First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method
Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ )...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Sun, L.J. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2023 |
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| Schlagwörter: |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Physics letters - Amsterdam : North-Holland Publ, 2011, 839 |
|---|---|
| Übergeordnetes Werk: |
volume:839 |
| DOI / URN: |
10.1016/j.physletb.2023.137801 |
|---|
| Katalog-ID: |
ELV009431020 |
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| 245 | 1 | 0 | |a First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method |
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| 520 | |a Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. | ||
| 650 | 4 | |a Lifetimes of | |
| 650 | 4 | |a Nova nucleosynthesis | |
| 650 | 4 | |a Bayesian analysis | |
| 650 | 4 | |a Markov chain Monte Carlo | |
| 700 | 1 | |a Fry, C. |4 oth | |
| 700 | 1 | |a Davids, B. |4 oth | |
| 700 | 1 | |a Esker, N. |4 oth | |
| 700 | 1 | |a Wrede, C. |4 oth | |
| 700 | 1 | |a Alcorta, M. |4 oth | |
| 700 | 1 | |a Bhattacharjee, S. |4 oth | |
| 700 | 1 | |a Bowry, M. |4 oth | |
| 700 | 1 | |a Brown, B.A. |4 oth | |
| 700 | 1 | |a Budner, T. |4 oth | |
| 700 | 1 | |a Caballero-Folch, R. |4 oth | |
| 700 | 1 | |a Evitts, L. |4 oth | |
| 700 | 1 | |a Friedman, M. |4 oth | |
| 700 | 1 | |a Garnsworthy, A.B. |4 oth | |
| 700 | 1 | |a Glassman, B.E. |4 oth | |
| 700 | 1 | |a Hackman, G. |4 oth | |
| 700 | 1 | |a Henderson, J. |4 oth | |
| 700 | 1 | |a Kirsebom, O.S. |4 oth | |
| 700 | 1 | |a Lighthall, J. |4 oth | |
| 700 | 1 | |a Machule, P. |4 oth | |
| 700 | 1 | |a Measures, J. |4 oth | |
| 700 | 1 | |a Moukaddam, M. |4 oth | |
| 700 | 1 | |a Park, J. |4 oth | |
| 700 | 1 | |a Pearson, C. |4 oth | |
| 700 | 1 | |a Pérez-Loureiro, D. |4 oth | |
| 700 | 1 | |a Ruiz, C. |4 oth | |
| 700 | 1 | |a Ruotsalainen, P. |4 oth | |
| 700 | 1 | |a Smallcombe, J. |4 oth | |
| 700 | 1 | |a Smith, J.K. |4 oth | |
| 700 | 1 | |a Southall, D. |4 oth | |
| 700 | 1 | |a Surbrook, J. |4 oth | |
| 700 | 1 | |a Weghorn, L.E. |4 oth | |
| 700 | 1 | |a Williams, M. |4 oth | |
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10.1016/j.physletb.2023.137801 doi (DE-627)ELV009431020 (ELSEVIER)S0370-2693(23)00135-1 DE-627 ger DE-627 rda eng 530 DE-600 UA 1000 rvk 33.40 bkl 33.50 bkl 39.22 bkl Sun, L.J. verfasserin (orcid)0000-0002-1619-7448 aut First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. Lifetimes of Nova nucleosynthesis Bayesian analysis Markov chain Monte Carlo Fry, C. oth Davids, B. oth Esker, N. oth Wrede, C. oth Alcorta, M. oth Bhattacharjee, S. oth Bowry, M. oth Brown, B.A. oth Budner, T. oth Caballero-Folch, R. oth Evitts, L. oth Friedman, M. oth Garnsworthy, A.B. oth Glassman, B.E. oth Hackman, G. oth Henderson, J. oth Kirsebom, O.S. oth Lighthall, J. oth Machule, P. oth Measures, J. oth Moukaddam, M. oth Park, J. oth Pearson, C. oth Pérez-Loureiro, D. oth Ruiz, C. oth Ruotsalainen, P. oth Smallcombe, J. oth Smith, J.K. oth Southall, D. oth Surbrook, J. oth Weghorn, L.E. oth Williams, M. oth Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 839 (DE-627)266015360 (DE-600)1466612-1 nnns volume:839 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHY SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2111 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 UA 1000 33.40 33.50 39.22 AR 839 |
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10.1016/j.physletb.2023.137801 doi (DE-627)ELV009431020 (ELSEVIER)S0370-2693(23)00135-1 DE-627 ger DE-627 rda eng 530 DE-600 UA 1000 rvk 33.40 bkl 33.50 bkl 39.22 bkl Sun, L.J. verfasserin (orcid)0000-0002-1619-7448 aut First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. Lifetimes of Nova nucleosynthesis Bayesian analysis Markov chain Monte Carlo Fry, C. oth Davids, B. oth Esker, N. oth Wrede, C. oth Alcorta, M. oth Bhattacharjee, S. oth Bowry, M. oth Brown, B.A. oth Budner, T. oth Caballero-Folch, R. oth Evitts, L. oth Friedman, M. oth Garnsworthy, A.B. oth Glassman, B.E. oth Hackman, G. oth Henderson, J. oth Kirsebom, O.S. oth Lighthall, J. oth Machule, P. oth Measures, J. oth Moukaddam, M. oth Park, J. oth Pearson, C. oth Pérez-Loureiro, D. oth Ruiz, C. oth Ruotsalainen, P. oth Smallcombe, J. oth Smith, J.K. oth Southall, D. oth Surbrook, J. oth Weghorn, L.E. oth Williams, M. oth Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 839 (DE-627)266015360 (DE-600)1466612-1 nnns volume:839 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHY SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2111 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 UA 1000 33.40 33.50 39.22 AR 839 |
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10.1016/j.physletb.2023.137801 doi (DE-627)ELV009431020 (ELSEVIER)S0370-2693(23)00135-1 DE-627 ger DE-627 rda eng 530 DE-600 UA 1000 rvk 33.40 bkl 33.50 bkl 39.22 bkl Sun, L.J. verfasserin (orcid)0000-0002-1619-7448 aut First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. Lifetimes of Nova nucleosynthesis Bayesian analysis Markov chain Monte Carlo Fry, C. oth Davids, B. oth Esker, N. oth Wrede, C. oth Alcorta, M. oth Bhattacharjee, S. oth Bowry, M. oth Brown, B.A. oth Budner, T. oth Caballero-Folch, R. oth Evitts, L. oth Friedman, M. oth Garnsworthy, A.B. oth Glassman, B.E. oth Hackman, G. oth Henderson, J. oth Kirsebom, O.S. oth Lighthall, J. oth Machule, P. oth Measures, J. oth Moukaddam, M. oth Park, J. oth Pearson, C. oth Pérez-Loureiro, D. oth Ruiz, C. oth Ruotsalainen, P. oth Smallcombe, J. oth Smith, J.K. oth Southall, D. oth Surbrook, J. oth Weghorn, L.E. oth Williams, M. oth Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 839 (DE-627)266015360 (DE-600)1466612-1 nnns volume:839 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHY SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2111 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 UA 1000 33.40 33.50 39.22 AR 839 |
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10.1016/j.physletb.2023.137801 doi (DE-627)ELV009431020 (ELSEVIER)S0370-2693(23)00135-1 DE-627 ger DE-627 rda eng 530 DE-600 UA 1000 rvk 33.40 bkl 33.50 bkl 39.22 bkl Sun, L.J. verfasserin (orcid)0000-0002-1619-7448 aut First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. Lifetimes of Nova nucleosynthesis Bayesian analysis Markov chain Monte Carlo Fry, C. oth Davids, B. oth Esker, N. oth Wrede, C. oth Alcorta, M. oth Bhattacharjee, S. oth Bowry, M. oth Brown, B.A. oth Budner, T. oth Caballero-Folch, R. oth Evitts, L. oth Friedman, M. oth Garnsworthy, A.B. oth Glassman, B.E. oth Hackman, G. oth Henderson, J. oth Kirsebom, O.S. oth Lighthall, J. oth Machule, P. oth Measures, J. oth Moukaddam, M. oth Park, J. oth Pearson, C. oth Pérez-Loureiro, D. oth Ruiz, C. oth Ruotsalainen, P. oth Smallcombe, J. oth Smith, J.K. oth Southall, D. oth Surbrook, J. oth Weghorn, L.E. oth Williams, M. oth Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 839 (DE-627)266015360 (DE-600)1466612-1 nnns volume:839 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHY SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2111 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 UA 1000 33.40 33.50 39.22 AR 839 |
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10.1016/j.physletb.2023.137801 doi (DE-627)ELV009431020 (ELSEVIER)S0370-2693(23)00135-1 DE-627 ger DE-627 rda eng 530 DE-600 UA 1000 rvk 33.40 bkl 33.50 bkl 39.22 bkl Sun, L.J. verfasserin (orcid)0000-0002-1619-7448 aut First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method 2023 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. Lifetimes of Nova nucleosynthesis Bayesian analysis Markov chain Monte Carlo Fry, C. oth Davids, B. oth Esker, N. oth Wrede, C. oth Alcorta, M. oth Bhattacharjee, S. oth Bowry, M. oth Brown, B.A. oth Budner, T. oth Caballero-Folch, R. oth Evitts, L. oth Friedman, M. oth Garnsworthy, A.B. oth Glassman, B.E. oth Hackman, G. oth Henderson, J. oth Kirsebom, O.S. oth Lighthall, J. oth Machule, P. oth Measures, J. oth Moukaddam, M. oth Park, J. oth Pearson, C. oth Pérez-Loureiro, D. oth Ruiz, C. oth Ruotsalainen, P. oth Smallcombe, J. oth Smith, J.K. oth Southall, D. oth Surbrook, J. oth Weghorn, L.E. oth Williams, M. oth Enthalten in Physics letters Amsterdam : North-Holland Publ, 2011 839 (DE-627)266015360 (DE-600)1466612-1 nnns volume:839 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OLC-PHY SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2004 GBV_ILN_2014 GBV_ILN_2111 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 UA 1000 33.40 33.50 39.22 AR 839 |
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Sun, L.J. @@aut@@ Fry, C. @@oth@@ Davids, B. @@oth@@ Esker, N. @@oth@@ Wrede, C. @@oth@@ Alcorta, M. @@oth@@ Bhattacharjee, S. @@oth@@ Bowry, M. @@oth@@ Brown, B.A. @@oth@@ Budner, T. @@oth@@ Caballero-Folch, R. @@oth@@ Evitts, L. @@oth@@ Friedman, M. @@oth@@ Garnsworthy, A.B. @@oth@@ Glassman, B.E. @@oth@@ Hackman, G. @@oth@@ Henderson, J. @@oth@@ Kirsebom, O.S. @@oth@@ Lighthall, J. @@oth@@ Machule, P. @@oth@@ Measures, J. @@oth@@ Moukaddam, M. @@oth@@ Park, J. @@oth@@ Pearson, C. @@oth@@ Pérez-Loureiro, D. @@oth@@ Ruiz, C. @@oth@@ Ruotsalainen, P. @@oth@@ Smallcombe, J. @@oth@@ Smith, J.K. @@oth@@ Southall, D. @@oth@@ Surbrook, J. @@oth@@ Weghorn, L.E. @@oth@@ Williams, M. @@oth@@ |
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Sun, L.J. |
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Sun, L.J. ddc 530 rvk UA 1000 bkl 33.40 bkl 33.50 bkl 39.22 misc Lifetimes of misc Nova nucleosynthesis misc Bayesian analysis misc Markov chain Monte Carlo First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method |
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First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method |
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first application of markov chain monte carlo-based bayesian data analysis to the doppler-shift attenuation method |
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First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method |
| abstract |
Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. |
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Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. |
| abstract_unstemmed |
Motivated primarily by the large uncertainties in the thermonuclear rate of the 30P ( p , γ ) 31 S reaction that limit our understanding of classical novae, we carried out lifetime measurements of 31S excited states using the Doppler Shift Lifetimes (DSL2) facility at the TRIUMF Isotope Separator and Accelerator (ISAC-II) facility. The 31S excited states were populated by the 3He ( 32 S , α ) 31 S reaction. The deexcitation γ rays were detected by a clover-type high-purity germanium detector in coincidence with the α particles detected by a silicon detector telescope. We have applied modern Markov chain Monte Carlo-based Bayesian statistical techniques to perform lineshape analyses of Doppler-shift attenuation method γ-ray data for the first time. We have determined the lifetimes of the two lowest-lying 31S excited states. First experimental upper limits on the lifetimes of four higher-lying states have been obtained. The experimental results were compared to shell-model calculations using five universal sd-shell Hamiltonians. Evidence for γ rays originating from the astrophysically important J π = 3 / 2 + , 260-keV 30P ( p , γ ) 31 S resonance with an excitation energy of E x = 6390.2 ( 7 ) keV in 31S has also been observed, although strong constraints on the lifetime will require better statistics. |
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First application of Markov chain Monte Carlo-based Bayesian data analysis to the Doppler-shift attenuation method |
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Fry, C. Davids, B. Esker, N. Wrede, C. Alcorta, M. Bhattacharjee, S. Bowry, M. Brown, B.A. Budner, T. Caballero-Folch, R. Evitts, L. Friedman, M. Garnsworthy, A.B. Glassman, B.E. Hackman, G. Henderson, J. Kirsebom, O.S. Lighthall, J. Machule, P. Measures, J. Moukaddam, M. Park, J. Pearson, C. Pérez-Loureiro, D. Ruiz, C. Ruotsalainen, P. Smallcombe, J. Smith, J.K. Southall, D. Surbrook, J. Weghorn, L.E. Williams, M. |
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|
| score |
7.3991537 |