First data with the Hybrid Array of Gamma Ray Detector (HAGRiD)
The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond t...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Smith, K. [verfasserIn] Baugher, T. [verfasserIn] Burcher, S. [verfasserIn] Carter, A.B. [verfasserIn] Cizewski, J.A. [verfasserIn] Chipps, K.A. [verfasserIn] Febbraro, M. [verfasserIn] Grzywacz, R. [verfasserIn] Jones, K.L. [verfasserIn] Munoz, S. [verfasserIn] Pain, S.D. [verfasserIn] Paulauskas, S.V. [verfasserIn] Ratkiewicz, A. [verfasserIn] Schmitt, K.T. [verfasserIn] Thornsberry, C. [verfasserIn] Toomey, R. [verfasserIn] Walter, D. [verfasserIn] Willoughby, H. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Nuclear instruments & methods in physics research / B - Amsterdam [u.a.] : Elsevier, 1984, 414, Seite 190-194 |
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| Übergeordnetes Werk: |
volume:414 ; pages:190-194 |
| DOI / URN: |
10.1016/j.nimb.2017.06.028 |
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| Katalog-ID: |
ELV005089042 |
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| 245 | 1 | 0 | |a First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) |
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| 520 | |a The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. | ||
| 650 | 4 | |a LaBr | |
| 650 | 4 | |a γ-Ray detectors | |
| 650 | 4 | |a Transfer reaction | |
| 650 | 4 | |a β-Decay | |
| 650 | 4 | |a HAGRiD | |
| 650 | 4 | |a VANDLE | |
| 650 | 4 | |a JENSA | |
| 650 | 4 | |a ORRUBA | |
| 700 | 1 | |a Baugher, T. |e verfasserin |4 aut | |
| 700 | 1 | |a Burcher, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Carter, A.B. |e verfasserin |4 aut | |
| 700 | 1 | |a Cizewski, J.A. |e verfasserin |4 aut | |
| 700 | 1 | |a Chipps, K.A. |e verfasserin |4 aut | |
| 700 | 1 | |a Febbraro, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Grzywacz, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Jones, K.L. |e verfasserin |4 aut | |
| 700 | 1 | |a Munoz, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Pain, S.D. |e verfasserin |4 aut | |
| 700 | 1 | |a Paulauskas, S.V. |e verfasserin |4 aut | |
| 700 | 1 | |a Ratkiewicz, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Schmitt, K.T. |e verfasserin |4 aut | |
| 700 | 1 | |a Thornsberry, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Toomey, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Walter, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Willoughby, H. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Nuclear instruments & methods in physics research / B |d Amsterdam [u.a.] : Elsevier, 1984 |g 414, Seite 190-194 |h Online-Ressource |w (DE-627)266014585 |w (DE-600)1466524-4 |w (DE-576)074959735 |7 nnns |
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10.1016/j.nimb.2017.06.028 doi (DE-627)ELV005089042 (ELSEVIER)S0168-583X(17)30703-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.40 bkl Smith, K. verfasserin aut First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) 2017 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. LaBr γ-Ray detectors Transfer reaction β-Decay HAGRiD VANDLE JENSA ORRUBA Baugher, T. verfasserin aut Burcher, S. verfasserin aut Carter, A.B. verfasserin aut Cizewski, J.A. verfasserin aut Chipps, K.A. verfasserin aut Febbraro, M. verfasserin aut Grzywacz, R. verfasserin aut Jones, K.L. verfasserin aut Munoz, S. verfasserin aut Pain, S.D. verfasserin aut Paulauskas, S.V. verfasserin aut Ratkiewicz, A. verfasserin aut Schmitt, K.T. verfasserin aut Thornsberry, C. verfasserin aut Toomey, R. verfasserin aut Walter, D. verfasserin aut Willoughby, H. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / B Amsterdam [u.a.] : Elsevier, 1984 414, Seite 190-194 Online-Ressource (DE-627)266014585 (DE-600)1466524-4 (DE-576)074959735 nnns volume:414 pages:190-194 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2098 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.40 Kernphysik AR 414 190-194 |
| spelling |
10.1016/j.nimb.2017.06.028 doi (DE-627)ELV005089042 (ELSEVIER)S0168-583X(17)30703-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.40 bkl Smith, K. verfasserin aut First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) 2017 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. LaBr γ-Ray detectors Transfer reaction β-Decay HAGRiD VANDLE JENSA ORRUBA Baugher, T. verfasserin aut Burcher, S. verfasserin aut Carter, A.B. verfasserin aut Cizewski, J.A. verfasserin aut Chipps, K.A. verfasserin aut Febbraro, M. verfasserin aut Grzywacz, R. verfasserin aut Jones, K.L. verfasserin aut Munoz, S. verfasserin aut Pain, S.D. verfasserin aut Paulauskas, S.V. verfasserin aut Ratkiewicz, A. verfasserin aut Schmitt, K.T. verfasserin aut Thornsberry, C. verfasserin aut Toomey, R. verfasserin aut Walter, D. verfasserin aut Willoughby, H. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / B Amsterdam [u.a.] : Elsevier, 1984 414, Seite 190-194 Online-Ressource (DE-627)266014585 (DE-600)1466524-4 (DE-576)074959735 nnns volume:414 pages:190-194 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2098 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.40 Kernphysik AR 414 190-194 |
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10.1016/j.nimb.2017.06.028 doi (DE-627)ELV005089042 (ELSEVIER)S0168-583X(17)30703-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.40 bkl Smith, K. verfasserin aut First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) 2017 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. LaBr γ-Ray detectors Transfer reaction β-Decay HAGRiD VANDLE JENSA ORRUBA Baugher, T. verfasserin aut Burcher, S. verfasserin aut Carter, A.B. verfasserin aut Cizewski, J.A. verfasserin aut Chipps, K.A. verfasserin aut Febbraro, M. verfasserin aut Grzywacz, R. verfasserin aut Jones, K.L. verfasserin aut Munoz, S. verfasserin aut Pain, S.D. verfasserin aut Paulauskas, S.V. verfasserin aut Ratkiewicz, A. verfasserin aut Schmitt, K.T. verfasserin aut Thornsberry, C. verfasserin aut Toomey, R. verfasserin aut Walter, D. verfasserin aut Willoughby, H. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / B Amsterdam [u.a.] : Elsevier, 1984 414, Seite 190-194 Online-Ressource (DE-627)266014585 (DE-600)1466524-4 (DE-576)074959735 nnns volume:414 pages:190-194 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2098 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.40 Kernphysik AR 414 190-194 |
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10.1016/j.nimb.2017.06.028 doi (DE-627)ELV005089042 (ELSEVIER)S0168-583X(17)30703-6 DE-627 ger DE-627 rda eng 530 DE-600 33.05 bkl 33.40 bkl Smith, K. verfasserin aut First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) 2017 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. LaBr γ-Ray detectors Transfer reaction β-Decay HAGRiD VANDLE JENSA ORRUBA Baugher, T. verfasserin aut Burcher, S. verfasserin aut Carter, A.B. verfasserin aut Cizewski, J.A. verfasserin aut Chipps, K.A. verfasserin aut Febbraro, M. verfasserin aut Grzywacz, R. verfasserin aut Jones, K.L. verfasserin aut Munoz, S. verfasserin aut Pain, S.D. verfasserin aut Paulauskas, S.V. verfasserin aut Ratkiewicz, A. verfasserin aut Schmitt, K.T. verfasserin aut Thornsberry, C. verfasserin aut Toomey, R. verfasserin aut Walter, D. verfasserin aut Willoughby, H. verfasserin aut Enthalten in Nuclear instruments & methods in physics research / B Amsterdam [u.a.] : Elsevier, 1984 414, Seite 190-194 Online-Ressource (DE-627)266014585 (DE-600)1466524-4 (DE-576)074959735 nnns volume:414 pages:190-194 GBV_USEFLAG_U SYSFLAG_U GBV_ELV GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_187 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2098 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik 33.40 Kernphysik AR 414 190-194 |
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Smith, K. @@aut@@ Baugher, T. @@aut@@ Burcher, S. @@aut@@ Carter, A.B. @@aut@@ Cizewski, J.A. @@aut@@ Chipps, K.A. @@aut@@ Febbraro, M. @@aut@@ Grzywacz, R. @@aut@@ Jones, K.L. @@aut@@ Munoz, S. @@aut@@ Pain, S.D. @@aut@@ Paulauskas, S.V. @@aut@@ Ratkiewicz, A. @@aut@@ Schmitt, K.T. @@aut@@ Thornsberry, C. @@aut@@ Toomey, R. @@aut@@ Walter, D. @@aut@@ Willoughby, H. @@aut@@ |
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Smith, K. |
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Smith, K. ddc 530 bkl 33.05 bkl 33.40 misc LaBr misc γ-Ray detectors misc Transfer reaction misc β-Decay misc HAGRiD misc VANDLE misc JENSA misc ORRUBA First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) |
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530 DE-600 33.05 bkl 33.40 bkl First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) LaBr γ-Ray detectors Transfer reaction β-Decay HAGRiD VANDLE JENSA ORRUBA |
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First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) |
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First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) |
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Smith, K. Baugher, T. Burcher, S. Carter, A.B. Cizewski, J.A. Chipps, K.A. Febbraro, M. Grzywacz, R. Jones, K.L. Munoz, S. Pain, S.D. Paulauskas, S.V. Ratkiewicz, A. Schmitt, K.T. Thornsberry, C. Toomey, R. Walter, D. Willoughby, H. |
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first data with the hybrid array of gamma ray detector (hagrid) |
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First data with the Hybrid Array of Gamma Ray Detector (HAGRiD) |
| abstract |
The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. |
| abstractGer |
The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. |
| abstract_unstemmed |
The structure of nuclei provides insight into astrophysical reaction rates that are difficult to measure directly. These studies are often performed with transfer reactions and β-decay measurements. These experiments benefit from particle-γ coincidence measurements which provide information beyond that of particle detection alone. The Hybrid Array of Gamma Ray Detectors (HAGRiD) of LaBr3(Ce) scintillators has been designed with this purpose in mind. The design of the array permits it to be coupled with particle detector systems, such as the Oak Ridge Rutgers University Barrel Array (ORRUBA) of silicon detectors and the Versatile Array of Neutron Detectors at Low Energy (VANDLE). It is also designed to operate with the Jet Experiments in Nuclear Structure and Astrophysics (JENSA) advanced target system. HAGRiD’s design avoids compromising the charged-particle angular resolution due to compact geometries which are often used to increase the γ efficiency in other systems. First experiments with HAGRiD coupled to VANDLE as well as ORRUBA and JENSA are discussed. |
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Baugher, T. Burcher, S. Carter, A.B. Cizewski, J.A. Chipps, K.A. Febbraro, M. Grzywacz, R. Jones, K.L. Munoz, S. Pain, S.D. Paulauskas, S.V. Ratkiewicz, A. Schmitt, K.T. Thornsberry, C. Toomey, R. Walter, D. Willoughby, H. |
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