measured with the Hyperion array at Texas A&M University's Cyclotron Facility to probe the relevant neutron capture reactions <sup>61,62,67,68</sup>Zn(n,<em>γ</em>). As an example, preliminary <em>γ</em>-decay probabilities are presented for <sup>69</sup>Zn.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123110"},"PeriodicalIF":1.7,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143868924","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-16DOI: 10.1016/j.nuclphysa.2025.123111
Weihua Yang , Chao Li
{"title":"The nuclear matter effect on parton distribution functions","authors":"Weihua Yang , Chao Li","doi":"10.1016/j.nuclphysa.2025.123111","DOIUrl":"10.1016/j.nuclphysa.2025.123111","url":null,"abstract":"<div><div>Parton distribution functions (PDFs) are important quantities in describing nucleon structures. They are universal and process-independent. As a matter of fact, nucleon PDFs are inevitably affected by nuclear matter during nuclear scattering process. In order to study the nuclear PDFs (nPDFs), in this paper, we introduce the nucleon pair PDFs (dPDFs) to describe parton distributions in the nucleon pair which is confined to a nucleus. We first of all construct the nuclear state in terms of the nucleonic states and calculate the operator definition of nPDFs. Neglecting the higher order corrections or multi-nucleon correlations, we find that nPDFs can be written as a sum of two terms which respectively correspond to PDFs and dPDFs. Nucleon pair PDFs which stem from nucleon-nucleon correlation are proportional to common nucleon PDFs but suppressed by a factor. Compared with the experimental data, we find that dPDFs can explain the behaviour of the EMC effect. We further calculate the Paschos-Wolfenstein ratio to study the nuclear matter effect on the extraction of weak mixing angle or <span><math><msup><mrow><mi>sin</mi></mrow><mrow><mn>2</mn></mrow></msup><mo></mo><msub><mrow><mi>θ</mi></mrow><mrow><mi>W</mi></mrow></msub></math></span> by using dPDFs.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123111"},"PeriodicalIF":1.7,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143842752","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-16DOI: 10.1016/j.nuclphysa.2025.123112
Weiping Liu , JUNA Collaboration
{"title":"Progress of underground nuclear astrophysics JUNA","authors":"Weiping Liu , JUNA Collaboration","doi":"10.1016/j.nuclphysa.2025.123112","DOIUrl":"10.1016/j.nuclphysa.2025.123112","url":null,"abstract":"<div><div>The Jinping Underground experiment for Nuclear Astrophysics (JUNA) takes advantage of the ultra-low background of the CJPL to conduct experiments for directly studying crucial reactions at stellar energies in the evolution of stars. In 2020, JUNA commissioned a mA level high current accelerator based on an ECR source, as well as high efficiency BGO and <sup>3</sup>He detectors. Direct measurements of key nuclear reactions, including <span><math><mmultiscripts><mrow><mi>Mg</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>25</mn></mrow></mmultiscripts><msup><mrow><mo>(</mo><mi>p</mi><mo>,</mo><mi>γ</mi><mo>)</mo></mrow><mrow><mn>26</mn></mrow></msup><mrow><mi>Al</mi></mrow></math></span>, <span><math><mmultiscripts><mrow><mi>F</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>19</mn></mrow></mmultiscripts><msup><mrow><mo>(</mo><mi>p</mi><mo>,</mo><mi>α</mi><mi>γ</mi><mo>)</mo></mrow><mrow><mn>16</mn></mrow></msup><mi>O</mi></math></span>, <span><math><mmultiscripts><mrow><mi>F</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>19</mn></mrow></mmultiscripts><msup><mrow><mo>(</mo><mi>p</mi><mo>,</mo><mi>γ</mi><mo>)</mo></mrow><mrow><mn>20</mn></mrow></msup><mrow><mi>Ne</mi></mrow></math></span>, <span><math><mmultiscripts><mrow><mi>C</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>12</mn></mrow></mmultiscripts><msup><mrow><mo>(</mo><mi>α</mi><mo>,</mo><mi>γ</mi><mo>)</mo></mrow><mrow><mn>16</mn></mrow></msup><mi>O</mi></math></span> and <span><math><mmultiscripts><mrow><mi>O</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>18</mn></mrow></mmultiscripts><msup><mrow><mo>(</mo><mi>α</mi><mo>,</mo><mi>γ</mi><mo>)</mo></mrow><mrow><mn>22</mn></mrow></msup><mrow><mi>Ne</mi></mrow></math></span>, were performed in JUNA with improved precision and closer to the Gamow window relative to previous measurements. These precise reaction rates provide valuable insights into the high precision astrophysics simulation.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123112"},"PeriodicalIF":1.7,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143860489","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-15DOI: 10.1016/j.nuclphysa.2025.123108
Shung-Ichi Ando
{"title":"Radiative α capture on 12C in cluster effective field theory: Short review","authors":"Shung-Ichi Ando","doi":"10.1016/j.nuclphysa.2025.123108","DOIUrl":"10.1016/j.nuclphysa.2025.123108","url":null,"abstract":"<div><div>Study of radiative <em>α</em> capture on <sup>12</sup>C, <sup>12</sup>C(<em>α</em>,<em>γ</em>)<sup>16</sup>O, in cluster effective field theory (EFT) is reviewed. A low energy EFT for <sup>12</sup>C(<em>α</em>,<em>γ</em>)<sup>16</sup>O at the Gamow-peak energy, <span><math><msub><mrow><mi>E</mi></mrow><mrow><mi>G</mi></mrow></msub><mo>=</mo><mn>0.3</mn></math></span> MeV, is constructed, and the theory is first applied to the study of elastic <em>α</em>-<sup>12</sup>C scattering at low energies. The effective range parameters are fitted to the precise phase shift data of the elastic scattering and the astrophysical <span><math><msub><mrow><mi>S</mi></mrow><mrow><mi>E</mi><mn>1</mn></mrow></msub></math></span> factor of the <em>E</em>1 transition of <sup>12</sup>C(<em>α</em>,<em>γ</em>)<sup>16</sup>O at <span><math><msub><mrow><mi>E</mi></mrow><mrow><mi>G</mi></mrow></msub></math></span> is estimated. For the study of the <em>E</em>2 transition of <sup>12</sup>C(<em>α</em>,<em>γ</em>)<sup>16</sup>O, we discuss a difficulty to determine the asymptotic normalization coefficient (ANC) of the subthreshold <span><math><msubsup><mrow><mn>2</mn></mrow><mrow><mn>1</mn></mrow><mrow><mo>+</mo></mrow></msubsup></math></span> state of <sup>16</sup>O from the elastic scattering data, and demonstrate the difficulty with the estimate of the astrophysical <span><math><msub><mrow><mi>S</mi></mrow><mrow><mi>E</mi><mn>2</mn></mrow></msub></math></span> factor of <sup>12</sup>C(<em>α</em>,<em>γ</em>)<sup>16</sup>O at <span><math><msub><mrow><mi>E</mi></mrow><mrow><mi>G</mi></mrow></msub></math></span>. We discuss the uncertainty in the estimate of the <em>S</em> factors at <span><math><msub><mrow><mi>E</mi></mrow><mrow><mi>G</mi></mrow></msub></math></span> in the present approach.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123108"},"PeriodicalIF":1.7,"publicationDate":"2025-04-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143838770","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-15DOI: 10.1016/j.nuclphysa.2025.123109
Chaitanya Anil Bokade, Bhaghyesh
{"title":"Bc meson masses and decays: Insights from a relativistic screened potential model","authors":"Chaitanya Anil Bokade, Bhaghyesh","doi":"10.1016/j.nuclphysa.2025.123109","DOIUrl":"10.1016/j.nuclphysa.2025.123109","url":null,"abstract":"<div><div>In this study, we undertake a comprehensive analysis of the <span><math><msub><mrow><mi>B</mi></mrow><mrow><mi>c</mi></mrow></msub></math></span> meson mass spectrum and decay properties using a relativistic screened potential model. We evaluate the spectra of <span><math><mi>S</mi><mo>,</mo><mi>P</mi><mo>,</mo><mi>D</mi></math></span> and <em>G</em> wave states, along with the decay constants, <em>E</em>1 and <em>M</em>1 transitions, leptonic and radiative leptonic decays. The magnetic moments for various <span><math><msub><mrow><mi>B</mi></mrow><mrow><mi>c</mi></mrow></msub></math></span> states are also calculated. The results are compared with available experimental data and with results from other theoretical models.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123109"},"PeriodicalIF":1.7,"publicationDate":"2025-04-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143842753","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-15DOI: 10.1016/j.nuclphysa.2025.123105
F. Wu (吴桐安) , C. Andreoiu , V. Karayonchev , C.M. Petrache , J.-M. Régis , A. Esmaylzadeh , C. Michelagnoli , M. Beuschlein , P. Spagnoletti , G. Colombi , J.M. Daugas , L. Domenichetti , P.E. Garrett , J. Jolie , M. Ley , S. Pannu , E. Taddei , M. von Tresckow
{"title":"Towards lifetime measurement of excited states in 120Sn using thermal neutron capture","authors":"F. Wu (吴桐安) , C. Andreoiu , V. Karayonchev , C.M. Petrache , J.-M. Régis , A. Esmaylzadeh , C. Michelagnoli , M. Beuschlein , P. Spagnoletti , G. Colombi , J.M. Daugas , L. Domenichetti , P.E. Garrett , J. Jolie , M. Ley , S. Pannu , E. Taddei , M. von Tresckow","doi":"10.1016/j.nuclphysa.2025.123105","DOIUrl":"10.1016/j.nuclphysa.2025.123105","url":null,"abstract":"<div><div>The intruder bands in Sn isotopes, based on the 2p-2h excitation across the <span><math><mi>Z</mi><mo>=</mo><mn>50</mn></math></span> proton shell gap, are well-known to exhibit shape coexistence near the neutron mid-shell region. The spectroscopic signatures are enhanced <em>E</em>0 transitions between the <span><math><msup><mrow><mn>0</mn></mrow><mrow><mo>+</mo></mrow></msup></math></span> band heads and enhanced <em>E</em>2 transitions within rotational bands built on these <span><math><msup><mrow><mn>0</mn></mrow><mrow><mo>+</mo></mrow></msup></math></span> band heads. However, lifetime information for the excited <span><math><msup><mrow><mn>0</mn></mrow><mrow><mo>+</mo></mrow></msup></math></span> states is incomplete. Experimental details for the neutron-capture reaction and analysis procedures are described, and the first result of the <span><math><msubsup><mrow><mn>2</mn></mrow><mrow><mn>1</mn></mrow><mrow><mo>+</mo></mrow></msubsup></math></span> lifetime demonstrates proper calibration of the setup.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123105"},"PeriodicalIF":1.7,"publicationDate":"2025-04-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143838769","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-14DOI: 10.1016/j.nuclphysa.2025.123099
D. Piatti, LUNA collaboration
{"title":"The challenging first direct measurement of the 65 keV resonance strength in the 17O(p,γ)18F reaction at LUNA","authors":"D. Piatti, LUNA collaboration","doi":"10.1016/j.nuclphysa.2025.123099","DOIUrl":"10.1016/j.nuclphysa.2025.123099","url":null,"abstract":"<div><div>A precise determination of the proton capture rates on oxygen is mandatory to predict the abundance ratios of oxygen isotopes in a stellar environment where the hydrogen burning is active. The <sup>17</sup>O(p,<em>γ</em>)<sup>18</sup>F reaction, in particular, plays a crucial role in AGB nucleosynthesis as well as in explosive hydrogen burning occurring in novae and type I supernovae. At the temperature of interest for the former scenario (20 MK ≤ T ≤ 80 MK) the main contribution to the astrophysical reaction rate comes from the <span><math><msub><mrow><mi>E</mi></mrow><mrow><mi>r</mi></mrow></msub></math></span> = 64.5 keV resonance. The strength of this resonance is presently determined only through indirect measurements, with an adopted value <em>ωγ</em> = (1.6 ± 0.3) × 10<sup>−11</sup> eV. A new high sensitivity setup has been installed at LUNA, located at Laboratori Nazionali del Gran Sasso. The underground location of LUNA 400kV guarantees a reduction of the cosmic ray background by several orders of magnitude. The residual background was further reduced by a dedicated shielding. On the other hand the 4<em>π</em>-BGO detector efficiency was optimized installing an aluminum target chamber and holder. With about 400 C accumulated on Ta<sub>2</sub>O<sub>5</sub> targets, with nominal <sup>17</sup>O enrichment of 90%, the LUNA collaboration has performed the first ever direct measurement of the 64.5 keV resonance strength.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123099"},"PeriodicalIF":1.7,"publicationDate":"2025-04-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143860490","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-11DOI: 10.1016/j.nuclphysa.2025.123101
T.K. Rana , Samir Kundu , S. Manna , K. Banerjee , P. Karmakar , T.K. Ghosh , G. Mukherjee , A. Sen , R. Pandey , P. Pant , Pratap Roy , R. Shil , S.S. Nayak , K. Rani , K. Atreya , D. Paul , R. Santra , A. Sultana , S. Pal , S. Basu , M.K. Dey
{"title":"First in-beam experiment in K500 superconducting cyclotron at VECC","authors":"T.K. Rana , Samir Kundu , S. Manna , K. Banerjee , P. Karmakar , T.K. Ghosh , G. Mukherjee , A. Sen , R. Pandey , P. Pant , Pratap Roy , R. Shil , S.S. Nayak , K. Rani , K. Atreya , D. Paul , R. Santra , A. Sultana , S. Pal , S. Basu , M.K. Dey","doi":"10.1016/j.nuclphysa.2025.123101","DOIUrl":"10.1016/j.nuclphysa.2025.123101","url":null,"abstract":"<div><div>Characterization of first beam from <em>K</em>500 cyclotron at VECC, Kolkata, was performed using the elastic scattering experiment with a <sup>197</sup>Au target. Two independent approaches have been used to calibrate the detector system to estimate beam energy and its energy spread. Apart from the beam characterization, the fragment emission mechanism, particularly the isospin equilibrium and isoscaling behaviour, has been studied using <sup>14</sup>N, <sup>16</sup>O and <sup>20</sup>Ne beams from the cyclotron. This article provides details of the beam characterization of the cyclotron and also an overview of the experiments conducted.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123101"},"PeriodicalIF":1.7,"publicationDate":"2025-04-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143838771","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Nuclear Physics APub Date : 2025-04-11DOI: 10.1016/j.nuclphysa.2025.123103
M. Feijoo-Fontán , A. Barrière , N. Mozumdar , H. Álvarez-Pol , J.L. Rodríguez-Sánchez , O. Sorlin , J. Benlliure , D. Cortina-Gil , R3B collaboration
{"title":"Development of a PID algorithm for the CALIFA detector to study multinucleon knockout reactions in exotic nuclei","authors":"M. Feijoo-Fontán , A. Barrière , N. Mozumdar , H. Álvarez-Pol , J.L. Rodríguez-Sánchez , O. Sorlin , J. Benlliure , D. Cortina-Gil , R3B collaboration","doi":"10.1016/j.nuclphysa.2025.123103","DOIUrl":"10.1016/j.nuclphysa.2025.123103","url":null,"abstract":"<div><div>Previous studies have shown a reduction in cross sections relative to theoretical predictions for single-nucleon knockout reactions, with varying conclusions about the dependence of this reduction on the N/Z ratio of the projectile. The (p,pX) knockout reactions studied with the R<sup>3</sup>B setup offer a unique opportunity for kinematically complete measurements using inverse kinematics. This work focuses on the development of an algorithm for performing particle identification using the CALIFA detector, of vital importance for the study of knocked-out clusters such as deuterium.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1059 ","pages":"Article 123103"},"PeriodicalIF":1.7,"publicationDate":"2025-04-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143826094","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}