Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo
Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed pro...
Ausführliche Beschreibung
Autor*in: |
Klepper, O. [verfasserIn] |
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Artikel |
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Sprache: |
Englisch |
Erschienen: |
1982 |
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Anmerkung: |
© Springer-Verlag 1982 |
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Übergeordnetes Werk: |
Enthalten in: Zeitschrift für Physik. A, Hadrons and nuclei - Springer-Verlag, 1975, 305(1982), 2 vom: Juni, Seite 125-130 |
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Übergeordnetes Werk: |
volume:305 ; year:1982 ; number:2 ; month:06 ; pages:125-130 |
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DOI / URN: |
10.1007/BF01415019 |
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Katalog-ID: |
OLC2029708720 |
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245 | 1 | 0 | |a Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo |
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520 | |a Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. | ||
650 | 4 | |a Evaporation | |
650 | 4 | |a Lower Limit | |
650 | 4 | |a Energy Distribution | |
650 | 4 | |a Mass Number | |
650 | 4 | |a Proton Decay | |
700 | 1 | |a Batsch, T. |4 aut | |
700 | 1 | |a Hofmann, S. |4 aut | |
700 | 1 | |a Kirchner, R. |4 aut | |
700 | 1 | |a Kurcewicz, W. |4 aut | |
700 | 1 | |a Reisdorf, W. |4 aut | |
700 | 1 | |a Roeckl, E. |4 aut | |
700 | 1 | |a Schardt, D. |4 aut | |
700 | 1 | |a Nyman, G. |4 aut | |
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10.1007/BF01415019 doi (DE-627)OLC2029708720 (DE-He213)BF01415019-p DE-627 ger DE-627 rakwb eng 530 VZ Klepper, O. verfasserin aut Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1982 Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. Evaporation Lower Limit Energy Distribution Mass Number Proton Decay Batsch, T. aut Hofmann, S. aut Kirchner, R. aut Kurcewicz, W. aut Reisdorf, W. aut Roeckl, E. aut Schardt, D. aut Nyman, G. aut Enthalten in Zeitschrift für Physik. A, Hadrons and nuclei Springer-Verlag, 1975 305(1982), 2 vom: Juni, Seite 125-130 (DE-627)129415375 (DE-600)189286-1 (DE-576)014793679 0939-7922 nnns volume:305 year:1982 number:2 month:06 pages:125-130 https://doi.org/10.1007/BF01415019 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_59 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_70 GBV_ILN_105 GBV_ILN_130 GBV_ILN_150 GBV_ILN_170 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2185 GBV_ILN_2192 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2360 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4313 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4336 GBV_ILN_4700 AR 305 1982 2 06 125-130 |
spelling |
10.1007/BF01415019 doi (DE-627)OLC2029708720 (DE-He213)BF01415019-p DE-627 ger DE-627 rakwb eng 530 VZ Klepper, O. verfasserin aut Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1982 Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. Evaporation Lower Limit Energy Distribution Mass Number Proton Decay Batsch, T. aut Hofmann, S. aut Kirchner, R. aut Kurcewicz, W. aut Reisdorf, W. aut Roeckl, E. aut Schardt, D. aut Nyman, G. aut Enthalten in Zeitschrift für Physik. A, Hadrons and nuclei Springer-Verlag, 1975 305(1982), 2 vom: Juni, Seite 125-130 (DE-627)129415375 (DE-600)189286-1 (DE-576)014793679 0939-7922 nnns volume:305 year:1982 number:2 month:06 pages:125-130 https://doi.org/10.1007/BF01415019 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_59 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_70 GBV_ILN_105 GBV_ILN_130 GBV_ILN_150 GBV_ILN_170 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2185 GBV_ILN_2192 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2360 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4313 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4336 GBV_ILN_4700 AR 305 1982 2 06 125-130 |
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10.1007/BF01415019 doi (DE-627)OLC2029708720 (DE-He213)BF01415019-p DE-627 ger DE-627 rakwb eng 530 VZ Klepper, O. verfasserin aut Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1982 Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. Evaporation Lower Limit Energy Distribution Mass Number Proton Decay Batsch, T. aut Hofmann, S. aut Kirchner, R. aut Kurcewicz, W. aut Reisdorf, W. aut Roeckl, E. aut Schardt, D. aut Nyman, G. aut Enthalten in Zeitschrift für Physik. A, Hadrons and nuclei Springer-Verlag, 1975 305(1982), 2 vom: Juni, Seite 125-130 (DE-627)129415375 (DE-600)189286-1 (DE-576)014793679 0939-7922 nnns volume:305 year:1982 number:2 month:06 pages:125-130 https://doi.org/10.1007/BF01415019 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_59 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_70 GBV_ILN_105 GBV_ILN_130 GBV_ILN_150 GBV_ILN_170 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2185 GBV_ILN_2192 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2360 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4313 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4336 GBV_ILN_4700 AR 305 1982 2 06 125-130 |
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10.1007/BF01415019 doi (DE-627)OLC2029708720 (DE-He213)BF01415019-p DE-627 ger DE-627 rakwb eng 530 VZ Klepper, O. verfasserin aut Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1982 Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. Evaporation Lower Limit Energy Distribution Mass Number Proton Decay Batsch, T. aut Hofmann, S. aut Kirchner, R. aut Kurcewicz, W. aut Reisdorf, W. aut Roeckl, E. aut Schardt, D. aut Nyman, G. aut Enthalten in Zeitschrift für Physik. A, Hadrons and nuclei Springer-Verlag, 1975 305(1982), 2 vom: Juni, Seite 125-130 (DE-627)129415375 (DE-600)189286-1 (DE-576)014793679 0939-7922 nnns volume:305 year:1982 number:2 month:06 pages:125-130 https://doi.org/10.1007/BF01415019 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_59 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_70 GBV_ILN_105 GBV_ILN_130 GBV_ILN_150 GBV_ILN_170 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2185 GBV_ILN_2192 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2360 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4313 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4336 GBV_ILN_4700 AR 305 1982 2 06 125-130 |
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10.1007/BF01415019 doi (DE-627)OLC2029708720 (DE-He213)BF01415019-p DE-627 ger DE-627 rakwb eng 530 VZ Klepper, O. verfasserin aut Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1982 Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. Evaporation Lower Limit Energy Distribution Mass Number Proton Decay Batsch, T. aut Hofmann, S. aut Kirchner, R. aut Kurcewicz, W. aut Reisdorf, W. aut Roeckl, E. aut Schardt, D. aut Nyman, G. aut Enthalten in Zeitschrift für Physik. A, Hadrons and nuclei Springer-Verlag, 1975 305(1982), 2 vom: Juni, Seite 125-130 (DE-627)129415375 (DE-600)189286-1 (DE-576)014793679 0939-7922 nnns volume:305 year:1982 number:2 month:06 pages:125-130 https://doi.org/10.1007/BF01415019 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_30 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_59 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_70 GBV_ILN_105 GBV_ILN_130 GBV_ILN_150 GBV_ILN_170 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2027 GBV_ILN_2185 GBV_ILN_2192 GBV_ILN_2221 GBV_ILN_2279 GBV_ILN_2360 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4277 GBV_ILN_4302 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4313 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4320 GBV_ILN_4323 GBV_ILN_4336 GBV_ILN_4700 AR 305 1982 2 06 125-130 |
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direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $ni+92mo |
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Direct and beta-delayed proton decay of very neutron-deficient rare-earth isotopes produced in the $ reaction^{58} $Ni+92Mo |
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Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. © Springer-Verlag 1982 |
abstractGer |
Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. © Springer-Verlag 1982 |
abstract_unstemmed |
Abstract Using on-line mass separation of evaporation residues from the $ reaction^{58} $Ni +92Mo→150Yb*, a proton line of 1,055±6 keV energy and 0.42±0.10 s half-life was observed at mass number 147. The origin of this activity is very likely the direct proton decay $ of^{147} $Tm. Beta-delayed protons registered at the same mass position show a pronounced peak structure in their energy distribution. A lower limit of their half-life was set to 1 s. © Springer-Verlag 1982 |
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score |
7.4014254 |