T.K. Rana , Deepak Pandit , S. Manna , Samir Kundu , K. Banerjee , A. Sen , R. Pandey , G. Mukherjee , T.K. Ghosh , S.S. Nayak , R. Shil , P. Karmakar , K. Atreya , K. Rani , D. Paul , R. Santra , A. Sultana , S. Basu , S. Pal , S. Sadhukhan , C. Bhattacharya
{"title":"Measurement of radiative decay width of the Hoyle state of 12C via 12C(p, p′)12C reaction","authors":"T.K. Rana , Deepak Pandit , S. Manna , Samir Kundu , K. Banerjee , A. Sen , R. Pandey , G. Mukherjee , T.K. Ghosh , S.S. Nayak , R. Shil , P. Karmakar , K. Atreya , K. Rani , D. Paul , R. Santra , A. Sultana , S. Basu , S. Pal , S. Sadhukhan , C. Bhattacharya","doi":"10.1016/j.nuclphysa.2025.123133","DOIUrl":null,"url":null,"abstract":"<div><div>The Hoyle state, the second excited state of <sup>12</sup>C at an excitation energy of 7.65 MeV, plays a vital role in nucleosynthesis. Its radiative decay width serves as a crucial channel for the formation of <sup>12</sup>C and all heavier elements in the Universe. To investigate this, exclusive experiments were conducted to measure the radiative decay width of the Hoyle state via the <sup>12</sup>C(p, p′)<sup>12</sup>C reaction. The radiative decay branching ratio <span><math><msub><mrow><mi>Γ</mi></mrow><mrow><mi>r</mi><mi>a</mi><mi>d</mi></mrow></msub></math></span>/Γ was determined to be 4.03(21) × 10<sup>−4</sup>. Based on the currently accepted values of <span><math><msub><mrow><mi>Γ</mi></mrow><mrow><mi>π</mi></mrow></msub><mo>(</mo><mi>E</mi><mn>0</mn><mo>)</mo><mo>/</mo><mi>Γ</mi></math></span> and <span><math><msub><mrow><mi>Γ</mi></mrow><mrow><mi>π</mi></mrow></msub><mo>(</mo><mi>E</mi><mn>0</mn><mo>)</mo></math></span>, the radiative width of the Hoyle state was calculated as 3.75(40) × 10<sup>−3</sup> eV.</div></div>","PeriodicalId":19246,"journal":{"name":"Nuclear Physics A","volume":"1060 ","pages":"Article 123133"},"PeriodicalIF":1.7000,"publicationDate":"2025-04-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear Physics A","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0375947425001198","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, NUCLEAR","Score":null,"Total":0}
引用次数: 0
Abstract
The Hoyle state, the second excited state of 12C at an excitation energy of 7.65 MeV, plays a vital role in nucleosynthesis. Its radiative decay width serves as a crucial channel for the formation of 12C and all heavier elements in the Universe. To investigate this, exclusive experiments were conducted to measure the radiative decay width of the Hoyle state via the 12C(p, p′)12C reaction. The radiative decay branching ratio /Γ was determined to be 4.03(21) × 10−4. Based on the currently accepted values of and , the radiative width of the Hoyle state was calculated as 3.75(40) × 10−3 eV.
期刊介绍:
Nuclear Physics A focuses on the domain of nuclear and hadronic physics and includes the following subsections: Nuclear Structure and Dynamics; Intermediate and High Energy Heavy Ion Physics; Hadronic Physics; Electromagnetic and Weak Interactions; Nuclear Astrophysics. The emphasis is on original research papers. A number of carefully selected and reviewed conference proceedings are published as an integral part of the journal.