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Isomeric state of 80Y and its role in the astrophysical rp-process. / Novikov, Yu N.; Schatz, H.; Dendooven, P.; Béraud, R.; Miehé, Ch; Seliverstov, D. M.; Vorobjev, G. K.; Baumann, P.; Borge, M. J.G.; Canchel, G.; Desagne, Ph; Emsallem, A.; Huang, W.; Huikari, J.; Jokinen, A.; Knipper, A.; Kolhinen, V.; Nieminen, A.; Oinonen, M.; Penttilä, H.; Peräjärvi, K.; Piqueras, I.; Rinta-Antila, S.; Szerypo, J.; Äystö, J.

в: European Physical Journal A, Том 11, № 3, 01.12.2001, стр. 257-261.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Novikov, YN, Schatz, H, Dendooven, P, Béraud, R, Miehé, C, Seliverstov, DM, Vorobjev, GK, Baumann, P, Borge, MJG, Canchel, G, Desagne, P, Emsallem, A, Huang, W, Huikari, J, Jokinen, A, Knipper, A, Kolhinen, V, Nieminen, A, Oinonen, M, Penttilä, H, Peräjärvi, K, Piqueras, I, Rinta-Antila, S, Szerypo, J & Äystö, J 2001, 'Isomeric state of 80Y and its role in the astrophysical rp-process', European Physical Journal A, Том. 11, № 3, стр. 257-261. https://doi.org/10.1007/s100500170062

APA

Novikov, Y. N., Schatz, H., Dendooven, P., Béraud, R., Miehé, C., Seliverstov, D. M., Vorobjev, G. K., Baumann, P., Borge, M. J. G., Canchel, G., Desagne, P., Emsallem, A., Huang, W., Huikari, J., Jokinen, A., Knipper, A., Kolhinen, V., Nieminen, A., Oinonen, M., ... Äystö, J. (2001). Isomeric state of 80Y and its role in the astrophysical rp-process. European Physical Journal A, 11(3), 257-261. https://doi.org/10.1007/s100500170062

Vancouver

Novikov YN, Schatz H, Dendooven P, Béraud R, Miehé C, Seliverstov DM и пр. Isomeric state of 80Y and its role in the astrophysical rp-process. European Physical Journal A. 2001 Дек. 1;11(3):257-261. https://doi.org/10.1007/s100500170062

Author

Novikov, Yu N. ; Schatz, H. ; Dendooven, P. ; Béraud, R. ; Miehé, Ch ; Seliverstov, D. M. ; Vorobjev, G. K. ; Baumann, P. ; Borge, M. J.G. ; Canchel, G. ; Desagne, Ph ; Emsallem, A. ; Huang, W. ; Huikari, J. ; Jokinen, A. ; Knipper, A. ; Kolhinen, V. ; Nieminen, A. ; Oinonen, M. ; Penttilä, H. ; Peräjärvi, K. ; Piqueras, I. ; Rinta-Antila, S. ; Szerypo, J. ; Äystö, J. / Isomeric state of 80Y and its role in the astrophysical rp-process. в: European Physical Journal A. 2001 ; Том 11, № 3. стр. 257-261.

BibTeX

@article{17b9585dc52e404cbcfc6c64b086149a,
title = "Isomeric state of 80Y and its role in the astrophysical rp-process",
abstract = "A careful investigation of the isomeric transition of the long-lived state at 228.5 keV excitation energy in 80Y has been done. The HIGISOL facility at the Jyv{\"a}skyl{\"a} isochronous cyclotron has been used. We used the electron magnetic transporter to prepare an appropriate source and to measure the electron spectra in clean background conditions. The measured internal conversion coefficient αΚ = 0.50 ± 0.07 allows unambiguous 1- identification for the 228.5 keV first excited isomeric state in 80Y. With a bare half-life of 6.8 ± 0.5 s found in this work, this state is strongly populated in the rp-process during X-ray bursts and has therefore to be taken into account in X-ray burst model calculations. However, because of the similarity of the β-decay half-lives of isomeric and ground states, we find a maximum reduction in the effective β-decay lifetime of 80Y of only 17 ± 2%. Our results pave the way for a future investigation of the impact of the isomeric state on the {"}effective{"} 80Y proton capture rate.",
author = "Novikov, {Yu N.} and H. Schatz and P. Dendooven and R. B{\'e}raud and Ch Mieh{\'e} and Seliverstov, {D. M.} and Vorobjev, {G. K.} and P. Baumann and Borge, {M. J.G.} and G. Canchel and Ph Desagne and A. Emsallem and W. Huang and J. Huikari and A. Jokinen and A. Knipper and V. Kolhinen and A. Nieminen and M. Oinonen and H. Penttil{\"a} and K. Per{\"a}j{\"a}rvi and I. Piqueras and S. Rinta-Antila and J. Szerypo and J. {\"A}yst{\"o}",
year = "2001",
month = dec,
day = "1",
doi = "10.1007/s100500170062",
language = "English",
volume = "11",
pages = "257--261",
journal = "European physical journal A. Hadrons and nuclei",
issn = "0939-7922",
publisher = "Springer Nature",
number = "3",

}

RIS

TY - JOUR

T1 - Isomeric state of 80Y and its role in the astrophysical rp-process

AU - Novikov, Yu N.

AU - Schatz, H.

AU - Dendooven, P.

AU - Béraud, R.

AU - Miehé, Ch

AU - Seliverstov, D. M.

AU - Vorobjev, G. K.

AU - Baumann, P.

AU - Borge, M. J.G.

AU - Canchel, G.

AU - Desagne, Ph

AU - Emsallem, A.

AU - Huang, W.

AU - Huikari, J.

AU - Jokinen, A.

AU - Knipper, A.

AU - Kolhinen, V.

AU - Nieminen, A.

AU - Oinonen, M.

AU - Penttilä, H.

AU - Peräjärvi, K.

AU - Piqueras, I.

AU - Rinta-Antila, S.

AU - Szerypo, J.

AU - Äystö, J.

PY - 2001/12/1

Y1 - 2001/12/1

N2 - A careful investigation of the isomeric transition of the long-lived state at 228.5 keV excitation energy in 80Y has been done. The HIGISOL facility at the Jyväskylä isochronous cyclotron has been used. We used the electron magnetic transporter to prepare an appropriate source and to measure the electron spectra in clean background conditions. The measured internal conversion coefficient αΚ = 0.50 ± 0.07 allows unambiguous 1- identification for the 228.5 keV first excited isomeric state in 80Y. With a bare half-life of 6.8 ± 0.5 s found in this work, this state is strongly populated in the rp-process during X-ray bursts and has therefore to be taken into account in X-ray burst model calculations. However, because of the similarity of the β-decay half-lives of isomeric and ground states, we find a maximum reduction in the effective β-decay lifetime of 80Y of only 17 ± 2%. Our results pave the way for a future investigation of the impact of the isomeric state on the "effective" 80Y proton capture rate.

AB - A careful investigation of the isomeric transition of the long-lived state at 228.5 keV excitation energy in 80Y has been done. The HIGISOL facility at the Jyväskylä isochronous cyclotron has been used. We used the electron magnetic transporter to prepare an appropriate source and to measure the electron spectra in clean background conditions. The measured internal conversion coefficient αΚ = 0.50 ± 0.07 allows unambiguous 1- identification for the 228.5 keV first excited isomeric state in 80Y. With a bare half-life of 6.8 ± 0.5 s found in this work, this state is strongly populated in the rp-process during X-ray bursts and has therefore to be taken into account in X-ray burst model calculations. However, because of the similarity of the β-decay half-lives of isomeric and ground states, we find a maximum reduction in the effective β-decay lifetime of 80Y of only 17 ± 2%. Our results pave the way for a future investigation of the impact of the isomeric state on the "effective" 80Y proton capture rate.

UR - http://www.scopus.com/inward/record.url?scp=0000596724&partnerID=8YFLogxK

U2 - 10.1007/s100500170062

DO - 10.1007/s100500170062

M3 - Article

AN - SCOPUS:0000596724

VL - 11

SP - 257

EP - 261

JO - European physical journal A. Hadrons and nuclei

JF - European physical journal A. Hadrons and nuclei

SN - 0939-7922

IS - 3

ER -

ID: 47745244