Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap

Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -8122...
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Autor*in:	Jaries, A. [verfasserIn] Stryjczyk, M. Kankainen, A. Eronen, T. Ge, Z. Mougeot, M. Raggio, A. Ruotsalainen, J.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2024

Anmerkung:	© The Author(s) 2024

Übergeordnetes Werk:	Enthalten in: The European physical journal - Springer Berlin Heidelberg, 1998, 60(2024), 2 vom: 17. Feb.
Übergeordnetes Werk:	volume:60 ; year:2024 ; number:2 ; day:17 ; month:02

Links:	Volltext

DOI / URN:	10.1140/epja/s10050-024-01248-z

Katalog-ID:	SPR054807107

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520			\|a Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value.
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700	1		\|a Ruotsalainen, J. \|0 (orcid)0000-0002-5589-2005 \|4 aut
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allfields	10.1140/epja/s10050-024-01248-z doi (DE-627)SPR054807107 (SPR)s10050-024-01248-z-e DE-627 ger DE-627 rakwb eng 530 VZ 33.40 bkl 33.50 bkl Jaries, A. verfasserin (orcid)0000-0002-5279-0820 aut Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. Stryjczyk, M. (orcid)0000-0001-6515-2409 aut Kankainen, A. (orcid)0000-0003-1082-7602 aut Eronen, T. (orcid)0000-0003-0003-6022 aut Ge, Z. (orcid)0000-0001-8586-6134 aut Mougeot, M. (orcid)0000-0003-1372-1205 aut Raggio, A. (orcid)0000-0002-5365-1494 aut Ruotsalainen, J. (orcid)0000-0002-5589-2005 aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 60(2024), 2 vom: 17. Feb. (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:60 year:2024 number:2 day:17 month:02 https://dx.doi.org/10.1140/epja/s10050-024-01248-z kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 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_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 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_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 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_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 VZ 33.50 VZ AR 60 2024 2 17 02
spelling	10.1140/epja/s10050-024-01248-z doi (DE-627)SPR054807107 (SPR)s10050-024-01248-z-e DE-627 ger DE-627 rakwb eng 530 VZ 33.40 bkl 33.50 bkl Jaries, A. verfasserin (orcid)0000-0002-5279-0820 aut Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. Stryjczyk, M. (orcid)0000-0001-6515-2409 aut Kankainen, A. (orcid)0000-0003-1082-7602 aut Eronen, T. (orcid)0000-0003-0003-6022 aut Ge, Z. (orcid)0000-0001-8586-6134 aut Mougeot, M. (orcid)0000-0003-1372-1205 aut Raggio, A. (orcid)0000-0002-5365-1494 aut Ruotsalainen, J. (orcid)0000-0002-5589-2005 aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 60(2024), 2 vom: 17. Feb. (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:60 year:2024 number:2 day:17 month:02 https://dx.doi.org/10.1140/epja/s10050-024-01248-z kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 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_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 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_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 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_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 VZ 33.50 VZ AR 60 2024 2 17 02
allfields_unstemmed	10.1140/epja/s10050-024-01248-z doi (DE-627)SPR054807107 (SPR)s10050-024-01248-z-e DE-627 ger DE-627 rakwb eng 530 VZ 33.40 bkl 33.50 bkl Jaries, A. verfasserin (orcid)0000-0002-5279-0820 aut Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. Stryjczyk, M. (orcid)0000-0001-6515-2409 aut Kankainen, A. (orcid)0000-0003-1082-7602 aut Eronen, T. (orcid)0000-0003-0003-6022 aut Ge, Z. (orcid)0000-0001-8586-6134 aut Mougeot, M. (orcid)0000-0003-1372-1205 aut Raggio, A. (orcid)0000-0002-5365-1494 aut Ruotsalainen, J. (orcid)0000-0002-5589-2005 aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 60(2024), 2 vom: 17. Feb. (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:60 year:2024 number:2 day:17 month:02 https://dx.doi.org/10.1140/epja/s10050-024-01248-z kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 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_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 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_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 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_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 VZ 33.50 VZ AR 60 2024 2 17 02
allfieldsGer	10.1140/epja/s10050-024-01248-z doi (DE-627)SPR054807107 (SPR)s10050-024-01248-z-e DE-627 ger DE-627 rakwb eng 530 VZ 33.40 bkl 33.50 bkl Jaries, A. verfasserin (orcid)0000-0002-5279-0820 aut Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. Stryjczyk, M. (orcid)0000-0001-6515-2409 aut Kankainen, A. (orcid)0000-0003-1082-7602 aut Eronen, T. (orcid)0000-0003-0003-6022 aut Ge, Z. (orcid)0000-0001-8586-6134 aut Mougeot, M. (orcid)0000-0003-1372-1205 aut Raggio, A. (orcid)0000-0002-5365-1494 aut Ruotsalainen, J. (orcid)0000-0002-5589-2005 aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 60(2024), 2 vom: 17. Feb. (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:60 year:2024 number:2 day:17 month:02 https://dx.doi.org/10.1140/epja/s10050-024-01248-z kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 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_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 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_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 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_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 VZ 33.50 VZ AR 60 2024 2 17 02
allfieldsSound	10.1140/epja/s10050-024-01248-z doi (DE-627)SPR054807107 (SPR)s10050-024-01248-z-e DE-627 ger DE-627 rakwb eng 530 VZ 33.40 bkl 33.50 bkl Jaries, A. verfasserin (orcid)0000-0002-5279-0820 aut Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap 2024 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © The Author(s) 2024 Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. Stryjczyk, M. (orcid)0000-0001-6515-2409 aut Kankainen, A. (orcid)0000-0003-1082-7602 aut Eronen, T. (orcid)0000-0003-0003-6022 aut Ge, Z. (orcid)0000-0001-8586-6134 aut Mougeot, M. (orcid)0000-0003-1372-1205 aut Raggio, A. (orcid)0000-0002-5365-1494 aut Ruotsalainen, J. (orcid)0000-0002-5589-2005 aut Enthalten in The European physical journal Springer Berlin Heidelberg, 1998 60(2024), 2 vom: 17. Feb. (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:60 year:2024 number:2 day:17 month:02 https://dx.doi.org/10.1140/epja/s10050-024-01248-z kostenfrei Volltext SYSFLAG_0 GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 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_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 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_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 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_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 VZ 33.50 VZ AR 60 2024 2 17 02
language	English
source	Enthalten in The European physical journal 60(2024), 2 vom: 17. Feb. volume:60 year:2024 number:2 day:17 month:02
sourceStr	Enthalten in The European physical journal 60(2024), 2 vom: 17. Feb. volume:60 year:2024 number:2 day:17 month:02
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authorswithroles_txt_mv	Jaries, A. @@aut@@ Stryjczyk, M. @@aut@@ Kankainen, A. @@aut@@ Eronen, T. @@aut@@ Ge, Z. @@aut@@ Mougeot, M. @@aut@@ Raggio, A. @@aut@@ Ruotsalainen, J. @@aut@@
publishDateDaySort_date	2024-02-17T00:00:00Z
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The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). 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spellingShingle	Jaries, A. ddc 530 bkl 33.40 bkl 33.50 Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
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topic_title	530 VZ 33.40 bkl 33.50 bkl Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
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title	Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
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title_full	Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
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title_sort	reinvestigation of $$^{91}$$sr and $$^{95}$$y atomic masses using the jyfltrap penning trap
title_auth	Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
abstract	Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. © The Author(s) 2024
abstractGer	Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. © The Author(s) 2024
abstract_unstemmed	Abstract We report on the precise mass measurements of the $$^{91}$$Sr and $$^{95}$$Y isotopes performed using the JYFLTRAP double Penning trap mass spectrometer. The mass-excess values from this work, $${\textrm{ME}(^{91}\textrm{Sr}) = -83645.5(13)}$$ keV and $${\textrm{ME}(^{95}\textrm{Y}) = -81226.4(10)}$$ keV, deviate by 6.5(52) keV and $$-18(7)$$ keV from the Atomic Mass Evaluation 2020 (AME20). In the case of $$^{91}$$Sr the new result disagrees with the ISOLTRAP value, while for $$^{95}$$Y, it agrees with the older JYFLTRAP value. © The Author(s) 2024
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title_short	Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap
url	https://dx.doi.org/10.1140/epja/s10050-024-01248-z
remote_bool	true
author2	Stryjczyk, M. Kankainen, A. Eronen, T. Ge, Z. Mougeot, M. Raggio, A. Ruotsalainen, J.
author2Str	Stryjczyk, M. Kankainen, A. Eronen, T. Ge, Z. Mougeot, M. Raggio, A. Ruotsalainen, J.
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doi_str	10.1140/epja/s10050-024-01248-z
up_date	2024-07-04T03:05:31.391Z
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Reinvestigation of $$^{91}$$Sr and $$^{95}$$Y atomic masses using the JYFLTRAP Penning trap

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