Zr/Nb isobar separation experiment for future 93Zr AMS measurement
93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in n...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lu, W. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015transfer abstract |
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| Umfang: |
5 |
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| Übergeordnetes Werk: |
Enthalten in: Editorial Comment - Unwala, Darius J. ELSEVIER, 2013, a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics, Amsterdam [u.a.] |
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| Übergeordnetes Werk: |
volume:361 ; year:2015 ; day:15 ; month:10 ; pages:491-495 ; extent:5 |
| Links: |
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| DOI / URN: |
10.1016/j.nimb.2015.01.071 |
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ELV023349832 |
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| 245 | 1 | 0 | |a Zr/Nb isobar separation experiment for future 93Zr AMS measurement |
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| 520 | |a 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. | ||
| 520 | |a 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. | ||
| 650 | 7 | |a Bragg curve |2 Elsevier | |
| 650 | 7 | |a Accelerator mass spectrometry |2 Elsevier | |
| 650 | 7 | |a 93Nb reduction chemistry |2 Elsevier | |
| 700 | 1 | |a Anderson, T. |4 oth | |
| 700 | 1 | |a Bowers, M. |4 oth | |
| 700 | 1 | |a Bauder, W. |4 oth | |
| 700 | 1 | |a Collon, P. |4 oth | |
| 700 | 1 | |a Kutschera, W. |4 oth | |
| 700 | 1 | |a Kashiv, Y. |4 oth | |
| 700 | 1 | |a Lachner, J. |4 oth | |
| 700 | 1 | |a Martschini, M. |4 oth | |
| 700 | 1 | |a Ostdiek, K. |4 oth | |
| 700 | 1 | |a Robertson, D. |4 oth | |
| 700 | 1 | |a Schmitt, C. |4 oth | |
| 700 | 1 | |a Skulski, M. |4 oth | |
| 700 | 1 | |a Steier, P. |4 oth | |
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10.1016/j.nimb.2015.01.071 doi GBV00000000000148A.pica (DE-627)ELV023349832 (ELSEVIER)S0168-583X(15)00095-6 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 610 VZ 44.85 bkl Lu, W. verfasserin aut Zr/Nb isobar separation experiment for future 93Zr AMS measurement 2015transfer abstract 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. Bragg curve Elsevier Accelerator mass spectrometry Elsevier 93Nb reduction chemistry Elsevier Anderson, T. oth Bowers, M. oth Bauder, W. oth Collon, P. oth Kutschera, W. oth Kashiv, Y. oth Lachner, J. oth Martschini, M. oth Ostdiek, K. oth Robertson, D. oth Schmitt, C. oth Skulski, M. oth Steier, P. oth Enthalten in Elsevier Unwala, Darius J. ELSEVIER Editorial Comment 2013 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam [u.a.] (DE-627)ELV011304669 volume:361 year:2015 day:15 month:10 pages:491-495 extent:5 https://doi.org/10.1016/j.nimb.2015.01.071 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_62 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 44.85 Kardiologie Angiologie VZ AR 361 2015 15 1015 491-495 5 045F 530 |
| spelling |
10.1016/j.nimb.2015.01.071 doi GBV00000000000148A.pica (DE-627)ELV023349832 (ELSEVIER)S0168-583X(15)00095-6 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 610 VZ 44.85 bkl Lu, W. verfasserin aut Zr/Nb isobar separation experiment for future 93Zr AMS measurement 2015transfer abstract 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. Bragg curve Elsevier Accelerator mass spectrometry Elsevier 93Nb reduction chemistry Elsevier Anderson, T. oth Bowers, M. oth Bauder, W. oth Collon, P. oth Kutschera, W. oth Kashiv, Y. oth Lachner, J. oth Martschini, M. oth Ostdiek, K. oth Robertson, D. oth Schmitt, C. oth Skulski, M. oth Steier, P. oth Enthalten in Elsevier Unwala, Darius J. ELSEVIER Editorial Comment 2013 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam [u.a.] (DE-627)ELV011304669 volume:361 year:2015 day:15 month:10 pages:491-495 extent:5 https://doi.org/10.1016/j.nimb.2015.01.071 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_62 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 44.85 Kardiologie Angiologie VZ AR 361 2015 15 1015 491-495 5 045F 530 |
| allfields_unstemmed |
10.1016/j.nimb.2015.01.071 doi GBV00000000000148A.pica (DE-627)ELV023349832 (ELSEVIER)S0168-583X(15)00095-6 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 610 VZ 44.85 bkl Lu, W. verfasserin aut Zr/Nb isobar separation experiment for future 93Zr AMS measurement 2015transfer abstract 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. Bragg curve Elsevier Accelerator mass spectrometry Elsevier 93Nb reduction chemistry Elsevier Anderson, T. oth Bowers, M. oth Bauder, W. oth Collon, P. oth Kutschera, W. oth Kashiv, Y. oth Lachner, J. oth Martschini, M. oth Ostdiek, K. oth Robertson, D. oth Schmitt, C. oth Skulski, M. oth Steier, P. oth Enthalten in Elsevier Unwala, Darius J. ELSEVIER Editorial Comment 2013 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam [u.a.] (DE-627)ELV011304669 volume:361 year:2015 day:15 month:10 pages:491-495 extent:5 https://doi.org/10.1016/j.nimb.2015.01.071 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_62 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 44.85 Kardiologie Angiologie VZ AR 361 2015 15 1015 491-495 5 045F 530 |
| allfieldsGer |
10.1016/j.nimb.2015.01.071 doi GBV00000000000148A.pica (DE-627)ELV023349832 (ELSEVIER)S0168-583X(15)00095-6 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 610 VZ 44.85 bkl Lu, W. verfasserin aut Zr/Nb isobar separation experiment for future 93Zr AMS measurement 2015transfer abstract 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. Bragg curve Elsevier Accelerator mass spectrometry Elsevier 93Nb reduction chemistry Elsevier Anderson, T. oth Bowers, M. oth Bauder, W. oth Collon, P. oth Kutschera, W. oth Kashiv, Y. oth Lachner, J. oth Martschini, M. oth Ostdiek, K. oth Robertson, D. oth Schmitt, C. oth Skulski, M. oth Steier, P. oth Enthalten in Elsevier Unwala, Darius J. ELSEVIER Editorial Comment 2013 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam [u.a.] (DE-627)ELV011304669 volume:361 year:2015 day:15 month:10 pages:491-495 extent:5 https://doi.org/10.1016/j.nimb.2015.01.071 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_62 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 44.85 Kardiologie Angiologie VZ AR 361 2015 15 1015 491-495 5 045F 530 |
| allfieldsSound |
10.1016/j.nimb.2015.01.071 doi GBV00000000000148A.pica (DE-627)ELV023349832 (ELSEVIER)S0168-583X(15)00095-6 DE-627 ger DE-627 rakwb eng 530 530 DE-600 610 VZ 610 VZ 44.85 bkl Lu, W. verfasserin aut Zr/Nb isobar separation experiment for future 93Zr AMS measurement 2015transfer abstract 5 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. 93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. Bragg curve Elsevier Accelerator mass spectrometry Elsevier 93Nb reduction chemistry Elsevier Anderson, T. oth Bowers, M. oth Bauder, W. oth Collon, P. oth Kutschera, W. oth Kashiv, Y. oth Lachner, J. oth Martschini, M. oth Ostdiek, K. oth Robertson, D. oth Schmitt, C. oth Skulski, M. oth Steier, P. oth Enthalten in Elsevier Unwala, Darius J. ELSEVIER Editorial Comment 2013 a journal on accelerators, instrumentation and techniques applied to research in nuclear and atomic physics, materials science and related fields in physics Amsterdam [u.a.] (DE-627)ELV011304669 volume:361 year:2015 day:15 month:10 pages:491-495 extent:5 https://doi.org/10.1016/j.nimb.2015.01.071 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_62 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 44.85 Kardiologie Angiologie VZ AR 361 2015 15 1015 491-495 5 045F 530 |
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zr/nb isobar separation experiment for future 93zr ams measurement |
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Zr/Nb isobar separation experiment for future 93Zr AMS measurement |
| abstract |
93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. |
| abstractGer |
93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. |
| abstract_unstemmed |
93Zr (t 1/2 =1.6Ma) is mostly produced by the main s-process in low-to-intermediate mass AGB stars. Large uncertainty exists in the current 92Zr(n,γ)93Zr Maxwellian Average cross section. This could have significant impact on nucleosynthesis calculations. Large amounts of 93Zr are also produced in nuclear reactors and pose long-term environmental radioactivity. Hence, measurement of 93Zr by the AMS is important for both fields above. We report here on progress in the development of AMS method to measure 93Zr. Compared with 98MeV beam energy, Zr/Nb isobar position separation was improved using 155.2MeV beam energy and Gas-Filled Magnet. Energy loss measurement with increased beam energy inside the detector indicates that higher beam energy can improve isobar energy loss separation. A chemical procedure to reduce the Nb content in Zr samples has been developed and tested. It reduces the 93Nb content by a factor of 1000. |
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