W.-J. Ong, H. Schatz, K. Kravvaris, S. Ahn, K. Childers, B. P. Crider, A. C. Dombos, C. Langer, R. Lewis, S. N. Liddick, S. Lyons, Z. Meisel, F. Montes, J. Pereira, D. Richman, K. Schmidt, A. Spyrou
{"title":"Mn64、Cr62 和 Fe65 的 β 延迟中子发射","authors":"W.-J. Ong, H. Schatz, K. Kravvaris, S. Ahn, K. Childers, B. P. Crider, A. C. Dombos, C. Langer, R. Lewis, S. N. Liddick, S. Lyons, Z. Meisel, F. Montes, J. Pereira, D. Richman, K. Schmidt, A. Spyrou","doi":"10.1103/physrevc.110.024321","DOIUrl":null,"url":null,"abstract":"The <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>β</mi></math>-decay properties of nuclei near the second nuclear “island of inversion” around neutron rich nuclei with neutron number 40 are important tests of nuclear structure models and interactions. In particular, the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>β</mi></math>-delayed neutron emission branch (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>P</mi><mi mathvariant=\"normal\">n</mi></msub></math>), is useful for investigating <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>β</mi></math>-strength and neutron-<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>γ</mi></math> competition above the neutron separation energies of the daughter nuclei. We report new constraints for <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><msub><mi>P</mi><mi mathvariant=\"normal\">n</mi></msub></math> values for three nuclei in the region: <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><msub><mi>P</mi><mi mathvariant=\"normal\">n</mi></msub><mo><</mo><mn>1</mn><mo>%</mo></mrow></math>), <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>64</mn></mmultiscripts></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><msub><mi>P</mi><mi mathvariant=\"normal\">n</mi></msub><mo>=</mo><mn>1.5</mn><mrow><mo>(</mo><mn>6</mn><mo>)</mo></mrow><mo>%</mo></mrow></math>), and <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Fe</mi><mprescripts></mprescripts><none></none><mn>65</mn></mmultiscripts></math> (<math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><msub><mi>P</mi><mi mathvariant=\"normal\">n</mi></msub><mo><</mo><mn>1</mn><mo>%</mo></mrow></math>), measured with the Neutron Emission Ratio Observer (NERO) neutron long counter system and the Beta Counting Station (BCS) at the National Superconducting Cyclotron Laboratory (NSCL). Our results resolve the large discrepancy between previous direct and indirect measurements for <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>64</mn></mmultiscripts></math> and confirm the predictions of global theoretical models when a statistical treatment of the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>γ</mi></math> and neutron decays of the daughter states is included. We also obtain improved half-lives for <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> [206(5) ms] and the short-lived isomer in the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Fe</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> daughter [112(7) ms] from <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>β</mi></math>-delayed <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>γ</mi></math> emission data obtained in the same experiment with the Summing NaI (SuN) total absorption spectrometer. Finally, we use <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mi>γ</mi></math> emission data to obtain a new upper limit for the <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mrow><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts><mspace width=\"0.16em\"></mspace><mi>β</mi></mrow></math>-decay population of the long-lived isomeric state in <math xmlns=\"http://www.w3.org/1998/Math/MathML\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math>.","PeriodicalId":20122,"journal":{"name":"Physical Review C","volume":"7 1","pages":""},"PeriodicalIF":3.1000,"publicationDate":"2024-08-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"β-delayed neutron emission of Mn64, Cr62, and Fe65\",\"authors\":\"W.-J. Ong, H. Schatz, K. Kravvaris, S. Ahn, K. Childers, B. P. Crider, A. C. Dombos, C. Langer, R. Lewis, S. N. Liddick, S. Lyons, Z. Meisel, F. Montes, J. Pereira, D. Richman, K. Schmidt, A. Spyrou\",\"doi\":\"10.1103/physrevc.110.024321\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>β</mi></math>-decay properties of nuclei near the second nuclear “island of inversion” around neutron rich nuclei with neutron number 40 are important tests of nuclear structure models and interactions. In particular, the <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>β</mi></math>-delayed neutron emission branch (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>P</mi><mi mathvariant=\\\"normal\\\">n</mi></msub></math>), is useful for investigating <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>β</mi></math>-strength and neutron-<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>γ</mi></math> competition above the neutron separation energies of the daughter nuclei. We report new constraints for <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><msub><mi>P</mi><mi mathvariant=\\\"normal\\\">n</mi></msub></math> values for three nuclei in the region: <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><msub><mi>P</mi><mi mathvariant=\\\"normal\\\">n</mi></msub><mo><</mo><mn>1</mn><mo>%</mo></mrow></math>), <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>64</mn></mmultiscripts></math> (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><msub><mi>P</mi><mi mathvariant=\\\"normal\\\">n</mi></msub><mo>=</mo><mn>1.5</mn><mrow><mo>(</mo><mn>6</mn><mo>)</mo></mrow><mo>%</mo></mrow></math>), and <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Fe</mi><mprescripts></mprescripts><none></none><mn>65</mn></mmultiscripts></math> (<math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><msub><mi>P</mi><mi mathvariant=\\\"normal\\\">n</mi></msub><mo><</mo><mn>1</mn><mo>%</mo></mrow></math>), measured with the Neutron Emission Ratio Observer (NERO) neutron long counter system and the Beta Counting Station (BCS) at the National Superconducting Cyclotron Laboratory (NSCL). Our results resolve the large discrepancy between previous direct and indirect measurements for <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>64</mn></mmultiscripts></math> and confirm the predictions of global theoretical models when a statistical treatment of the <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>γ</mi></math> and neutron decays of the daughter states is included. We also obtain improved half-lives for <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> [206(5) ms] and the short-lived isomer in the <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Fe</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math> daughter [112(7) ms] from <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>β</mi></math>-delayed <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>γ</mi></math> emission data obtained in the same experiment with the Summing NaI (SuN) total absorption spectrometer. Finally, we use <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mi>γ</mi></math> emission data to obtain a new upper limit for the <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mrow><mmultiscripts><mi>Cr</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts><mspace width=\\\"0.16em\\\"></mspace><mi>β</mi></mrow></math>-decay population of the long-lived isomeric state in <math xmlns=\\\"http://www.w3.org/1998/Math/MathML\\\"><mmultiscripts><mi>Mn</mi><mprescripts></mprescripts><none></none><mn>62</mn></mmultiscripts></math>.\",\"PeriodicalId\":20122,\"journal\":{\"name\":\"Physical Review C\",\"volume\":\"7 1\",\"pages\":\"\"},\"PeriodicalIF\":3.1000,\"publicationDate\":\"2024-08-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Physical Review C\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1103/physrevc.110.024321\",\"RegionNum\":2,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"Physics and Astronomy\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physical Review C","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1103/physrevc.110.024321","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Physics and Astronomy","Score":null,"Total":0}
β-delayed neutron emission of Mn64, Cr62, and Fe65
The -decay properties of nuclei near the second nuclear “island of inversion” around neutron rich nuclei with neutron number 40 are important tests of nuclear structure models and interactions. In particular, the -delayed neutron emission branch (), is useful for investigating -strength and neutron- competition above the neutron separation energies of the daughter nuclei. We report new constraints for values for three nuclei in the region: (), (), and (), measured with the Neutron Emission Ratio Observer (NERO) neutron long counter system and the Beta Counting Station (BCS) at the National Superconducting Cyclotron Laboratory (NSCL). Our results resolve the large discrepancy between previous direct and indirect measurements for and confirm the predictions of global theoretical models when a statistical treatment of the and neutron decays of the daughter states is included. We also obtain improved half-lives for [206(5) ms] and the short-lived isomer in the daughter [112(7) ms] from -delayed emission data obtained in the same experiment with the Summing NaI (SuN) total absorption spectrometer. Finally, we use emission data to obtain a new upper limit for the -decay population of the long-lived isomeric state in .
期刊介绍:
Physical Review C (PRC) is a leading journal in theoretical and experimental nuclear physics, publishing more than two-thirds of the research literature in the field.
PRC covers experimental and theoretical results in all aspects of nuclear physics, including:
Nucleon-nucleon interaction, few-body systems
Nuclear structure
Nuclear reactions
Relativistic nuclear collisions
Hadronic physics and QCD
Electroweak interaction, symmetries
Nuclear astrophysics